prompt_front: Now, answer the following question based on the text below, only give me the answer and do not output any other words.

Question: What is the maximum radius of the emitting region for the black body model?

Read the following text and answer briefly.

Context 1: \section{Introduction}

The publicly available XMM-Newton slew data covers to date around 35\%
of the sky  The soft band (0 2$-$2 keV) sensitivity limit of the slews
(6$\times10^{-13}$\,ergs cm$^{-2}$ s$^{-1}$) is close to that of the
ROSAT All-Sky Survey (RASS; Voges et al \ 1999), and in the medium
(2$-$12 keV) band, the slew data goes significantly deeper
(4$\times10^{-12}$\,ergs cm$^{-2}$ s$^{-1}$) than all other previous
large area surveys  Over 7700 individual sources have so far been
detected to a positional accuracy of 8\arcsec   For details on the
the construction and
characteristics of the first released XMM-Newton slew survey
catalogue, see Saxton et al  (2008)  For details of the initial
science results from the slew survey, see Read et al  (2006) 

The comparison of XMM-Newton slew data with the RASS is now giving,
for the first time, the opportunity to find exotic, extreme
high-variability X-ray bursting objects, e g  tidal disruption
candidates (Esquej et al  2007), and also Galactic novae, flare stars,
and flaring white dwarfs, plus eclipsing binaries, AGN and blazars  It
is only with such a large-area survey as the XMM-Newton Slew Survey,
that transient events as these have a chance of being caught 

One such rare event, XMMSL1~J060636 2-694933, which we here show to be
a new Classical Nova, was discovered in an XMM-Newton slew from 18th
July 2006 at a very high count rate of 23 3\,ct s$^{-1}$ (EPIC-pn:
0 2$-$2\,keV)  

Classical novae (see Bode \& Evans 2008 for a review) occur in
interacting binary systems consisting of a white dwarf primary star
and a lower-mass secondary star  The nova itself is a cataclysmic
nuclear explosion caused by the accretion of material (via Roche Lobe
overflow or wind accretion) from the secondary star onto the surface
of the white dwarf; here the pressure and temperature at the base of
the accreted material becomes sufficient to trigger a thermonuclear
runaway  A recent review of the thermonuclear processes powering
classical novae can be found in Starrfield et al \ (2008)   The
accreted material is partially expelled, obscuring the X-ray emission
from the surface of the white dwarf  At later stages, the ejected
material expands further and becomes optically thin, revealing the
nuclear burning on the surface of the white dwarf   This emission
peaks in the soft X-ray regime and it is known as the super-soft
source (SSS) state (Krautter 2008)  Models of the classical nova SSS
state can be found in Tuchman \& Truran (1998) and Sala \& Hernanz
(2005) 

Though many classical novae have been observed in X-rays in their SSS
states (Ness et al \ (2007) for example discuss several examples observed with
Swift), it is in the optical band, early in their outbursts, that
classical novae are almost always discovered  This is because they are
intrinsically optically bright and easily found in inexpensive
wide-area shallow surveys   XMMSL1~J060636 2-694933 is very unusual
therefore in that it has been discovered, as we shall see, later in
its evolution, in the SSS X-ray state 

In this paper we describe the XMM-Newton slew observations
(Section~2), and the follow-up X-ray observations by the Swift XRT
(Section~3) and XMM-Newton (Section~4)  Multiwavelength observations
with Swift-UVOT, Magellan and ASAS are described in Section~5  We then
present a discussion of the results (Section~6), and conclusions 



\begin{table*}[t]
  \caption[]
  {Details of the four XMM-Newton Slew observations and the single (Rev \,1378) 
    dedicated XMM-Newton pointed observation  XMM-Newton revolution, date and observation ID 
    are tabulated, together with the 0 2$-$2 0\,keV X-ray properties of XMMSL1~J060636 2-694933;  
    position, background-subtracted counts, exposure, count-rate, and detection likelihood  For the 
    Rev \,1378 dedicated observation, these properties are given for all the EPIC cameras combined   
    For the slew observations, only the EPIC-pn values are given  In the first two slews the source 
    was not detected, and upper limits are shown in the table }
  \centering
\begin{tabular}{lccccrrrr}
\hline
Rev  & Date & Obs \,ID & RA(J2000)   & Dec(J2000) & Counts         & Exposure & Count rate  & Lik  \\ 
     & (UT) &        &     &            &                & (s) & (s$^{-1}$)  &      \\ \hline 
 351 (slew) & 07/11/01 &  9035100003  &        &               & $<$3 6     & 8 8 & $<$0 41 & $<$$\sim$8      \\
 750 (slew) & 12/01/04 &  9075000003  &        &               & $<$3 2     & 17 3 & $<$0 18 & $<$$\sim$8      \\  
1210 (slew )& 18/07/06 &  9121000003  & 06:06:36 2 & -69:49:33 & 228 8$\pm$14 1 & 9 8 & 23 4$\pm$1 4 & 1777 1   \\ 
1246 (slew) & 28/09/06 &  9121460003  & 06:06:36 5 & -69:49:38 &  12 9$\pm$2 4  & 3 4 &  3 8$\pm$0 7 &   54 7   \\
\vspace{-3 5mm}\\
\hline 
1378 (pointed) & 19/06/07 &  0510010501  & 06:06:36 5 & -69:49:37 & 1511 0$\pm$44 8 & 8940 0 &  0 20$\pm$0 01 & 4630 4          \\
\hline
\end{tabular}
\label{slewtable}
\end{table*}

\section{XMM-Newton slew observations}

XMMSL1~J060636 2-694933 was discovered in XMM-Newton slew 9121000003
from revolution 1210 on 18th July 2006  Details of the standard
XMM-Newton slew data reduction and analysis used, plus the
source-searching and catalogue cross-correlation etc , are presented
in Saxton et al   (2008) 

The source passed through the EPIC-pn detector in 14\,s, at a small
off-axis angle, such that an effective vignetting-corrected soft band
(0 2$-$2\,keV) exposure time of 9 8\,s was achieved   A total of 229
source counts lie within a radius of 20\arcsec, yielding a (EPIC-pn:
0 2$-$2\,keV) count rate of 23 4\,ct s$^{-1}$ 

The source is seen to have no cross-correlation identifications in the
RASS, and no other multiwavelength candidates within 30\arcsec\ in
Simbad\footnote{http://simbad u-strasbg fr/simbad/},
NED\footnote{http://nedwww ipac caltech edu/index html}, and
HEASARC\footnote{http://heasarc gsfc nasa gov/}  The position of the
source in the sky is such that it lies apparently at the outer eastern
edge of the LMC 

XMM-Newton has slewed over this region of sky a number of times, and
though nothing was detected in previous slews from 7th November 2001
and 12th January 2004, the source was seen again on 28th September
2006 (rev \,1246, 72 days after the rev \,1210 discovery), at the same
position, but at a reduced flux level (3 8\,ct s$^{-1}$; EPIC-pn:
0 2$-$2\,keV)   i e  it had reduced in flux by a factor of $\approx$6
in 72 days  XMM-Newton has not slewed over this area of sky since
rev \,1246  Details of the relevant XMM-Newton slews, together with
the (0 2$-$2\,keV) EPIC-pn source position, detected source counts,
count rate and detection likelihood are given in
Table~\ref{slewtable} 

The fact that XMMSL1 J060636 2-694933 is detected in the total-band
(0 2$-$12\,keV) and the soft-band (0 2$-$2\,keV), whilst effectively
zero counts are seen in the hard-band (2$-$12\,keV), is immediately
indicative of the source being very soft  

The moderately high count rate indicates that the spectrum is affected
by pile-up (the on-axis limit is 6\,ct s$^{-1}$ for EPIC-pn full-frame
mode
\footnote{http://xmm esac esa int/external/xmm\_user\_support/documentation
  /uhb\_2 5/index html})  This distorts the spectrum and makes
quantitative spectral analysis of the slew data difficult  We
minimized these effects by following the standard procedure, i e 
ignoring the central part of the Point Spread Function (PSF), and
extracted an event spectrum (containing single and double events) of
the source from within an annulus of 5\arcsec$-$30\arcsec\ radius,
centred on the source position  Unresolved problems associated with
the motion of sources across the detector still exist within slew
data, and approximations currently have to be made when calculating
the associated effective area and detector response matrix files  In
order to perform qualitative spectral analysis, an effective area file
was generated by averaging the individual core-removed effective area
files at 9 different positions along the detector track made by the
source  This accounts for the removal of the piled-up core, and takes
the vignetting and PSF variations into account to a good
approximation   Individual BACKSCAL values have been set by hand, as
have the EXPOSURE values, estimated by calculating the distance
travelled by the source in detector coordinates and finding the time
taken to do this, given a 90\,deg\,hr$^{-1}$ slew speed, then
subtracting the appropriate fractions for chip gaps and bad pixels 
For the response matrix, we used the equivalent canned detector
response matrix for the vignetting-weighted average source position,
for single plus double events and for full-frame mode:
epn\_ff20\_sdY6\_v6 9 rmf  A background spectrum was extracted from a
much larger circular region close to the source and at a similar
off-axis angle 

To fit the slew spectral data, and indeed all the high-energy spectra
in the present paper, the
XSPEC\footnote{http://heasarc gsfc nasa gov/docs/xanadu/xspec/}
spectral fitting package has been used  As $\chi^2$ minimization is
not valid when fitting spectra of low statistical quality, for the
fitting of the slew spectrum (and all the spectral fitting in the
present paper), C-statistics have been used  To take into account the
absorbing column along the line of sight, the {\em wabs} model with
the {\em wilm} cosmic abundance table (Wilms et al \ 2000) has been
used throughout the paper  All the errors quoted in the present paper
are 90\% confidence intervals, unless otherwise stated 

The rev \,1210 slew spectrum shows that the source is very soft, and
appears consistent with a 63$_{-10}^{+12}$\,eV black body, absorbed by
a hydrogen column density of
8 2$_{-4 1}^{+5 4}\times10^{20}$\,cm$^{-2}$  The fit is good, with a
P-statistic value of 0 11, obtained via the XSPEC {\em goodness}
command for this fit, based on 5000 random simulations  The best-fit
hydrogen column is equal to the full Galactic hydrogen column in the
direction of the source (8 0$\pm{1 1}\times10^{20}$\,cm$^{-2}$; Dickey
\& Lockman, 1990, calculated via the FTOOL {\em
  nh}\footnote{http://heasarc gsfc nasa gov/lheasoft/ftools/fhelp/nh txt}) 
The slew spectrum, plus the best fit simple black body model and the
deviations from the model, are shown in Fig \,\ref{slewspec}  The
observed count rate corresponds to a (0 2$-$2\,keV) flux, corrected
for the removal of the saturated PSF core, of
4 8$^{+2 7}_{-1 6}\times10^{-11}$\,ergs cm$^{-2}$ s$^{-1}$ (an
increase in flux over the RASS upper limit, assuming the same spectral
model, by a factor of more than 500) 

Simple power-law, thermal Bremmstrahlung, and other optically thin hot
plasma models are unable to fit the spectrum adequately well   Given
that we later are able to identify the source as a nova (Section~5 2),
then the black-body model will likely be a good approximation 
Furthermore, as we have obtained here a moderate number of slew
counts, the more physically realistic, though more complex atmosphere
model for CO white dwarfs of MacDonald \& Vennes (1991), provided by
K \,Page (private communication), was attempted   This model, used
e g  to model the nova V1974 Cyg (Balman et al \ 1998), yielded a
marginal fit (and not formally a more statistically significant fit;
P-statistic = 0 03, based on 5000 random simulations), with an
effective temperature of 70$^{+8}_{-6}$\,eV, an $N_{\rm H}$ of
3 7$^{+3 2}_{-2 5}$$\times$$10^{20}$\,cm$^{-2}$, and a PSF-corrected
(0 2$-$2\,keV) flux of 4 5$^{+1 3}_{-1 8}\times10^{-11}$\,ergs
cm$^{-2}$ s$^{-1}$  Note that a smaller $N_{\rm H}$ (though perhaps
still consistent with the full Galactic hydrogen column) is now
obtained using the white dwarf atmosphere model  (Note that the
MacDonald \& Vennes (1991) ONe white dwarf atmosphere model was also
attempted, but yielded a marginally worse fit than the CO white dwarf
atmosphere model; only the CO atmosphere model has been used in the
subsequent analysis) 

It is well known (e g  Krautter et al \ 1996) that, because of the
energy-dependent opacity in the white dwarf atmosphere, fits to super
soft source novae spectra with black body models give larger fluxes
and lower temperatures than atmosphere models fit to the same spectra,
and this is seen in the present case  Thus the black body model
requires a larger $N_{\rm H}$ to fit the same data than the atmosphere
model, as is seen  

