cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.5255/ukda-sn-6912-3
title: Understanding Society: Innovation Panel, Waves 1-5, 2008-2012: Special Licence Access, Local Education Authorities
DOI: 10.5255/ukda-sn-6913-3
title: Understanding Society: Innovation Panel, Waves 1-5, 2008-2012: Special Licence Access, Strategic Health Authorities
DOI: 10.5255/ukda-sn-6914-3
title: Understanding Society: Innovation Panel, Waves 1-5, 2008-2012: Special Licence Access, Primary Care Organisations
DOI: 10.5255/ukda-sn-6915-3
title: Understanding Society: Innovation Panel, Waves 1-5, 2008-2012: Special Licence Access, Output Area Classification (OAC)
DOI: 10.5255/ukda-sn-6916-3
title: Understanding Society: Innovation Panel, Waves 1-5, 2008-2012: Special Licence Access, Travel to Work Areas
DOI: 10.4225/08/5200456cd09b5
title: Parkes observations for project P262 semester 2004JANT

description: Timing of young pulsars
DOI: 10.4125/pd0043th
title: Approach to the Core Structure of the Polycyclic Alkaloid Palhinine A

description: A synthesis of the tricyclic partly substituted core structure of palhinine A was achieved. To reach the bicyclo[2.2.2]octane motif a domino Michael reaction was employed as a key step. After Arndt–Eistert homologation and intramolecular aldol reaction the isotwistane core could be obtained after simple functional-group manipulations.
DOI: 10.4125/pd0044th
title: Addition of Terminal Alkynes to Aromatic Nitriles Catalyzed by Divalent 
Lanthanide Amides Supported by Amidates: Synthesis of Ynones

description: An efficient protocol has been established for the synthesis of conjugated ynones via addition of terminal alkynes to aromatic nitriles, which is catalyzed by novel divalent lanthanide amide complexes. All the reactions gave the products in good to excellent yields at room temperature under solvent-free conditions without any additives. The novel lanthanide amide catalysts were also synthesized and structurally characterized for the first time.
DOI: 10.4125/pd0045th
title: A Domino Palladium Catalysis: Synthesis of 7-Methyl-5H-dibenzo[a,c][7]
annulen-5-ones

description: A domino Pd-catalyzed reaction of 1-(2-bromophenyl)ethanones for the synthesis of novel 7-methyl-5H-dibenzo[a,c][7]annulen-5-ones, a carbon core structure present in colchicinoid natural products, is presented. The reaction is proposed to proceed via intermolecular homobiaryl coupling and intramolecular aldol condensation.
DOI: 10.4125/pd0046th
title: A Practical, Ligand-Free, Palladium-Catalyzed Isocyanide Insertion Reaction for the Construction of Novel Ring-Fused Quinazolinones

description: A high-yielding, ligand-free, palladium-catalyzed isocyanide insertion reaction for the synthesis of phthalazino[1,2-b]quinazolinones from the readily obtainable quinazolinones has been developed. Easily handled and relatively low-cost palladium(II) acetate was used as the catalyst, without an additional ligand. Preparation of the quinazolinones involved the cascade reaction of isatoic anhydrides, phenylhydrazines and 2-bromobenzaldehyde catalyzed by p-toluenesulfonic acid in one pot. This novel protocol may be applicable for the synthesis of other important ring-fused heterocyclic compounds.
DOI: 10.4125/pd0048th
title: Highly Regioselective Allylic Substitution Reactions Catalyzed by an Air-Stable (π-Allyl)iridium Complex Derived from Dinaphthocyclooctatetraene and a Phosphoramidite Ligand

description: An air-stable (π-allyl)iridium complex derived from dinaphthocyclooctatetraene and a phosphoramidite ligand has been synthesized and found to be highly efficient in iridium-catalyzed allylic substitution reactions. This catalyst features excellent regioselectivity and high stability. When NaCH(CO2Me)2 was used as the nucleophile, the catalyst loading in allylic alkylation reactions can be as low as 0.01 mol%.
DOI: 10.4225/08/5200460faa552
title: Parkes observations for project P262 semester 2004OCTS

description: Timing of young pulsars
DOI: 10.4231/d3319s29k
title: Seismic earth pressures on retaining wall on pile in sand with clay layer underneath (GC03)

description: A series of dynamic centrifuge experiments on a standard cantilever wall supported on piles were performed to evaluate their seismic performance. The supporting soil was a compacted low plasticity clay and the backfill was a medium dense sand. The main objective is to evaluate the accuracy of current design standards and analysis procedures
DOI: 10.4231/d36q1sh1b
title: Seismic Behavior of Modern Reinforced Concrete Structural Walls (Specimen PW2)

