cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25491/x7q8-t797
title: GTEX-U8XE-1526-SM-4E3HT

description: Sample ID: GTEX-U8XE-1526-SM-4E3HT
DOI: 10.25491/xs29-q338
title: GTEX-X4XX-0126-SM-3NMC2

description: Sample ID: GTEX-X4XX-0126-SM-3NMC2
DOI: 10.25549/uschist-dt-m183722
title: The Daily Southern Californian, Vol. 6, No. 22, April 30, 1915

description: The Daily Southern Californian, Vol. 6, No. 22, April 30, 1915.
DOI: 10.25549/uschist-dt-m185026
title: Daily Trojan, Vol. 26, No. 56, January 02, 1935

description: Daily Trojan, Vol. 26, No. 56, January 02, 1935.
DOI: 10.25549/uschist-dt-m190286
title: Daily Trojan, Vol. 61, No. 28, October 22, 1969

description: Daily Trojan, Vol. 61, No. 28, October 22, 1969.
DOI: 10.25919/5bb0e84d63fb2
title: Parkes observations for project P892 semester 2016OCTS_BPSR_10

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: 10.25919/5bb0e89a9bdc3
title: Parkes observations for project P892 semester 2016OCTS_BPSR_11

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: 10.25919/5bb0e8e67e188
title: Parkes observations for project P934 semester 2016OCTS_BPSR_01

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: 10.25919/5bb0e9316e171
title: Parkes observations for project P934 semester 2016OCTS_BPSR_02

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: 10.25919/5bb0e97cad053
title: Parkes observations for project P934 semester 2016OCTS_BPSR_03

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: 10.25919/5bb0e9c6cf24d
title: Parkes observations for project P892 semester 2016OCTS_BPSR_21

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: 10.25919/5bb0ea1353925
title: Parkes observations for project P892 semester 2016OCTS_BPSR_22

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: 10.25919/5bb0ea6133d39
title: Parkes observations for project P892 semester 2016OCTS_BPSR_23

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: 10.25491/0hm3-v413
title: GTEX-P4QS-0526-SM-2I3ET

description: Sample ID: GTEX-P4QS-0526-SM-2I3ET
DOI: 10.25491/121c-m914
title: GTEX-P4QS-1126-SM-3NMD5

description: Sample ID: GTEX-P4QS-1126-SM-3NMD5
DOI: 10.25491/16xw-zs86
title: GTEX-ZTPG-2226-SM-57WF9

description: Sample ID: GTEX-ZTPG-2226-SM-57WF9
DOI: 10.25491/2gtp-0e45
title: GTEX-ZTSS-0004-SM-4YCCS

description: Sample ID: GTEX-ZTSS-0004-SM-4YCCS
DOI: 10.25491/35fk-db66
title: GTEX-X4XX-1126-SM-3NMBY

description: Sample ID: GTEX-X4XX-1126-SM-3NMBY
DOI: 10.25491/37v5-0f11
title: GTEX-ZTPG-1526-SM-51MTF

description: Sample ID: GTEX-ZTPG-1526-SM-51MTF
DOI: 10.25491/5d1e-wv52
title: GTEX-UJHI-0326-SM-4IHJE

description: Sample ID: GTEX-UJHI-0326-SM-4IHJE
DOI: 10.25491/6meb-t714
title: GTEX-YB5K-2226-SM-4WWG1

description: Sample ID: GTEX-YB5K-2226-SM-4WWG1
DOI: 10.25491/78e2-t454
title: GTEX-RNOR-0011-R1A-SM-5SI8F

description: Sample ID: GTEX-RNOR-0011-R1A-SM-5SI8F
DOI: 10.25491/88zt-5j34
title: GTEX-RNOR-0011-R4A-SM-3GAD3

description: Sample ID: GTEX-RNOR-0011-R4A-SM-3GAD3
DOI: 10.25491/8t5r-4x51
title: GTEX-YBZK-0326-SM-59HLN

description: Sample ID: GTEX-YBZK-0326-SM-59HLN
DOI: 10.25491/8w2b-ma92
title: GTEX-P4QS-1026-SM-3NMCW

description: Sample ID: GTEX-P4QS-1026-SM-3NMCW
DOI: 10.25491/a29w-7c20
title: GTEX-X4XY-0011-R6B-SM-46MVB

description: Sample ID: GTEX-X4XY-0011-R6B-SM-46MVB
DOI: 10.25491/amf5-jn44
title: GTEX-X4XX-0726-SM-4QARS

description: Sample ID: GTEX-X4XX-0726-SM-4QARS
DOI: 10.25491/b98x-d890
title: GTEX-ZTPG-1326-SM-51MSQ

description: Sample ID: GTEX-ZTPG-1326-SM-51MSQ
DOI: 10.25491/c33d-6w34
title: GTEX-ZTPG-2326-SM-57WFL

description: Sample ID: GTEX-ZTPG-2326-SM-57WFL
DOI: 10.25491/cj8k-s135
title: GTEX-ZTPG-1626-SM-5DUX2

description: Sample ID: GTEX-ZTPG-1626-SM-5DUX2
DOI: 10.25491/ck3b-4k95
title: GTEX-X4XX-3026-SM-3NMB2

description: Sample ID: GTEX-X4XX-3026-SM-3NMB2
DOI: 10.25491/db0f-jt10
title: GTEX-P4QS-0626-SM-3NMD1

description: Sample ID: GTEX-P4QS-0626-SM-3NMD1
DOI: 10.25491/dj75-we85
title: GTEX-RNOR-0011-R5A-SM-2TF4J

description: Sample ID: GTEX-RNOR-0011-R5A-SM-2TF4J
DOI: 10.25491/dn2z-8m70
title: GTEX-RNOR-0011-R7A-SM-2TF4V

