cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25919/5bb0f42810f67
title: Parkes observations for project P892 semester 2016OCTS_BPSR_44

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: 10.25919/5bb0f472be87a
title: Parkes observations for project P892 semester 2016OCTS_BPSR_45

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: 10.25919/5bb0f4be7b521
title: Parkes observations for project P938 semester 2016OCTS

description: We propose a targeted, 357-hr search of two nearby galaxies with high star-formation rates (SFRs) for fast radio bursts (FRBs). The primary aim of this carefully designed experiment is to test the hypothesis that FRBs are correlated with SFR, and originate in the nearby Universe at typical distances of ~100 Mpc. This hypothesis is supported by leading models for FRBs that invoke extreme forms of young neutron-star emission, and by arguments based on signatures of FRB propagation. If the hypothesis is true, we expect ~20 FRB detections in our observations. In the case of a null result, we will show that FRBs are highly likely to originate at distances beyond ~175 Mpc. Our observations will also allow for the most sensitive search to date (by a factor of 30) for supergiant pulses from extragalactic analogues of the Crab pulsar. By using the 20cm Multibeam receiver, with the central beam pointed at the galaxies of interest, we will additionally perform a standard FRB search in all beams with an expected yield of one serendipitous event. Although we have no guarantee of a higher FRB detection rate than a truly blind survey, our experimental design ensures that we will finish with substantially greater insight into the FRB population.
DOI: 10.25919/5bb0f50ad0a00
title: Parkes observations for project P938 semester 2016OCTS_BPSR_01

description: We propose a targeted, 357-hr search of two nearby galaxies with high star-formation rates (SFRs) for fast radio bursts (FRBs). The primary aim of this carefully designed experiment is to test the hypothesis that FRBs are correlated with SFR, and originate in the nearby Universe at typical distances of ~100 Mpc. This hypothesis is supported by leading models for FRBs that invoke extreme forms of young neutron-star emission, and by arguments based on signatures of FRB propagation. If the hypothesis is true, we expect ~20 FRB detections in our observations. In the case of a null result, we will show that FRBs are highly likely to originate at distances beyond ~175 Mpc. Our observations will also allow for the most sensitive search to date (by a factor of 30) for supergiant pulses from extragalactic analogues of the Crab pulsar. By using the 20cm Multibeam receiver, with the central beam pointed at the galaxies of interest, we will additionally perform a standard FRB search in all beams with an expected yield of one serendipitous event. Although we have no guarantee of a higher FRB detection rate than a truly blind survey, our experimental design ensures that we will finish with substantially greater insight into the FRB population.
DOI: 10.25919/5bb0f5558fba9
title: Parkes observations for project P938 semester 2016OCTS_BPSR_02

description: We propose a targeted, 357-hr search of two nearby galaxies with high star-formation rates (SFRs) for fast radio bursts (FRBs). The primary aim of this carefully designed experiment is to test the hypothesis that FRBs are correlated with SFR, and originate in the nearby Universe at typical distances of ~100 Mpc. This hypothesis is supported by leading models for FRBs that invoke extreme forms of young neutron-star emission, and by arguments based on signatures of FRB propagation. If the hypothesis is true, we expect ~20 FRB detections in our observations. In the case of a null result, we will show that FRBs are highly likely to originate at distances beyond ~175 Mpc. Our observations will also allow for the most sensitive search to date (by a factor of 30) for supergiant pulses from extragalactic analogues of the Crab pulsar. By using the 20cm Multibeam receiver, with the central beam pointed at the galaxies of interest, we will additionally perform a standard FRB search in all beams with an expected yield of one serendipitous event. Although we have no guarantee of a higher FRB detection rate than a truly blind survey, our experimental design ensures that we will finish with substantially greater insight into the FRB population.
DOI: 10.25919/5bb0f59fa71f6
title: Parkes observations for project P938 semester 2016OCTS_BPSR_03

