cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25491/9xd5-ks48
title: GTEX-UJMC-1226-SM-4IHLI

description: Sample ID: GTEX-UJMC-1226-SM-4IHLI
DOI: 10.25491/bjy7-j635
title: GTEX-UJMC-0626-SM-4IHJQ

description: Sample ID: GTEX-UJMC-0626-SM-4IHJQ
DOI: 10.25491/bwmb-5612
title: GTEX-P78B-0008-SM-48TE1

description: Sample ID: GTEX-P78B-0008-SM-48TE1
DOI: 10.25491/c56z-ck90
title: GTEX-UJMC-1826-SM-3GADT

description: Sample ID: GTEX-UJMC-1826-SM-3GADT
DOI: 10.25491/czav-rg22
title: GTEX-P78B-0426-SM-2I5F5

description: Sample ID: GTEX-P78B-0426-SM-2I5F5
DOI: 10.25491/d6sv-bj08
title: GTEX-P4QT-1826-SM-2S1NJ

description: Sample ID: GTEX-P4QT-1826-SM-2S1NJ
DOI: 10.25491/egzm-m676
title: GTEX-YEC3-1426-SM-4WWEM

description: Sample ID: GTEX-YEC3-1426-SM-4WWEM
DOI: 10.25491/ff4j-vj04
title: GTEX-RTLS-0526-SM-2TF64

description: Sample ID: GTEX-RTLS-0526-SM-2TF64
DOI: 10.25491/fghp-8851
title: GTEX-RTLS-0826-SM-2TF5Q

description: Sample ID: GTEX-RTLS-0826-SM-2TF5Q
DOI: 10.25491/fm24-ww08
title: GTEX-YEC3-1126-SM-5IFIH

description: Sample ID: GTEX-YEC3-1126-SM-5IFIH
DOI: 10.25491/g2ve-h044
title: GTEX-UJMC-1026-SM-4IHKN

description: Sample ID: GTEX-UJMC-1026-SM-4IHKN
DOI: 10.25491/ga2p-j456
title: GTEX-P78B-0626-SM-2S1O5

description: Sample ID: GTEX-P78B-0626-SM-2S1O5
DOI: 10.25491/gacc-ak29
title: GTEX-RTLS-1126-SM-46MUQ

description: Sample ID: GTEX-RTLS-1126-SM-46MUQ
DOI: 10.25491/hny2-f357
title: GTEX-UJMC-0326-SM-3GAE2

description: Sample ID: GTEX-UJMC-0326-SM-3GAE2
DOI: 10.25491/hzz1-1g40
title: GTEX-RTLS-0426-SM-2TF5K

description: Sample ID: GTEX-RTLS-0426-SM-2TF5K
DOI: 10.25491/j1re-j786
title: GTEX-X585-1426-SM-4E3JO

description: Sample ID: GTEX-X585-1426-SM-4E3JO
DOI: 10.25491/j9es-5150
title: GTEX-UJMC-0926-SM-4IHLK

description: Sample ID: GTEX-UJMC-0926-SM-4IHLK
DOI: 10.25491/jztd-qp67
title: GTEX-RTLS-0626-SM-2TF6G

description: Sample ID: GTEX-RTLS-0626-SM-2TF6G
DOI: 10.25491/k44t-0w37
title: GTEX-RTLS-0226-SM-2TF5E

description: Sample ID: GTEX-RTLS-0226-SM-2TF5E
DOI: 10.25491/kf2q-h221
title: GTEX-ZTTD-0526-SM-57WDV

description: Sample ID: GTEX-ZTTD-0526-SM-57WDV
DOI: 10.25491/m0jq-yq44
title: GTEX-X585-0011-R8A-SM-46MUX

description: Sample ID: GTEX-X585-0011-R8A-SM-46MUX
DOI: 10.25491/mvk7-0p43
title: GTEX-UJMC-0526-SM-3GAE3

description: Sample ID: GTEX-UJMC-0526-SM-3GAE3
DOI: 10.25491/myh4-xj20
title: GTEX-X585-0011-R4B-SM-46MVH

description: Sample ID: GTEX-X585-0011-R4B-SM-46MVH
DOI: 10.25491/mz4c-gz86
title: GTEX-P4QT-2426-SM-3NMCL

description: Sample ID: GTEX-P4QT-2426-SM-3NMCL
DOI: 10.25491/phv0-7904
title: GTEX-P4QT-2026-SM-3NMCJ

description: Sample ID: GTEX-P4QT-2026-SM-3NMCJ
DOI: 10.25491/px0h-nw92
title: GTEX-UJMC-1126-SM-3GADP

description: Sample ID: GTEX-UJMC-1126-SM-3GADP
DOI: 10.25491/qr19-pz75
title: GTEX-ZTTD-2626-SM-57WEX

