BEE-spoke-data/govdocs1-by-extension huggingface dataset:
148                          EXPEDITION  TO  THE
birds observed were the Canada jay,* blue jay,t hairy wood-pecker, Indian hen, golden plover,! and woodcock. We killed five pheasants on the 7th of September; on the 4th, we heard, near Rainy Lake, the notes of the whip-poor-will. A rail was also seen, but it disappeared too soon to enable Mr. Say to determine the species.
The mosquitoes, which troubled us but little after we left Red river, were replaced near the height of land, by some dipterous insects belonging to two distinct species of the genus Simulium.|| Their punctures were equally severe with those of the mosquitoes, but they were not so numerous ; they principally attacked the face and neck, sometimes, however, they crept under our clothes; they seemed to prefer warm and dry weather, differing in this respect from the mosquitoes, which prefer a humid atmosphere.
A number of aquatic plants were observed in Cats-tail river; among these was one resembling our splatterdock,fi but smaller; its leaf always floats, but never projects above the water; its flower and seed-vessel are smaller than those which we have generally seen. Besides these there is a small plant, the leaf-stalks of which are elongated; its leaf, which is small, floats upon the water. We saw another plant with small yellow flowers, and leaves very much divided; its stalk projected six or eight inches above the surface of the water.**
The Kamanatekwoya receives no tributary, of any im-
* Garrulus Canadensis.                f Garrulus cristatus.
$ "Vanellus Helveticus of authors, according to Ord's reprint of Wilson's Ornithology.                           Tetrao umbellus.
|| One of these is the S. venustum, Say, Jour. Acad. Nat. Sci. vol. 3, p. 28.
1 Nuphar lutea.                * Ranunculus delphinefolius, Torrey.
From: Farid Yared [faridyared@cox.net]
Sent: Saturday, January 03, 2004 5:39 PM
To: rule-comments@sec.gov
Subject: Naked short selling should not be allowed

"Naked short positions are non existing shares borrowed without interest 
payments for the sole purpose of selling down the price of the shares. Drug 
cartels, the mafia and terror organizations use them for money laundry purposes. 
Yes you read correctly. Naked short positions carry no expenses, since the 
shares they are borrowed from don't exist and solely are invented as a vehicle 
to bring down share prices. "
 
 
Brokerage houses and their specialists should not be allowed to do the above. 
But I guess since it's harder to catch them, the SEC will do nothing about 
this. Or will they? How about creating a database where every short transaction 
by anybody includes a tracking record of the borrowed shares. Is this too hard 
for the SEC to accomplish? allowing a computer to do the work of the 
undermanned SEC?
 
Or is the SEC rather content with catching the little fish caught red handed 
while allowing the big fish to continue to steal millions and billions and 
use the stolen money to pay off the lawyers defending them against the SEC. 
If the SEC suspects a market maker or specialist of causing the public to 
lose 10 million while a specialist or a client gains 10 million, does a 1 
million dollar settlement make sense? As a true deterrent, the settlement 
should be a severe penalty that costs the firm more than the amount of 

damage it caused.
That will make them think twice before doing it again. Fining them 1 million 
for 10 million in damage will encourage them to keep looking for these zero 
cost, 90% profit transactions.
 
The trial should be for putting the company out of business permanently.
 
 
Enraged small investor,
Farid Yared
Paul Cleggett-Halleim
NASA Headquarters, Washington, D.C.                  May 17, 1990
(Phone:  202/453-1548)

George H. Diller
Kennedy Space Center, Fla.
(Phone:  407/867-2468)


RELEASE:  90-70

ULYSSES SPACECRAFT ARRIVES AT CAPE TO BEGIN LAUNCH PREPARATIONS


     Ulysses, a spacecraft that eventually will explore the sun, 
arrived at Cape Canaveral Air Force Station, Fla., today to begin 
preparations for a launch in October aboard Space Shuttle 
Discovery.

     The Ulysses mission is a NASA-European Space Agency (ESA) 
cooperative project to study the sun, the solar wind and 
interstellar space.  The spacecraft's instruments will study the 
phenomena near the Sun's north and south polar regions, which 
never have been examined by spacecraft.

     The 814-pound satellite, riding aboard an Air France 747 
cargo plane, arrived this morning after about a 10-hour flight 
from Amsterdam in the Netherlands.  Ulysses was taken to NASA's 
Hangar AO prior to beginning final assembly and checkout.

     In July, after fueling at the Explosive Safe Area, Ulysses 
will be transported to the Vertical Processing Facility at KSC to 
be mated with a dual upper stage, a Payload Assist Module coupled 
to an Inertial Upper Stage.

     Ulysses will be carried aboard the Space Shuttle Discovery 
on mission STS-41, scheduled to be launched from Pad B at Complex 
39 on Oct. 5.  The launch opportunity extends for 19 days.  
Discovery is now undergoing preparation for the mission in the 
KSC orbiter processing facility.

     No upper stage propulsion system has enough energy to lift 
the spacecraft directly from Earth over the sun's poles.  
Therefore, Ulysses will be launched on an interplanetary 
trajectory, arriving at Jupiter in February 1992.  

     Ulysses will use Jupiter's gravity to leave the ecliptic 
plane and achieve a flight trajectory which will take Ulysses 
toward the southern pole of the sun.  The satellite then will 
make its first solar polar approach in May 1994.  

     Ulysses' orbit will cross the sun's equator in February 1995 
and continue toward the solar north pole, reaching there in May 
1995.  The mission will conclude in October 1995, 5 years after 
launch.

     The science instruments aboard Ulysses are furnished by the 
United States and Europe.  The ESA spacecraft was built by 
Dornier in the Federal Republic of Germany.  The NASA Jet 
Propulsion Laboratory (JPL), Pasadena, Calif., is managing the 
U.S portion of the mission.  Communications with the spacecraft 
will be through NASA's Deep Space Network tracking stations, 
operated by JPL.