description: We propose a targeted, 357-hr search of two nearby galaxies with high star-formation rates (SFRs) for fast radio bursts (FRBs). The primary aim of this carefully designed experiment is to test the hypothesis that FRBs are correlated with SFR, and originate in the nearby Universe at typical distances of ~100 Mpc. This hypothesis is supported by leading models for FRBs that invoke extreme forms of young neutron-star emission, and by arguments based on signatures of FRB propagation. If the hypothesis is true, we expect ~20 FRB detections in our observations. In the case of a null result, we will show that FRBs are highly likely to originate at distances beyond ~175 Mpc. Our observations will also allow for the most sensitive search to date (by a factor of 30) for supergiant pulses from extragalactic analogues of the Crab pulsar. By using the 20cm Multibeam receiver, with the central beam pointed at the galaxies of interest, we will additionally perform a standard FRB search in all beams with an expected yield of one serendipitous event. Although we have no guarantee of a higher FRB detection rate than a truly blind survey, our experimental design ensures that we will finish with substantially greater insight into the FRB population.
DOI: 10.25919/5bb0f5eb718d5
title: Parkes observations for project P892 semester 2016OCTS_BPSR_69

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: 10.25491/02t4-bt72
title: GTEX-ZTX8-1026-SM-5EGHD

description: Sample ID: GTEX-ZTX8-1026-SM-5EGHD
DOI: 10.25491/1qfc-5z20
title: GTEX-RU1J-0426-SM-46MUK

description: Sample ID: GTEX-RU1J-0426-SM-46MUK
DOI: 10.25491/212r-tw37
title: GTEX-X5EB-0626-SM-46MVQ

description: Sample ID: GTEX-X5EB-0626-SM-46MVQ
DOI: 10.25491/29k7-5j82
title: GTEX-ZTX8-1126-SM-51MRM

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title: GTEX-RU1J-0626-SM-4WAWY

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DOI: 10.25491/2zy4-v163
title: GTEX-YEC3-2426-SM-5IFJR

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DOI: 10.25491/3a81-yk82
title: GTEX-UPJH-0001-SM-3NMDE

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title: GTEX-YEC3-2326-SM-5IFJF

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DOI: 10.25491/7p8n-7n16
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title: GTEX-X5EB-1026-SM-46MVU

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DOI: 10.25491/8a1z-mh11
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title: GTEX-RU1J-0826-SM-46MUU

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DOI: 10.25491/8tbn-8f34
title: GTEX-UPIC-1526-SM-4IHLU

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DOI: 10.25491/98x6-sq73
title: GTEX-P78B-1726-SM-3P5ZV

description: Sample ID: GTEX-P78B-1726-SM-3P5ZV
DOI: 10.25491/9pjm-3z17
title: GTEX-RU1J-0326-SM-46MUM

description: Sample ID: GTEX-RU1J-0326-SM-46MUM
DOI: 10.25491/a80z-rx70
title: GTEX-RU1J-1426-SM-46MUV

description: Sample ID: GTEX-RU1J-1426-SM-46MUV
DOI: 10.25491/aehb-rw49
title: GTEX-P78B-2526-SM-3P5ZY

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DOI: 10.25491/b4d5-cz97
title: GTEX-RU1J-1026-SM-46MUR

description: Sample ID: GTEX-RU1J-1026-SM-46MUR
DOI: 10.25491/b6x5-nv73
title: GTEX-UPIC-1126-SM-4IHLO

description: Sample ID: GTEX-UPIC-1126-SM-4IHLO
DOI: 10.25491/bjc7-7622
title: GTEX-RU1J-1326-SM-46MUL

description: Sample ID: GTEX-RU1J-1326-SM-46MUL
DOI: 10.25491/bvbe-hq86
title: GTEX-P78B-1026-SM-3NMC4

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DOI: 10.25491/bxz6-2152
title: GTEX-PLZ4-0006-SM-2S1NY

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DOI: 10.25491/c3ex-ms96
title: GTEX-ZTX8-1426-SM-5DUVO

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DOI: 10.25491/ck2j-j918
title: GTEX-YEC4-0001-SM-4W1Y6

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DOI: 10.25491/d3qp-zz66
title: GTEX-UPIC-0826-SM-3GADQ

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DOI: 10.25491/ehgq-j912
title: GTEX-P78B-2226-SM-3P5ZZ

description: Sample ID: GTEX-P78B-2226-SM-3P5ZZ
DOI: 10.25491/empw-4s89
title: GTEX-X5EB-0826-SM-46MVS

description: Sample ID: GTEX-X5EB-0826-SM-46MVS
DOI: 10.25491/et9g-7719
title: GTEX-ZTX8-1626-SM-51MRY

description: Sample ID: GTEX-ZTX8-1626-SM-51MRY
DOI: 10.25491/f1k8-3r25
title: GTEX-YEC4-0008-SM-4W1YR