The model normalizations, corrected for the removal
of the saturated PSF core, can be used to derive an approximate
distance to the source   If we assume a typical emitting region for
the white dwarf atmosphere to be of spherical radius 10$^{9}$\,cm,
then, for the black body model, this distance turns out to be
20$^{+31}_{-10}$\,kpc  The effects discussed above however can lead to
usage of the black body model giving rise to an underestimation of the
distance   For the white dwarf atmosphere model, a larger distance of
71$^{+27}_{-23}$\,kpc is obtained  Both estimates are consistent with
the distance to the LMC ($\sim$50\,kpc, see Section~6), and assuming a
distance of 50\,kpc, the black body derived flux corresponds to a
(pile-up corrected) 0 2$-$2\,keV X-ray luminosity of
1 4$^{+0 8}_{-0 5}\times10^{37}$\,ergs s$^{-1}$ 


\begin{figure}
\centering
\includegraphics[bb=100 20 575 700,clip,width=6 0cm,angle=270]{12082f1 ps}
\caption{XMM-Newton Slew spectrum of XMMSL1 J060636 2-694933 from
  XMM-Newton revolution 1210   The data points (crosses; adjacent data
  bins having been grouped together for the plot to have a significance of at least
  3) have been fitted with a black body model (kT=63\,eV; see text) 
  The solid line shows the best fit to the spectrum  The ratio of the
  data to the best fit model is shown in the lower panel }
\label{slewspec}
\end{figure}


\section{Swift XRT X-ray observations}

We requested and received a prompt observation with Swift of this
source before it moved out of the Swift visibility window in April
2007  We received over 14\,ksec of Swift-XRT time in 7
separate observations and the details of these observations are listed
in Table~\ref{xrttable}  All of the observations were in photon
counting mode and none of the observations showed any times of
significant high-BG flux  In none of the observations did the source
position coincide with any of the dead (micrometeorite-induced)
detector columns  The analysis has been performed using HEASOFT
v6 1 2  The individual XRT observations were astrometrically-corrected
and then stacked to ascertain a best Swift-XRT position $-$ this was
found to be 06 06 37 00 -69 49 33 9 (with a 90\% error radius of
4 0\arcsec)  Source counts were then extracted from each observation
from a circle of radius of 40\arcsec\ at this position  Background
counts were extracted from each observation from large-radius
off-source circles close to the source position  Source counts and
count rates for the individual XRT observations are given in
Table~\ref{xrttable} 


\begin{table}
  \caption[]{Details of the Swift-XRT observations (observation ID, observation date and 
    cleaned exposure time) are tabulated, together with the total (0 2$-$2 0\,keV) background-subtracted 
    counts and count rate from XMMSL1 J060636 2-694933 (see text) }
  \centering
\begin{tabular}{ccrrr}
\hline
ID          & Date     & Exp  & Counts       & Count rate       \\ 
            &   (UT)   &  (s) &              & (s$^{-1}$)        \\ \hline 
00030895001 & 28/02/07 & 1955 & 23 9$\pm$5 1 & 0 0122$\pm$0 0026  \\
00030895002 & 07/03/07 & 1796 & 15 8$\pm$4 2 & 0 0088$\pm$0 0024 \\
00030895003 & 08/03/07 & 1651 & 10 9$\pm$3 6 & 0 0066$\pm$0 0022 \\
00030895004 & 08/03/07 & 2547 & 20 6$\pm$4 8 & 0 0081$\pm$0 0019 \\
00030895005 & 10/03/07 & 2550 & 29 5$\pm$5 7 & 0 0116$\pm$0 0022 \\
00030895006 & 20/03/07 &  552 &  8 6$\pm$3 2 & 0 0156$\pm$0 0057 \\
00030895007 & 22/03/07 & 3391 & 24 4$\pm$5 4 & 0 0072$\pm$0 0016 \\
\hline
\end{tabular}
\label{xrttable}
\end{table}

The observation naturally fell into three time-separated groups, those
of obs \,1, obs \,2-5 and obs \,6-7  A similar analysis applied to
these groups (where the statistics are improved) gives rise to source
counts and count rates of 76 7$\pm$9 3\,counts and
0 0090$\pm$0 0011\,ct~s$^{-1}$ (for obs \,2-5), and
33 0$\pm$6 2\,counts and 0 0084$\pm$0 0016\,ct~s$^{-1}$ (for
obs \,6-7)  (Analysis of all the data together yields
133 6$\pm$12 3\,counts and 0 0092$\pm$0 0009\,ct~s$^{-1}$)  

A spectrum was extracted from all the Swift-XRT data from a 40\arcsec\
radius circle, using grades 0$-$12, centred on the Swift-XRT position 
A background spectrum was extracted again from all the Swift-XRT data,
from large-radius off-source circles close to the source position  An
ARF file was created using {\em xrtmkarf} and the appropriate RMF
(swxpc0to12\_20010101v008 rmf) from the Swift-XRT Calibration Database
was obtained 

Standard spectral models were again fit to the spectral data using
XSPEC  Again, C-statistics were used, as was the {\em wabs} absorption
model with the {\em wilm} cosmic abundance table  It was again 
obvious that only a very soft spectrum would be appropriate for the
data, and the only simple model that was able to fit the data
adequately was a black-body model of temperature
$kT$=$59^{+14}_{-10}$\,eV, with an absorbing hydrogen column of
9 5$^{+5 0}_{-3 9}$$\times$$10^{20}$\,cm$^{-2}$  No sufficiently constrained parameters could
be obtained using the CO white dwarf atmosphere model (MacDonald \&
Vennes 1991)  The Swift-XRT spectrum, together with the best-fit black
body model is shown in Fig \,\ref{xrtspec}  The corresponding
(0 2$-$2 0\,keV) flux is 2 7$^{+0 7}_{-1 2}\times10^{-13}$\,ergs
cm$^{-2}$ s$^{-1}$ (i e  a reduction by more than a factor 100 from
the XMM-Newton slew discovery flux), and the X-ray luminosity, for the
assumed distance of 50\,kpc, is 8 0$^{+2 2}_{-3 5}\times10^{34}$\,ergs
s$^{-1}$ 

\begin{figure}
\centering
\includegraphics[bb=100 15 580 710,clip,width=6 0cm,angle=270]{12082f2 ps}
\caption{Swift-XRT spectrum from XMMSL1 J060636 2-694933  The data
  points (crosses; adjacent data bins having been grouped together for
  the plot to have a significance of at least 3) have been fitted with
  a black body model (kT=59\,eV; see text)  The source has faded by a
  factor of $>100$ since the XMM-Newton revolution 1210 slew
  discovery  The solid line show the best fit to the spectra   The
  ratio of the data to the best fit model is shown in the lower panel 
}
\label{xrtspec}
\end{figure}

A cautious estimate of the size of the emitting region can be obtained
from the model normalization; the assumed distance of 50\,kpc yields a
maximum radius of 4 5$\times$10$^{8}$\,cm (the fit normalization is
essentially unconstrained at the lower bound)   Though great care
should be taken in interpreting this result, as the black body model
is possibly overestimating the luminosity, this obtained radius is
still consistent with that of moderately massive ($>$1 1$M_{\odot}$)
white dwarfs (Hamada \& Salpeter 1961), i e \,the whole white dwarf
surface may still be emitting at 59\,eV 

\section{Dedicated XMM-Newton observations}

We were granted an XMM-Newton Target of Opportunity (ToO) observation,
once the source became again visible to XMM-Newton, and a 10\,ks
XMM-Newton EPIC observation was made on 19th June 2007 (see
Table~\ref{slewtable})  All the XMM-Newton EPIC data, i e   the data
from the two MOS cameras and the single pn camera, were taken in
full-frame mode with the thin filter in place   These data from the
three EPIC instruments have been reprocessed using the standard
procedures in XMM-Newton SAS (Science Analysis System) $-$ v 7 1 0 
Periods of high-background, of which there were very few, were
filtered out of each dataset by creating a high-energy 10$-$15\,keV
lightcurve of single events over the entire field of view, and
selecting times when this lightcurve peaked above 0 75\,ct s$^{-1}$
(for pn) or 0 25\,ct s$^{-1}$ (for MOS)  This resulted in
$\approx$9 4(8 0)\,ks of low-background MOS(pn) data  Details of this dedicated
XMM-Newton observation, together with source position, and
(0 2$-$2\,keV) all-EPIC combined (pn, MOS1, MOS2) detected source
counts, count rate and detection likelihood are given in
Table~\ref{slewtable} 

Source spectra, containing single and double events, were extracted
from the datasets from circles (none of the data were now piled up)
centred on the source position  An extraction radius, estimated from
where the radial surface brightness profile was seen to fall to the
surrounding background level, was set to 30\arcsec  Background spectra
were extracted from each cleaned dataset from a 40\arcsec$-$80\arcsec\
annulus centred on the source position  Point sources seen to
contaminate these larger-area background spectra were removed from the
background spectra to a radius of 60\arcsec  ARF files were created
for the source spectra, and were checked to confirm that the correct
extraction area calculations had been performed  Finally RMF response
files were generated 
 
Standard spectral models were again fit to the spectral data using
XSPEC  Once again it was obvious that only a very soft model would fit the data; the only
simple model that was able to fit the data well (a P-statistic = 0 17,
based on 5000 random simulations) was a black-body model of
temperature $kT$=70$^{+3}_{-4}$\,eV, with an absorbing hydrogen column
of 6 9$^{+1 0}_{-1 6}\times10^{20}$\,cm$^{-2}$  The spectrum, together with this best-fit
model are shown in Fig \,\ref{xmmspec}  The corresponding
(0 2$-$2 0\,keV) flux is only marginally less than the Swift-XRT value
at 2 2$^{+0 8}_{-0 9}\times10^{-13}$\,ergs cm$^{-2}$ s$^{-1}$ and the
X-ray luminosity (for the assumed distance of 50\,kpc) is
6 7$^{+2 5}_{-2 8}\times10^{34}$\,ergs s$^{-1}$ 

\begin{figure}
\centering
\includegraphics[bb=110 15 570 705,clip,width=6 0cm,angle=270]{12082f3 ps}
\caption{XMM-Newton ToO spectrum from XMMSL1 J060636 2-694933  The
  data points (crosses; adjacent data bins having been grouped
  together for the plot to have a significance of at least 3)) have
  been fitted again with a black body model (kT=70\,eV) (see text) 
  EPIC-pn data is shown in black, with EPIC-MOS1 in red and EPIC-MOS2
  in green  The solid lines show the best fit to the spectra   The
  ratios of the data to the best fit model are shown in the lower
  panel }
\label{xmmspec}
\end{figure}

Given that, in this XMM-Newton ToO observation, we had obtained a
larger number of counts ($\raisebox{-1mm}{$\stackrel{>}{\sim}$}$1500 over the 3 EPIC cameras), the
physically more realistic CO white dwarf atmosphere model (MacDonald \&
Vennes 1991) was also attempted  This yielded a marginal fit (and formally
a no more statistically significant fit; P-statistic = 0 04, based on
5000 random simulations), with an effective temperature of
73$^{+3}_{-2}$\,eV, and an $N_{\rm H}$ of
3 4$^{+0 8}_{-0 8}$$\times$$10^{20}$\,cm$^{-2}$  Again, usage of the black body model results
in a larger fitted $N_{\rm H}$ and a lower fitted temperature than
with the atmosphere model  


As before, the model normalization can be used to obtain a cautious
estimate of the size of the emitting region  For the assumed distance
of 50\,kpc, then the black body model returns an emitting region
radius of only 1 3$\pm$0 2$\times$10$^{8}$\,cm   Again care should be
taken, as this may be an overestimation, the black body model having
perhaps overestimated the luminosity  For the white dwarf atmosphere
model, a smaller radius of 0 4$\pm$0 1$\times$10$^{8}$\,cm is
obtained  Note further that the assumption of a larger distance (see
Section~6) would result in a proportionally larger emitting radius 
The range in allowed radius therefore is quite large, and it is not
impossible for for the whole of the white dwarf surface to be emitting
at 70\,eV  If this is the case, then the white dwarf would have to be
at the high end of the mass range ($>$1 2$M_{\odot}$; Hamada \&
Salpeter 1961)  It may be the case then that we are at this point at,
or close to the end of the SSS phase, where the effective temperature
has reached a maximum (Sala \& Hernanz 2005), as is tentatively seen
in the spectral fitting results, and where the photospheric radius has
reached a minimum, close to the white dwarf radius 


\subsection{X-ray variability}

The full (XMM-Newton slew plus Swift-XRT plus XMM-Newton ToO) X-ray
lightcurve of XMMSL1 J060636 2-694933 is shown in
Fig \,\ref{lightcurve}  The calculated (0 2$-$2 0\,keV) flux values
are shown plotted against the number of days since the rev \,1210
XMM-Newton Slew discovery  The first two data points are the
rev \,1210 and the rev \,1246 XMM-Newton Slew observations  Then the
three nested Swift-XRT points are shown and finally the XMM-Newton ToO
observation  The level of RASS upper limit is shown to the bottom
left  The (0 2$-$2 0\,keV) X-ray flux is seen to have dropped by more
than two orders of magnitude in 230 days since the discovery, but is
then seen to have levelled off for the next 120 days, at a level still
$\approx$3 times that of the RASS  Finally, no evidence for any
short-term variability (using time bins down to 100\,s) is seen in the
highest statistic continuous X-ray lightcurve (the $\approx$8 0\,ksec
background-filtered EPIC-pn lightcurve) obtained from the 19/06/07
XMM-Newton observation 

\begin{figure}
\centering
\includegraphics[bb=60 60 550 454,clip,width=8 7cm]{12082f4 ps}
\caption{The full X-ray lightcurve of XMMSL1 J060636 2-694933  Plotted
  are the calculated (0 2$-$2 0\,keV) flux values versus time  The
  first point is the rev \,1210 XMM-Newton Slew observation, then the
  rev \,1246 XMM-Newton Slew observation  The three nested Swift-XRT points
  are shown next and finally the XMM-Newton ToO observation  The RASS upper
  limit is shown bottom left  }
\label{lightcurve}
\end{figure}