	- end -

     NASA news releases and other information are available 
electronically on CompuServe and GEnie, the General Electric 
Network for Information Exchange.  For information on CompuServe, 
call 1-800/848-8199 and ask for representative 176.  For 
information on GEnie, call 1-800/638-9636.
TITLE:   GCN GRB OBSERVATION REPORT
NUMBER:  120
SUBJECT: SGR1900+14 field optical observations
DATE:    98/06/30 17:05:16 GMT
FROM:    Arne A Henden at USNO/USRA  <aah@nofs.navy.mil>

A. Henden, C. Luginbuhl and F. Vrba (U.S. Naval Observatory Flagstaff
Station) report that they have obtained extensive I-band and J-band
observations of the near-IR sources and surrounding field associated
with SGR1900+14 both before and after the recent onset of activity.
None of the observations coincide with bursts detected by BATSE, and no
unusual photometric behavior has been detected though reductions are
ongoing.  A new eclipsing binary has been detected nearby, however, at
RA 19:07:16.85 DEC +09:18:50.4 (J2000), about 39.0 arcseconds SE of
the M supergiant pair.  The binary is about I=19.1 out of eclipse,
and has been observed through several eclipses of about 0.4mag depth.
The period is either about 1.07day or some integer fraction.
This binary appears as the star labelled 'J' in Figure 1 of
Vrba et. al. ApJ 468:225 (1996).  We bring this star to the attention of
other observers in the hope that it not send anyone on a wild goose
chase if it is detected as a variable in observations of this
gamma-ray burst location.

This message is quotable in publications.
From: Jordan, Andy (HRSA)
Sent: Thursday, April 17, 2008 5:15 PM
To: Patterson, Katherine (HRSA); Josephdegoes, Stephanie (HRSA)
Subject: FW: Comments period Extension Needed for FQHs

 

-----Original Message-----
From: Trujillo, Charlene [mailto:charlene.trujillo@colostate.edu]
Sent: Thursday, April 17, 2008 4:07 PM
To: Jordan, Andy (HRSA)
Subject: FW: Comments period Extension Needed for FQHs

-----Original Message-----
From: Trujillo, Charlene
Sent: Thursday, April 17, 2008 2:04 PM
To: 'John_East@allard.senate.gov'
Subject: Comments period Extension Needed for FQHs

Thank you for your time and commitment to serving our community. I am currently a Board Member for Pueblo Community Health Center, I am also a consumer.

My point of view as a consumer: 
Having a child that need's medication and medical care monthly. I would not know what or where to seek medical care for my child. With out the help of PCHC. With the high cost of medical care, I was faced with paying for private medical care or keeping a roof over my family. I'm personally thankful for having the caring professional staff at PCHC.
Providers can seek employment in a private establishment, but they stay here to serve the uninsured like my self. I am grateful for all of the hard work the center provides on a daily bases.

My point of view as a Board Member: 
This would be detrimental to our community. Tier #2 would eliminate our eligibility for expansion to serve our uninsured in our community.
Pueblo Community Health Center would not be allowed to recruit or maintain providers. Pueblo Colorado now has around 30,000 uninsured Families living right here in our community!

I ask that when you voice you vote that you think for your community, and the uninsured consumer local clinic serve. 

Once again that you for your time.    

Consumer and Board Member at Pueblo Community Health Center.

Gracias/Thank You
Charlene Trujillo
 Bilingual Nutrition Educator
Colorado State University, Extension
212  West 12 th Street
Pueblo, Colorado 81003
719-583-4993 Fax 719-583-6582
E-Mail charlene.trujillo@colostate.edu
000
WGUS84 KEPZ 060345
FLSEPZ

FLOOD ADVISORY
NATIONAL WEATHER SERVICE EL PASO TX
938 PM MDT SAT AUG 5 2006

NMC051-060545-
938 PM MDT SAT AUG 5 2006

THE NATIONAL WEATHER SERVICE IN EL PASO HAS ISSUED A

* FLOOD ADVISORY FOR...
  SOUTH CENTRAL SIERRA COUNTY IN NEW MEXICO

* UNTIL 1145 PM MDT

* AT 938 PM MDT A SPOTTER REPORTED THAT THREE QUARTERS OF AN INCH OF 
RAIN FELL IN THE LAST HOUR IN HILLSBORO AND MODERATE RAIN WAS STILL 
OCCURRING. THE SPOTTER ALSO INDICATED THAT THE PERCHA CREEK WAS NEAR 
BANKFULL. NATIONAL WEATHER SERVICE DOPPLER RADAR INDICATED THAT 
LIGHT TO MODERATE RAIN MAY PERSIST FOR ANOTHER HOUR OR SO. THIS 
RAISES THE POSSIBILITY OF STREAM AND ARROYO FLOODING AS WELL AS 
FLOODING ON STATE HIGHWAY 152.

PERSONS IN THE HILLSBORO AND KINGSTON AREAS AS WELL AS THOSE
NEAR THE PERCHA CREEK SHOULD BE ALERT TO RISING WATERS AND BE
PREPARED TO MOVE TO HIGHER GROUND IF THE CREEK COMES OUT OF ITS
BANKS. 

LAT...LON 3262 10770 3261 10730 3301 10734 3301 10773

$$

MACBLAIN
From: Schierloh, Lee B [PVTC] [mailto:lee.b.schierloh@smithbarney.com]
Sent: Thursday, June 24, 2004 11:21 AM
To: 'chairmanoffice@sec.gov'
Subject: Fund Governance

Dear Chairman Donaldson,

Once again I find myself questioning the role of government in day to day
business affairs. Maybe it goes deeper than this to include the concept of
"free enterprise"
in general. At what point does a regulatory body begin over-stepping its
bounds and start regulating in the "name
of regulating"? 

The recent SEC vote on fund governance smacks of this.

Having faithfully served my constituency- "my clients" for
the last eighteen years, I find it hard to see how their interests are
"best" being served by negatively impacting their fund performance. In
forcing independent directors
on the fund industry you in many cases increase their
cost of doing business and take fund management away
from the task of managing fund assets-their prime purpose
for being.

Numerous studies have shown that fund performance is
negatively impacted by independent boards. It makes sense. Who has a greater
incentive to push for better performance? A vested director or an
independent. Ironically, or not, funds with vested directors have lower
fees on average. Maybe they want better pricing and 
performance too.

Call my argument simplistic and naive, I'm just trying to get the best
performance I can get for my clients. If that occurs on a more regularly
basis with independent boards and directors, I'm all for it. But its not the
case. The facts dispel the rationale for making these changes time and time
again.

Unfortunately for us dog soldiers the generals got it wrong again. 

Yours Truly,
Lee B. Schierloh

P.S.
I hope you take no offense to my position on this issue, as I hold you in
very high regard.

