cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25919/5bb0ee881d008
title: Parkes observations for project P892 semester 2016OCTS_BPSR_37

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: 10.25919/5bb0eed53f804
title: Parkes observations for project P892 semester 2016OCTS_BPSR_38

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: 10.25919/5bb0ef1fe9eb1
title: Parkes observations for project P892 semester 2016OCTS_BPSR_39

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: 10.25919/5bb0ef6b85bad
title: Parkes observations for project P892 semester 2016OCTS_BPSR_40

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: 10.25491/15z3-t840
title: GTEX-ZTTD-0008-SM-51MQV

description: Sample ID: GTEX-ZTTD-0008-SM-51MQV
DOI: 10.25491/2gqc-6h45
title: GTEX-X585-0011-R1B-SM-46MVE

description: Sample ID: GTEX-X585-0011-R1B-SM-46MVE
DOI: 10.25491/2p6m-hs38
title: GTEX-ZTTD-0626-SM-4YCCY

description: Sample ID: GTEX-ZTTD-0626-SM-4YCCY
DOI: 10.25491/2yka-yr98
title: GTEX-UJMC-0426-SM-4IHJF

description: Sample ID: GTEX-UJMC-0426-SM-4IHJF
DOI: 10.25491/33yn-b328
title: GTEX-YEC3-0526-SM-5IFHN

description: Sample ID: GTEX-YEC3-0526-SM-5IFHN
DOI: 10.25491/3b1z-pr41
title: GTEX-X4XY-1626-SM-46MVN

description: Sample ID: GTEX-X4XY-1626-SM-46MVN
DOI: 10.25491/4fhv-mw18
title: GTEX-P4QT-0626-SM-3NMCP

description: Sample ID: GTEX-P4QT-0626-SM-3NMCP
DOI: 10.25491/4xyy-7m90
title: GTEX-P4QT-1626-SM-2S1NP

description: Sample ID: GTEX-P4QT-1626-SM-2S1NP
DOI: 10.25491/564m-9788
title: GTEX-X585-0011-R10A-SM-46MUY

description: Sample ID: GTEX-X585-0011-R10A-SM-46MUY
DOI: 10.25491/594v-y106
title: GTEX-YEC3-0626-SM-5IFHZ

description: Sample ID: GTEX-YEC3-0626-SM-5IFHZ
DOI: 10.25491/5qxy-n321
title: GTEX-RTLS-0326-SM-2TF6A

description: Sample ID: GTEX-RTLS-0326-SM-2TF6A
DOI: 10.25491/5y8c-8024
title: GTEX-RNOR-2426-SM-48FDY

description: Sample ID: GTEX-RNOR-2426-SM-48FDY
DOI: 10.25491/5yzb-9r96
title: GTEX-UJMC-0005-SM-3GACU

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DOI: 10.25491/79d8-vv09
title: GTEX-YEC3-0626-SM-4YCFE

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DOI: 10.25491/834m-xf59
title: GTEX-UJHI-1526-SM-3DB99

description: Sample ID: GTEX-UJHI-1526-SM-3DB99
DOI: 10.25491/87sz-3522
title: GTEX-RNOR-2226-SM-2TF5O

description: Sample ID: GTEX-RNOR-2226-SM-2TF5O
DOI: 10.25491/8ffj-kz24
title: GTEX-UJMC-0008-SM-4IHKK

description: Sample ID: GTEX-UJMC-0008-SM-4IHKK
DOI: 10.25491/8scv-r844
title: GTEX-ZTTD-0006-SM-51MSJ

description: Sample ID: GTEX-ZTTD-0006-SM-51MSJ
DOI: 10.25491/8srh-g291
title: GTEX-P4QT-0726-SM-3NMCM

description: Sample ID: GTEX-P4QT-0726-SM-3NMCM
DOI: 10.25491/9d4g-sa59
title: GTEX-ZTSS-1226-SM-51MSZ

description: Sample ID: GTEX-ZTSS-1226-SM-51MSZ
DOI: 10.25491/9jzz-9w91
title: GTEX-YEC3-0726-SM-4YCD1

description: Sample ID: GTEX-YEC3-0726-SM-4YCD1
DOI: 10.25491/9pag-eq74
title: GTEX-RNOR-2326-SM-2TF4I

description: Sample ID: GTEX-RNOR-2326-SM-2TF4I
DOI: 10.25491/a63j-z043
title: GTEX-YEC3-0826-SM-5P9JF

description: Sample ID: GTEX-YEC3-0826-SM-5P9JF
DOI: 10.25491/cmny-bx82
title: GTEX-YEC3-0726-SM-5IFIW

description: Sample ID: GTEX-YEC3-0726-SM-5IFIW
DOI: 10.25491/devc-3s45
title: GTEX-X585-0011-R11B-SM-46MUZ

