cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25919/5bb0ff1de8b99
title: Parkes observations for project P892 semester 2016OCTS_BPSR_56

description: SUPERBx is an extension to the SUPERB survey which looks at the highest Galactic latitudes in a search for fast radio bursts (FRBs). Our most recent results show that there is a strong Galactic latitude dependence to FRB detectability with the detection rate being 4 times higher ~45 degrees and higher above the plane; this is where SUPERBx will focus its efforts from now on. SUPERBx uses optimised GPU codes to search for pulsars and fast radio bursts (FRBs), making discoveries in real time. Handling our data as it comes in is essential for the SKA Phase I era so this work applies directly to the high-data rates of next generation telescopes. The FRBs discovered (we have already discovered four FRBs in this project) will have much more associated information than all previous detections. Firstly our discovery lag is ~1 second, rather than months/years. The Parkes observations will be shadowed by other radio telescopes (in particular the refurbished Molonglo which has now reached a level of performance where it has independently discovered 3 FRBs in 2016) to allow localisation of the discovered FRBs, and a host of optical and high-energy telescopes will then be triggered as appropriate. This is key for identifying FRB host galaxies, so as to solve the mystery of their progenitors and to exploit their many uses as tools for precision cosmology measurements.
DOI: 10.25919/5bb0ff698ee3a
title: Parkes observations for project P892 semester 2016OCTS_BPSR_57

description: SUPERBx is an extension to the SUPERB survey which looks at the highest Galactic latitudes in a search for fast radio bursts (FRBs). Our most recent results show that there is a strong Galactic latitude dependence to FRB detectability with the detection rate being 4 times higher ~45 degrees and higher above the plane; this is where SUPERBx will focus its efforts from now on. SUPERBx uses optimised GPU codes to search for pulsars and fast radio bursts (FRBs), making discoveries in real time. Handling our data as it comes in is essential for the SKA Phase I era so this work applies directly to the high-data rates of next generation telescopes. The FRBs discovered (we have already discovered four FRBs in this project) will have much more associated information than all previous detections. Firstly our discovery lag is ~1 second, rather than months/years. The Parkes observations will be shadowed by other radio telescopes (in particular the refurbished Molonglo which has now reached a level of performance where it has independently discovered 3 FRBs in 2016) to allow localisation of the discovered FRBs, and a host of optical and high-energy telescopes will then be triggered as appropriate. This is key for identifying FRB host galaxies, so as to solve the mystery of their progenitors and to exploit their many uses as tools for precision cosmology measurements.
DOI: 10.25919/5bb0ffb630298
title: Parkes observations for project P574 semester 2016OCTS

description: We request time to observe 260 pulsars on a regular basis in order to provide the accurate ephemerides necessary for the detection and characterisation of gamma-ray pulsars with the Fermi satellite. The main science goals are to increase the number of known gamma-ray pulsars (both radio loud and radio quiet), to determine accurate pulse profiles, and to characterise their high energy (phase-resolved) spectra. In the radio, the observations will also allow us to find glitches, characterise timing noise, investigate dispersion and rotation measure variability, and enhance our knowledge of single pulse phenomenology. To date, we
are (co-)authors on 50 papers arising from the collaboration and P574 data. The data have contributed to the PhD theses of students from the Bordeaux group and Stanford and are remain in active use (detailed within).
DOI: 10.25919/5bb10004f3705
title: Parkes observations for project P789 semester 2016OCTS

description: Recently there has been great success at Parkes discovering millisecond pulsars (MSPs), a class that includes some of the most interesting and scientifically valuable pulsars known. In the last few years we have discovered more than 40 MSPs though the High Time Resolution Universe Survey (P630) and Fermi searches (P675/P814). Here we propose to carry out precision timing of these sources to fully exploit these discoveries. Additionally, continue to study the most significant of the discoveries from the Parkes Multibeam Pulsar Survey (P268). 
To maximise scientific impact we have combined the most important sources from various previous proposals into this project, reducing total observation time required and easing the burden on the scheduler.
DOI: 10.25491/01zv-w318
title: GTEX-ZUA1-1926-SM-5E45E

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DOI: 10.25491/0rct-bg42
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DOI: 10.25491/0wtc-qp78
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DOI: 10.25491/10wp-1k33
title: GTEX-RU72-3026-SM-5SI7Y

description: Sample ID: GTEX-RU72-3026-SM-5SI7Y
DOI: 10.25491/1c8s-9f17
title: GTEX-UPK5-2326-SM-3P5Z8

description: Sample ID: GTEX-UPK5-2326-SM-3P5Z8
DOI: 10.25491/2wxk-js74
title: GTEX-PLZ6-0008-SM-48TD5