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DOI: 10.25491/f4zv-0d93
title: GTEX-P78B-1826-SM-3P5YX

description: Sample ID: GTEX-P78B-1826-SM-3P5YX
DOI: 10.25491/hzep-2p68
title: GTEX-ZTX8-1326-SM-4YCEL

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DOI: 10.25491/j1tf-ck87
title: GTEX-PLZ4-0008-SM-48TE6

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DOI: 10.25491/jg0z-7q72
title: GTEX-X5EB-0326-SM-4QASF

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DOI: 10.25491/k560-8260
title: GTEX-ZTX8-1226-SM-4YCE9

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DOI: 10.25491/kxdj-8782
title: GTEX-X5EB-0926-SM-46MVT

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DOI: 10.25491/m230-x567
title: GTEX-YEC3-2526-101809-SM-5CVLT

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DOI: 10.25491/m3zt-2441
title: GTEX-UPIC-1426-SM-4IHLQ

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DOI: 10.25491/n2fr-vt66
title: GTEX-ZTX8-1726-SM-51MSB

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DOI: 10.25491/p01n-aw09
title: GTEX-YEC3-2126-SM-5CVLR

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DOI: 10.25491/qdsx-vg28
title: GTEX-X5EB-0726-SM-46MVR

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DOI: 10.25491/rv2b-e424
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DOI: 10.25491/s314-ae53
title: GTEX-X5EB-0526-SM-46MVP

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DOI: 10.25491/sf5v-kr89
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DOI: 10.25491/vk1b-gv65
title: GTEX-UPIC-0926-SM-4IHLV

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DOI: 10.25491/vp2b-pk95
title: GTEX-YEC3-2526-SM-5CVLS

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title: GTEX-RTLS-2626-SM-46MUJ

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DOI: 10.25491/z4jz-3627
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DOI: 10.25491/z745-0n83
title: GTEX-ZTX8-0726-SM-59HL9

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DOI: 10.25491/zv3g-2k29
title: GTEX-RU1J-0226-SM-2TF5Y

description: Sample ID: GTEX-RU1J-0226-SM-2TF5Y
DOI: 10.25919/5bb0f63787c13
title: Parkes observations for project P938 semester 2016OCTS_BPSR_10

description: We propose a targeted, 357-hr search of two nearby galaxies with high star-formation rates (SFRs) for fast radio bursts (FRBs). The primary aim of this carefully designed experiment is to test the hypothesis that FRBs are correlated with SFR, and originate in the nearby Universe at typical distances of ~100 Mpc. This hypothesis is supported by leading models for FRBs that invoke extreme forms of young neutron-star emission, and by arguments based on signatures of FRB propagation. If the hypothesis is true, we expect ~20 FRB detections in our observations. In the case of a null result, we will show that FRBs are highly likely to originate at distances beyond ~175 Mpc. Our observations will also allow for the most sensitive search to date (by a factor of 30) for supergiant pulses from extragalactic analogues of the Crab pulsar. By using the 20cm Multibeam receiver, with the central beam pointed at the galaxies of interest, we will additionally perform a standard FRB search in all beams with an expected yield of one serendipitous event. Although we have no guarantee of a higher FRB detection rate than a truly blind survey, our experimental design ensures that we will finish with substantially greater insight into the FRB population.
DOI: 10.25919/5bb0f681e93a5
title: Parkes observations for project P938 semester 2016OCTS_BPSR_11