\section{Multi-wavelength Follow-up}

\subsection{Swift UVOT}

For the Feb/Mar 2007 Swift observations, we arranged for both the
Swift UVOT-B filter and the UVOT-UVW2 filters to be used in an
approximate exposure time ratio of 1:5, thus ensuring roughly equal
numbers of counts in the two bands (though there is a spectral type
dependency here)  Swift UVOT images in these two filters of the area
of sky around XMMSL1 J060636 2-694933 are shown in Fig \,\ref{uvot} 

Prior to the Swift UVOT observations, a `best-guess' to the possible
candidate optical/IR counterpart would have been the USNO-A2 0 source
0150-04066298 (B~mag: 17 4, R~mag: 16 1), seen 4\arcsec\ south of the
XMM-Newton slew position  The UVOT images however immediately showed
that the optically fainter source at position RA, Dec (J2000) = 06 06
36 4, -69 49 34 3 (error radius: ~0 5\arcsec) was a very strong UVW2
source and very blue, and was very likely the true counterpart to
XMMSL1~J060636 2-694933  (The UVW2 filter spans approximately
800\AA\,, centred at $\approx$1900\AA)

\begin{figure}
\centering
\includegraphics[bb=-82 210 695 585,clip,width=8 7cm]{12082f5 ps}
\caption{Swift UVOT images of the field around XMMSL1 J060636 2-694933 from observation
  00030895002  Left shows the UVOT B-filter and right shows the the
  UVOT UVW2-filter  The large circle is a 20\arcsec\ radius circle around
  the XMM-Newton Slew position  The small circle in the UVW2 image around the
  bright source is reproduced in the B image, indicating that a faint
  optical source is also visible at this position }
\label{uvot}
\end{figure}

The Swift UVOT pipeline processed data were analysed using the UVOT
photometry package {\em uvotsource} released with
FTOOLs\footnote{http://heasarc nasa gov/lheasoft/ftools/ftools\_menu html} 
This package performs aperture photometry on pre-specified source and
background regions, accounting for photometric- (via PSF fitting) and
coincidence loss- effects using the UVOT calibration files  Source
counts were extracted using a 5\arcsec\ radius aperture centred on the
source, while for the background we used a 10\arcsec\ radius aperture
located in a nearby source-free region   We used a larger background
aperture to effectively smooth over the modulo-8 fixed pattern noise
present in UVOT observations and to improve the statistics of the
background counts  Source counts were converted to UVOT UV-magnitudes
using the UVW2 zero-point calibration released with version~2 8 (Build
22) of the CALDB  The source is seen (see Fig \,\ref{uvotlc}) to be
roughly constant over the short duration of the Swift observations,
with a suggestion of a decline towards the end  This is in keeping
with the general form of the X-ray lightcurve (Fig \,\ref{lightcurve})
at this time 

\begin{figure}
\centering
\includegraphics[bb=80 70 535 380,clip,width=8 7cm]{12082f6 ps}
\caption{Variation of the UVW2 magnitude of the bright UV source
  during the Swift observations  The same time axis as
  Fig \,\ref{lightcurve} has been used to aid comparison, and a zoom
  is also shown  The UVW2 filter was only employed during observations
  00030895002, 00030895004, 00030895005, 00030895006 \& 00030895007
  (hence the points span the dates 07/03/07 to 22/03/07)  The errors here are 1-$\sigma$  }
\label{uvotlc}
\end{figure}

It is possible to include the UVOT-detected flux with the XRT spectrum
described in Section~3  UVOT files, created using {\em uvot2pha} for
the five observations (00030895002, 00030895004, 00030895005,
00030895006 \& 00030895007) where the UVW2 filter was employed, were
incorporated into {\em xspec}, along with the appropriate response
file (swuw2\_20041120v104 rsp) from the Swift-XRT Calibration
Database  We attempted to fit a single black-body spectrum to the
Swift-XRT+UV data (again using C-statistics, the {\em wabs} absorption
model and the {\em wilm} cosmic abundance table, plus the inclusion of
the {\em xspec-redden} component to model the absorption in the UV
band)  The best fit however, with a much lower temperature of
$kT$=$36^{+3}_{-4}$\,eV, is a very poor fit to the data; we obtain a
{\em goodness} P-statistic value of 0 00, based on 5000 random
simulations  This notwithstanding, a flux in the UVW2
(1 57$-$7 77\,eV) band of 3 5$\pm{0 2}\times10^{-13}$\,ergs cm$^{-2}$
s$^{-1}$ can be obtained, corresponding to a UVW2 luminosity, for the
assumed distance of 50\,kpc, of 1 0$\pm{0 1}\times10^{35}$\,ergs
s$^{-1}$ 

The very poor single black-body fit above, plus the large change in
fitted temperature is strongly suggestive that a model other than, or
in addition to the XRT-derived kT=59\,eV black body model (Section~3)
should be used to describe the UVW2 data  As we have no UV data other
than in the UVW2 filter, all that can be done is to apply the
XRT-derived black body model to the UVW2+XRT data, and in doing this,
a large flux excess with respect to the XRT-derived black body model
is seen in the UVW2 band  This is shown in Fig \ref{xrtuvotspec}  This
excess in UV emission (most of the $10^{35}$\,ergs s$^{-1}$ discussed
above) is likely due to a combination of residual post-nova nuclear
burning on the surface of the white dwarf, plus accretion in the disk,
including from emission lines  The situation is likely to be rather
complex, depending on the structure of both the ejecta and the
accretion disk, and is beyond the scope of the present work, where we
only have sparse UV data   For a review of the UV emission from
classical novae, see Shore (2008) 


\begin{figure}
\centering
\includegraphics[bb=100 15 580 710,clip,width=6 0cm,angle=270]{12082f7 ps}
\caption{Swift-XRT spectrum (black) from XMMSL1 J060636 2-694933, plus
  the best-fit black-body model to this spectrum (Section~3; Fig \,2),
  but extending into the UV to the Swift-UVOT UVW2 flux points (coloured)
  (see text)  The data points are plotted such that adjacent data
  bins have been grouped together to have a significance of at least
  3  The solid line show the best fit to the Swift-XRT spectrum  The
  ratio of the data to the best fit model is shown in the lower
  panel }
\label{xrtuvotspec}
\end{figure}


\subsection{Magellan optical observations}

On Nov ~13, 14, and 15, 2007, XMMSL1~J060636 2--694933 was observed
with the Low--Dispersion Survey Spectrograph 3 (LDSS3) mounted on the
Magellan Clay telescope  Images were obtained through the Sloan
$g^\prime$, $r^\prime$ and $i^\prime$ filters  On Nov ~15, 2007
conditions were photometric and the Landolt field RU 149A was observed
to flux calibrate the data in the $g^\prime$, $r^\prime$ and
$i^\prime$--bands   The Landolt (1992) magnitudes of the standards
were converted to Sloan magnitudes using the transformations presented
in Smith et al \ (2002)  All the images were debiased and flatfielded
using dome flatfield frames  We applied aperture photometry on each of
the images using DAOPHOT in \textsc{IRAF}\footnote{\textsc {iraf} is
  distributed by the National Optical Astronomy Observatories} to
compute the instrumental magnitudes of the stars  Differential
photometry of the optical counterpart to XMMSL1~J060636 2-694933
(marked by an arrow in Fig ~\ref{magellan}) was performed with respect
to the field star (marked with a `c' in Fig ~\ref{magellan})  This was the
brightest isolated and unsaturated star common to all frames   The
calibrated brightness of this comparison star is $g'= 18 42 \pm 0 04$,
$r'= 17 85 \pm 0 06$ and $i'=17 58 \pm 0 07$ 

\begin{figure}
\centering
\includegraphics[bb=35 215 575 575,clip,width=8 7cm]{12082f8 ps}
\caption{Magellan Clay LDSS3 finder chart  The counterpart to
  XMMSL1~J060636 2-694933 (and the bright Swift-UVOT UVW2-filter
  source; Figs \ref{uvot}\&\ref{uvotlc}) is marked with an arrow  The comparison star is
  shown marked with a 'c' }
\label{magellan}
\end{figure}

In addition to the imaging observations described above, we have
obtained spectroscopic observations on Nov ~13, 14, and 15, 2007 using
the VPH All grism, which has 660 lines per mm, and employing a
1\arcsec\ wide slit  This set-up provides a mean dispersion of 2\AA\,
per pixel  For a slit width of 1 arcsecond and a mean seeing close to
1\arcsec, the mean spectral resolution is $\approx$10\AA  On Nov ~13, 2007
we took 4 exposures of 450\,s each, on Nov ~14, 2007 we took 2
exposures of 900\,s each, and on Nov ~15, 2007 we took one 1200\,s
exposure with the slit at the parallactic angle  The spectra were bias
and flatfield corrected, and extracted in \textsc{IRAF}  The
instrumental response was corrected using the spectrophotometric flux
calibrators LTT 3218 (Nov ~13), H600 (Nov ~14) and LTT 9293 (Nov ~15) 
Significant differences in the flux around H$\alpha$ are apparent with
the flux being 50\% higher during the Nov ~15, 2007 with respect to
the Nov ~13, 2007 observations  Since there is no evidence for
brightening in the $r^\prime$ images we attribute the difference to
the fact that the source was not observed at the parallactic angle on
Nov ~13 and 14, 2007  We exported the one dimensional spectra to the
spectral analysis software package \textsc{molly} for further
analysis 

\begin{figure}
\centering
\includegraphics[bb=70 30 600 800,clip,width=6 8cm,angle=270]{12082f9 ps}
\caption{Magellan Clay averaged optical spectrum of the optical source
  associated with XMMSL1 J060636 2-694933  The flux scaling is
  approximate  The prominent strong emission lines are marked (see
  text)  }
\label{optspec}
\end{figure}

We have averaged all spectra (see Fig ~\ref{optspec})  We find several
strong emission lines  The strongest of these emission lines are best
interpreted as due to [OIII] 4958 9\AA\, and 5006 9\AA\,, He~II at
4685 8\AA\, and a blend of the H$\alpha$ plus the [NII] at 6548 1\AA\,
and 6583 4\AA\,, lines found often in novae (Williams 1992)  In this
case the main [OIII] lines appear redshifted by approximately 2000\,km
s$^{-1}$  We interprete this as due to clumpy outflows in the nova
shell  The integrated light from different outflowing parts can also
explain the substructure that is present in the [OIII] lines  The
outflow velocities that we obtain for the H$\alpha$ and H$\beta$ lines
is $\approx$350\,km s$^{-1}$, hence less than that for the [OIII]
lines   Note that, if XMMSL1~J060636 2-694933 does reside within the
LMC, then the systematic line-of-sight recession velocity of the LMC,
262$\pm$3 4\,km~s$^{-1}$ (van der Marel et al \ 2002), should be taken
into account; i e \,a good fraction of the observed H$\alpha$ and H$\beta$
recession would then be due to the recession of the LMC itself 

\subsection{Long-term Optical light curve}

Analysis of archival robotic optical survey data from 3-minute CCD
exposures (pixel size 14\arcsec 8), obtained with a 70\,mm (200\,mm
focal length) f/2 8 telephoto lens in the course of the All Sky
Automated Survey (ASAS; Pojmanski 2002) show that the visual magnitude
of this source rose from m$_{V}\raisebox{-1mm}{$\stackrel{>}{\sim}$}$14 to m$_{V}$$\approx$12 between
Sep ~18, 2005 and Sep ~30, 2005, and then declined rapidly thereafter (see
Fig \ref{optlc})  ASAS did not detect any significant emission from
the source after around November 2005, the source having dimmed below
the limiting magnitude of ASAS 

The decline from the brightest data point ($\approx$2 2 magnitudes in
10 days, then a further $\sim$1 3 magnitudes in 46 days) suggests that
this is a nova of the 'very fast' speed class (Warner 1995, Downes
et al \ 2001)  We estimate that the time that the light curve takes to
decline 2 magnitudes below maximum observed brightness is
8$\pm$2\,days (see Section~6) 

\begin{figure}
\centering
\includegraphics[bb=30 78 453 549,clip,width=7 8cm,angle=270]{12082f10 ps}
\caption{All Sky Automated Survey V-band magnitudes of the optical counterpart 
to XMMSL1~J060636 2-694933, during outburst (late September 2005) and afterwards }
\label{optlc}
\end{figure}