--------------------------------------------------------------
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PUBLIC INFORMATION OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109.  TELEPHONE (818) 354-5011



FOR IMMEDIATE RELEASE		November 20, 1989

	Radar astronomers at the Jet Propulsion Laboratory (JPL),
the Harvard-Smithsonian Center for Astrophysics and the Arecibo
Observatory obtained images of a newly-discovered asteroid as it
passed near the Earth in late August, revealing a two-part form. 
These are the first views of the surface of a small asteroid.
	The images show an irregular double body about a mile long,
rotating like a propeller about every four hours.  Theorists have
speculated that some asteroids could consist of two (or more)
bodies of similar size pulled together by their weak mutual
gravity.  "It is remarkable that the first images of a planetary
body this small should show a double-lobed object," said JPL's
Dr. Steven Ostro, leader of the radar astronomy team.
	The asteroid, designated 1989 PB, came within 2 1/2 million
miles of Earth (eleven times as far as the Moon) in late August,
a few days after the radar observing sessions. 
 	It had been discovered August 9 by JPL optical astronomer
Eleanor Helin and her associates, working at the Palomar
Observatory; Helin quickly alerted the radar team so that their
observations, conducted at the Arecibo Observatory's 1,000-foot
radar/radio telescope in Puerto Rico, could be made in the close pass.


	Orbiting the Sun about every 400 days, 1989 PB travels from
beyond the orbit of Mars to a zone between Venus and Mercury and
back.  Although the asteroid passes near Earth's orbit
frequently, it will not come within several million miles of our
planet again for about half a century.
	Both the radar and the optical observations were part of the
Planetary Astronomy Program of NASA's Office of Space Science and
Applications.  The Arecibo Observatory is part of the National
Astronomy and Ionosphere Center, operated by Cornell University
for the National Science Foundation.  The radar team included Dr.
John Chandler and Dr. Irwin Shapiro of the Harvard-Smithsonian
Center for Astrophysics and Alice Hine of Arecibo Observatory.
	Planetary radar astronomy, which has been used to study the
Moon and the inner planets and, more recently, many asteroids and
outer-planet satellites, is very different from optical
techniques.  While planets and asteroids are seen through the
optical telescope in reflected sunlight (and asteroids look like
tiny points at best), radar provides its own calibrated
illumination, permitting precise measurement of range and motion
from many small reflecting elements of the object.  Computer
processing can turn these data into a two-dimensional image.
	These first images of 1989 PB have picture elements less
than 1,000 feet across, comparing favorably with typical Voyager
spacecraft images, Ostro said. "Within a few months, he added,
"detailed analyses will let us reconstruct the asteroid's three-
dimensional shape, make some statements about how tightly gravity
is holding the two lobes together, and begin to formulatetheories about how it was formed."
#####
#.11/20/89jhw
To: zzz
Subject: permission request
cc: zzz

Dear Webmaster:

Unfortunately this came to my attention.zzz
Unfortunately this was brought to my attention.zzz

May I have permission to put the left handed image of DNA at

     zzz

that is,

     zzz

on my Left Handed DNA Hall of Fame page?

     http://www.ccrnp.ncifcrf.gov/~toms/LeftHanded.DNA.html

Your entry is at:

    http://www.ccrnp.ncifcrf.gov/~toms/LeftHanded.DNA.html#zzz

and permanently at:

    http://www.ccrnp.ncifcrf.gov/~toms/Leftyear2005.html#zzz

This is a non-commercial use.  I have put the example up so you can see how
it is presented.  I can add a copyright statement if you need one.

Information about my permissions policy is at
http://www.ccrnp.ncifcrf.gov/~toms/leftpolicy.html

Please note that your image is the mirror image of DNA found in biological
systems on earth.

Please also note the tongue-in-cheek nature of the page!

Thank you!

  Dr. Thomas D. Schneider
  National Institutes of Health
  National Cancer Institute
  Center for Cancer Research Nanobiology Program
  Molecular Information Theory Group
  Frederick, Maryland  21702-1201
  toms@ncifcrf.gov
  permanent email: toms@alum.mit.edu (use only if first address fails)
  http://www.ccrnp.ncifcrf.gov/~toms/

PS: Take a look at this page:
http://www.ccrnp.ncifcrf.gov/~toms/sciencetiff.html
It may help!!

PPS:
Definition of tongue-in-cheek:
http://kidshealth.org/kid/talk/come_from/tongue_cheek.html
1230YORKAVENUE4NEWYORK,N.Y.10021

June 16, 1976

Dr. F. H. C. Crick
MRC Laboratory of Molecular Biology
University Postgraduate Medical School
Hills Road
Cambridge,  CB2 2&H, England

Dear Francis and Odile:

     I am very sorry that it had to take so long for me to write to you
and thank you for the very nice couple of days I spent in Cambridge which
you had organized so well for me.  I have to thank Odile particularly for
the exquisite food she cooked for me.  I liked your two houses and the garden
across the road, a unique and quite imaginative manner of living.

    The reason for the long delay is that on arrival at the airport
something very unexpected happened to me, namely, I lost the vision in my
right eye.  After arriving in New York a detachment of the retina was found
which required prompt operation.  Fortunately, I fell into the hands of a good
surgeon and already have almost full vision again in the eye.  It has been a
trying time not being able to read and write for several weeks, and it was a
disturbing end to a very pleasant visit to Europe including the better part
which I spent in England.

    Now let me turn to something that has bothered me, namely, that you
felt that the joining of different organisms in the eukaryotic cell was a
chance event.  Yet, in most cases, what we see at present seems to me to be a
"marriage of convenience",
day examples,        and this was why I looked for a background in present-
      such as the case of the lichens where fungi + algae yields a

diversified group of symbionts.  Essentially it seems that the initial reaction
is a phagocytosis of bacteria or other cells which serve as food in primitive
eukaryotes.  Thus, as I see it, symbiosis is the result of an abortive phago-
cy-tosis where instead of being digested, the organism is more or less modified
to become a helper since it can add to the metabolic means of the host, for
example, nitrogen fixation or photosynthesis (Cf. enclosed copy of a paper
given at the Ochoa birthday festival last year).

    I am grateful to have been prompted by your doubt about' seeing some-
thing special in this symbiotic aggregation to have spent some time reviewing
it.  I hope that you might agree that often it may be choice rather than chance.