description: We propose a targeted, 357-hr search of two nearby galaxies with high star-formation rates (SFRs) for fast radio bursts (FRBs). The primary aim of this carefully designed experiment is to test the hypothesis that FRBs are correlated with SFR, and originate in the nearby Universe at typical distances of ~100 Mpc. This hypothesis is supported by leading models for FRBs that invoke extreme forms of young neutron-star emission, and by arguments based on signatures of FRB propagation. If the hypothesis is true, we expect ~20 FRB detections in our observations. In the case of a null result, we will show that FRBs are highly likely to originate at distances beyond ~175 Mpc. Our observations will also allow for the most sensitive search to date (by a factor of 30) for supergiant pulses from extragalactic analogues of the Crab pulsar. By using the 20cm Multibeam receiver, with the central beam pointed at the galaxies of interest, we will additionally perform a standard FRB search in all beams with an expected yield of one serendipitous event. Although we have no guarantee of a higher FRB detection rate than a truly blind survey, our experimental design ensures that we will finish with substantially greater insight into the FRB population.
DOI: 10.25919/5bb0f6ccd1bec
title: Parkes observations for project P938 semester 2016OCTS_BPSR_12

description: We propose a targeted, 357-hr search of two nearby galaxies with high star-formation rates (SFRs) for fast radio bursts (FRBs). The primary aim of this carefully designed experiment is to test the hypothesis that FRBs are correlated with SFR, and originate in the nearby Universe at typical distances of ~100 Mpc. This hypothesis is supported by leading models for FRBs that invoke extreme forms of young neutron-star emission, and by arguments based on signatures of FRB propagation. If the hypothesis is true, we expect ~20 FRB detections in our observations. In the case of a null result, we will show that FRBs are highly likely to originate at distances beyond ~175 Mpc. Our observations will also allow for the most sensitive search to date (by a factor of 30) for supergiant pulses from extragalactic analogues of the Crab pulsar. By using the 20cm Multibeam receiver, with the central beam pointed at the galaxies of interest, we will additionally perform a standard FRB search in all beams with an expected yield of one serendipitous event. Although we have no guarantee of a higher FRB detection rate than a truly blind survey, our experimental design ensures that we will finish with substantially greater insight into the FRB population.
DOI: 10.25919/5bb0f718739c5
title: Parkes observations for project P938 semester 2016OCTS_BPSR_13

description: We propose a targeted, 357-hr search of two nearby galaxies with high star-formation rates (SFRs) for fast radio bursts (FRBs). The primary aim of this carefully designed experiment is to test the hypothesis that FRBs are correlated with SFR, and originate in the nearby Universe at typical distances of ~100 Mpc. This hypothesis is supported by leading models for FRBs that invoke extreme forms of young neutron-star emission, and by arguments based on signatures of FRB propagation. If the hypothesis is true, we expect ~20 FRB detections in our observations. In the case of a null result, we will show that FRBs are highly likely to originate at distances beyond ~175 Mpc. Our observations will also allow for the most sensitive search to date (by a factor of 30) for supergiant pulses from extragalactic analogues of the Crab pulsar. By using the 20cm Multibeam receiver, with the central beam pointed at the galaxies of interest, we will additionally perform a standard FRB search in all beams with an expected yield of one serendipitous event. Although we have no guarantee of a higher FRB detection rate than a truly blind survey, our experimental design ensures that we will finish with substantially greater insight into the FRB population.
DOI: 10.25919/5bb0f76343eb9
title: Parkes observations for project P938 semester 2016OCTS_BPSR_04

description: We propose a targeted, 357-hr search of two nearby galaxies with high star-formation rates (SFRs) for fast radio bursts (FRBs). The primary aim of this carefully designed experiment is to test the hypothesis that FRBs are correlated with SFR, and originate in the nearby Universe at typical distances of ~100 Mpc. This hypothesis is supported by leading models for FRBs that invoke extreme forms of young neutron-star emission, and by arguments based on signatures of FRB propagation. If the hypothesis is true, we expect ~20 FRB detections in our observations. In the case of a null result, we will show that FRBs are highly likely to originate at distances beyond ~175 Mpc. Our observations will also allow for the most sensitive search to date (by a factor of 30) for supergiant pulses from extragalactic analogues of the Crab pulsar. By using the 20cm Multibeam receiver, with the central beam pointed at the galaxies of interest, we will additionally perform a standard FRB search in all beams with an expected yield of one serendipitous event. Although we have no guarantee of a higher FRB detection rate than a truly blind survey, our experimental design ensures that we will finish with substantially greater insight into the FRB population.
DOI: 10.25919/5bb0f7ae37903
title: Parkes observations for project P892 semester 2016OCTS_BPSR_62

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.