description: Sample ID: GTEX-ZTTD-2626-SM-57WEX
DOI: 10.25491/qsxt-r656
title: GTEX-X585-0011-R2B-SM-46MVF

description: Sample ID: GTEX-X585-0011-R2B-SM-46MVF
DOI: 10.25491/r4ff-tr56
title: GTEX-YEC3-1226-SM-5IFI8

description: Sample ID: GTEX-YEC3-1226-SM-5IFI8
DOI: 10.25491/rm1b-cq37
title: GTEX-ZTTD-2826-SM-4YCFA

description: Sample ID: GTEX-ZTTD-2826-SM-4YCFA
DOI: 10.25491/rqx7-rc54
title: GTEX-UJMC-0726-SM-3GADX

description: Sample ID: GTEX-UJMC-0726-SM-3GADX
DOI: 10.25491/ssyj-m947
title: GTEX-X585-0226-SM-4QAS2

description: Sample ID: GTEX-X585-0226-SM-4QAS2
DOI: 10.25491/v02g-bh64
title: GTEX-ZTTD-1026-SM-51MRD

description: Sample ID: GTEX-ZTTD-1026-SM-51MRD
DOI: 10.25491/vb1a-9251
title: GTEX-RTLS-0926-SM-2TF5X

description: Sample ID: GTEX-RTLS-0926-SM-2TF5X
DOI: 10.25491/w69y-5x67
title: GTEX-YEC3-0826-SM-4WWFP

description: Sample ID: GTEX-YEC3-0826-SM-4WWFP
DOI: 10.25491/wmf4-gn21
title: GTEX-X585-0011-R3B-SM-46MVG

description: Sample ID: GTEX-X585-0011-R3B-SM-46MVG
DOI: 10.25491/yy89-9f34
title: GTEX-P78B-0005-SM-2I5GM

description: Sample ID: GTEX-P78B-0005-SM-2I5GM
DOI: 10.25491/zzes-4k65
title: GTEX-ZTTD-1126-SM-51MRP

description: Sample ID: GTEX-ZTTD-1126-SM-51MRP
DOI: 10.25549/uschist-dt-m183801
title: The Daily Southern Californian, Vol. 5, No. 23, October 23, 1914

description: The Daily Southern Californian, Vol. 5, No. 23, October 23, 1914.
DOI: 10.25549/uschist-dt-m185110
title: The Southern California Trojan, Vol. 7, No. 44, December 03, 1915

description: The Southern California Trojan, Vol. 7, No. 44, December 03, 1915.
DOI: 10.25549/uschist-dt-m189574
title: Daily Trojan, Vol. 61, No. 46, November 18, 1969

description: Daily Trojan, Vol. 61, No. 46, November 18, 1969.
DOI: 10.25919/5bb0f17b49b8b
title: Parkes observations for project P892 semester 2016OCTS_BPSR_16

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: 10.25919/5bb0f1c74e4a1
title: Parkes observations for project P892 semester 2016OCTS_BPSR_17

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: 10.25919/5bb0f212592aa
title: Parkes observations for project P892 semester 2016OCTS_BPSR_18

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: 10.25919/5bb0f25d5f67b
title: Parkes observations for project P892 semester 2016OCTS_BPSR_19

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: 10.25919/5bb0f2a9c642d
title: Parkes observations for project P892 semester 2016OCTS_BPSR_20

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: 10.25919/5bb0f2f4dae07
title: Parkes observations for project P892 semester 2016OCTS_BPSR_36

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: 10.25919/5bb0f33fed96f
title: Parkes observations for project P892 semester 2016OCTS_BPSR_41

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: 10.25491/18bq-2a98
title: GTEX-YEC3-1926-SM-5IFIT

description: Sample ID: GTEX-YEC3-1926-SM-5IFIT
DOI: 10.25491/1dpz-2597
title: GTEX-P78B-1126-SM-3P615

description: Sample ID: GTEX-P78B-1126-SM-3P615
DOI: 10.25491/1f6g-cr28
title: GTEX-ZTX8-0626-SM-59HKC

description: Sample ID: GTEX-ZTX8-0626-SM-59HKC
DOI: 10.25491/1fjt-ta82
title: GTEX-YEC3-1426-SM-5PNXW

description: Sample ID: GTEX-YEC3-1426-SM-5PNXW
DOI: 10.25491/33f7-tv71
title: GTEX-RTLS-1226-SM-46MUP

description: Sample ID: GTEX-RTLS-1226-SM-46MUP
DOI: 10.25491/3awv-5668
title: GTEX-P78B-0826-SM-3NMCA

description: Sample ID: GTEX-P78B-0826-SM-3NMCA
DOI: 10.25491/3nnk-3x38
title: GTEX-ZTX8-0326-SM-59HLA