description: Sample ID: GTEX-X585-0011-R11B-SM-46MUZ
DOI: 10.25491/dxtj-5z91
title: GTEX-RTLS-0008-SM-48FET

description: Sample ID: GTEX-RTLS-0008-SM-48FET
DOI: 10.25491/dz4y-nv55
title: GTEX-P4QT-0526-SM-2I3EX

description: Sample ID: GTEX-P4QT-0526-SM-2I3EX
DOI: 10.25491/e0cx-3888
title: GTEX-P4QT-1626-SM-5S2UR

description: Sample ID: GTEX-P4QT-1626-SM-5S2UR
DOI: 10.25491/ecdm-jk08
title: GTEX-RTLS-0126-SM-447CA

description: Sample ID: GTEX-RTLS-0126-SM-447CA
DOI: 10.25491/eq10-5p52
title: GTEX-P4QT-1326-SM-3NMD3

description: Sample ID: GTEX-P4QT-1326-SM-3NMD3
DOI: 10.25491/f1s5-3907
title: GTEX-ZTSS-1926-SM-57WEW

description: Sample ID: GTEX-ZTSS-1926-SM-57WEW
DOI: 10.25491/gqch-bn47
title: GTEX-X585-0008-SM-46MU4

description: Sample ID: GTEX-X585-0008-SM-46MU4
DOI: 10.25491/k2c0-a834
title: GTEX-RTLS-0006-SM-2TF58

description: Sample ID: GTEX-RTLS-0006-SM-2TF58
DOI: 10.25491/k2wj-3230
title: GTEX-YEC3-0526-SM-4YCF2

description: Sample ID: GTEX-YEC3-0526-SM-4YCF2
DOI: 10.25491/mb40-5z51
title: GTEX-ZTSS-2026-SM-5987K

description: Sample ID: GTEX-ZTSS-2026-SM-5987K
DOI: 10.25491/n5qr-m224
title: GTEX-UJHI-1626-SM-3DB9A

description: Sample ID: GTEX-UJHI-1626-SM-3DB9A
DOI: 10.25491/nvtg-2395
title: GTEX-X585-0002-SM-46MVA

description: Sample ID: GTEX-X585-0002-SM-46MVA
DOI: 10.25491/p5rr-sx08
title: GTEX-P4QT-1526-SM-3NMCT

description: Sample ID: GTEX-P4QT-1526-SM-3NMCT
DOI: 10.25491/pprx-8805
title: GTEX-UJMC-0226-SM-4IHLH

description: Sample ID: GTEX-UJMC-0226-SM-4IHLH
DOI: 10.25491/rc6f-p658
title: GTEX-ZTSS-1426-SM-5985P

description: Sample ID: GTEX-ZTSS-1426-SM-5985P
DOI: 10.25491/rdw3-6458
title: GTEX-X4XY-1726-SM-46MVO

description: Sample ID: GTEX-X4XY-1726-SM-46MVO
DOI: 10.25491/t65r-4r49
title: GTEX-P4QT-1426-SM-3NMCX

description: Sample ID: GTEX-P4QT-1426-SM-3NMCX
DOI: 10.25491/tjxp-5071
title: GTEX-YEC3-0226-SM-5IFJO

description: Sample ID: GTEX-YEC3-0226-SM-5IFJO
DOI: 10.25491/w2ky-q881
title: GTEX-RNOR-1326-SM-48FDE

description: Sample ID: GTEX-RNOR-1326-SM-48FDE
DOI: 10.25491/wa9e-4q82
title: GTEX-ZTSS-1526-SM-51MTC

description: Sample ID: GTEX-ZTSS-1526-SM-51MTC
DOI: 10.25491/xdff-wa65
title: GTEX-X585-0005-SM-46MV3

description: Sample ID: GTEX-X585-0005-SM-46MV3
DOI: 10.25491/y3qd-kq86
title: GTEX-UJHI-1926-SM-3DB8Z

description: Sample ID: GTEX-UJHI-1926-SM-3DB8Z
DOI: 10.25491/yah0-x366
title: GTEX-ZTTD-0001-SM-4YCD5

description: Sample ID: GTEX-ZTTD-0001-SM-4YCD5
DOI: 10.25491/zvp8-hm35
title: GTEX-UJHI-1726-SM-3DB9B

description: Sample ID: GTEX-UJHI-1726-SM-3DB9B
DOI: 10.25491/zybe-ve92
title: GTEX-YEC3-0426-SM-5IFK1

description: Sample ID: GTEX-YEC3-0426-SM-5IFK1
DOI: 10.25549/uschist-dt-m173611
title: Daily Trojan, Vol. 147, No. 38, October 18, 2002