description: Sample ID: GTEX-RNOR-0011-R7A-SM-2TF4V
DOI: 10.25491/dqrb-xg33
title: GTEX-YBZK-0005-SM-59HKG

description: Sample ID: GTEX-YBZK-0005-SM-59HKG
DOI: 10.25491/dtr9-7038
title: GTEX-X4XY-0008-SM-46MVL

description: Sample ID: GTEX-X4XY-0008-SM-46MVL
DOI: 10.25491/e44k-ac35
title: GTEX-UJHI-0226-SM-4IHJL

description: Sample ID: GTEX-UJHI-0226-SM-4IHJL
DOI: 10.25491/e9md-ap05
title: GTEX-P4QS-0726-SM-3NMCZ

description: Sample ID: GTEX-P4QS-0726-SM-3NMCZ
DOI: 10.25491/ekv8-hx29
title: GTEX-ZTPG-2626-SM-57WFX

description: Sample ID: GTEX-ZTPG-2626-SM-57WFX
DOI: 10.25491/f09s-w920
title: GTEX-X4XX-0926-SM-46MV7

description: Sample ID: GTEX-X4XX-0926-SM-46MV7
DOI: 10.25491/fjq8-gq48
title: GTEX-YB5K-2126-SM-4WWDJ

description: Sample ID: GTEX-YB5K-2126-SM-4WWDJ
DOI: 10.25491/g90j-mh92
title: GTEX-RNOR-0326-SM-2TF51

description: Sample ID: GTEX-RNOR-0326-SM-2TF51
DOI: 10.25491/grf0-ye75
title: GTEX-RNOR-0011-R3A-SM-5SI8E

description: Sample ID: GTEX-RNOR-0011-R3A-SM-5SI8E
DOI: 10.25491/jp1v-9y65
title: GTEX-RNOR-0011-R3A-SM-2TF5J

description: Sample ID: GTEX-RNOR-0011-R3A-SM-2TF5J
DOI: 10.25491/m5qs-dm86
title: GTEX-RNOR-0126-SM-2TF57

description: Sample ID: GTEX-RNOR-0126-SM-2TF57
DOI: 10.25491/m6ny-jj34
title: GTEX-YB5K-2526-SM-62LEW

description: Sample ID: GTEX-YB5K-2526-SM-62LEW
DOI: 10.25491/p2a5-0797
title: GTEX-UJHI-0126-SM-4IHLP

description: Sample ID: GTEX-UJHI-0126-SM-4IHLP
DOI: 10.25491/pck6-ct02
title: GTEX-UJHI-0008-SM-4IHL1

description: Sample ID: GTEX-UJHI-0008-SM-4IHL1
DOI: 10.25491/qr01-qr78
title: GTEX-UJHI-0426-SM-3DB8Y

description: Sample ID: GTEX-UJHI-0426-SM-3DB8Y
DOI: 10.25491/qx8c-0239
title: GTEX-X4XY-0006-SM-46MV2

description: Sample ID: GTEX-X4XY-0006-SM-46MV2
DOI: 10.25491/rber-tr67
title: GTEX-YB5K-2326-SM-5IFHD

description: Sample ID: GTEX-YB5K-2326-SM-5IFHD
DOI: 10.25491/sy42-0v04
title: GTEX-P4QS-0926-SM-48TBS

description: Sample ID: GTEX-P4QS-0926-SM-48TBS
DOI: 10.25491/t1qg-9253
title: GTEX-X4XX-2926-SM-3NMB1

description: Sample ID: GTEX-X4XX-2926-SM-3NMB1
DOI: 10.25491/t335-fd13
title: GTEX-YB5K-2426-SM-5IFHP

description: Sample ID: GTEX-YB5K-2426-SM-5IFHP
DOI: 10.25491/vc8v-3r10
title: GTEX-P4QS-0226-SM-3NB1U

description: Sample ID: GTEX-P4QS-0226-SM-3NB1U
DOI: 10.25491/wce4-f949
title: GTEX-P4QS-1326-SM-3NMCD

description: Sample ID: GTEX-P4QS-1326-SM-3NMCD
DOI: 10.25491/wdqx-av94
title: GTEX-ZTPG-2026-SM-5O999

description: Sample ID: GTEX-ZTPG-2026-SM-5O999
DOI: 10.25491/wj6f-0x77
title: GTEX-UJHI-0006-SM-3DB8H

description: Sample ID: GTEX-UJHI-0006-SM-3DB8H
DOI: 10.25491/x59r-s685
title: GTEX-P4QS-0326-SM-2I3EU

description: Sample ID: GTEX-P4QS-0326-SM-2I3EU
DOI: 10.25491/xmhy-yy81
title: GTEX-U8XE-2026-SM-3DB8S

description: Sample ID: GTEX-U8XE-2026-SM-3DB8S
DOI: 10.25491/zmkj-5v92
title: GTEX-YB5K-2026-SM-4VDT3

description: Sample ID: GTEX-YB5K-2026-SM-4VDT3
DOI: 10.25491/zz5v-yp48
title: GTEX-X4XX-1026-SM-4QARO

description: Sample ID: GTEX-X4XX-1026-SM-4QARO
DOI: 10.25919/5bb0eaac19614
title: Parkes observations for project P892 semester 2016OCTS_BPSR_24

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: 10.25919/5bb0eaf708f46
title: Parkes observations for project P892 semester 2016OCTS_BPSR_25

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: 10.25919/5bb0eb414854b
title: Parkes observations for project P892 semester 2016OCTS_BPSR_26

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: 10.25919/5bb0eb8ca0b78
title: Parkes observations for project P892 semester 2016OCTS_BPSR_27

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.