description: Sample ID: GTEX-ZTX8-0326-SM-59HLA
DOI: 10.25491/3p6x-3c66
title: GTEX-ZTX8-0002-SM-4YCEU

description: Sample ID: GTEX-ZTX8-0002-SM-4YCEU
DOI: 10.25491/4v4z-e179
title: GTEX-P78B-1626-SM-2S1O1

description: Sample ID: GTEX-P78B-1626-SM-2S1O1
DOI: 10.25491/56b2-3h48
title: GTEX-UPIC-0326-SM-4IHJ9

description: Sample ID: GTEX-UPIC-0326-SM-4IHJ9
DOI: 10.25491/65tv-h292
title: GTEX-X5EB-0008-SM-46MU3

description: Sample ID: GTEX-X5EB-0008-SM-46MU3
DOI: 10.25491/6m6r-p306
title: GTEX-X585-2426-SM-46MW2

description: Sample ID: GTEX-X585-2426-SM-46MW2
DOI: 10.25491/7fch-ac66
title: GTEX-YEC3-2126-SM-4YCDB

description: Sample ID: GTEX-YEC3-2126-SM-4YCDB
DOI: 10.25491/832t-1t82
title: GTEX-RU1J-0003-SM-3K2A8

description: Sample ID: GTEX-RU1J-0003-SM-3K2A8
DOI: 10.25491/83kb-w140
title: GTEX-RU1J-0006-SM-2TF6M

description: Sample ID: GTEX-RU1J-0006-SM-2TF6M
DOI: 10.25491/b84w-1939
title: GTEX-X585-3126-SM-4QASH

description: Sample ID: GTEX-X585-3126-SM-4QASH
DOI: 10.25491/c2g2-1n30
title: GTEX-UPIC-0005-SM-3GACV

description: Sample ID: GTEX-UPIC-0005-SM-3GACV
DOI: 10.25491/dby1-1y86
title: GTEX-ZTX8-0526-SM-59HLD

description: Sample ID: GTEX-ZTX8-0526-SM-59HLD
DOI: 10.25491/djc8-0e35
title: GTEX-ZTX8-0426-SM-59HLG

description: Sample ID: GTEX-ZTX8-0426-SM-59HLG
DOI: 10.25491/dtrj-5906
title: GTEX-ZTX8-0008-SM-4YCDV

description: Sample ID: GTEX-ZTX8-0008-SM-4YCDV
DOI: 10.25491/dwfb-ta54
title: GTEX-UPIC-0626-SM-4IHK2

description: Sample ID: GTEX-UPIC-0626-SM-4IHK2
DOI: 10.25491/ea3x-3998
title: GTEX-X585-3026-SM-46MWF

description: Sample ID: GTEX-X585-3026-SM-46MWF
DOI: 10.25491/f455-2160
title: GTEX-YEC3-2026-SM-5CVLQ

description: Sample ID: GTEX-YEC3-2026-SM-5CVLQ
DOI: 10.25491/fbzj-b020
title: GTEX-UJMC-2026-SM-3GADR

description: Sample ID: GTEX-UJMC-2026-SM-3GADR
DOI: 10.25491/fnn9-3v87
title: GTEX-X585-2526-SM-4QAS1

description: Sample ID: GTEX-X585-2526-SM-4QAS1
DOI: 10.25491/gdvs-nr33
title: GTEX-P78B-1326-SM-3P611

description: Sample ID: GTEX-P78B-1326-SM-3P611
DOI: 10.25491/gvwe-3119
title: GTEX-UJMC-1926-SM-3GADS

description: Sample ID: GTEX-UJMC-1926-SM-3GADS
DOI: 10.25491/hntt-mc05
title: GTEX-P78B-0726-SM-2S1O2

description: Sample ID: GTEX-P78B-0726-SM-2S1O2
DOI: 10.25491/jg0t-9r08
title: GTEX-YEC3-1726-SM-5IFIK

description: Sample ID: GTEX-YEC3-1726-SM-5IFIK
DOI: 10.25491/jt46-z468
title: GTEX-X5EB-0004-SM-46MWA

description: Sample ID: GTEX-X5EB-0004-SM-46MWA
DOI: 10.25491/ke7d-q486
title: GTEX-UPIC-0526-SM-4WWCQ

description: Sample ID: GTEX-UPIC-0526-SM-4WWCQ
DOI: 10.25491/kjg6-zn39
title: GTEX-ZTX8-0006-SM-4YCE4

description: Sample ID: GTEX-ZTX8-0006-SM-4YCE4
DOI: 10.25491/m8rd-1041
title: GTEX-RTLS-1326-SM-46MUN