description: Daily Trojan, Vol. 147, No. 38, October 18, 2002.
DOI: 10.25549/uschist-dt-m176738
title: The Daily Southern Californian, Vol. 10, No. 33, April 18, 1913

description: The Daily Southern Californian, Vol. 10, No. 33, April 18, 1913.
DOI: 10.25549/uschist-dt-m176884
title: The Daily Southern Californian, Vol. 9, No. 25, October 28, 1912

description: The Daily Southern Californian, Vol. 9, No. 25, October 28, 1912.
DOI: 10.25549/uschist-dt-m183500
title: The Daily Southern Californian, Vol. 6, No. 20, April 23, 1915

description: The Daily Southern Californian, Vol. 6, No. 20, April 23, 1915.
DOI: 10.25549/uschist-dt-m183645
title: The Daily Southern Californian, Vol. 3, No. 1, September 11, 1913

description: The Daily Southern Californian, Vol. 3, No. 1, September 11, 1913.
DOI: 10.25549/uschist-dt-m183878
title: The Daily Southern Californian, Vol. 4, No. 13, March 03, 1914

description: The Daily Southern Californian, Vol. 4, No. 13, March 03, 1914.
DOI: 10.25549/uschist-dt-m184949
title: The Yellow Dog, Vol. 3.2, No. 1, May 08, 1934

description: The Yellow Dog, Vol. 3.2, No. 1, May 08, 1934.
DOI: 10.25549/uschist-dt-m185187
title: The Daily Southern Californian, Vol. 3, No. 67, January 23, 1914

description: The Daily Southern Californian, Vol. 3, No. 67, January 23, 1914.
DOI: 10.25549/uschist-dt-m186887
title: Daily Trojan, Vol. 55, No. 93, April 08, 1964

description: Daily Trojan, Vol. 55, No. 94 [sic, i.e. 93], April 08, 1964.
DOI: 10.25549/uschist-dt-m187350
title: Daily Trojan, Vol. 151, No. 59, April 19, 2004

description: Daily Trojan, Vol. 145 [sic i.e. 151], No. 59, April 19, 2004.
DOI: 10.25549/uschist-dt-m190077
title: Daily Trojan, Vol. 90, No. 20, March 05, 1981

description: Daily Trojan, Vol. 90, No. 20, March 05, 1981.
DOI: 10.25919/5bb0efb6affc2
title: Parkes observations for project P892 semester 2016OCTS_BPSR_31

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: 10.25919/5bb0f002ccecf
title: Parkes observations for project P892 semester 2016OCTS_BPSR_32

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: 10.25919/5bb0f04e52286
title: Parkes observations for project P892 semester 2016OCTS_BPSR_15

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: 10.25919/5bb0f09954e7d
title: Parkes observations for project P860 semester 2016OCTS

description: This is a request for observing time for the initial follow-up of pulsar discoveries from the low-latitude Galactic plane section of the HTRU survey (P630). We have already discovered 88 pulsars from 93% of processed data. With data processing on-going, we expect that processing and data review should be complete by the end of the upcoming semester. Extrapolation and population synthesis shows that the Galactic plane survey should result in a further 15-20 discoveries.

The discovery of pulsars is just a first step and interesting science can usually only be revealed when a follow-up timing campaign is carried out. One year of initial timing is the minimal timespan required to fully-characterise any newly-discovered pulsars, essential for deriving pulsar parameters such as the characteristic age, magnetic ?eld strength, spin-down rate, as well as to detect any unexpected behaviour of the pulsar which might result from emission instabilities.

This follow-up timing project is necessary for identifying any interesting pulsar systems discovered from the HTRU Galactic plane survey. Since all of the pulsars on the observing list here are followed-up for the first time, they will produce completely new and exciting results. In addition, this timing project will enable a large-scale examination of the Galactic plane pulsar population, exploring the true boundaries of pulsar phase space. Given the large number of discoveries expected and the long integration length required, this dedicated follow-up timing campaign is vital for achieving our science goals.
DOI: 10.25919/5bb0f0e3cb573
title: Parkes observations for project P860 semester 2016OCTS_BPSR_01

description: This is a request for observing time for the initial follow-up of pulsar discoveries from the low-latitude Galactic plane section of the HTRU survey (P630). We have already discovered 88 pulsars from 93% of processed data. With data processing on-going, we expect that processing and data review should be complete by the end of the upcoming semester. Extrapolation and population synthesis shows that the Galactic plane survey should result in a further 15-20 discoveries.

The discovery of pulsars is just a first step and interesting science can usually only be revealed when a follow-up timing campaign is carried out. One year of initial timing is the minimal timespan required to fully-characterise any newly-discovered pulsars, essential for deriving pulsar parameters such as the characteristic age, magnetic ?eld strength, spin-down rate, as well as to detect any unexpected behaviour of the pulsar which might result from emission instabilities.