description: A series of four experiments were conducted to study the behavior of planar reinforced concrete walls representative of modern buildings in seismic zones. Tests were designed per the ACI 318 building code. Demands on the wall simulated earthquake loads expected to occur in mid-rise buildings. The test specimens simulated the lower three stories of a ten-story wall, with demands at the third floor boundary selected to simulate the loads in the upper seven stories. The four tests investigated the following parameters: i) shear demand, accomplished by varying the simulated load distribution of the wall, ii) reinforcement layout, with longitudinal reinforcement concentrated in boundary elements or distributed evenly along the length of the wall, and iii) the use of lap splices in the expected plastic hinge region of the wall. Experiment 2 is considered the reference specimen. Each of the other specimens is altered from Experiment 2 for one of the parameters listed.

Experiment 2 is described by the following:
* Boundary element longitudinal reinforcement distribution.
* Uniform lateral load distribution (effective height = 0.50H)
* Spliced longitudinal reinforcement at base of wall.
DOI: 10.4225/08/520046c57a7ca
title: Parkes observations for project P262 semester 2004MAYT

description: Timing of young pulsars
DOI: 10.4231/d3hx15r0d
title: Lateral Testing of Bridge Abutment Backwall with 8' Sandy backfill Test 1

description: A reinforced concrete abutment backwall specimen with dimensions of 15 ft in width, 8.5 ft in height and 3ft in thickness was pushed under quasi static lateral loading into a 8.0 ft high, densely compacted SE 30 backfill material according to Caltrans bridge design specifications. Wingwalls were simulated using sheets of plywood material furnished with several layers of PVC foil to minimize  wall soil interface friction. A set of 6 actuators was installed between the backwall and a high capacity reaction block in horizontal and diagonal arrangements to displace the wall laterally and prevent any uplift movement. The test was controlled using the MTS Flextest GT software.  The backfill material was compacted with a vibratory roller to an average compaction of 96%. The backfill was also furnished with low strength gypsum columns to investigate the location of the soil failure surface.  The test was performed under displacement control with increasing displacement of up to 12.5 inches. Small loading-reloading cycles were applied at each displacement level, but not allowing soil gapping.
DOI: 10.4225/08/51fb2899b9c02
title: Parkes observations for project P439 semester 2003SEPT

description: Properties of neutron star kicks
DOI: 10.4225/08/51fb29511fa82
title: Parkes observations for project P439 semester 2004OCTS

description: Properties of neutron star kicks
DOI: 10.4225/08/51fb3659bf957
title: Parkes observations for project P439 semester 2005OCTS

description: Properties of neutron star kicks
DOI: 10.4225/08/51fb6784e1070
title: GFLOWS Lab Chemistry

description: Lab chemistry results of sampled bore locations in the Musgrave province, South Australia.
DOI: 10.4225/08/520b31d2c7031
title: Parkes observations for project P456 semester 2004OCTS

description: A millisecond pulsar timing array
DOI: 10.6073/pasta/93c45ac08504682c755fcaef5260c361
title: High-Resolution Orthorectified Imagery from 2008, Niwot Ridge LTER Project Area, Colorado
DOI: 10.6073/pasta/a0deef7b86d2b509d846793960b105a5
title: High-Resolution Orthorectified Imagery from 2008, Niwot Ridge LTER Project Area, Colorado
DOI: 10.4225/08/5200479487e4b
title: Parkes observations for project P262 semester 2005OCTS

description: Timing of young pulsars
DOI: 10.4231/d3th8bn1x
title: 2d Shake ST3 ( Test on Nevada Sand Saturated with viscous fluid) June 2013

description: soil cylindrical specimen is saturated with viscous fluid and subjected to 2d base shaking in order to identify the dynamic properties of the soil.
DOI: 10.4225/08/520048114d49e
title: Parkes observations for project P262 semester 2005APRS

description: Timing of young pulsars
DOI: 10.4231/d3pr7mt75
title: Phase 1: Headland H60 - water depth h=0.6 m: Measurements of radial wave propagation, wave runup, landslide kinematics and deposit