description: Sample ID: GTEX-RTLS-1326-SM-46MUN
DOI: 10.25491/msbn-ya64
title: GTEX-RTLS-2426-SM-46MUO

description: Sample ID: GTEX-RTLS-2426-SM-46MUO
DOI: 10.25491/nmkd-v945
title: GTEX-P78B-0626-SM-5S2W4

description: Sample ID: GTEX-P78B-0626-SM-5S2W4
DOI: 10.25491/nysq-8e87
title: GTEX-YEC3-1326-SM-5PNXV

description: Sample ID: GTEX-YEC3-1326-SM-5PNXV
DOI: 10.25491/pmn2-b885
title: GTEX-RU1J-0008-SM-46MV9

description: Sample ID: GTEX-RU1J-0008-SM-46MV9
DOI: 10.25491/q6qc-hv41
title: GTEX-RTLS-2326-SM-46MUH

description: Sample ID: GTEX-RTLS-2326-SM-46MUH
DOI: 10.25491/qfxb-n062
title: GTEX-UPIC-0226-SM-3GADO

description: Sample ID: GTEX-UPIC-0226-SM-3GADO
DOI: 10.25491/qz4m-hj12
title: GTEX-X585-1826-SM-4QAS3

description: Sample ID: GTEX-X585-1826-SM-4QAS3
DOI: 10.25491/raah-w010
title: GTEX-X585-1226-SM-46MW7

description: Sample ID: GTEX-X585-1226-SM-46MW7
DOI: 10.25491/s2y2-fw81
title: GTEX-P78B-0526-SM-2I5F7

description: Sample ID: GTEX-P78B-0526-SM-2I5F7
DOI: 10.25491/s67k-n274
title: GTEX-X5EB-0006-SM-46MV5

description: Sample ID: GTEX-X5EB-0006-SM-46MV5
DOI: 10.25491/sghh-wr20
title: GTEX-ZTX8-0226-SM-5E44D

description: Sample ID: GTEX-ZTX8-0226-SM-5E44D
DOI: 10.25491/t51k-3k93
title: GTEX-ZTTD-2726-SM-57WFA

description: Sample ID: GTEX-ZTTD-2726-SM-57WFA
DOI: 10.25491/ta2p-fk68
title: GTEX-UJMC-1326-SM-4IHLS

description: Sample ID: GTEX-UJMC-1326-SM-4IHLS
DOI: 10.25491/tz4n-xx41
title: GTEX-RU1J-0126-SM-2TF6Y

description: Sample ID: GTEX-RU1J-0126-SM-2TF6Y
DOI: 10.25491/v7b6-zz82
title: GTEX-YEC3-2026-SM-4WWFL

description: Sample ID: GTEX-YEC3-2026-SM-4WWFL
DOI: 10.25491/vhad-jw68
title: GTEX-P78B-0926-SM-2I5FA

description: Sample ID: GTEX-P78B-0926-SM-2I5FA
DOI: 10.25491/watc-km87
title: GTEX-P78B-1626-SM-5SI85

description: Sample ID: GTEX-P78B-1626-SM-5SI85
DOI: 10.25491/xftg-b668
title: GTEX-UPIC-0002-SM-3NMDC

description: Sample ID: GTEX-UPIC-0002-SM-3NMDC
DOI: 10.25491/zd1w-b138
title: GTEX-YEC3-1926-SM-4WWF5

description: Sample ID: GTEX-YEC3-1926-SM-4WWF5
DOI: 10.25549/uschist-dt-m176663
title: The Daily Southern Californian, Vol. 10, No. 28, April 08, 1913

description: The Daily Southern Californian, Vol. 10, No. 28, April 08, 1913.
DOI: 10.25549/uschist-dt-m183425
title: The Southern California Trojan, Vol. 7, No. 9, September 30, 1915

description: The Southern California Trojan, Vol. 7, No. 9, September 30, 1915.
DOI: 10.25549/uschist-dt-m184723
title: Daily Trojan, Vol. 25, No. 122, April 26, 1934

description: Daily Trojan, Vol. 25, No. 122, April 26, 1934
DOI: 10.25549/uschist-dt-m187179
title: The Southern California Trojan, Vol. 7, No. 83, March 09, 1916

description: The Southern California Trojan, Vol. 7, No. 83, March 09, 1916.
DOI: 10.25549/uschist-dt-m190473
title: Daily Trojan, Vol. 61, No. 4, September 18, 1969

description: Daily Trojan, Vol. 61, No. 4, September 18, 1969.
DOI: 10.25919/5bb0f39150e3b
title: Parkes observations for project P892 semester 2016OCTS_BPSR_42

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: 10.25919/5bb0f3dcea1d5
title: Parkes observations for project P892 semester 2016OCTS_BPSR_43

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.