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title: GTEX-UTHO-0011-R11A-SM-3GIJE

description: Sample ID: GTEX-UTHO-0011-R11A-SM-3GIJE
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title: GTEX-PLZ6-0226-SM-3P61I

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DOI: 10.25491/6kvp-b219
title: GTEX-RU72-3126-SM-46MUB

description: Sample ID: GTEX-RU72-3126-SM-46MUB
DOI: 10.25491/7j2f-3116
title: GTEX-X8HC-0126-SM-4E3JW

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title: GTEX-PLZ6-0006-SM-2I5FQ

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DOI: 10.25491/k69s-dr70
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DOI: 10.25491/pm7z-5b48
title: GTEX-RU72-2626-SM-4GIE1

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title: GTEX-X88G-0006-SM-47JX5

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DOI: 10.25491/r11p-hd87
title: GTEX-YECK-0226-SM-4W215

description: Sample ID: GTEX-YECK-0226-SM-4W215
DOI: 10.25491/rt74-sw27
title: GTEX-X88G-0008-SM-47JWN

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title: GTEX-PLZ6-0006-SM-33HBZ

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title: GTEX-PLZ6-0126-SM-48TC6

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title: GTEX-X88G-0426-SM-47JZ5

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DOI: 10.25491/stf2-ae40
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DOI: 10.25491/vfan-qj07
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description: Sample ID: GTEX-RUSQ-0006-SM-2TF6P
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DOI: 10.25491/zd82-se44
title: GTEX-X88G-0126-SM-47JZ3

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DOI: 10.25549/uschist-dt-m173906
title: Daily Trojan, Vol. 103, No. 14, January 30, 1987

description: Daily Trojan, Vol. 103, No. 14, January 30, 1987.
DOI: 10.25549/uschist-dt-m183505
title: The Daily Southern Californian, Vol. 5, No. 29, November 05, 1914

description: The Daily Southern Californian, Vol. 5, No. 29, November 05, 1914.
DOI: 10.25549/uschist-dt-m183973
title: The Daily Southern Californian, Vol. 5, No. 21, October 21, 1914

description: The Daily Southern Californian, Vol. 5, No. 21, October 21, 1914.
DOI: 10.25549/uschist-dt-m184806
title: Daily Trojan, Vol. 25, No. 89, March 05, 1934

description: Daily Trojan, Vol. 25, No. 89, March 05, 1934.
DOI: 10.25549/uschist-dt-m186627
title: Daily Trojan, Vol. 26, No. 1, September 19, 1934

description: Daily Trojan, Vol. 26, No. 1, September 19, 1934.
DOI: 10.25549/uschist-dt-m189591
title: Daily Trojan, Vol. 90, No. 20, March 04, 1981

description: Daily Trojan, Vol. 90, No. 20, March 04, 1981.
DOI: 10.25919/5bb100524912d
title: Parkes observations for project P456 semester 2016OCTS_BPSR_01

description: The Parkes Pulsar Timing Array (PPTA) project has three primary goals: (a) detection of gravitational waves from astronomical sources, (b) establishment of a pulsar timescale, and (c) improvement of our understanding of Solar-system dynamics. The PPTA is the oldest of three international pulsar timing groups. We have the smallest telescope and the smallest group, but the best measurements and the best results. Our bound on the strength of the incoherent gravitational wave background is the only bound which significantly constrains theoretical models. We have maintained our leading position because: we have the southern sky; we have a small but well-focussed group; we have the best-calibrated receivers; and we have been able to observe with an almost regular cadence of 15 to 20 days at three different wavelengths. With this proposal we aim to maintain our pre-eminent position in the field.

Unlike most observing proposals, this is a continuing proposal for which the observations will continue to improve bounds on gravitational waves until they are finally detected. Continued Parkes observations will remain valuable until the first stage of the SKA is able to offer the same sensitivity as Parkes and the same observing time. Even after the gravitational wave background is detected we will want to continue observations in support of the nascent field of gravitational wave astronomy!
DOI: 10.25919/5bb100a130cc5
title: Parkes observations for project P934 semester 2016OCTS_BPSR_07

description: On the smallest scales, the warm interstellar medium contains surprisingly complex structure, including extremely overdense filaments and blobs of plasma that remain intact for months, despite physical processes that should cause them to disperse on short (week) time scales.   It is possible that magnetization plays a role in confining this plasma.     On these AU length scales the plasma is best probed by observing the scintillations of compact background radio sources such as pulsars and quasars.   Recent observations show that overdensities are confined to narrow regions along lines of sight.  Over the last decade, improvements in the analysis of scintillation have enabled better characterization of these structures.     These studies however have focused on the ISM in the solar-system neighbourhood and the Galactic plane.    Here we propose to observe pulsars at high galactic latitudes to extend the sample lines of sight.  We will determine if the scattering regions are confined to the Galactic plane or persist into the halo of the galaxy.   We will also search for (or place limits on) magnetic field variations within these scattering regions and discrete structures.  Our observations will also provide important constraints on the scintillation of fast radio bursts, extragalactic sources which may be magnified by the similar structures to those studied here.
DOI: 10.25919/5bb100ec67c0c
title: Parkes observations for project P892 semester 2016OCTS_BPSR_51