This follow-up timing project is necessary for identifying any interesting pulsar systems discovered from the HTRU Galactic plane survey. Since all of the pulsars on the observing list here are followed-up for the first time, they will produce completely new and exciting results. In addition, this timing project will enable a large-scale examination of the Galactic plane pulsar population, exploring the true boundaries of pulsar phase space. Given the large number of discoveries expected and the long integration length required, this dedicated follow-up timing campaign is vital for achieving our science goals.
DOI: 10.25919/5bb0f12f445a9
title: Parkes observations for project P860 semester 2016OCTS_BPSR_02

description: This is a request for observing time for the initial follow-up of pulsar discoveries from the low-latitude Galactic plane section of the HTRU survey (P630). We have already discovered 88 pulsars from 93% of processed data. With data processing on-going, we expect that processing and data review should be complete by the end of the upcoming semester. Extrapolation and population synthesis shows that the Galactic plane survey should result in a further 15-20 discoveries.

The discovery of pulsars is just a first step and interesting science can usually only be revealed when a follow-up timing campaign is carried out. One year of initial timing is the minimal timespan required to fully-characterise any newly-discovered pulsars, essential for deriving pulsar parameters such as the characteristic age, magnetic ?eld strength, spin-down rate, as well as to detect any unexpected behaviour of the pulsar which might result from emission instabilities.

This follow-up timing project is necessary for identifying any interesting pulsar systems discovered from the HTRU Galactic plane survey. Since all of the pulsars on the observing list here are followed-up for the first time, they will produce completely new and exciting results. In addition, this timing project will enable a large-scale examination of the Galactic plane pulsar population, exploring the true boundaries of pulsar phase space. Given the large number of discoveries expected and the long integration length required, this dedicated follow-up timing campaign is vital for achieving our science goals.
DOI: 10.25491/1d81-e057
title: GTEX-X585-0011-R5A-SM-46MVI

description: Sample ID: GTEX-X585-0011-R5A-SM-46MVI
DOI: 10.25491/1pg9-bz02
title: GTEX-ZTTD-1226-SM-51MS2

description: Sample ID: GTEX-ZTTD-1226-SM-51MS2
DOI: 10.25491/2g0w-vt85
title: GTEX-X585-0426-SM-4E3JZ

description: Sample ID: GTEX-X585-0426-SM-4E3JZ
DOI: 10.25491/2qsd-7887
title: GTEX-ZTTD-1426-SM-4YCEX

description: Sample ID: GTEX-ZTTD-1426-SM-4YCEX
DOI: 10.25491/2qyq-8r48
title: GTEX-P4QT-2626-SM-2I3FM

description: Sample ID: GTEX-P4QT-2626-SM-2I3FM
DOI: 10.25491/3rv9-c084
title: GTEX-P4QT-1726-SM-2S1NQ

description: Sample ID: GTEX-P4QT-1726-SM-2S1NQ
DOI: 10.25491/41a4-q698
title: GTEX-ZTTD-0326-SM-57WFW

description: Sample ID: GTEX-ZTTD-0326-SM-57WFW
DOI: 10.25491/4kcx-k114
title: GTEX-RTLS-0726-SM-46MV4

description: Sample ID: GTEX-RTLS-0726-SM-46MV4
DOI: 10.25491/5yvr-0z72
title: GTEX-ZTTD-1726-SM-57WEL

description: Sample ID: GTEX-ZTTD-1726-SM-57WEL
DOI: 10.25491/6gck-za36
title: GTEX-RTLS-0626-SM-5SI7Z

description: Sample ID: GTEX-RTLS-0626-SM-5SI7Z
DOI: 10.25491/6j9w-qq79
title: GTEX-X585-1026-SM-46MW6

description: Sample ID: GTEX-X585-1026-SM-46MW6
DOI: 10.25491/6vme-0v28
title: GTEX-YEC3-0926-SM-5Q5AC

description: Sample ID: GTEX-YEC3-0926-SM-5Q5AC
DOI: 10.25491/6xnc-fa48
title: GTEX-YEC3-1026-SM-5IFI5

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DOI: 10.25491/7gwb-ks11
title: GTEX-P78B-0226-SM-3NB1Z

description: Sample ID: GTEX-P78B-0226-SM-3NB1Z
DOI: 10.25491/82zp-hp14
title: GTEX-YEC3-1326-SM-4WWEL

description: Sample ID: GTEX-YEC3-1326-SM-4WWEL
DOI: 10.25491/82zz-kr07
title: GTEX-X585-0011-R6A-SM-46MVJ

description: Sample ID: GTEX-X585-0011-R6A-SM-46MVJ
DOI: 10.25491/98q1-4025
title: GTEX-YEC3-1426-101806-SM-5PNXX

description: Sample ID: GTEX-YEC3-1426-101806-SM-5PNXX