cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.23725/p390-k390
title: NWD296878.b38.irc.v1.cram

description: TOPMed: NWD296878.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/p7pr-jr66
title: NWD212065.b38.irc.v1.cram

description: TOPMed: NWD212065.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/pdhm-zt52
title: NWD207548.b38.irc.v1.cram

description: TOPMed: NWD207548.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/q0fn-6075
title: NWD380927.b38.irc.v1.cram

description: TOPMed: NWD380927.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/qjj0-a215
title: NWD125203.b38.irc.v1.cram

description: TOPMed: NWD125203.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/sdhn-zm23
title: NWD296872.b38.irc.v1.cram

description: TOPMed: NWD296872.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/tajp-5j52
title: NWD296394.b38.irc.v1.cram

description: TOPMed: NWD296394.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/tqdt-f516
title: NWD125366.b38.irc.v1.cram

description: TOPMed: NWD125366.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/twv9-2g92
title: NWD210876.b38.irc.v1.cram

description: TOPMed: NWD210876.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/vk78-7f29
title: NWD125036.b38.irc.v1.cram

description: TOPMed: NWD125036.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/w6hk-7h88
title: NWD211600.b38.irc.v1.cram

description: TOPMed: NWD211600.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/wbhy-gf74
title: NWD129070.b38.irc.v1.cram

description: TOPMed: NWD129070.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/x5m6-f693
title: NWD140418.b38.irc.v1.cram

description: TOPMed: NWD140418.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/xe9a-cm02
title: NWD296710.b38.irc.v1.cram

description: TOPMed: NWD296710.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/xes6-0f62
title: NWD137552.b38.irc.v1.cram

description: TOPMed: NWD137552.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/ydxf-m170
title: NWD208851.b38.irc.v1.cram

description: TOPMed: NWD208851.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/zr9g-c183
title: NWD125369.b38.irc.v1.cram

description: TOPMed: NWD125369.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.25549/pcra-c14-195024
title: Beware!, 1963
title: Берегитесь!, 1963

description: An essay protesting against the AUECB (All-Union Council of Evangelical Christian-Baptists), December 1963. Листовка-протест против ВСЕХБ (Всесоюзный совет Евангельских Христиан-Баптистов), декабрь 1963 год.
DOI: 10.25549/uschist-c104-179646
title: Daily Trojan, Vol. 166, No. 4, January 16, 2009

description: Daily Trojan, Vol. 166, No. 4, January 16, 2009.
DOI: 10.25549/uschist-c104-181292
title: Daily Trojan, Vol. 168, No. 36, October 15, 2009

description: Daily Trojan, Vol. 168, No. 36, October 15, 2009.
DOI: 10.25549/uschist-c104-185428
title: Daily Trojan, Vol. 36, No. 64, February 08, 1945

description: Daily Trojan, Vol. 36, No. 64, February 08, 1945.
DOI: 10.25549/uschist-c104-195657
title: Daily Trojan, vol. 177, no. 19, Sep 25, 2012

description: Daily Trojan, vol. 177, no. 19, Sep 25, 2012.
DOI: 10.25549/uschist-c104-196721
title: Daily Trojan, vol. 175, no. 11, Jan 26, 2012

description: Daily Trojan, vol. 175, no. 11, Jan 26, 2012.
DOI: 10.25549/uschist-c104-198268
title: Daily Trojan, vol. 174, no. 37, Oct 13, 2011

description: Daily Trojan, vol. 174, no. 37, Oct 13, 2011.
DOI: 10.25549/uschist-c104-199378
title: Daily Trojan, vol. 172, no. 42, Mar 24, 2011

description: Daily Trojan, vol. 172, no. 42, Mar 24, 2011.
DOI: 10.25549/uschist-c104-200640
title: Daily Trojan, vol. 171, no. 57, Nov 12, 2010

description: Daily Trojan, vol. 171, no. 57, Nov 12, 2010.
DOI: 10.25549/uschist-c104-202382
title: Daily Trojan, vol. 162, no. 20, Sep 25, 2007

description: Daily Trojan, vol. 162, no. 20, Sep 25, 2007.
DOI: 10.25549/uschist-c104-204998
title: Daily Trojan, vol. 180, no. 24, Sep 30, 2013

description: Daily Trojan, vol. 180, no. 24, Sep 30, 2013.
DOI: 10.25549/uschist-c104-206038
title: Daily Trojan, vol. 181, no. 27, Feb 25, 2014