\section{Discussion}

The optical spectrum, showing lines of [OIII] 4958 9\AA\, and
5006 9\AA\,, He~II at 4685 8\AA\, and a blend of the H$\alpha$ plus
[NII] at 6548 1\AA\, and 6583 4\AA\, suggests that
XMMSL1~J060636 2-694933 was a nova, observed (in Nov 2007) in the late
A$_{0}$ auroral phase  The fact that the observed [OIII] lines are not
in the more usual, optically thin 3:1 ratio, can be explained in terms
of a clumpy outflow scenario, whereby individual clumps of both
rest-frame and redward-shifted material are observed, and the
superposition of these account for the observed [OIII] ratio (note
further that density enhancements can change observed [OIII] ratios to
more like $\sim$1:1)  Clumps of material are often seen in nova ejecta
(e g  Shara et al \ 1997), and outflows of speeds around 2000\,km
s$^{-1}$ are not uncommon in novae (e g  in nova LMC 1991; Schwartz
et al \ 2001) 

XMMSL1~J060636 2-694933 was likely at its onset (in Oct 2005) a very
fast, Fe~{\sc ii} nova (Section~3 and Williams et al \ 1991; Williams
et al \ 1994)  An accurate classification now however is not possible,
so late after maximum brightness  The soft ($kT_{\rm
  eff}$$\approx$60--70\,eV) X-ray spectrum indicates that the nova was
in a super-soft source (SSS) state (Krautter 2008) during its
discovery (in July 2006), and throughout its X-ray decline (by more
than two orders of magnitude) in the observations of Sept 2006, March
2007 and June 2007   Such a state originates from nuclear burning on
the surface of the white dwarf, and measurements of the intensity,
duration, and temperature can be used to estimate the distance to the
nova and the mass of the white dwarf (e g  Balman et al \ 1998; Lanz
et al \ 2005)  Indeed, we believe (Section~4) that the white dwarf
within XMMSL1~J060636 2-694933 may be quite massive
($>$1 2$M_{\odot}$) 

As discussed earlier, classical novae are almost always discovered
optically in the early phases of their outbursts 
XMMSL1~J060636 2-694933 is very unusual therefore in that it has been
discovered first in X-rays  As such, it is useful to compare it with
XMMSL1~J070542 7-381442 (also known as V598 Pup; Read et al \ 2008),
another nova recently discovered (in X-rays) in the XMM-Newton slew
survey  With a peak $m_{V}$ of $\ltsim12$, XMMSL1~J060636 2-694933 is
not a particularly bright nova (c f  V598 Pup, which reached an
m$_{V}$ of $\raisebox{-1mm}{$\stackrel{<}{\sim}$}$4), and so it is not surprising that it went
unnoticed, only being discovered in X-rays during the later (here
291\,days after the outburst), optically thin nebular phase, when
classical novae are typically observed as soft X-ray sources  Though
this delay should be taken as a upper limit, it is long when compared
to V598 Pup ($\raisebox{-1mm}{$\stackrel{<}{\sim}$}$127 days), but may instead be more similar to the
delays of $\sim$200 days seen in V1974 Cyg (Krautter et al \ 1996),
$\sim$6 months of V382 Vel (Orio et al \ 2002), and 6$-$8 months of
V1494 Aql (Drake et al \ 2003)  In their X-ray monitoring of optical
novae in M31, Pietsch et al \ (2007) detect 11 out of 34 novae in
X-rays within a year after their optical outbursts  Seven novae are
seen to be X-ray bright, several (3$-$9) years after outburst, and
three novae showed very short X-ray outbursts, starting within
50\,days of outburst, but lasting only two to three months 
XMMSL1~J060636 2-694933 therefore is not particularly unusual 

A method to estimate the distance to the nova is to use the relation
between the absolute magnitude at maximum brightness and the time that
the light curve takes to decline 2 magnitudes below maximum
brightness, $t_{2}$ (Della Valle \& Livio 1995)  We have no
information over the 12 days between the data point of maximum
brightness and the lower limit prior to this (Fig \,\ref{optlc}), and
therefore we have no exact outburst date, nor exact apparent
magnitude at outburst   Assuming for the moment though that we have
caught the outburst exactly in the Sep ~30, 2005 observation, then we
can estimate (Sect ~5 3) $t_{2}$ to be 8$\pm$2\,days, and using this,
we can estimate (Della Valle \& Livio 1995) the absolute magnitude at
maximum brightness $M_{V}$ to be --8 7$\pm$0 6  An absolute magnitude
of $M_{V}$=--8 7 implies a peak luminosity $\sim$7 times the Eddington
luminosity for a 1\,$M_{\odot}$ white dwarf  This is quite typical of
novae 

With $A_{V}$=0 39$^{+0 05}_{-0 09}$ (90\% error), as derived (Predehl
\& Schmitt 1995) from $N_{\rm
  H}$=6 9$^{+1 0}_{-1 6}\times10^{20}$\,cm$^{-2}$ (from the highest
statistic spectral fit; the XMM-Newton ToO observation), and with
$M_{V}$=--8 7$\pm$0 6, and a peak $m_{V}$ of 12 0, we can derive a
distance to XMMSL1~J060636 2-694933 of 115$^{+43}_{-30}$\,kpc   As
discussed above however, we are unsure as to the exact outburst date
and the maximum brightness at outburst  Our assumed peak $m_{V}$ of
12 0 is almost certainly an underestimation  Although we have no
information in the 12 days prior to Sep ~30, 2005, a simple linear
extrapolation of the early October lightcurve back prior to Sep ~30,
2005 suggests that the actual peak $m_{V}$ was somewhere between 9 and
12  The corresponding distance estimates are then between 29 and
115\,kpc (with a mid-point $m_{V}$=10 5 value yielding a distance
estimate of 58\,kpc)  Many methods have been used to estimate the
distance to the LMC (e g   Kovacs 2000, Nelson et al \ 2000), but a
value of around 50\,kpc appears to be quite robust  Our distance
estimate is certainly consistent with that of the LMC, though the
errors are quite large   It does appear to be the case however, that
our distance estimate places the source far outside of our own Galaxy 
This, together with the source's position on the sky (at the eastern
edge of the LMC) and the sizable ($\sim$Galactic) X-ray hydrogen
column densities obtained from the spectral fits, suggest strongly
that XMMSL1~J060636 2-694933 lies within the LMC itself   Note further
that the (pile-up corrected) spectral model normalizations to the
initial Slew discovery data (Sect ~2) also imply an approximate
distance to XMMSL1~J060636 2-694933 of $\sim$50\,kpc 

The source had, at the time of the slew detection, an absorbed
(0 2$-$2\,keV) X-ray flux of 4 8$^{+2 7}_{-1 6}\times10^{-11}$\,ergs
cm$^{-2}$ s$^{-1}$, corresponding to a 0 2$-$2\,keV X-ray luminosity
(at 50\,kpc) of 1 4$^{+0 8}_{-0 5}\times10^{37}$\,ergs s$^{-1}$ 
Assuming instead for the moment a distance more like 100\,kpc (though
this is thought to be well beyond the LMC, e g  Kovacs 2000), then the
(0 2$-$2\,keV) X-ray luminosity of
5 7$^{+3 0}_{-1 9}\times$$10^{37}$\,erg s$^{-1}$ obtained is at the high end of the X-ray luminosities of
classical SSS-phase novae discussed e g \,in Orio et al \ (2002) and
Ness et al \ (2007)  As discussed though, we have very likely missed
the outburst peak, and as such, our more probable assumed distance of
50\,kpc gives rise to a more typical SSS-phase X-ray luminosity   The
luminosities of 7$-$8$\times$$10^{34}$\,erg s$^{-1}$, obtained during
the Swift and pointed XMM-Newton observations, are more typical of
novae at later times, when the emission can also sometimes be
described by a thermal plasma, rather than a black-body type spectrum,
or a more mixed spectrum, due to the complex structure of the ejecta
and the accretion disk (Krautter 2008, Shore 2008) 


\section{Conclusions}

A bright X-ray source, XMMSL1~J060636 2-694933, was detected in an
XMM-Newton slew on 18 July 2006 at a position where no previous X-ray
source had been seen  The XMM-Newton slew data, plus follow-up dedicated
XMM-Newton and Swift observations, plus optical imaging and
spectroscopic data acquired with the Magellan Clay telescope and 
All-Sky Automated Survey (ASAS) data were used to classify the new object
as a nova, and to examine its properties  The primary conclusions are
as follows:

  \begin{itemize}

  \item The soft X-ray spectrum indicates that the nova was in a
    super-soft source (SSS) state at its discovery in July 2007
    (XMM-Newton slew) and through its X-ray decline (by over two
    orders of magnitude) in September 2006 (XMM-Newton slew), March
    2007 (Swift) and June 2007 (XMM-Newton) 

  \item The Magellan optical spectrum (Nov 2007) of the source
    indicates that it was very likely then a nova in the late
    A$_{0}$ auroral phase 

  \item The very fast optical decline (ASAS) during the nova's onset
    (Oct 2005), indicates that the initial nova was likely of speed class
    'very fast' 

  \item The very fast speed, together with the absolute magnitude at
    maximum brightness and the X-ray absorption, give rise to a
    distance to the source far beyond our own Galaxy  The large
    distance, together with the source's position in the sky, at the
    eastern edge of the LMC, and the spectral information from the
    X-ray data, are very suggestive that the nova is situated within
    the LMC itself 

  \item Analysis of XMM-Newton slew data is continuing to provide a
    powerful means of finding new X-ray transient objects 

\end{itemize}

\begin{acknowledgements}

  The XMM-Newton project is an ESA Science Mission with instruments
  and contributions directly funded by ESA Member States and the USA
  (NASA)  The XMM-Newton project is supported by the Bundesministerium
  f\"ur Wirtschaft und Technologie/Deutsches Zentrum f\"ur Luft- und
  Raumfahrt (BMWI/DLR, FKZ 50 OX 0001), the Max-Planck Society and the
  Heidenhain-Stiftung  AMR and PE acknowledge the support of STFC
  funding, and PGJ of the Netherlands Organisation for Scientific
  Research  The ASAS project is supported by the N2030731/1328 grant
  from the MNiSzW  We thank the referee (G \,Sala) for very useful
  comments and several references that have improved the paper
  notably  We thank Kim Page for providing the white dwarf atmosphere
  model, and we thank her and Graham Wynn for useful discussions  The
  use of the spectral analysis software package \textsc{molly} written
  by Tom Marsh is also acknowledged  MM acknowledges support by a
  Miller Institute Research Fellowship during the time in which part
  of the work was completed 

\end{acknowledgements}


Context 3: Sir Simon William English  (born 30 December 1961) is a New Zealand former National Party politician who served as the 39th prime minister of New Zealand from 2016 to 2017  He had previously served as the 17th deputy prime minister of New Zealand and minister of finance from 2008 to 2016 under John Key and the Fifth National Government 

A farmer and public servant before entering politics, English was elected to the New Zealand Parliament in  as the National Party's candidate in the Wallace electorate  He was elevated to Cabinet in 1996 and in 1999 was made minister of finance, although he served for less than a year due to his party's loss at the 1999 general election  In October 2001, English replaced Jenny Shipley as the leader of the National Party (and consequently as Leader of the Opposition)  He led the party to its worst defeat at the 2002 general election, and as a consequence, in October 2003 he was replaced as leader by Don Brash 

In November 2006, after Brash's resignation, English became deputy leader under John Key  After National's victory at the 2008 general election, he became deputy prime minister and was also made minister of finance for the second time  Under English's direction New Zealand's economy maintained steady growth during National's three terms of government  He became a list-only MP after stepping down as an electorate MP at the 2014 general election 

John Key resigned as leader of the National Party and prime minister in December 2016  English won the resulting leadership election unopposed and was sworn in as prime minister on 12 December 2016  His tenure was only ten months, and included a three-month election campaign  In the 2017 general election, National won the largest number of seats but fell short of a majority  The parties holding the balance of power declined to support the existing government, and English was subsequently replaced as prime minister by Jacinda Ardern, leader of the Labour Party  English initially continued on as Leader of the Opposition, but resigned as leader of the National Party on 27 February 2018 and left parliament two weeks later 

Early life
English was born on 30 December 1961 at Lumsden Maternity Centre in Lumsden  He is the eleventh of twelve children of Mervyn English and Norah (née O'Brien) English  His parents purchased Rosedale, a mixed sheep and cropping farm in Dipton, Southland from Mervyn's uncle, Vincent English, a bachelor, in 1944  English was born in the maternity unit at Lumsden 

English attended St Thomas's School in Winton, then boarded at St  Patrick's College in Upper Hutt, where he became head boy  He played in the first XV of the school's rugby team  English went on to study commerce at the University of Otago, where he was a resident at Selwyn College, and then completed an honours degree in English literature at Victoria University of Wellington 

After finishing his studies, English returned to Dipton and farmed for a few years  From 1987 to 1989, he worked in Wellington as a policy analyst for the New Zealand Treasury, at a time when the free market policies favoured by Labour's finance minister Roger Douglas (known collectively as "Rogernomics") were being implemented 

English joined the National Party in 1980, while at Victoria University  He served for a period as chairman of the Southland branch of the Young Nationals, and became a member of the Wallace electorate committee  After moving to Wellington, he served for periods on the Island Bay and Miramar electorate committees, respectively 