description: SUPERBx is an extension to the SUPERB survey which looks at the highest Galactic latitudes in a search for fast radio bursts (FRBs). Our most recent results show that there is a strong Galactic latitude dependence to FRB detectability with the detection rate being 4 times higher ~45 degrees and higher above the plane; this is where SUPERBx will focus its efforts from now on. SUPERBx uses optimised GPU codes to search for pulsars and fast radio bursts (FRBs), making discoveries in real time. Handling our data as it comes in is essential for the SKA Phase I era so this work applies directly to the high-data rates of next generation telescopes. The FRBs discovered (we have already discovered four FRBs in this project) will have much more associated information than all previous detections. Firstly our discovery lag is ~1 second, rather than months/years. The Parkes observations will be shadowed by other radio telescopes (in particular the refurbished Molonglo which has now reached a level of performance where it has independently discovered 3 FRBs in 2016) to allow localisation of the discovered FRBs, and a host of optical and high-energy telescopes will then be triggered as appropriate. This is key for identifying FRB host galaxies, so as to solve the mystery of their progenitors and to exploit their many uses as tools for precision cosmology measurements.
DOI: 10.25919/5bb1013709936
title: Parkes observations for project P892 semester 2016OCTS_BPSR_52

description: SUPERBx is an extension to the SUPERB survey which looks at the highest Galactic latitudes in a search for fast radio bursts (FRBs). Our most recent results show that there is a strong Galactic latitude dependence to FRB detectability with the detection rate being 4 times higher ~45 degrees and higher above the plane; this is where SUPERBx will focus its efforts from now on. SUPERBx uses optimised GPU codes to search for pulsars and fast radio bursts (FRBs), making discoveries in real time. Handling our data as it comes in is essential for the SKA Phase I era so this work applies directly to the high-data rates of next generation telescopes. The FRBs discovered (we have already discovered four FRBs in this project) will have much more associated information than all previous detections. Firstly our discovery lag is ~1 second, rather than months/years. The Parkes observations will be shadowed by other radio telescopes (in particular the refurbished Molonglo which has now reached a level of performance where it has independently discovered 3 FRBs in 2016) to allow localisation of the discovered FRBs, and a host of optical and high-energy telescopes will then be triggered as appropriate. This is key for identifying FRB host galaxies, so as to solve the mystery of their progenitors and to exploit their many uses as tools for precision cosmology measurements.
DOI: 10.25919/5bb101825ca39
title: Parkes observations for project P455 semester 2016OCTS

description: This project is to continue timing and profile studies of the first double-pulsar system, a unique laboratory for gravitational physics. Recent results, including the first measurements of higher-order light-propagation effects and of the relativistic deformation of the orbit, highlight the importance of a long term observational campaign for this remarkable system. The main aims of this proposal are 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 geometry and map the pulsar beams via geodetic precession.
DOI: 10.25491/0ceh-mw51
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DOI: 10.25491/0jxb-a150
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DOI: 10.25491/1gxb-4v08
title: GTEX-UTHO-0011-R6A-SM-3GIJW

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title: GTEX-UTHO-0426-SM-3GAED

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title: GTEX-PLZ6-1326-SM-3NB24

description: Sample ID: GTEX-PLZ6-1326-SM-3NB24
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title: GTEX-ZV68-0011-R7a-SM-51MT4

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title: GTEX-YECK-1626-SM-5IFHQ

description: Sample ID: GTEX-YECK-1626-SM-5IFHQ
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title: GTEX-UTHO-0011-R5A-SM-3GIJD

description: Sample ID: GTEX-UTHO-0011-R5A-SM-3GIJD
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title: GTEX-YECK-1426-SM-5IFHE

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title: GTEX-X8HC-0626-SM-4E3HQ

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description: Sample ID: GTEX-ZV68-0011-R2a-SM-4YCDK
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title: GTEX-X8HC-1026-SM-46MWH

description: Sample ID: GTEX-X8HC-1026-SM-46MWH
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description: Sample ID: GTEX-X8HC-1426-SM-46MWC
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title: GTEX-UTHO-1226-SM-3GAEE

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DOI: 10.25491/crv4-fe36
title: GTEX-PLZ6-0526-SM-3P61C

description: Sample ID: GTEX-PLZ6-0526-SM-3P61C
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title: GTEX-RUSQ-0226-SM-47JWT

description: Sample ID: GTEX-RUSQ-0226-SM-47JWT
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title: GTEX-ZV68-0126-SM-59HKS

description: Sample ID: GTEX-ZV68-0126-SM-59HKS
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title: GTEX-YECK-1326-SM-4W1ZF