description: The landslide tsunami generator (LTG) was deployed in the curved headland scenario with a water depth of 0.6 m.  The curved headland configuration consists of the LTG mounted to a ramp with an opposing headland ramp 5.52 m from the toe of the landslide ramp.  The center of the opposing headland had a 90˚ bend.   Both the landslide ramp and the opposing headland ramp were built at a slope of 1:2 (vertical:horizontal) or α = 27.1˚.  Wave gauges were strategically placed in the basin along rays at various angles from the landslide source to describe the tsunami wave angular dependence.  A hybrid system of runup wave gauges and camera recordings focused on the runup slope measured the wave runup.  The deformable landside material consisted of naturally rounded river gravel.  The landslide surface kinematics were recorded with a planar particle image velocimetry (PIV) setup.  The landslide deposit was scanned with a multi-transducer acoustic (MTA) array.
DOI: 10.4225/08/51fc6531ab0cb
title: Parkes observations for project P050 semester 1991AUGT

description: 70cm pulsar survey and timing
DOI: 10.4225/08/51fc91c2619f8
title: Parkes observations for project P050 semester 1991DECT

description: 70cm Pulsar Survey and Timing
DOI: 10.4225/08/51fcc37e343b4
title: Parkes observations for project P050 semester 1991Q2

description: 75cm pulsar survey
DOI: 10.4225/08/51fcd3f988614
title: Parkes observations for project P050 semester 1992APRT

description: 70cm Pulsar Survey and Timing
DOI: 10.4225/08/51fd0676687c1
title: Parkes observations for project P050 semester 1992AUGT

description: 70cm Pulsar Survey and Timing
DOI: 10.4225/08/520048d7143bf
title: Parkes observations for project P262 semester 2006APRS

description: Young pulsars are of interest in several different ways: they are sometimes
associated with supernova remnants, they sometimes have high-energy
(optical, X-ray, gamma-ray) pulsed emission, and they usually have
significant period variations and often suffer glitches. We propose frequent
monitoring of the period of about 35 mostly young pulsars to provide
a database for high-energy, ATCA and LBA observations of pulsars and to
investigate variations in their period.
DOI: 10.4225/08/51fd2b3d97148
title: Parkes observations for project P050 semester 1992DECT

description: 70cm Pulsar Survey and Timing
DOI: 10.4225/08/51fd4f28ee33d
title: Parkes observations for project P050 semester 1993APRT

description: 70cm Pulsar Survey and Timing
DOI: 10.4225/08/51fdb3b37a372
title: Parkes observations for project P050 semester 1994AUGT

description: Parkes Southern Pulsar Survey
DOI: 10.4225/08/51fdc6f65d59c
title: Parkes observations for project P050 semester 1994DECT

description: Parkes Southern Pulsar Survey
DOI: 10.4225/08/51ff254a2498a
title: Parkes observations for project P427 semester 2007OCTS

description: Timing the dozen pulsars discovered in P303 is ensuring high quality results: (a) the peculiarities (in position or projected acceleration) of all the 5 millisecond pulsars in NGC6752 suggested the presence of non thermal dynamics in the core, perhaps due to black-holes of intermediate mass; (b) the eclipsing pulsar in NGC6397 appears the best laboratory for studying formation and evolution of exotic binaries. We propose to continue our timing project focusing mostly on NGC6752 at 20cm (in order to measure additional parameters useful to constrain the existence of a black-hole) and NGC6397 at 10cm (for studying the eclipse region and orbital secular evolution).  We also request observations in order to confirm candidates resulting from the ongoing reprocessing of the data with a code sensitive to pulsars in close binaries.
DOI: 10.6073/pasta/734611a8520b00b0e428dcdccc45d855
title: Gaviota Fire Perimeter (Santa Barbara County, CA), June 9, 2004 - From Geospatial Multi-Agency Coordination Group (GeoMAC)
DOI: 10.4225/08/51ff266eaaf24
title: Parkes observations for project P427 semester 2008OCTS

description: Timing the dozen pulsars discovered in P303 is ensuring high quality results: (a) the peculiarities (in position or projected acceleration) of all the 5 millisecond pulsars in NGC6752 suggested the presence of non thermal dynamics in the core, perhaps due to black-holes of intermediate mass; (b) the eclipsing pulsars in NGC6397 and NGC6266 appear promising laboratories for studying formation and evolution of exotic binaries. We propose to continue our timing project focusing mostly on NGC6752 at 20cm (in order to measure additional parameters useful to constrain the existence of a black-hole), NGC6397 at 10cm (for studying the eclipse region and orbital secular evolution) and NGC6266 at 20cm (for investigating the cluster's proper motion and dynamics and the eclipsing pulsar).  We also request time for performing some tests of timing observations of these sources with the new back-ends available at Parkes (APSR, DFB3, 13x1024 digital filterbank) and for performing pilot observations of a new deeper than ever search of NGC6752, NGC6397 and of few other suitable clusters.
DOI: 10.4225/08/51ff3112d2be9
title: Parkes observations for project P427 semester 2011APRS