Fourth National Government (1990–1999)

At the 1990 general election, English stood as the National candidate in Wallace, replacing the retiring Derek Angus, and was elected with a large majority  He would hold this seat, renamed Clutha-Southland in 1996, until 2014  He and three other newly elected National MPs (Tony Ryall, Nick Smith, and Roger Sowry) were soon identified as rising stars in New Zealand politics, and at various points were dubbed the "brat pack", the "gang of four", and the "young Turks"  In his first term in parliament, English chaired a select committee into social services  He was made a parliamentary under-secretary in 1993, serving under the Minister of Health 

First period in cabinet (1996–1999)
In early 1996, English was elevated to cabinet by Prime Minister Jim Bolger, becoming the Minister for Crown Health Enterprises and Associate Minister of Education (to Wyatt Creech)  He was 34 at the time, becoming the cabinet's youngest member  After the 1996 general election, the National Party was forced into a coalition with New Zealand First to retain government  In the resulting cabinet reshuffle, English emerged as Minister of Health  However, as a condition of the coalition agreement, NZ First's Neil Kirton (a first-term MP) was made Associate Minister of Health, effectively becoming English's deputy  This arrangement was described in the press as a "shotgun marriage", and there were frequent differences of opinion between the two ministers  After their relationship became unworkable, Kirton was sacked from the role in August 1997, with the agreement of NZ First leader Winston Peters 

As Minister of Health, English was responsible for continuing the reforms to the public health system that National had begun after the 1990 general election  The reforms were unpopular, and health was perceived as one of the government's weaknesses, with the health portfolio consequently being viewed as a challenge  English believed that the unpopularity of the reforms was in part due to a failure in messaging, and encouraged his National colleagues to avoid bureaucratic and money-focused language (such as references to "balance sheets" and "user charges") and instead talk about the improvements to services the government's reforms would bring  He also rejected the idea that public hospitals could be run as commercial enterprises, a view which some of his colleagues had previously promoted 

By early 1997, as dissatisfaction with Bolger's leadership began to grow, English was being touted as a potential successor, along with Jenny Shipley and Doug Graham  His age (35) was viewed as the main impediment to a successful leadership run  National's leadership troubles were resolved in December 1997, when Bolger resigned and Shipley was elected to the leadership unopposed  English had been a supporter of Bolger as leader, but Shipley reappointed him Minister of Health in her new cabinet 

English was promoted to Minister of Finance in a reshuffle in January 1999, a position which was at the time subordinate to the Treasurer, Bill Birch  After a few months, the pair switched positions as part of Birch's transition to retirement, with English assuming the senior portfolio  In early interviews, he emphasised his wish to be seen as a pragmatist rather than an ideologue, and said that the initiatives of some of his predecessors (Roger Douglas's "Rogernomics" and Ruth Richardson's "Ruthanasia") had focused on "fruitless, theoretical debates" when "people just want to see problems solved" 

Opposition (1999–2008)

After the National Party lost the 1999 election to Helen Clark's Labour Party, English continued on in the shadow cabinet as National's spokesperson for finance



ground_truth: 4.5x10^8 cm.

prompt_front: Now, answer the following question based on the text below, only give me the answer and do not output any other words.

Question: What did the court in In re Ferguson conclude about the transformation prong of the Bilski test?

Read the following text and answer briefly.