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title: GTEX-RUSQ-0126-SM-47JWV

description: Sample ID: GTEX-RUSQ-0126-SM-47JWV
DOI: 10.25491/jxnf-w453
title: GTEX-X8HC-0726-SM-46MWG

description: Sample ID: GTEX-X8HC-0726-SM-46MWG
DOI: 10.25491/k4yr-8693
title: GTEX-ZV68-0006-SM-4YCEJ

description: Sample ID: GTEX-ZV68-0006-SM-4YCEJ
DOI: 10.25491/kz65-6b14
title: GTEX-X8HC-0008-SM-46MU6

description: Sample ID: GTEX-X8HC-0008-SM-46MU6
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title: GTEX-ZV68-0011-R6a-SM-51MSR

description: Sample ID: GTEX-ZV68-0011-R6a-SM-51MSR
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title: GTEX-RUSQ-0526-SM-2TF72

description: Sample ID: GTEX-RUSQ-0526-SM-2TF72
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title: GTEX-PLZ6-0826-SM-3P61K

description: Sample ID: GTEX-PLZ6-0826-SM-3P61K
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title: GTEX-ZV68-0008-SM-4YCCV

description: Sample ID: GTEX-ZV68-0008-SM-4YCCV
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title: GTEX-UTHO-0726-SM-3GAEN

description: Sample ID: GTEX-UTHO-0726-SM-3GAEN
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title: GTEX-PLZ6-0926-SM-3P5ZQ

description: Sample ID: GTEX-PLZ6-0926-SM-3P5ZQ
DOI: 10.25491/rrsm-wr10
title: GTEX-UTHO-0011-R4A-SM-3GIJP

description: Sample ID: GTEX-UTHO-0011-R4A-SM-3GIJP
DOI: 10.25491/sfmm-c158
title: GTEX-ZV68-0226-SM-59HJF

description: Sample ID: GTEX-ZV68-0226-SM-59HJF
DOI: 10.25491/te0r-d104
title: GTEX-PLZ6-0626-SM-3P61B

description: Sample ID: GTEX-PLZ6-0626-SM-3P61B
DOI: 10.25491/tpss-qq22
title: GTEX-RUSQ-0926-SM-47JWU

description: Sample ID: GTEX-RUSQ-0926-SM-47JWU
DOI: 10.25491/vh45-br75
title: GTEX-PLZ6-0426-SM-5IJDW

description: Sample ID: GTEX-PLZ6-0426-SM-5IJDW
DOI: 10.25491/wcxz-6965
title: GTEX-RUSQ-1026-SM-2TF6V

description: Sample ID: GTEX-RUSQ-1026-SM-2TF6V
DOI: 10.25491/wjwg-z542
title: GTEX-X8HC-1526-SM-46MWD

description: Sample ID: GTEX-X8HC-1526-SM-46MWD
DOI: 10.25491/xv4k-bd97
title: GTEX-X88G-0226-SM-4GIE4

description: Sample ID: GTEX-X88G-0226-SM-4GIE4
DOI: 10.25491/ynd9-eg80
title: GTEX-X8HC-1326-SM-46MWB

description: Sample ID: GTEX-X8HC-1326-SM-46MWB
DOI: 10.25491/z3jq-sj66
title: GTEX-X8HC-0226-SM-4E3K1

description: Sample ID: GTEX-X8HC-0226-SM-4E3K1
DOI: 10.25491/z5bg-9k88
title: GTEX-YECK-2826-SM-5IFHF

description: Sample ID: GTEX-YECK-2826-SM-5IFHF
DOI: 10.25491/zme5-d077
title: GTEX-RUSQ-0826-SM-47JWW

description: Sample ID: GTEX-RUSQ-0826-SM-47JWW
DOI: 10.25491/ztqs-8n57
title: GTEX-PLZ6-0626-SM-5K7WJ

description: Sample ID: GTEX-PLZ6-0626-SM-5K7WJ
DOI: 10.25549/uschist-dt-m183806
title: The Southern California Trojan, Vol. 7, No. 42, December 01, 1915

description: The Southern California Trojan, Vol. 7, No. 42, December 01, 1915.
DOI: 10.25549/uschist-dt-m185115
title: The Daily Southern Californian, Vol. 4, No. 10, February 25, 1914

description: The Daily Southern Californian, Vol. 4, No. 10, February 25, 1914.
DOI: 10.25549/uschist-dt-m190482
title: Daily Trojan, Vol. 61, No. 10, September 26, 1969

description: Daily Trojan, Vol. 61, No. 10, September 26, 1969.