With many good wishes to you both,

Sincerely,

Fritz Eptnann
TITLE:   GCN GRB OBSERVATION REPORT
NUMBER:  1273
SUBJECT: GRB011121, possible supernova association
DATE:    02/03/15 17:16:11 GMT
FROM:    Peter Garnavich at U of Notre Dame  <pgarnavi@miranda.phys.nd.edu>

P. M.  Garnavich, S. T. Holland (Notre Dame), S. Jha, R. P. Kirshner, 
   D. Bersier, and K. Z. Stanek (CfA)

We have reanalyzed R-band images of GRB 011121 obtained with the
Walter Baade 6.5m Magellan telescope on 2001 Dec. 4.32  in light
of the recently released HST images taken near the same time
(Bloom, GCN 1260). The brightness of the afterglow in the Magellan
data deviated from the steep powerlaw decline seen in the
first three days after the burst and we attributed this to contamination
from the host galaxy (e.g. Phillips et al. GCN 1164). However the Magellan
magnitude of R=23.0+\-0.1, obtained by point-spread-function fitting is
consistent with the WFPC2 magnitude of f702w=23.16+\-0.08 which
has minimal host contamination. Both observations are nearly
2 magnitudes brighter than the early-time extrapolation. 

The full light curve is well fit by an initial powerlaw with
index of 1.71+\-0.05  plus the light curve of SN 1998bw stretched
and faded to a redshift of z=0.36 (Infante et al. GCN 1152). The
Dec. 4 data is 10 days after explosion in the rest frame, while
SN 1998bw peaked 17 days after GRB 980425, so later epochs
may show a small rise in the f702w magnitude before final
fading. The light curve can be viewed at

http://www.nd.edu/~pgarnavi/grb011121/grb011121_sn.ps

Assuming a flat cosmology with Omega_m=0.3 and a Hubble
parameter of 65 km/s/Mpc, we derive an absolute magnitude for
the possible supernova on Dec. 4 of Mv=-19.3+\-0.2 (corrected
for a large Galactic extinction but not for host extinction), consistent
with SN 1998bw near maximum.  These observations could be strong
evidence for a SN-GRB connection.

This message may be cited.
"Venite&#059; O come let us sing /","sm1885/16900","16983","001.gif","1","1","","001.tif"
"Venite&#059; O come let us sing /","sm1885/16900","16983","002.gif","2","2","","002.tif"
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"Venite&#059; O come let us sing /","sm1885/16900","16983","005.gif","5","5","","005.tif"
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"Venite&#059; O come let us sing /","sm1885/16900","16983","007.gif","7","7","","007.tif"
"Venite&#059; O come let us sing /","sm1885/16900","16983","008.gif","8","8","","008.tif"
"Venite&#059; O come let us sing /","sm1885/16900","16983","009.gif","9","9","","009.tif"
Subject: FVFE01 RJTD 120910
FVFE01 RJTD 120910
VA ADVISORY
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AT
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FROM JMA NWP MODEL.
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NXT ADVISORY: WE WILL ISSUE FURTHER ADVISORY IF VA IS DETECTED IN
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ELLITE IMAGERY=

.
A collection of particle data acquired from several spacecraft with use of 
the instruments by TASPD SINP MSU has been restored and presented on Internet 
due to efforts of many people.

TASPD staff members from the Heliosphere Physics Lab Tamara Styopina, 
Tatyana Khotilovskaya and Lidiya Ryabova have made the most significant 
contribution to converting the data tables from old papers into 
the computer-readable files for non-geocentric spacecraft.  Sergey Ermakov 
has performed the manual digitization of the trajectory data for 
these spacecraft and the initial correction of these coordinate data 
for the sake of their better smoothing.  Together with Dr. Eugene Chuchkov 
and Dr. Vladimir Tulupov, he input a lot of corrections into the time-tags 
of a huge-size data set from GRANAT.  Dr. Vladimir Tulupov and 
Dr. Boris Scherbovsky gave the notes concerning specifics of 
the historically used sensors, which is necessary for proper 
understanding of the presented data.  From the very beginning, 
a head of the Lab Dr. Nickolay Kontor supported an idea of this work 
by all means; many things could not be done without his participation.

A head of the Magnetosphere Physics Lab, Dr. Elmar Sosnovets has supported 
restoration of the data collection from COSMOS-900 and participated in all 
most essential discussions.  Dr. Lyudmila Tverskaya has leaded a part of work 
relevant to rectification of a huge data set from COSMOS-900.  
Tatyana Lukina and Dr. Tatyana Ivanova performed this tremendous work.

Dr. Nickolay Pavlov made a lot of programming, data rectification works, 
preparing documentation, organizing work, etc.

Prof. Boris Tverskoy, a head of TASPD till 1997, supported this work.

Dr. Nickolay Khevinson from IKI RAN and Dr. Alexander Sheikhet from NPO 
Lavochkina have provided us with the exact elements of the GRANAT's orbit.

It should be notices the useful work of the World Data Center B whose printed 
issues of particle datasets from Russian spacecraft, published in 70s, helped 
us a lot in preparing a part of the collection.
The work has been supported by NASA, grant NAG5-4656.  All participants 
from TASPD are very thankful to those colleagues from the USA who trusted 
us in this initiative.  The grant gave us a new exceptional opportunity 
to realize the initial idea with a good modern equipment.

It was very pleasant to cooperate with Dr. Joseph King from NSSDC/GSFC, NASA.  
His suggestions, and the fruitful discussions of many aspects of data 
organization that took place with him and his colleagues, gave us a lot of 
new understanding of the scheme of a data collection oriented onto user's 
needs.  His patience and his approach that directed to data standardization 
but, nevertheless, leaves a room for individuality of each data contributor 
are really exceptional.  Dr. Nataliya Papitashvili made a lot for deriving 
the final form of the data collection and porting its copy to NSSDC.

Nick Pavlov, 1999
Bartsch, L. A., Rada, R. G., and Sullivan, J. F., 1996, A comparison of solids
collected in sediment traps and automated water samplers: Hydrobiologia, v.
323, no. 1, p. 61-66.

Abstract

Many telemetry transmitter attachments disrupt downy insulation, and may
bias survival studies during cold weather by making ducklings more
susceptible to chilling. We compared thermal responses of untreated 1-day-old
mallards (Anas platyrhynchos) to ducklings carrying external sutured
backpack or subcutaneously implanted transmitters. Ducklings carrying
external transmitters showed areas of increased surface temperature in
thermographic images. However, open-circuit respirometry studies at 5, 10,
15, 20, and 25 C and wind speeds of 0.1, 0.2, 0.5, and 1 m/s indicated no
biologically significant differences in total heat production, net heat
production, or short-term body mass loss. These results do not exclude the
possibility of other negative effects of transmitters on duckling behavior and
survival.