Context 2: Xpp-pdf support utility
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PATENT, TRADEMARK
& COPYRIGHT !
Reproduced with permission from BNA’s Patent,Trademark 11/20/09, 11/20/2009  Copyright ஽ 2009 by The Bu-reau of National Affairs, Inc  (800-372-1033) http://www bna com As the patent community anticipates a decision by the U S  Supreme Court on subject matter patentability, recent rulings by the Federal Circuit and the Board of Patent Appeals and Interferences suggest strategies for preparing method patent applications that will sur- vive the Federal Circuit’s ‘‘machine-or-transformation’’ test 
The Changing Landscape of Method Claims in the Wake of In re Bilski:What We Can Learn from Recent Decisions of Federal Courts and the Board ofPatent Appeals rulings on software-based and other business methodpatent applications 
On review before the high court is the en banc ruling ‘‘Pure’’ business methods are out  Algorithms by the U S  Court of Appeals for the Federal Circuit1 are out  Machines and data transformations that, in order to be eligible for patent protection, an in- ventive method must either be tied to a machine or re- While the patent community waits for the Supreme cite a transformation of an article 2 This ‘‘machine-or- Court’s decision in Bilski v  Kappos, No  08-964 (U S 
transformation’’ test replaced the Freeman-Walter- argued Nov  9, 2009) (79 PTCJ 33, 11/13/09), patent ap- Abele3 test and the ‘‘useful, concrete and tangible plicants seeking to write patentable claims are stuckwith trying to conform to the lower courts’ most recent 1 In re Bilski, 545 F 3d 943, 88 USPQ2d 1385 (Fed  Cir 
2008) (en banc) (77 PTCJ 4, 11/7/08) 
2 ‘‘The machine-or-transformation test is a two-branched Adriana Suringa Luedke and Bridget M  Hay- inquiry; an applicant may show that a process claim satisfies den are lawyers at Dorsey & Whitney, Min- § 101 either by showing that his claim is tied to a particular neapolis  Luedke can be reached at machine, or by showing that his claim transforms an article ’’ leudke adriana@dorsey com  Hayden can be reached at hayden bridget@dorsey com  3 In re Freeman, 573 F 2d 1237, 197 USPQ 464 (C C P A 
1978); In re Walter, 618 F 2d 758, 205 USPQ 397 (C C P A 
COPYRIGHT ஽ 2009 BY THE BUREAU OF NATIONAL AFFAIRS, INC 
result’’ inquiry advocated in State Street,4 each of gregating, and selling real estate property and claims which had been applied by the Federal Circuit and its reciting a method of performing tax-deferred real estate predecessor court in various cases, and both of which property exchanges were not statutory under Section 101  Since no machine was recited, the only issue be- In this article, we examine the 2008 decision of the fore the court was whether the claims met the ‘‘trans- Federal Circuit, federal district court decisions, and de- formation’’ prong of the Bilski test 13 The court held cisions of Patent and Trademark Office’s Board of that the claims ‘‘involve[d] only the transformation or Patent Appeals and Interferences  Based upon the out- manipulation of legal obligations and relationships’’ comes in these cases, we offer guidance as to what is that did not qualify under Bilski 14 patent-eligible under 35 U S C  § 101, strategies for pre- Concerning the recitation of the ‘‘creation of deed- senting methods in patent applications and claiming shares’’ in some of the claims, the court found that the these methods, and possible ‘‘fixes’’ for applications deedshares themselves were not physical objects, but drafted pre-Bilski that must now withstand scrutiny un- only represented intangible legal ownership interests in der the new machine-or-transformation test 
property 15 Therefore, the creation of deedshares wasnot sufficient to establish patent eligibility under Bil- A number of recent federal court and board decisions have applied the patent eligibility test set forth in Bilski, implemented step to an otherwise obvious method was not sufficient to avoid invalidity of the claim  In KingPharmeuticals Inc  v  Eon Labs Inc ,17 the district court held invalid claims to a method of increasing the oral Several cases have addressed (and rejected) claims bioavailability of metaxalone because the claims were obvious over the prior art asserted by the accused in- In In re Ferguson,6 the Federal Circuit reviewed the board’s rejection of claims directed to a method of mar- Two dependent claims added a step of informing the keting a product and a ‘‘paradigm’’ for marketing soft- patient of certain results, which the patentee argued ware as nonstatutory subject matter under Section was not obvious  The court rejected this argument, con- 101 7 The appellate court affirmed the board’s rejection, cluding that ‘‘[b]ecause the food effect is an inherent concluding that the method claims were neither tied to property of the prior art and, therefore, unpatentable, a particular machine or apparatus nor did they trans- then informing a patient of that inherent property is form a particular article into a different state or thing 8 The court defined a machine broadly as ‘‘a concrete The court also commented that the added step of in- thing, consisting of parts, or of certain devices or com- forming the patient did not meet the patent eligibility binations of devices,’’ which did not include the ‘‘shared standard set forth in Bilski because the step did not re- marketing force’’ to which the method claims were quire use of a machine or transform the metaxalone into a different state or thing 19 Notably, this conclusion The claims directed to a ‘‘paradigm’’ were non- runs counter to the Supreme Court’s instruction that statutory because the claims did not fall within any of claims are to be examined ‘‘as a whole’’ and not dis- the four statutory categories (machines, manufactures, sected into old and new elements and that are evaluated compositions of matter and processes)  Concerning the two closest possible categories, the court concluded Recent board decisions have been consistent with the that the claimed paradigm was not a process, because holdings of the federal courts  For example, in Ex parte no act or series of acts was required, and was not a Roberts,21 the board found ineligible under Section 101 manufacture, because it was not a tangible article re- a ‘‘method of creating a real estate investment instru- sulting from a process of manufacture 10 Concerning ment adapted for performing tax-deferred exchanges’’ the recitation of a ‘‘marketing company’’ in the para- because the claim did not satisfy either the machine or digm claims, the court concluded that the patent appli- cants did ‘‘no more than provide an abstract idea—a Similarly, in Ex parte Haworth,23 a method for ‘‘at- business model for an intangible marketing com- tempting to collect payments from customers having delinquent accounts concurrently with a partner that In Fort Properties Inc  v  American Master Lease owns the delinquent accounts’’ was found to be patent LLC,12 the California district court held that claims re- ineligible because the claim wording was ‘‘broad in that citing a series of transactions involving acquiring, ag- 1980); In re Abele, 684 F 2d 902, 214 USPQ 682 (C C P A 
4 State Street Bank & Trust Co  v  Signature Financial 16 See Ex parte Roberts , 2009-004444 at 4-5 (B P A I  June Group, 149 F 3d 1368, 1370, 47 USPQ2d 1596 (Fed  Cir  1998) 19, 2009) (holding a ‘‘method of creating a real estate invest- ment instrument adapted for performing tax-deferred ex- changes’’ patent ineligible as not passing the machine-or- 7 The court accepted the board’s definition of ‘‘paradigm’’ 17 593 F  Supp 2d 501 (E D N Y  2009) 
to mean ‘‘a pattern, example or model ’’ Id  at 1362 
20 See Diamond v  Diehr, 450 U S  175, 188 (1981) 
21 No  2009-004444 (B P A I  June 19, 2009) 
12 2009 WL 249205, *5 (C D  Cal  Jan  22, 2009) 
23 No  2009-000350 (B P A I  July 30, 2009) 
it refers generally to extending an offer, receiving an machine  Accordingly, the process claims       are not acceptance, and paying a commission’’ and did not in- voke, recite or limit the method of implementation us-ing any particular machine or apparatus 24 The court also evaluated similar claims that recited the use of a ‘‘comparator’’ to perform the recited pixel- B  Software Claims Not Expressly Tied to a ‘Particular by-pixel comparison and held that this recitation also did not mandate a machine 29 While the court acknowl-edged that software was offered as one ‘‘option,’’ the Other cases have addressed software methods where court concluded that the claimed function of the com- the claim language was either not expressly tied to com- parator could also be performed in one’s mind or on pa- puter hardware components or the ties to computer per such that a machine was not required  The court components were somewhat ambiguous  In several further noted that, even though the ‘‘comparator’’ was cases, courts have rejected the recitation of generic defined as a ‘‘device,’’ ‘‘the use of the term ‘device’ is computer components as sufficient to satisfy the ‘‘ma- not synonymous with machine ’’30 As a result, none of chine’’ prong of the Bilski test  A number of these deci- the claims at issue met the ‘‘machine’’ prong of the Bil- sions also addressed the ‘‘transformation’’ prong of the Concerning the ‘‘transformation’’ prong, the court re- In Research Corporation Technology Inc  v  Mi- lied in particular upon the Abele decision in expanding crosoft Corp ,25 the district court considered the patent the requirements of this test by requiring that the eligibility of method claims in six patents directed to claimed transformation process be both ‘‘(1) limited to methods of halftoning of gray scale images by using a transformation of specific data, and 2) limited to a vi- pixel-by-pixel comparison of the image against a blue sual depiction representing specific objects or sub- noise mask  Relying on the Federal Circuit’s Bilski stances ’’31 It then concluded that a number of the analysis as well as a decision of its predecessor court, patent claims did not meet the second prong of this ex- In re Abele,26 the judge concluded that a number of the panded test because the claims did not ‘‘require any vi- sual depiction or subsequent display’’ even though the transformation test set forth in Bilski 27 claimed method did transform specific image data 32 Concerning the ‘‘machine’’ prong, the district court The district court also found other claims patent- found that the pixel-by-pixel comparison recited in the eligible under Section 101 because these claims recited claims did not require the use of a machine, but could the use of the comparison data ‘‘to produce a halftoned ‘‘dictate[d] a transformation of specific data, and [were] be done on a sheet of paper using a pen  The com- further limited to a visual depiction which represents parison uses formulas and numbers to generate a bi- specific objects ’’33 Thus, the patent eligibility of the nary value to determine the placement of a dot at a claims turned on whether the claims recited the use of location  Formulas and numbers not tied to a particu- the transformed data to generate a display 
lar machine cannot be patented, under the machine In DealerTrack Inc  v  Huber,34 the district court prong, even with a field-of-use limitation because granted a summary judgment of invalidity under § 101 they represent fundamental principles, and to do so of patent claims directed to ‘‘a computer aided method’’ would preempt the entire field  The patent claims      
of managing a credit application reciting the following do not mandate the use of a machine to achieve their algorithmic and algebraic ends  Simply because adigital apparatus such as a computer, calculator, or [A] receiving credit application data from a remote the like could assist with this comparison does not render it patent eligible material  RCT’s argument [B] selectively forwarding the credit application data that a pixel by its nature is electronic and therefore to remote funding source terminal devices; necessitates a machine is a post solution argumentand the Court rejects it  The claim construction specifies that the comparison is of a value to a mask 29 The term ‘‘comparator’’ was construed by the court to be (or set of values) to determine whether the dot is a ‘‘device (or collection of operations, as in software) that com- turned on at a specific location  This process does pares an input number (called the operand) to a number pre- not require a particular machine  The Bilski test is stored in the comparator (called the threshold) and produces clear: the process claims must be tied to a particular as output a binary value (such as ‘‘0,’’ zero) if the input is alge-braically less than the threshold [the result of comparing anoperand against a fixed threshold and setting an operand less 24 Id  at 9-10  See also, e g , Ex parte Farnes, 2009-002770 than the threshold to one value and an operand greater than (B P A I  June 2, 2009) (rejecting a method claim for develop- or equal to the threshold to another value], and produces the ing a solution to a customer experience issue including steps opposite binary value (such as ‘‘1,’’ one) if the input is algebra- of: ‘‘identifying a target customer,’’ ‘‘defining a current cus- ically greater than or equal to the threshold ’’ Id  at *17 (em- tomer experience,’’ ‘‘summarizing values and benefits’’ to pro- vide to the customer, and ‘‘identifying metrics for measuring success’’); Ex parte Salinkas, 2009-002768 (B P A I  May 18, 31 Id  at *9  Notably, Bilski concluded that the Abele visual 2009) (finding patent ineligible a method of launching a depiction was ‘‘sufficient’’ to establish transformation (545 knowledge network involving ‘‘selecting an executive spon- F 3d at 963), while the Research Corporation court went fur- sor,’’ ‘‘forming a core team of experts,’’ and ‘‘providing pre- ther by making visual depiction ‘‘required’’ to establish trans- 25 2009 WL 2413623 (D  Ariz  July 28, 2009) (78 PTCJ 432, 26 684 F 2d 902, 214 USPQ 682 (C C P A  1982) 
34 2009 WL 2020761 (C D  Cal  July 7, 2009) (78 PTCJ 341, PATENT, TRADEMARK & COPYRIGHT JOURNAL [C] forwarding funding decision data from at least tation of ‘over the Internet’ suffices to tie a process one of the remote funding source terminal de- claim to a particular machine’’ and concluded that it vices to the remote application entry and display The internet continues to exist despite the addition [D] wherein the selectively forwarding the credit ap- or subtraction of any particular piece of hardware  It may be supposed that the internet itself, rather than [E] sending at least a portion of a credit application any underlying computer or set of computers, is the to more than one of said remote funding sources ‘‘machine’’ to which plaintiff refers  Yet the internet is an abstraction  If every computer user in the world [F] sending at least a portion of a credit application unplugged from the internet, the internet would to more than one of said remote funding sources cease to exist, although every molecule of every ma- sequentially until a finding [sic ] source returns a chine remained in place  One can touch a computer or a network cable, but one cannot touch ‘‘the inter- [G] sending       a credit application       after a prede- Additionally, the court found that the recitation of the [H] sending the credit application from a first remote internet in this case merely constituted ‘‘insignificant funding source to a second remote funding extra-solution activity’’ and therefore did not qualify as a ‘‘particular machine’’ under Bilski 41 ‘‘[T]ossing in In concluding that the claim did not satisfy the Bilski references to internet commerce’’ was not sufficient to machine-or-transformation test, the court held that the render ‘‘a mental process for collecting data and weigh- claimed central processor, remote application and dis- ing values’’ patent-eligible 42 Additionally, ‘‘limiting’’ play device, and remote funding source terminal device the claim to use over the Internet was not a meaningful could be ‘‘any device’’ and did not constitute a ‘‘’par- limitation, such that the claims ‘‘broadly preempt the ticular machine’ within the meaning of Bilski ’’35 The fundamental mental process of fraud detection using court relied upon several board decisions to support its associations between credit cards ’’43 premise that ‘‘claims reciting the use of general purpose processors or computers do not satisfy the test ’’36 claim,44 notwithstanding the Federal Circuit’s holding In Cybersource Corp  v  Retail Decisions Inc ,37 the in In re Beauregard,45 the district court concluded that district court held claims for ‘‘a method for verifying the ‘‘there is at present no legal doctrine creating a special validity of a credit card transaction over the Internet’’ ‘‘Beauregard claim’’ that would exempt the claim from and ‘‘a computer readable medium containing program the analysis of Bilski ’’ Moreover, ‘‘[s]imply appending instructions for detecting fraud in a credit card transac- ‘A computer readable media including program instruc- tion       over the Internet’’ invalid under § 101 based tions’ to an otherwise non-statutory process claim is in- upon the court’s interpretation of Bilski 
sufficient to make it statutory ’’46 Consequently, this Concerning the method claim, the court considered claim also failed the Bilski test 
both the ‘‘transformation’’ and ‘‘machine’’ prongs of the In at least one instance, the U S  International Trade Bilski test  In concluding that there was no transforma- Commission has interpreted the ‘‘machine’’ prong of tion, the court focused on the intangibility of the ma- Bilski less stringently than did the district courts in the nipulated data  According to the court, transformation cases discussed above  In In the Matter of Certain Video is limited to transformation of a physical article or sub- Game Machines and Related Three-Dimensional Point- stance  Accordingly, the method claim did not qualify ing Devices,47 the accused infringer filed a motion for because the data representing credit cards did not rep- summary judgment alleging that the asserted claims resent tangible articles but instead an intangible series impermissibly sought to patent a mathematical algo- of rights and obligations existing between the account rithm  According to the movant, the recitations of a ‘‘3D pointing device,’’ ‘‘handheld device,’’ or ‘‘free space Concerning whether the claimed method was tied to pointing device’’ were not sufficient to tie the claims to a particular machine, the court assessed whether ‘‘reci- a particular machine, but served ‘‘only to limit the field-of-use of the claimed mathematical algorithm and [did] not otherwise impart patentability on the claimed math- Id  at *3  The court relied upon the holdings in Ex parte Gutta, No  2008-3000 at 5-6 (B P A I  Jan  15, 2009) (stating In denying the motion for summary judgment, the ‘‘[t]he recitation in the preamble of ‘[a] computerized method ITC first noted that, ‘‘[w]hile the ultimate determination performed by a data processor’ adds nothing more than a gen- of whether the asserted claims are patentable under eral purpose computer that is associated with the steps of the § 101 is a question of law, the Federal Circuit has ac- process in an unspecified manner ’’); Ex parte Nawathe, No 
2007-3360, 2009 WL 327520, *4 (B P A I  Feb  9, 2009) (finding‘‘the computerized recitation purports to a general purpose processor [], as opposed to a particular computer specifically programmed for executing the steps of the claimed method ’’); and Ex parte Cornea-Hasegan, No  2008-4742 at 9-10 (B P A I 
Jan  13, 2009) (indicating the appellant does not dispute ‘‘the recitation of a processor does not limit the process steps to any 44 Claims having this format are called ‘‘Beauregard’’ specific machine or apparatus ’’)  The court also cited Cyber- claims and were found to not be barred by the traditional source Corp  v  Retail Decisions Inc , (discussed below), in sup- printed matter rule in In re Beauregard, 53 F 3d 1583, 1584, 35 port of its interpretation of the required ‘‘particular machine ’’ 37 620 F  Supp  2d 1068, 92 USPQ2d 1011 (N D  Cal  2009) 47 2009 WL 1070801 (U S I T C  2009) 
knowledged that ‘there may be cases in which the legal given a dataset of feature vectors associated with the question as to patentable subject matter may turn on subsidiary factual issues’ ’’ (citation omitted)  In con- for each binary partition under consideration, rank- struing the claims, the tribunal found that there was a ing features using two-category feature ranking; and genuine dispute as to whether the claimed ‘‘devices’’represented a ‘‘particular machine’’ under the Bilski while the predetermined number of features has not test and whether the claimed ‘‘two-dimensional rota- yet been selected: picking a binary partition p; tional transform’’ was merely a mathematical calcula- selecting a feature based on the ranking for binary tion or instead meant ‘‘changing the mathematical rep- resentation of a two-dimensional quantity from oneframe of reference to a differently-oriented frame of ref- adding the selected feature to an output list if not al- erence’’ as asserted by the patentee  Additionally, the ready present in the output list and removing the se- dispute over the meaning of the claimed ‘‘two- lected feature from further consideration for the bi- dimensional rotational transform’’ also raised a dis- puted issue as to whether this element recited a trans- Notably, while the independent claim failed the formation that would qualify under the ‘‘transforma- machine-or-transformation test, its dependent claim tion’’ prong of Bilski  Given these disputed issues, the was eligible because it recited, ‘‘further comprising us- ITC concluded that it was inappropriate to grant sum- ing the selected features in training a classifier for clas- mary judgment as to the patent eligibility of the claims 
