cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25919/5bb0fbdae0ea2
title: Parkes observations for project P939 semester 2016OCTS

description: Since the work of Keith et al. (2013), we have known that the Parkes Pulsar Timing Array (PPTA) pulsar J1603-7202 showed a clear extreme scattering event (ESE), which lasted about 260 days. As the dynamic spectra for PPTA observations improved, Coles et al. (2015) found that this ESE showed a clear increase in turbulence and used that to show that it must be much more compact than the normal ionised interstellar medium (IISM). Now, with an extra year of data, we have fitted a scattering model to the entire data set. This model provides: the orbital inclination angle; the distance to the scattering region; and the velocity of the IISM. The low inclination angle suggests that the companion is a heavy white dwarf, or possibly a neutron star. However these measurements, and other properties of the ESE such as its velocity and structure, are poorly constrained because the scatter in our data is large. The scatter originates from changes in the IISM over timescales much smaller than our ~12 year observing span. To mitigate this scatter, it is necessary to thoroughly observe this pulsar over one orbital period (~6.3 days). This will allow us to confirm the mass of the companion, and to characterise the nature of the ESE that continues to dominate the scattering environment in the direction of this pulsar.
DOI: 10.25919/5bb0fc248df58
title: Parkes observations for project P892 semester 2016OCTS_BPSR_58

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: 10.25919/5bb0fc6f3ad98
title: Parkes observations for project P892 semester 2016OCTS_BPSR_59

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: 10.25919/5bb0fcbc1d49f
title: Parkes observations for project P892 semester 2016OCTS_BPSR_60

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: 10.25919/5bb0fd06ed2d9
title: Parkes observations for project P456 semester 2016OCTS

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: 10.25919/5bb0fd563c0d9
title: Parkes observations for project P892 semester 2016OCTS_BPSR_66

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: 10.25919/5bb0fda150618
title: Parkes observations for project P892 semester 2016OCTS_BPSR_67

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: 10.25491/0v9n-6582
title: GTEX-PLZ5-0926-SM-4RGM9

description: Sample ID: GTEX-PLZ5-0926-SM-4RGM9
DOI: 10.25491/0w6r-qf82
title: GTEX-ZUA1-1526-SM-59HLS

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DOI: 10.25491/1tfe-qe02
title: GTEX-YEC4-2526-SM-4W1Z2

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title: GTEX-RU72-1026-SM-46MUG

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title: GTEX-YEC4-1926-SM-5IFHJ

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title: GTEX-PLZ5-1526-SM-3P5ZX

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title: GTEX-X62O-2226-SM-46MW3

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DOI: 10.25491/8w61-a008
title: GTEX-X638-0226-SM-47JZ9

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title: GTEX-X638-0426-SM-47JY2

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title: GTEX-UPK5-0426-SM-3GAEK

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DOI: 10.25491/9q49-tm14
title: GTEX-RU72-0626-SM-46MUI

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title: GTEX-UPK5-1226-SM-4IHL8

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title: GTEX-UPK5-1626-SM-4JBHI

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DOI: 10.25491/dg9h-c736
title: GTEX-UPK5-1526-SM-4JBJA

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DOI: 10.25491/dn39-t371
title: GTEX-RU72-0926-SM-2TF6B

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DOI: 10.25491/dxv2-q423
title: GTEX-ZUA1-1026-SM-4YCEA

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DOI: 10.25491/ecsc-ay68
title: GTEX-UPK5-2026-SM-4JBIM

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DOI: 10.25491/ffme-0q19
title: GTEX-X638-0326-SM-47JY1

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DOI: 10.25491/fwww-tv97
title: GTEX-PLZ5-1126-SM-3P613

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DOI: 10.25491/gmhy-8847
title: GTEX-YEC4-2426-SM-57WFO

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DOI: 10.25491/h1xx-8w78
title: GTEX-PLZ5-0926-SM-3TW8L

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DOI: 10.25491/hpds-nz70
title: GTEX-YEC4-1326-SM-5IFHG

description: Sample ID: GTEX-YEC4-1326-SM-5IFHG
DOI: 10.25491/hvnd-2r30
title: GTEX-X638-0126-SM-47JZ8

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DOI: 10.25491/hxwt-6g40
title: GTEX-RU72-1326-SM-2TF6T

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DOI: 10.25491/j0ac-9r97
title: GTEX-RU72-1126-SM-2TF6H

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DOI: 10.25491/kj78-pm96
title: GTEX-ZUA1-0326-SM-5NQA3

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DOI: 10.25491/kwkh-9m63
title: GTEX-UPK5-1426-SM-4JBHH

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DOI: 10.25491/mwee-me23
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DOI: 10.25491/p11y-yr20
title: GTEX-RU72-1226-SM-2TF6N

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DOI: 10.25491/q3ss-3d65
title: GTEX-UPK5-0326-SM-5SI81

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DOI: 10.25491/qe57-ks34
title: GTEX-RU72-1426-SM-46MUF

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DOI: 10.25491/r5nx-ss30
title: GTEX-ZUA1-0626-SM-4YCCW

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DOI: 10.25491/r9q1-8877
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DOI: 10.25491/rz1w-1r78
title: GTEX-PLZ5-1626-SM-3NB21

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DOI: 10.25491/ss83-j732
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title: GTEX-YEC4-2126-SM-5IFJH

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title: GTEX-UPK5-1326-SM-4IHLE

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DOI: 10.25549/uschist-dt-m173628
title: Daily Trojan, Vol. 159, No. 34, October 09, 2006

description: Daily Trojan, Vol. 159, No. 34, October 09, 2006.
DOI: 10.25549/uschist-dt-m176743
title: The Daily Southern Californian, Vol. 9, No. 9, September 30, 1912

description: The Daily Southern Californian, Vol. 9, No. 9, September 30, 1912.
DOI: 10.25549/uschist-dt-m176889
title: The Daily Southern Californian, Vol. 10, No. 10, February 26, 1913

description: The Daily Southern Californian, Vol. 10, No. 10, February 26, 1913.
DOI: 10.25549/uschist-dt-m183650
title: The Daily Southern Californian, Vol. 5, No. 47, December 18, 1914

description: The Daily Southern Californian, Vol. 5, No. 47, December 18, 1914.
DOI: 10.25549/uschist-dt-m183883
title: The Daily Southern Californian, Vol. 6, No. 15, April 06, 1915

description: The Daily Southern Californian, Vol. 6, No. 15, April 06, 1915.
DOI: 10.25549/uschist-dt-m184954
title: Daily Trojan, Vol. 26, No. 59, January 07, 1935

description: Daily Trojan, Vol. 26, No. 59, January 07, 1935.
DOI: 10.25549/uschist-dt-m185192
title: The Daily Southern Californian, Vol. 3, No. 62, January 15, 1914

description: The Daily Southern Californian, Vol. 3, No. 62, January 15, 1914.
DOI: 10.25549/uschist-dt-m190082
title: Summer Trojan, Vol. 60, No. 4, June 27, 1969

description: Summer Trojan, Vol. 60, No. 4, June 27, 1969.
DOI: 10.25919/5bb0fdeec1ac4
title: Parkes observations for project P892 semester 2016OCTS_BPSR_68

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: 10.25919/5bb0fe3a89cfc
title: Parkes observations for project P892 semester 2016OCTS_BPSR_53

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: 10.25919/5bb0fe85dce69
title: Parkes observations for project P892 semester 2016OCTS_BPSR_54

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: 10.25919/5bb0fed0d8340
title: Parkes observations for project P892 semester 2016OCTS_BPSR_55

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.