description: Timing of the dozen pulsars discovered by us in P303 is ensuring high quality results: (a) the peculiarities (in position or projected acceleration) of all the 5 millisecond pulsars in NGC6752 suggested the presence of non thermal dynamics in the core, perhaps due to black-holes of intermediate mass; (b) the eclipsing pulsar in NGC6397 is a stereotype for studying the late evolution of exotic binaries. We propose to continue our timing project focusing mostly on NGC6752 at 20cm (in order to measure additional parameters useful to constrain the existence of a black-hole) and NGC6397 at 10cm (for studying the orbital secular evolution, the eclipse region, and the mechanisms leading to the ejection of matter from the binary system).
DOI: 10.4225/08/51ff34a4b22de
title: Parkes observations for project P427 semester 2007APRS

description: Timing the dozen pulsars discovered in P303 is ensuring high quality results: (a) the peculiarities (in position or projected acceleration) of all the 5 millisecond pulsars in NGC6752 suggested the presence of non thermal dynamics in the core, perhaps due to black-holes of intermediate mass; (b) the eclipsing pulsar in NGC6397 appears the best laboratory for studying formation and evolution of exotic binaries. We propose to continue our timing project focusing mostly on NGC6752 at 20cm (in order to measure additional parameters useful to constrain the existence of a black-hole) and NGC6397 at 10cm (for studying the eclipse region and orbital secular evolution).  We also request observations in order to confirm candidates resulting from reprocessing of the data with a code sensitive to pulsars in close binaries.
DOI: 10.4225/08/51ff3509e93bd
title: Parkes observations for project P427 semester 2009OCTS

description: Timing the dozen pulsars discovered in P303 is ensuring high quality results: (a) the peculiarities (in position or projected acceleration) of all the 5 millisecond pulsars in NGC6752 suggested the presence of non thermal dynamics in the core, perhaps due to black-holes of intermediate mass; (b) the eclipsing pulsar in NGC6397 is a stereotype for studying the late evolution of exotic binaries. We propose to continue our timing project focusing mostly on NGC6752 at 20cm (in order to measure additional parameters useful to constrain the existence of a black-hole) and NGC6397 at 10cm (for studying the eclipse region and the orbital secular evolution). We also request time for performing pilot observations for a new deeper than ever search for millisecond pulsars in a subset of suitable clusters. This revamped search (as well as the requested timing observations) will exploit the new back-ends (APSR and DFB4) now available at Parkes.
DOI: 10.4225/08/51ff382042c9d
title: Parkes observations for project P427 semester 2010APRS

description: Timing the dozen pulsars discovered in P303 is ensuring high quality results: (a) the peculiarities (in position or projected acceleration) of all the 5 millisecond pulsars in NGC6752 suggested the presence of non thermal dynamics in the core, perhaps due to black-holes of intermediate mass; (b) the eclipsing pulsar in NGC6397 is a stereotype for studying the late evolution of exotic binaries. We propose to continue our timing project focusing mostly on NGC6752 at 20cm (in order to measure additional parameters useful to constrain the existence of a black-hole) and NGC6397 at 10cm (for studying the eclipse region and the orbital secular evolution). We also request time for performing observations for a new deeper than ever search for millisecond pulsars in a subset of suitable clusters. This revamped search (as well as the requested timing observations) will exploit the new back-ends (APSR and DFB4) now available at Parkes.
DOI: 10.4225/08/51ff399aa6b9e
title: Parkes observations for project P427 semester 2009APRS

description: Timing the dozen pulsars discovered in P303 is ensuring high quality results: (a) the peculiarities (in position or projected acceleration) of all the 5 millisecond pulsars in NGC6752 suggested the presence of non thermal dynamics in the core, perhaps due to black-holes of intermediate mass; (b) the eclipsing pulsars in NGC6397 and NGC6266 are primary targets for studying the late evolution of exotic binaries. We propose to continue our timing project focusing mostly on NGC6752 at 20cm (in order to measure additional parameters useful to constrain the existence of a black-hole), NGC6397 at 10cm (for studying the eclipse region and the orbital secular evolution) and NGC6266 at 20cm (for investigating the cluster's proper motion and dynamics and the eclipsing pulsar).  We also request time for performing pilot observations for a new deeper than ever search for millisecond pulsars in a subset of suitable clusters. This revamped search will exploit the new back-ends (APSR and DFB4) now available at Parkes.
DOI: 10.4225/08/51ff493514316
title: Parkes observations for project P427 semester 2010OCTS