Keywords

Anas platyrhynchos, evaporative cooling, mallards, metabolic rate,
radiotelemetry, recruitment, radio transmitters, metabolism chamber,
oxygen-consumption, wild mallards, wind, behavior, temperature,
canvasbacks, animals, ducks
VA1659

1.  BERNARD ROAD, VIEW OF QUARTERS #51 FROM SOUTH
2.  BERNARD ROAD, GENERAL VIEW OF QUARTERS #51 FROM WEST
3.  BERNARD ROAD, VIEW OF QUARTERS #51 & #53 FROM WEST
4.  BERNARD ROAD, VIEW OF QUARTERS #41-#47 FROM SOUTH
5.  BERNARD ROAD, GENERAL VIEW OF QUARTERS #47A & B FROM SOUTH
6.  BERNARD ROAD, VIEW OF QUARTERS #37-#29 FROM SOUTH
7.  BERNARD ROAD, GENERAL VIEW OF QUARTERS #37-A & B FROM SOUTHEAST
8.  INGALLS ROAD, GENERAL VIEW FROM CORNER OF INGALLS ROAD AND FRANK LANE LOOKING NORTHEAST
9.  INGALLS ROAD, BUILDING #95/93 FROM NORTHEAST
10.  INGALLS ROAD, VIEW OF #95 FROM EAST
11.  INGALLS ROAD, VIEW OF #89/91 FROM NORTHEAST
12.  INGALLS ROAD, VIEW OF #89 FROM SOUTHEAST
13.  INGALLS ROAD, VIEW OF #85/87 FROM NORTHEAST
14.  INGALLS ROAD, VIEW OF #87 FROM NORTHEAST
15.  INGALLS ROAD, VIEW OF #85 FROM SOUTHEAST WITH #89 IN THE BACKGROUND
16.  INGALLS ROAD, VIEW OF #83 FROM NORTHEAST
17.  INGALLS ROAD, VIEW OF #81/83 FROM NORTHEAST
18.  INGALLS ROAD, VIEW OF #81/83 FROM SOUTHEAST
19.  INGALLS ROAD, VIEW OF #75 FROM NORTHEAST
20.  INGALLS ROAD, VIEW OF #73 FROM NORTHEAST
21.  INGALLS ROAD, GENERAL VIEW TO HOUSES SOUTH OF #73 FROM NORTHEAST
22.  INGALLS ROAD, VIEW OF #67/69 FROM NORTHEAST
23.  INGALLS ROAD, VIEW OF #67 FROM SOUTHEAST
24.  INGALLS ROAD, VIEW OF #65/63 FROM NORTHEAST
25.  INGALLS ROAD, VIEW OF #63/65 FROM SOUTHEAST
26.  INGALLS ROAD, VIEW OF #61/59 FROM NORTHEAST
27.  INGALLS ROAD, VIEW OF #59/61 FROM SOUTHEAST
28.  INGALLS ROAD, VIEW OF #57/55 FROM NORTHEAST
29.  INGALLS ROAD, VIEW OF #55/57 FROM SOUTHEAST
30.  INGALLS ROAD, DETAIL OF ALLEGORICAL ANGEL KEYSTONE ON SECOND FLOOR
31.  INGALLS ROAD, VIEW OF TYPICAL KEYSTONE ON FIRST FLOOR
32.  INGALLS ROAD, DETAIL OF KEYSTONE
33.  FENWICK ROAD, GENERAL VIEW OF #29 AND #33 FROM SOUTHWEST
34.  FENWICK ROAD, VIEW OF #29 FROM SOUTH
35.  FENWICK ROAD, VIEW OF #33 FROM SOUTHWEST
36.  TIDBALL ROAD, QUARTERS #18
37.  AERIAL VIEW
38.  AERIAL VIEW
39.  AERIAL VIEW
40.  AERIAL VIEW
41.  AERIAL VIEW
42.  AERIAL VIEW
43.  AERIAL VIEW
44.  AERIAL VIEW
45.  AERIAL VIEW
46.  AERIAL VIEW
47.  AERIAL VIEW
48.  AERIAL VIEW
49.  AERIAL VIEW
50.  AERIAL VIEW
51.  AERIAL VIEW
52.  AERIAL VIEW
53.  AERIAL VIEW
54.  AERIAL VIEW
55.  AERIAL VIEW
56.  AERIAL VIEW
57.  AERIAL VIEW
58.  AERIAL VIEW
59.  AERIAL VIEW
60.  AERIAL VIEW
61.  AERIAL VIEW
62.  AERIAL VIEW
63.  AERIAL VIEW
64.  AERIAL VIEW
65.  AERIAL VIEW
66.  AERIAL VIEW
67.  AERIAL VIEW
68.  AERIAL VIEW
69.  AERIAL VIEW
70.  AERIAL VIEW
71.  AERIAL VIEW
UNA:+.?*'
UNB+UNOC:4+sender-id+receiver-id+20090105:1901+interchg-ref'
UNH+msg-refnum-abc+IFTMCS:D:05B:UN:::++++AIAG MOSS'
BGM+705:::Bill of Lading+19298:5:B+9'
DTM+132:20070807120000:204'
DTM+133:20070720120000:204'
DTM+137:20070711120000:204'
TSR+27+2:172++9'
MOA+44:287782:EUR'
MOA+40:193248:EUR'
FTX+AAR+++This cargo is to be cleared at Charleston prior to movement to Spring Hill. GO date is 15 days from VSL ARR for CAD and 15 days FM ARR Inland for Inbond'
FTX+AAA+++auto parts'
LOC+73+NLRTM::6'
TOD++CC+FCA::4'
RFF+BM:APLU706026315'
RFF+BN:842987:18'
DTM+171:20070811120000:204'
RFF+UC:VLU-1175007:18'
RFF+CT:contract123'
RFF+AAJ:DO123'
RFF+RF:98304982:18'
RFF+OP:88732'
RFF+SRN:2178883:20'
RFF+UCN:VLU-1175007:18'
TCC+see UN rec 23:132:::C++100236'
LOC+57+NLRTM:::Rotterdam'
TDT+20+42+1:vessel++APLU::182:American Presidents Line+++vessel:::APL Egypt:US'
LOC+7+USMRC::6:Spring Hill, TN+:::TN+:::US'
LOC+88+NLRTM::6:Rotterdam'
LOC+12+USCHS::6:Port of Charleston+1601'
LOC+9+42157::112:Rotterdam'
NAD+CA+123456789::16++Quick Carrier, Inc.+100 Main St+Your Town+MD:::+20878+US'
NAD+CB+234598776::16++Global CB+100 Main Street+Anytown+Maryland:::+20878+US'
CTA+IC+:James Broker'
COM+james.broker@example.com:EM'
NAD+FW+2356::163++ABC Freight Forwarder+ABC Freight Forwarder+Mytown+Maryland:::+20878+US'
CTA+IC+:Freddy Forward'
COM+FForward@example.com:EM'
NAD+MI'
CTA+IC+:Martin Material'
COM+martin@example.com:ME'
NAD+SE+321777392::16++Acme Auto Supplier GMBH+Mototren Kaiser Kreisel+Kaiserslautern+Rhineland-Palatinate:::+67663+DE'
CTA+SR+:Joe Sales'
COM+301 555 3432:TE'
RFF+ABR:98734927:18'
RFF+ED:983:18'
RFF+EX:9849483:18'
RFF+EP:30982:18'
NAD+SF+498994588::16++Acme Auto Supplier GMBH+Mototren Kaiser Kreisel+Kaiserslautern+Rhineland-Palatinate:::+67663+DE'
CTA+IC+:Joyce ShipFrom'
COM+301 555-1232:TE'
NAD+ST+964475835::16++Any Logistics Mngt, Inc+3830 Main Street+Cherry Hill+TN:::+37174+US'
CTA+IC+:Sally Shiptu'
COM+sally@example.com:EM'
CTA+NT'
GID+1+22:box'
TMD+3++1'
LOC+28+US::5'
PIA+1+AS123:AB'
PIA+1+buyerID123:GB'
PIA+1+1:BL'
PIA+1+drawing1:DR'
PIA+1+ec8:EC'
PIA+5+8708.80.6590:HS'
PIA+1+pserv123:MP'
PIA+1+ver1:AA'
PIA+1+MAT1:BM'
PIA+1+0:BQ'
PIA++VEN12345:VN'
FTX+AAA+++cylinder heads'
MEA+AAY+ABJ+MTQ:20'
MEA+PD+G+KG:8628'
DIM+AAZ+cm:225:146:91'
PCI++Packages 1 to 22, individuallly labeled.'
DGS+49+4'
FTX+AAD+++dangerous stuff'
EQD+CN+APLU3011360::5+21+1++5'
TMD+3++1'
MEA+AAX+AAD+KG:8628'
MEA+AAX+SQ+M:22'
SEL+690545+SH:::Adam Opel'
UNT+83+msg-refnum-abc'
UNZ+1+interchg-ref'
000
WUUS54 KBRO 132244
SVRBRO
TXC061-215-132315-
/O.NEW.KBRO.SV.W.0062.070813T2244Z-070813T2315Z/