sifying data into categories ’’ In view of the specifica- A similar conclusion was reached in Versata Soft- tion, the board indicated that the ‘‘classifier’’ was a par- ware Inc  v  Sun Microsystems Inc ,48 in which the dis- ticular machine ‘‘in that it performs a particular data trict court denied the defendant’s motion for summary classification function that is beyond mere general pur- judgment of invalidity under Section 101 based upon pose computing ’’53 The board also concluded that the the Bilski court’s refusal ‘‘to adopt a broad exclusion claim ‘‘transforms a particular article into a different over software or any other such category of subject state or thing, namely by transforming an untrained matter beyond the exclusion of claims drawn to funda- classifier into a trained classifier ’’54 In Ex parte Casati,55 the board reversed the examin- Less stringent ‘‘machine’’ prong analyses are also er’s Section 101 rejection of a method claim reciting: found at the board level  For example, in Ex parteSchrader,50 the board held patent-eligible under Bilski A method of analyzing data and making predictions, reading process execution data from logs for a busi- A method for obtaining feedback from consumers re- ceiving an advertisement from an ad provided by anad provider through an interactive channel, the collecting the process execution data and storing the process execution data in a memory defining a ware-house; creating a feedback panel including at least one feed-back response concerning said advertisement; and analyzing the process execution data; generatingprediction models in response to the analyzing; and providing said feedback panel to said consumers, using the prediction models to predict an occurrence said feedback panel being activated by a consumer to of an exception in the business process 
provide said feedback response concerning said ad-vertisement to said ad provider through said interac- In this case, giving consideration to the specification, which ‘‘unequivocally describes the data warehouse aspart of the overall system apparatus, and subsequent Here, the board found ‘‘interactive channel’’ to be descriptions describe the memory/warehouse device in part of an ‘‘overall patent eligible system of appara- terms of machine executable functions,’’ the board con- tuses’’ when viewed in the context of the specification, cluded that ‘‘one of ordinary skill in the art would un- which included ‘‘the Internet and World Wide Web, In- derstand that the claimed storing of process execution teractive Television, and self service devices, such as In- data in a memory defining a warehouse constitutes formation Kiosks and Automated Teller Machines ’’51 patent-eligible subject matter under § 101 because the In another recent decision, Ex parte Forman,52 the memory/warehouse element ties the claims to a particu- board found a ‘‘computer-implemented feature selec- tion method’’ including a ‘‘classifier’’ eligible under Other recent board decisions have reached the oppo- Section 101 because it satisfied both the machine and transformation prong  Here, the ‘‘classifier’’ was recitedin a dependent claim, in which its independent claim re-cited: 53 Id  at 13 
54 Id  See also Ex parte Busche, No  2008-004750 (B P A I 
A computer-implemented feature selection method May 28, 2009) (holding a process claim and a computer pro- for selecting a predetermined number of features for gram product claim, each reciting training a machine, ‘‘are di- a set of binary partitions over a set of categories rected to machines that have such structure as may be adaptedby training ’’) 55 No  2009-005786 (B P A I  July 31, 2009) 
48 2009 WL 1084412, *1 (E D  Tex  March 31, 2009) 
56 Id  at 7  See also Ex parte Dickerson, No  2009-001172 at 49 Citing Bilski, 545 F 3d at 959 n  23 
16 (B P A I  July 9, 2009) (holding claims that ‘‘recite a comput- 50 No  2009-009098 (B P A I  Aug  31, 2009) 
erized method which includes a step of outputting information from a computer       are tied to a particular machine or appa- 52 No  2008-005348 (B P A I  Aug  17, 2009) 
PATENT, TRADEMARK & COPYRIGHT JOURNAL implemented methods ineligible under the Bilski test transformation test applied to this type of claim 63 because the claims failed to tie the method steps to any Then, applying the Bilski test, the board concluded that concrete parts, devices, or combinations of devices  For the claim did not qualify  According to the board, the example, in Ex parte Holtz,57 the board found ineligible under Section 101 a ‘‘method for comparing file tree de-scriptions’’ because the claim ‘‘obtains data (a file struc- does not transform physical subject matter and is not ture), compares data (file structures), generates a tied to a particular machine        Limiting the claims change log, and optimizes the change log without tying to computer readable media does not add any practi- these steps to any concrete parts, devices, or combina- cal limitation to the scope of the claim  Such a field- tions of devices’’ and the ‘‘file structures’’ did not repre- of-use limitation is insufficient to render an other- Similarly, in Ex parte Gutta,58 the board held ineli- gible under § 101 a ‘‘method for identifying one or moremean items for a plurality of items       having a sym- II  The Current Scope of Patent Eligibility bolic value of a symbolic attribute,’’ concluding that the These recent cases establish that some types of meth- claim ‘‘computes a variance and selects a mean item ods are clearly patent-eligible under Section 101, others without tying these steps to any concrete parts, devices, clearly are not eligible, and yet others may be depend- or combinations of devices’’ and ‘‘symbolic values are ing on how they are described and claimed 
neither physical objects nor do they represent physicalobjects ’’ First, the eligibility of system and apparatus claims is largely unaffected by the Bilski decision, with the ca- In contrast to the district court’s decision in Cyber- veat that such claims may be more closely scrutinized source Corp , discussed supra, in a recent board deci- for compliance with Diamond v  Diehr and Gottschalk sion, Ex parte Bodin,59 ‘‘a computer program product’’ v  Benson, which prohibit patenting of a claim directed was found to be patent-eligible subject matter as being to ‘‘laws of nature, natural phenomena, [or] abstract embodied in a ‘‘computer readable medium ’’ Here, the board considered whether the phrase ‘‘recorded on the Also, methods that are performed at least in part by a recording medium’’ as it is recited in the body of the machine qualify for patent eligibility under Section 101 
claims was the same as ‘‘recorded on a computer- Thus, for example, some computer-implemented and readable medium ’’ Acknowledging the differences be- software-related inventions remain patentable as long tween a statutory claim to a data structure stored on a as they are properly described and claimed as being computer readable medium compared to a nonstatutory performed by a computer or computer components 
claim to a data structure that referred to ideas reflected The tie to a machine, however, cannot merely be im- in nonstatutory processes, the board stated: ‘‘[w]hen plicit based upon the description and context of the ap- functional descriptive material is recorded on some plication or general language in the preamble of the computer-readable medium, it becomes structurally claim  Instead, the use of a machine to perform one or and functionally interrelated to the medium and will be more of the claimed functions must be expressly de- statutory in most cases since use of technology permits scribed in the body of the claim so as to be a meaning- the function of the descriptive material to be real- ful limitation on the claim  If a method claim can be read in such a way that all functions can be performed Similarly, in Ex parte Azuma,61 a claim to a ‘‘com- by a human, it will likely not pass the machine prong of puter program product       comprising: a computer us- able medium’’ was found to be directed to statutory The ‘‘Interim Examination Instructions for Evaluat- subject matter under § 101 because the language ‘‘com- ing Subject Matter Eligibility Under 35 U S C  § 101’’ re- puter usable medium’’ referred to tangible storage me- cently issued by the Patent and Trademark Office con- dia, such as a server, floppy drive, main memory and firm that the recitation of a general purpose computer hard disk as disclosed by appellant’s specification, and is sufficient to satisfy Section 101 where the general did not ‘‘implicate the use of a carrier wave ’’ purpose computer is ‘‘programmed to perform the pro- In an older decision, Ex parte Cornea-Hasegan,62 cess steps,       in effect, becom[ing] a special purpose however, the Board seemingly came to the opposite conclusion, holding that a claim reciting ‘‘a computer Concerning data transformation, there seems to be readable media including program instructions which agreement of the Federal Circuit and at least one dis- when executed by a processor cause the processor to trict court that a method that is both limited to transfor- perform’’ a series of steps was not patent-eligible under mation of specific data and limited to a visual depiction Bilski  The board first determined that ‘‘analysis of a representing specific objects or substances qualifies un- ‘manufacture’ claim and a ‘process’ claim is the sameunder 63 Id  at 11 
57 No  2008-004440 at 12-13 (B P A I  Aug  24, 2009) 
65 Diamond v  Diehr, 450 U S  175, 185, 205 USPQ 488 58 No  2008-004366 at 10-11 (B P A I  Aug  10, 2009) 
(1980); Gottschalk v  Benson, 409 U S  63, 67, 175 USPQ 673 59 No  2009-002913 (B P A I  Aug  5, 2009) 
60 Id  at 10 (comparing In re Lowry, 32 F 3d 1579, 1583-84, 66 ‘‘Interim Examination Instructions for Evaluating Sub- 32 USPQ2d 1031 (Fed  Cir  1994) to In re Warmerdam, 33 F 3d ject Matter Eligibility Under 35 U S C  § 101,’’ U S  Patent and 1354, 1361-62, 31 USPQ2d 1754 (Fed  Cir  1994)) 
Trademark Office, Aug  24, 2009, at 6 (78 PTCJ 530, 8/28/09) 
61 No  2009-003902 at 10 (B P A I  Sept  14, 2009) 
The authors’ recent experiences with examiners suggest that 62 No  2008-004742 (B P A I  Jan  13, 2009) 
the examiners are following these instructions 
der Section 101 67 Thus, claims analogous to those in In Concerning claims directed to computer program re Abele68 in which ‘‘data clearly represented physical products, one district court has held that appending ‘‘A and tangible objects, namely the structure of bones, or- computer readable media including program instruc- gans, and other body tissues [so as to recite] the trans- tions’’ to an otherwise non-statutory process claim is in- formation of that raw data into a particular visual depic- sufficient to make it statutory 72 The board has also tion of a physical object on a display’’ are patent- held ineligible claims to ‘‘a computer readable me- dia ’’73 The board has, however, also upheld the eligibil-ity of ‘‘a computer program product’’ as being embod- ied in a computer readable medium 74 Given these in- Bilski has had a significant impact in eliminating consistent decisions, the patent eligibility of claims in patent protection for inventions that are performed en- tirely by humans or can be interpreted as such if read Concerning claims directed to generalized computer broadly  This includes claims that describe processes processing functions, several Board decisions suggest for creating or manipulating legal and financial docu- that, absent a tie to a concrete real-world application, ments and relationships  In this area in particular, many such claims are likely to be deemed an ‘‘algorithm’’ un- pending applications filed prior to Bilski are no longer der Benson and therefore held to be non-statutory  75 patent-eligible, and many issued patents are no longer Any recitation of a specific field of use for the claimed valid  This retroactive impact of the Bilski decision is process or use of the outcome of such processes are troubling, given the investment in these patents and ap- also more likely to be found ‘‘field-of-use’’ or ‘‘post- plications, which have now been rendered essentially solution activity’’ limitations insufficient to render the worthless despite the suggestion in the Federal Circuit’s claim patent-eligible  Thus, the more tied a claimed pro- earlier State Street decision, now overruled, that such cess is to tangible results or particular applications (not claims qualified for patent protection 
just fields of use), the more likely it is to qualify under Inventions that do not fit within the four statutory categories are also not patent-eligible  The Federal Cir-cuit and the board have rejected claims directed to ‘‘a III  Presenting and Claiming Methods in Patent signal,’’ ‘‘a paradigm,’’ ‘‘a user interface’’ and ‘‘a corr-elator’’ on the basis that these items did not qualify as a ‘‘machine, manufacture, composition of matter or pro- Several strategies for describing and claiming meth- cess’’ under § 101  70 There is also an increasing focus ods or processes in patent applications may avoid or on the tangibility of the claimed invention in that, to minimize potential Section 101 problems 
qualify as a ‘‘machine’’ or ‘‘manufacture’’ under Section First, the description provided in a patent application should include well-defined steps or functions associ-ated with method or process  For example, when the claims include ‘‘initiating’’ method steps, a description Remaining areas of uncertainty concerning the scope of well-defined physical steps or functions for initiating of Section 101 include (1) what qualifies under Bilski as should be provided, and a concrete item, machine, de- a ‘‘transformation of an article or data,’’ (2) whether vice, or component that is responsible for the initiating claims to computer programs (Beauregard claims) function should be identified  For claiming ‘‘identify- qualify, and (3) whether internal computer processing ing’’ method steps, provide specific parameters for functionality not tied to a specific application or tan- making the identification, such as according to a speci- fied measurement 76 Where data is involved, the source Concerning data transformation, other than Abele- and type of data should be specified 
style claims discussed above, what qualifies as a data or Also, drawings should be provided that depict the article transformation remains unclear  Claims that concrete item, device, component or combination have been held not to meet the transformation prong in- thereof, and each method or process step or function clude claims directed to the creation or manipulation of should be linked expressly to at least one item, device data representing an intangible series of rights and ob- or component in the drawings that performs the step or ligations (e g , credit card data) and claims directed to function  Broadening language indicating that other the transformation or manipulation of legal obligations components may also be used to perform the function and relationships  Beyond these specific examples, it is may also be included to avoid an unduly narrow inter- difficult to predict what will or will not qualify as a data or article transformation under Bilski 
The claims should affirmatively claim the device, ma- chine or component performing each step or function 
67 In re Bilski, 545 F 3d at 963; Research Corporation Tech- For computer or software-related inventions, the de- nologies, 2009 WL 2413623 at *9 
scription should specify that the software functionality 68 The claimed process involved graphically displaying vari- ances of data from average values wherein the data was X-rayattenuation data produced in a two dimensional field by a com- 72 Cybersource Corp , 620 F  Supp  2d at 1080 
puted tomography scanner  See In re Bilski, 545 F 3d at 962- 73 Cornea-Hasegan, No  2008-004742 
74 Ex parte Bodin, No  2009-002913 (B P A I  Aug  5, 2009) 
69 In re Bilski, 545 F 3d at 963 
75 E g , Ex parte Greene, No  2008-004073 (B P A I  Apr  24, 70 In re Nuijten 500 F 3d 1346, 1357, 84 USPQ2d 1495 (Fed 
2009); Daughtrey, No  2008-000202; Ex parte Arning, No 
Cir  2007) (74 PTCJ 631, 9/28/07) (signal); In re Ferguson, 558 2008-003008 (B P A I  Mar  30, 2009); Cybersource Corp , 620 F 3d 1359, 1366, 90 USPQ2d 1035 (Fed  Cir  2009) (77 PTCJ F  Supp 2d at 1080 (concerning claim 2) 
489, 3/13/09) (paradigm); Ex parte Daughtrey, No  2008- 76 See Brief of American Bar Association as Amicus Curiae 000202 (B P A I  Apr  8, 2009) (user interface); Ex parte Laba- Supporting Respondent, Bilski v  Kappos, No  08-964, ABA die, No  2008-004310 (B P A I  May 6, 2009) (correlator) 
Amicus Br  at 12-13 (U S  amicus brief filed Oct  2, 2009) (78 71 E g , Nuijten, 500 F 3d at 1356-7 
PATENT, TRADEMARK & COPYRIGHT JOURNAL is performed by a computer or computer components 
patent or published application, the option of importing Specificity as to the type of computer component per- subject matter into the specification is limited to ‘‘non- forming each function may be helpful in establishing essential’’ subject matter  In other words, the specifica- eligibility under the Bilski test 
tion can only be amended to disclose a machine for per-forming process steps as long as one skilled in the art IV  Fixing Pre-Bilski Applications to Meet the New would recognize from the original disclosure that the process is implemented by a machine  The key in mak- For patent applications filed prior to the Bilski deci- ing this type of amendment is avoiding (or overcoming) sion, it can be challenging to meet the new require- a rejection under 35 U S C  § 112, para  1, for lack of ments for patent eligibility, particularly when no ma- chine or transformations were expressly described in If incorporation by reference is not an option, a patent applicant may submit evidence, such as a decla- In some cases, there may be sufficient explicit de- ration by the inventor or a duly qualified technical ex- scription of a machine, e g , a computer, such that the pert, demonstrating that one skilled in the art would un- machine can be added into the body of the claims  For derstand the disclosed method to be one performed by example, patent applications for computer-related in- a machine  Unlike attorney argument, which can be dis- ventions sometimes contain a generic description of regarded, such evidence must be considered by the ex- computers that are used to perform the claimed method, and such a generic description may be suffi- One other option is to reformat the claims  Since Bil- cient to impart patent eligibility to the claims when the ski ostensibly does not apply to system and apparatus general-purpose computer is programmed to become a claims, in some instances it may be possible for an ap- plicant to convert his method claims into system claims For patent applications lacking in an explicit descrip- to avoid application of the Bilski test  This strategy, tion of any machine, however, the application may in- however, is unlikely to succeed where the patent speci- corporate by reference patents or publications that can fication does not describe such a system for implement- be used to bolster the specification and provide support ing the method and therefore does not provide the req- for the requisite claim amendments  When an applica- uisite disclosure of the claimed invention under Section tion incorporates by reference a U S  patent or pub- lished U S  patent application, any description from the incorporated references, whether or not the subject The future of the Bilski machine-or-transformation matter is ‘‘essential’’ to support the claims, may be im- test now rests with the Supreme Court  Regardless of ported into the specification  This option may enable the outcome of the appeal, however, it is clear that the importation of the requisite description of a machine, scope of statutory subject matter under Section 101 has which can then also be recited in the claims 77 When been narrowed  The Supreme Court now has a chance the document incorporated by reference is not a U S 
to clarify what has been excluded; it may even reject ormodify the Bilski machine-or-transformation test  How 77 Manual of Patent Examining Procedure, Eighth Ed , Rev 
this will affect the development and protection of cur- 7/2008, at § 608 01(P); see also 37 C F R  § 1 57 
rent and future technologies remains to be seen 
Source: http://www dorsey com/files/upload/luedke_bna_patent_journal_nov09 pdf
(resolução 404 2012 retificação 19062012)
RESOLUÇÃO Nº 404 , DE 12 DE JUNHO DE 2012 Dispõe sobre padronização dos procedimentos administrativos na lavratura de Auto de Infração, na expedição de notificação de autuação e de notificação de penalidade de multa e de advertência, por infração de responsabilidade de proprietário e de condutor de veículo e da identificação de condutor infrator, e dá outras providências 
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Context 3:  He was elected deputy leader of the party in February 2001, following the resignation of Wyatt Creech, with Gerry Brownlee being his unsuccessful opponent 