description: Timing of the dozen pulsars discovered by us in P303 is ensuring high quality results: (a) the peculiarities (in position or projected acceleration) of all the 5 millisecond pulsars in NGC6752 suggested the presence of non thermal dynamics in the core, perhaps due to black-holes of intermediate mass; (b) the eclipsing pulsar in NGC6397 is a stereotype for studying the late evolution of exotic binaries. We propose to continue our timing project focusing mostly on NGC6752 at 20cm (in order to measure additional parameters useful to constrain the existence of a black-hole) and NGC6397 at 10cm (for studying the eclipse region and the orbital secular evolution).
DOI: 10.4225/08/51ff609630eb4
title: Parkes observations for project P455 semester 2004MAYT

description: Timing & geodetic precession in the double pulsar & the DNS PSR J1756-2251
DOI: 10.4225/08/51ff622fa9f85
title: Parkes observations for project P455 semester 2004OCTS

description: Timing & geodetic precession in the double pulsar & the DNS PSR J1756-2251
DOI: 10.4225/08/51ff639fec863
title: Parkes observations for project P455 semester 2005APRS

description: Timing & geodetic precession in the double pulsar and the DNS PSR J1756-2251
DOI: 10.4225/08/51ff67b33f74b
title: Parkes observations for project P455 semester 2005OCTS

description: Timing & geodetic precession in the double pulsar and two relativistic binaries
DOI: 10.4225/08/51ff6d270a807
title: Parkes observations for project P455 semester 2006APRS

description: This project is to continue timing and profile monitoring of the first 
double-pulsar system and two other relativistic binaries discovered in
our surveys. These systems provide unique laboratories for
gravitational physics. In order to exploit them, we had combined
the previous projects P455 & P400 into one request.  In addition to the
double pulsar we want to continue our studies of the double neutron
star PSR J1756-2251, and the relativistic binary J1141-6545. We
aim to provide the strongest tests to date for general relativity and
to measure for the first time the moment-of-inertia of a neutron star.
Additionally, we will determine the system geometries and map the
pulsar beams via geodetic precession.
DOI: 10.4225/08/51ff6f826d6d9
title: Parkes observations for project P455 semester 2006OCTS

description: This project is to continue timing and profile monitoring of the first 
double-pulsar system and two other relativistic binaries discovered in
our surveys. These systems provide unique laboratories for
gravitational physics. In addition to the
double pulsar we want to continue our studies of the double neutron
star PSR J1756-2251, and the relativistic binary J1141-6545. We
aim to provide the strongest tests to date for general relativity and
to measure for the first time the moment-of-inertia of a neutron star.
Additionally, we will determine the system geometries and map the
pulsar beams via geodetic precession.
DOI: 10.4225/08/51ff71969ad4b
title: Parkes observations for project P455 semester 2007APRS

description: This project is to continue timing and profile monitoring of the first 
double-pulsar system and two other relativistic binaries discovered in
our surveys. These systems provide unique laboratories for
gravitational physics. In addition to the
double pulsar we want to continue our studies of the double neutron
star PSR J1756-2251, and the relativistic binary J1141-6545. We
aim to provide the strongest tests to date for general relativity and
to measure for the first time the moment-of-inertia of a neutron star.
Additionally, we will determine the system geometries and map the
pulsar beams via geodetic precession.
DOI: 10.4225/08/51ff75e389e1a
title: Parkes observations for project P455 semester 2007OCTS

description: This project is to continue timing and profile monitoring of the first 
double-pulsar system and two other relativistic binaries discovered in
our surveys. These systems provide unique laboratories for
gravitational physics. In addition to the
double pulsar we want to continue our studies of the double neutron
star PSR J1756-2251, and the relativistic binary J1141-6545. We
aim to provide the strongest tests to date for general relativity and
to measure for the first time the moment-of-inertia of a neutron star.
Additionally, we will determine the system geometries and map the
pulsar beams via geodetic precession.
DOI: 10.4225/08/51ff7e76c18ff
title: Parkes observations for project P455 semester 2008APRS

description: This project is to continue timing and profile monitoring of the first 

double-pulsar system and two other relativistic binaries discovered in

our surveys. These systems provide unique laboratories for

gravitational physics. In addition to the
 double pulsar we want to continue our studies of the double neutron
 star PSR J1756-2251, and the relativistic binary J1141-6545. We
 aim to provide the strongest tests to date for general relativity and
 to measure for the first time the moment-of-inertia of a neutron star.

Additionally, we will determine the system geometries and map the

pulsar beams via geodetic precession.