BULLETIN - EAS ACTIVATION REQUESTED
SEVERE THUNDERSTORM WARNING
NATIONAL WEATHER SERVICE BROWNSVILLE TX
544 PM CDT MON AUG 13 2007

THE NATIONAL WEATHER SERVICE IN BROWNSVILLE HAS ISSUED A

* SEVERE THUNDERSTORM WARNING FOR...
  WEST CENTRAL CAMERON COUNTY IN DEEP SOUTH TEXAS...
  SOUTHEASTERN HIDALGO COUNTY IN DEEP SOUTH TEXAS...
  THIS INCLUDES THE CITIES OF...WESLACO...MERCEDES...EDCOUCH...
  DONNA...

* UNTIL 615 PM CDT

* AT 535 PM CDT...NATIONAL WEATHER SERVICE DOPPLER RADAR INDICATED A
  SEVERE THUNDERSTORM CAPABLE OF PRODUCING DIME SIZE HAIL...AND
  DAMAGING WINDS IN EXCESS OF 60 MPH.  THIS STORM WAS LOCATED NEAR
  MERCEDES...AND MOVING SOUTHWEST AT 10 MPH.

* THE SEVERE THUNDERSTORM WILL BE NEAR...
  MERCEDES BY 600 PM CDT...
  WESLACO BY 605 PM CDT...
  DONNA BY 610 PM CDT...
  PROGRESO BY 615 PM CDT...

THIS IS A DANGEROUS STORM. IF YOU ARE IN ITS PATH...PREPARE
IMMEDIATELY FOR DAMAGING WINDS...DESTRUCTIVE HAIL...AND DEADLY CLOUD
TO GROUND LIGHTNING. PEOPLE OUTSIDE SHOULD MOVE TO A SHELTER...
PREFERABLY INSIDE A STRONG BUILDING BUT AWAY FROM WINDOWS.

LAT...LON 2623 9780 2632 9797 2609 9815 2598 9793

$$

PHILO
Comments for Review of NuMI RAW system 

                           Oct  24, 2001

                   from    Russ Rucinski
                       ------------------------

The piping diagram conforms with the ISA piping standard and is readily understood by 
those familiar with process piping.
 
The cooling water to the adsorber pile shielding has multiple parallel paths (and 
parallel/redundant paths) without an obvious means to equalize or set desired flow 
rates to the modules.  It understood that the amount of energy deposited will vary 
among the different modules.  I further understand that efforts were probably made 
to design in the correct flow impedances.  It is worth designing in a convenient 
means of adding valves should flow balancing be necessary.
 
As mentioned by a different reviewer in the meeting, if the purpose of the expansion 
tank (at H5 on drg. ME-406229, rev.B) in the adsorber raw system is to separate out 
evolved gas, the flow should be in one end of the tank and out the other.
 
Alternatively, an experience I have had with gas in water systems is that the air 
collects in the top of the full flow filters on the suction side of the pump.  That 
is a bleed off point that we commonly use.  You may consider moving the expansion
tank at H5 to a large port connection on your filter at E5.
 
The back pressure regulator on the expansion tanks should be replaced by a manual 
flow control valve.  The back pressure regulator and supply regulator will fight 
each other.
 
You probably should have plans to have a gas analyzer connection to the vent line 
of your expansion tank to determine the level of H2 in the nitrogen.
 
I agree with your decision not to rely on flow measurement as an alarm or interlock point.
 