Leader of the Opposition
In October 2001, after months of speculation, Jenny Shipley resigned as leader of the National Party after being told she no longer had the support of the party caucus  English was elected as her replacement unopposed (with Roger Sowry as his deputy), and consequently became Leader of the Opposition  However, he did not openly organise against Shipley, and according to The Southland Times "there was almost an element of 'aw, shucks, I'll do it then' about Mr English's ascension" 

Aged 39 when he was elected, English became the second-youngest leader in the National Party's history, after Jim McLay (who was 38 when elected in 1984)  He also became only the third Southlander to lead a major New Zealand political party, after Joseph Ward and Adam Hamilton  However, English failed to improve the party's performance  In the 2002 election, National suffered its worst electoral defeat ever, gaining barely more than twenty percent of the vote  English described it as "the worst day of my political life"  Both party insiders and the general public were split as to how much to blame him for the loss, but most of the party believed that English would be able to rebuild National's support 

By late 2003, however, National's performance in opinion polls remained poor  The party had briefly increased its popularity in the year following the election, but by October its support had fallen to levels only slightly better than what it achieved in the last ballot  English also appeared in a boxing match for a charity against entertainer Ted Clarke  This did not boost his polling or that of the National party either, with suggestions that it devalued his image as a serious politician  Don Brash, former governor of the Reserve Bank and a relative newcomer to politics, began to build up support to replace English  On 28 October, Brash gained sufficient backing in Caucus to defeat English in a leadership contest 

Shadow cabinet roles and deputy leader
On 2 November 2003, when Brash changed responsibilities for certain MPs, English became National's spokesman for education, ranked at fifth place in the party's parliamentary hierarchy  He remained in parliament after the 2005 election  In his new shadow education portfolio, English performed strongly, and remained a party favourite despite his election defeat as leader in 2002, eventually being returned to the finance portfolio in August 2004 as deputy spokesman (while still retaining responsibility for education) 

In November 2006, Brash resigned as leader  English was considered as a potential replacement leader (running against John Key) or deputy leader (against incumbent Gerry Brownlee) in the ensuing leadership election  However, a contest was avoided when the MPs agreed a Key/English ticket would run unopposed in a display of party unity  English took over the deputy leadership and the finance portfolio in the Key shadow cabinet 

Fifth National Government (2008–2017)

Deputy Prime Minister and Minister of Finance (2008–2016)

At the 2008 election, English was re-elected by his electorate, winning by a margin of about 15,500 votes  He became Deputy Prime Minister of New Zealand and Minister of Finance in the fifth National Government, being sworn into office on 19 November 2008 and continued to serve in those roles until becoming Prime Minister on 12 December 2014  He was also made Minister of Infrastructure in National's first term of government and Minister responsible for Housing New Zealand Corporation and minister responsible for the New Zealand flag consideration process in its third 

He was comfortably re-elected in Clutha-Southland in the 2011 election but opted to run as a party-list candidate in 2014  

The pairing of John Key as leader of the National Party and English as his deputy has been compared to that of Bob Hawke and Paul Keating (in Australia) and Tony Blair and Gordon Brown (in the UK) 

English acceded to the role of Finance Minister in the continuing wake of the financial crisis  In response to New Zealand's rising debt, English made budget deficit-reduction his main priority  His first budget outlined three focuses in New Zealand's financial recovery: "improving the business environment and removing roadblocks to growth; investment in productive infrastructure; and improving the way government works"  One of his first acts was creating the National Infrastructure Unit, charged with formulating a plan for infrastructure projects and investments  He commissioned a government-wide spending review, with an aim to reducing government expenditure—with the exceptions of a two-year stimulus package and long-term increases on infrastructure spending 

In April 2011, the Opposition criticised English for suggesting that New Zealand businesses could use New Zealand's low wages to help it compete with Australia  The National Government campaigned for re-election in 2011 on its economic record  The Government boasted growth for five consecutive quarters up to mid-2010, totalling 1 6% of real GDP 

Strong growth resulted in a surplus of $473 million for the 2015/16 financial year, projected to rise to $8 5 billion by 2020/21  In his 2016 Economic and Fiscal Update address, English stated that reducing debt and tackling the costs of the 2016 Kaikōura earthquake were higher priorities than reducing rates of tax 

Allowances issue
In 2009, the media, including TVNZ and TV3 revealed that English was receiving about NZ$900 a week as part of a living allowance for ministers, to live in his own NZ$1 2 million Wellington home  At the time, English also received $276,200 in his annual salary as Deputy Prime Minister  It was also revealed other ministers with homes in the capital city were also claiming accommodation allowances  On 3 August 2009, Prime Minister John Key started a review of the housing allowances claimed by cabinet ministers  English subsequently paid back $12,000 and only claimed about $24,000 a year in living allowances  The Auditor-General's office said in September 2009 that they were making "preliminary enquiries" into parliamentary housing expenses in response to a letter of complaint from Progressive party leader Jim Anderton  Two days later English stated that he would no longer take up any housing allowance and had paid back all the allowance he had received since the November 2008 election 

Prime Minister (2016–2017)

John Key resigned on 12 December, and endorsed English as his successor in the resulting leadership election  Following the drop-out of both Judith Collins and Jonathan Coleman from the leadership election, English was sworn in as the 39th Prime Minister of New Zealand on 12 December 2016 

English appointed his first cabinet on 18 December  In a reshuffle, he appointed Steven Joyce to succeed him as Finance Minister, while most ministerial portfolios remained the same 

In February 2017, English did not attend Waitangi Day commemorations at the historic treaty grounds, reportedly in response to the Ngāpuhi iwi's decision to stop the Prime Minister from speaking at the marae



ground_truth: It required the transformation to be limited to specific data and a visual depiction representing specific objects or substances.

prompt_front: Now, answer the following question based on the text below, only give me the answer and do not output any other words.

Question: When did the 2017 general election be held?

Read the following text and answer briefly.

Context 3:  Ngāpuhi have protested the Government's negotiation of the Trans Pacific Partnership Agreement (TPPA), which the iwi believe infringes upon Māori sovereignty, and thus does not adhere to the Treaty of Waitangi  English had been invited to attend in an official capacity; his non-attendance was criticised by a Ngāpuhi elder and Opposition leader Andrew Little 

In his first overseas trip as Prime Minister, English travelled to Europe to discuss trade ties, including a prospective New Zealand–European Union free trade agreement  He first travelled to London on 13 January 2017 to meet British Prime Minister Theresa May  Discussing trade relations, English said the two nations were "natural partners" and would "continue to forge ties" after the UK's withdrawal from the EU  He also arranged to meet with London Mayor Sadiq Khan, Belgian Prime Minister Charles Michel and German Chancellor Angela Merkel   In a meeting with Merkel, English received crucial backing from Germany for a trade deal with the EU  On 16 January, English stated that his government would continue to promote TPPA, despite the United States' decision to withdraw from the agreement  He explained that Southeast Asian countries would now be treated as a priority in negotiations—he also asserted that the United States was ceding influence to China by its rejection of the trade pact 

At a press conference at the Beehive on 1 February 2017, English announced that the 2017 general election would be held on 23 September  The Prime Minister later confirmed that his party would approach ACT, United Future and the Māori Party if confidence and supply agreements were required to form a government following the election  In his second cabinet reshuffle on 24 April, English appointed Gerry Brownlee as his new Foreign Affairs Minister; he also promoted Nikki Kaye to the portfolio of Education Minister, and moved Mark Mitchell into the cabinet to become Defence Minister  The reshuffle was perceived as an election preparation 

On 13 February 2017, English welcomed Australian Prime Minister Malcolm Turnbull to Wellington  The two leaders reaffirmed their shared trade agenda, and discussed changes to the Australian citizenship pathway which will affect permanent residents originating from New Zealand 

On 19 June, it was reported that Todd Barclay, who succeeded English as MP for Clutha-Southland, had clandestinely recorded one of his employee's conversations the previous year, and that John Key's leaders' budget was used to pay a confidential settlement after the employee resigned  English admitted that he had been aware of the illegal recording and the settlement, and thus implicated in the scandal 

During the 2017 National campaign launch, English introduced a $379 million social investment package including digital learning academies for high school students, more resources for mathematics, and boosting support for teaching second languages in schools, and maintaining National Standards in the school curriculum  Prime Minister English also sought to defend National's financial management and economic track record and claimed that the opposition Labour Party would raise taxes  Early opinion polling had forecast a poor showing in the election for the Labour Party, but in early August 37-year-old Jacinda Ardern took over as Labour leader and seemingly energised younger voters 

At the 2017 general election, National won the largest share of the party vote (44 4%) and the largest number of seats (56) in the House Representatives  However, National lacked enough seats to govern alone due to two of the party's support partners, the Māori Party and United Future, losing their parliamentary seats  In response, English stated that the party would be entering into talks to form a coalition with New Zealand First  Following talks with the two largest parties, New Zealand First entered a coalition arrangement with the Labour Party  English was succeeded as prime minister by Jacinda Ardern on 26 October 

Opposition (2017–2018)

Leader of the Opposition
English was re-elected as National Party leader on 24 October 2017  At the time of his re-election, English announced his intention to stay on as leader until the next general election  On 13 February 2018, however, he stood down as National Party leader due to personal reasons, and instructed the party to put into motion the processes to elect a new leader  He also retired from Parliament  English's resignation followed weeks of speculation that he would step aside for a new leader  On 27 February, he was succeeded as party leader by Simon Bridges as the result of the leadership election held that day 

Post-premiership 
In 2018, English joined the board of Australian conglomerate, Wesfarmers  English serves in Chairmanships of Mount Cook Alpine Salmon, Impact Lab Ltd and Manawanui Support Ltd  He is also a director of The Instillery, Centre for Independent Studies and The Todd Corporation Limited, and is a member of the Impact Advisory Group of Macquarie Infrastructure and Real Assets 

Political and social views

English is regarded as more socially conservative than his predecessor, John Key  He has stated his opposition to voluntary euthanasia and physician-assisted suicide, same-sex civil unions, and the decriminalisation of prostitution  As Prime Minister he opposed any "liberalisation" of abortion law 

In 2004, English voted against a bill to establish civil unions for both same-sex and opposite-sex couples  In 2005, he voted for the Marriage (Gender Clarification) Amendment Bill, which would have amended the Marriage Act to define marriage as only between a man and a woman  English voted against the Marriage (Definition of Marriage) Amendment Bill, a bill that legalised same-sex marriage in New Zealand  However, in December 2016 he stated, "I'd probably vote differently now on the gay marriage issue  I don't think that gay marriage is a threat to anyone else's marriage" 

In 2009, English voted against the Misuse of Drugs (Medicinal Cannabis) Amendment Bill, a bill aimed at amending the Misuse of Drugs Act so that cannabis could be used for medical purposes 

Personal life 
English met his future wife, Mary Scanlon, at university  She was studying medicine at the time, and became a general practitioner  Both her parents were immigrants, her father being Samoan and her mother Italian, born on the island of Stromboli  They have six children: a daughter and five sons 

English is a practising Roman Catholic, but has stated that he considers his religious beliefs personal and thus separate from politics 

In June 2002, English took part in TV3's Fight For Life, a celebrity boxing fundraiser to raise money for the Yellow Ribbon anti-youth-suicide campaign, influenced by the death of a teenage nephew in 1997  He lost a split decision to former university colleague Ted Clarke 

Honours
In the 2018 Queen's Birthday Honours, English was appointed a Knight Companion of the New Zealand Order of Merit, for services of over 27 years to the State 



ground_truth: 23 September.