Your expansion tanks seem to fall outside of the scope of ASME boiler and pressure 
vessel code, but to save yourself time and energy with the safety committees, you might 
consider putting a diverter valve and an additional relief valve on such.  It will allow 
you the means to pull off the relief and test it periodically.
 
I think the connections to the ejector pump may be incorrect.  The horn drain should go 
into the throat of the ejector pump.  The pump flow goes through the venturi.
 
Submitted by Russ Rucinski, NUMI reviewer
SIGHTS OF PARIS.
321'
other's business, that few have any acquaintance with their
neighbours above and below them.
The circumscribed limits of the city, and the density of
its population, enable the Parisians to make a glittering
display in the streets, in the brilliancy and taste of which
they no doubt outdo any other people in the world. The
close vicinity of its inhabitants, and the facility with which
they get into the streets, and the tens of thousands of induce-
ments that tempt them there, tend to the concentration of
fashion and gaiety in the principal avenues and arcades,
which, in the pleasant evenings of spring and summer,
seem converted into splendid and brilliant salons, with the
appearance of continuous and elegant soires. To these
scenes all Parisians and all foreigners are alike admitted,
to see and enjoy the myriads of sights to be seen in the
shop-windows, as well as to most of the splendid collections
of works of literature and the arts, which, being under the
Government control, are free to the inspection of all who
wish to see them. Amidst most of these I have been, like
thousands of others, a visitor and admirer for two years,
seeking for information and amusementfor study and con-
templationalone ; or enjoying them in company with my
little children, or travelling friends, for whose aid and amuse-
ment I have as often given my time.
The reader will here see that I have before me the ma-
terials for another book, but as the object of this work is
attained, and its limits approached, with my known aversion
to travel over frequented ground, I must refer him to
other pens than mine for what I might have written had I
the room for it, and had it not been written twenty times
before.
The little bit of my life thus spent in the capital of
France, though filled with anxieties and grief, has had its
pleasant parts, having seen much to instruct and amuse
me, and having also met with, as in London, many warm
friends, to whom I shall feel attached as long as I live. In
the English society in Paris I met a number of my London
VOL. II.                                                                                           Y
.~)~; ~
#730
	ThterVieWer~	~
	Person interviewed~	~ ~	- -~--
816 Walnut Street, North Little Rock, Arkansas
A;7A  84
~ _____

	I was plowing when they surrendered. I had just learned to plows and was putting up some land, My young master come home and was telling me the War was ended and we was all free,

I was born in Lauderdale County, Mississippi, I think lt was about Vi)~V)
1854, My fathers name ~ ~ my mothers ~  I knew them both.

My mother belonged to Sterling and my father belonged to a man nan~d Huf Richmond Huff.

	We lived in Lauderdale County. Huff wou.ldn t sell my father and my people wouldnt t sell my mother, They lived about a mile or so apart. They didnt marry in them days. The niggers didnt, that Is, Father would just corne every Saturday night to see my mother. His cabin was about three miles from hers. We moved fromLauderdale County to Scott County, Mississippi, arid that separated mama and papa. They never did meet again. Of courses I mean it was the white people that moved, but they carried mains and us with them, Papa and mama never did meet again before freedom, and they didnt

meet afterwards,

	My mother had twelve children.--.eight girls and four boys, She had one by a man named Peter ~aith, ~ She was away from her husband then. She had four by my fathertwo boys and two girls;~y fathers name was Peter Huff, My mothers name was Mary Sterling~ I never did see my father no more after we moved away from him,
1~x~-s1ave Storiss	Page Two	150
(Texas)

long tails gins to shoot, d~,n it look like all de stars had came out of Heaven, and did dey fall! De stars not ai]. what fell. De white folks and de niggere fell on d.ere knees, prayin to Gawd to save dem iffen de world commt to a end, and de women folks all iun down in de cellar and stayed t 111 rnornizi  . Old Marse say tt was in 1833, and. he say dem stars lail a!hilo and quit awhile, like de showers when it rains.

	Bout a year after freedc~a Old Marse give us a piece of land for a church and dis was de school  t . De preacher s name was Christmas Crawford  and dat de reason I members it, it so funx~y to us. De nigger teacher n~zaed Nimron. De nigger. has de blueback speller. and larns rithmetic, too.

	On Thanksgivin Day de niggere goes round to de white folks houses and. gives a ~ like dis:

ufDe old bee make de honeycinb, De youx~g bee make de honey De nigger make de cotton and corn, And de white folks glt de mone~r.

t ~De raccoon he a curious man, H. never works till dark; Nothin ever sturbe he mind, Till he hear old Towser bark.

	Den de white folks asks us in and help ourselves to de cake or wine or whatever dey has, and. we does dis on Christmas, to.

	We had a song wed. sing when wes thinkin of crnin to Texas:

tJell putfor de South, for seven-up and loo,

Ohime in, n igge is  w m t you come  I ong  too?
No use talkin when de nigger wants to go,
Where de corn top blossoms and canebrakes grow.
Come long, cuba, and dance de polka juba,
Way down South, where de corn tapa grow.

	I, ~ t d I Ike t o be in old Alabama t o d te  btit Old. Marse and Miscue gone  and

it aint no use goin dere no more.
#ifndef TSIM_L1CPS
#define TSIM_L1CPS
///////////////////////////////////////////////////////////////////////////////
// File: tsim_l1cps.hpp
//
// Purpose:   Header File for CPS objects Finder
// Input  :   CPS Cluster Chunk info
// Output :   CPS Object (Type=electron/EM, Addr=address)
//
// Created:   07-JUNE-99  A. Lucotte
// History:
///////////////////////////////////////////////////////////////////////////////
#include "edm/Event.hpp"
#include "edm/TKey.hpp"
#include "unpack_evt/SysID.hpp"
#include "unpack_evt/Channel.hpp"
#include<math.h>
#include<stdlib.h>
#include<iostream.h>
#include"CPS_L1Object.hpp"
//=========================================================
// CPS L1 Cluster Class
//=========================================================
typedef unsigned int MYBYTE;
class tsim_l1cps{
public:
  tsim_l1cps();
  ~tsim_l1cps();
  int Get_L1ObjectCount();
  void CPS_L1ObjectForm();
  void Read_L1Object( int L1Object );
  void read_L1_CPS(Event &, D0MCH::SysID) ;
  std::vector<D0MCH::Channel> create_CPSL1Chunk(Event &, D0MCH::SysID);
  CPS_L1Object & operator[]( int i );      // Return _cps_l1object[i]
private:
  int _l1ObjectCount;                      // Count L1 Objects
  CPS_L1Object _cps_l1object[ 512 ];       // List of L1 Objects
  vector<Channel> _cpsl1chunk[];                     // CPS L1 Chunk Output
};
// Bit Packing Function (from Mrinmoy) //
inline MYBYTE mask(MYBYTE j){
  MYBYTE maskbits=1;
  for (MYBYTE i=1; i<j; i++){
    maskbits = maskbits + (1<<i);
  }
  return maskbits;
};
//    Packed word for CPS layer
//      - Format:
//    --------------------------------------------------------------------------------
//   |31 30 29 28 27 26 25 24 23 22 21 20 19 18 17 16 15 14 13 12 11 10 09 08 07 06 05
//   |--------------------------------------------------------------------------------
//   |NS| Front End |  Cluster address      |ty| width  |lo|hi|MIP bit pattern=000 |
//    --------------------------------------------------------------------------------
inline MYBYTE CPS_PACK(int side , int fend, int addr, int type, int widt,
		       int tlow , int thig ){
  MYBYTE i= (  (side & mask(1))<<31 )|
             ( (fend & mask(4))<<27 )|
             ( (addr & mask(8))<<19 )|
             ( (type & mask(1))<<18 )|
             ( (widt & mask(3))<<15 )|
             ( (tlow & mask(1))<<14 )|
             ( (thig & mask(1))<<13 );
  return i;
};
// UnPacked word for CPS axial layer data at PP//
inline void CPS_UNP(MYBYTE pword, int& side ,
		    int& fend, int& addr, int& type,
		    int& widt, int& tlow , int& thig ){
  side = ((pword>>31) & mask(1));
  fend = ((pword>>27) & mask(4));
  addr = ((pword>>19) & mask(8));
  type = ((pword>>18) & mask(1));
  widt = ((pword>>15) & mask(3));
  tlow = ((pword>>14) & mask(1));
  thig = ((pword>>13) & mask(1));
};
#endif
000
WGUS82 KMFL 100103
FLSMFL
FLC043-101615-
FLOOD STATEMENT 
NATIONAL WEATHER SERVICE MIAMI FL 
900 PM EDT THU JUN 09 2005


...A RIVER FLOOD WARNING REMAINS IN EFFECT FOR THE FISHEATING CREEK 
AT PALMDALE...

ABUNDANT RAINS DURING THE PAST WEEK HAVE SATURATED THE GROUND AROUND SOUTH
FLORIDA,ESPECIALLY ACROSS GLADES AND HIGHLANDS COUNTIES. THIS HAS RESULTED
IN FLOOD LEVEL CONDITIONS AT FISHEATING CREEK. MOIST TROPICAL RAINS WILL
CONTINUE THROUGH THIS WEEKEND POSSIBLY EXACERBATING THE SITUATION.

FOR FISHEATING CREEK NEAR PALMDALE, THE LATEST STAGE IS 7.0 FEET AT 07 AM
THURSDAY.  MINOR FLOODING IS FORECAST. THE STAGE WILL REMAIN AT OR SLIGHTLY
ABOVE FLOOD STAGE THROUGH 8 PM MONDAY.

FISHEATING CREEK EXCEEDED THE FLOOD STAGE OF 7.0 FEET AT 03 AM THURSDAY.
WITH THE LEVEL AT 7.0 FEET,UP STREAM CAMPGROUND ROADS AND FACILITIES WILL
REMAIN FLOODED.

REPORT ANY FLOODING TO THE NEAREST LAW ENFORCEMENT AGENCY OR YOUR COUNTY 
EMERGENCY MANGEMENT. THEY WILL RELAY YOUR REPORT TO THE NATIONAL WEATHER SERVICE
OFFICE.



DO NOT DRIVE VEHICLES THROUGH AREAS WHERE WATER COVERS THE ROAD.  

STAY TUNED TO NOAA WEATHER RADIO FOR ADDITIONAL INFORMATION AND UPDATES.

$$
                               FLD  OBSERVED         FORECAST 7AM     
LOCATION                       STG  STG  DAY TIME    FRI    SAT    SUN

LAKE OKEECHOBEE/FISHEATING CREEK
  PALMDALE                       7  7.0  THU 07 AM   7.0    7.0    7.0
"Before supper quadrille","sm/sm1879/00100","00105","001.gif","1","1","","001.tif"
"Before supper quadrille","sm/sm1879/00100","00105","002.gif","2","2","","002.tif"
"Before supper quadrille","sm/sm1879/00100","00105","003.gif","3","3","","003.tif"
"Before supper quadrille","sm/sm1879/00100","00105","004.gif","4","4","","004.tif"
"Before supper quadrille","sm/sm1879/00100","00105","005.gif","5","5","","005.tif"
"Before supper quadrille","sm/sm1879/00100","00105","006.gif","6","6","","006.tif"
"Before supper quadrille","sm/sm1879/00100","00105","007.gif","7","7","","007.tif"
"Before supper quadrille","sm/sm1879/00100","00105","008.gif","8","8","","008.tif"
"Before supper quadrille","sm/sm1879/00100","00105","009.gif","9","9","","009.tif"
"Before supper quadrille","sm/sm1879/00100","00105","010.gif","10","10","","010.tif"
"Before supper quadrille","sm/sm1879/00100","00105","011.gif","11","11","","011.tif"
"Before supper quadrille","sm/sm1879/00100","00105","012.gif","12","12","","012.tif"
"Before supper quadrille","sm/sm1879/00100","00105","013.gif","13","13","","013.tif"
"Before supper quadrille","sm/sm1879/00100","00105","014.gif","14","14","","014.tif"
"Before supper quadrille","sm/sm1879/00100","00105","015.gif","15","15","","015.tif"
"Before supper quadrille","sm/sm1879/00100","00105","016.gif","16","16","","016.tif"
"Before supper quadrille","sm/sm1879/00100","00105","017.gif","17","17","","017.tif"
"Before supper quadrille","sm/sm1879/00100","00105","018.gif","18","18","","018.tif"
"Before supper quadrille","sm/sm1879/00100","00105","019.gif","19","19","","019.tif"
"Before supper quadrille","sm/sm1879/00100","00105","020.gif","20","20","","020.tif"
"Before supper quadrille","sm/sm1879/00100","00105","021.gif","21","21","","021.tif"