description: Daily Trojan, vol. 181, no. 27, Feb 25, 2014.
DOI: 10.25549/uschist-c104-207759
title: Daily Trojan, vol. 183, no. 46, Oct 30, 2014

description: Daily Trojan, vol. 183, no. 46, Oct 30, 2014.
DOI: 10.25549/uschist-c104-217001
title: Daily Trojan, vol. 184, no. 20, Feb 11, 2015

description: Daily Trojan, vol. 184, no. 20, Feb 11, 2015.
DOI: 10.23725/1a15-m158
title: NWD297233.b38.irc.v1.cram

description: TOPMed: NWD297233.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/2296-t390
title: NWD125936.b38.irc.v1.cram

description: TOPMed: NWD125936.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/36nn-4n09
title: NWD212490.b38.irc.v1.cram

description: TOPMed: NWD212490.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/37jd-1r46
title: NWD213157.b38.irc.v1.cram

description: TOPMed: NWD213157.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/4djn-as12
title: NWD213025.b38.irc.v1.cram

description: TOPMed: NWD213025.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/4mpr-je45
title: NWD213547.b38.irc.v1.cram

description: TOPMed: NWD213547.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/4q3c-hm17
title: NWD213062.b38.irc.v1.cram

description: TOPMed: NWD213062.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/4s7x-qa98
title: NWD382491.b38.irc.v1.cram

description: TOPMed: NWD382491.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/5m89-cr40
title: NWD217570.b38.irc.v1.cram

description: TOPMed: NWD217570.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/66v7-8w80
title: NWD144845.b38.irc.v1.cram

description: TOPMed: NWD144845.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/6gb1-sy19
title: NWD382309.b38.irc.v1.cram

description: TOPMed: NWD382309.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/728n-bs77
title: NWD218827.b38.irc.v1.cram

description: TOPMed: NWD218827.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/7nqf-ej86
title: NWD381843.b38.irc.v1.cram

description: TOPMed: NWD381843.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/7r6c-2d88
title: NWD381722.b38.irc.v1.cram

description: TOPMed: NWD381722.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/81vn-mr72
title: NWD125889.b38.irc.v1.cram

description: TOPMed: NWD125889.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/8adf-1g34
title: NWD212295.b38.irc.v1.cram

description: TOPMed: NWD212295.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/98j7-8t67
title: NWD382450.b38.irc.v1.cram

description: TOPMed: NWD382450.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/9kx8-fn32
title: NWD125655.b38.irc.v1.cram

description: TOPMed: NWD125655.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/9zwx-0t16
title: NWD212574.b38.irc.v1.cram

description: TOPMed: NWD212574.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/b42w-6035
title: NWD297220.b38.irc.v1.cram

description: TOPMed: NWD297220.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/bfdv-qm65
title: NWD144991.b38.irc.v1.cram

description: TOPMed: NWD144991.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/bgn4-8k22
title: NWD297445.b38.irc.v1.cram

description: TOPMed: NWD297445.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/cf6r-8g79
title: NWD144090.b38.irc.v1.cram

description: TOPMed: NWD144090.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/cp40-k494
title: NWD382185.b38.irc.v1.cram

description: TOPMed: NWD382185.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/cpyr-rk92
title: NWD144080.b38.irc.v1.cram

description: TOPMed: NWD144080.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/d0ag-4941
title: NWD296935.b38.irc.v1.cram

description: TOPMed: NWD296935.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/d28x-4c13
title: NWD297140.b38.irc.v1.cram

description: TOPMed: NWD297140.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/dnq2-r449
title: NWD297636.b38.irc.v1.cram

description: TOPMed: NWD297636.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/dzap-7h42
title: NWD220603.b38.irc.v1.cram

description: TOPMed: NWD220603.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/fegs-g452
title: NWD125492.b38.irc.v1.cram

description: TOPMed: NWD125492.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/g10y-2k14
title: NWD212589.b38.irc.v1.cram

description: TOPMed: NWD212589.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/j5ep-d813
title: NWD297129.b38.irc.v1.cram

description: TOPMed: NWD297129.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/jjfs-0425
title: NWD212611.b38.irc.v1.cram

description: TOPMed: NWD212611.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/jjrc-7017
title: NWD297635.b38.irc.v1.cram

description: TOPMed: NWD297635.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/jtga-6b22
title: NWD125897.b38.irc.v1.cram

description: TOPMed: NWD125897.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/mxf4-h651
title: NWD125984.b38.irc.v1.cram

description: TOPMed: NWD125984.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/nex0-z017
title: NWD212367.b38.irc.v1.cram

description: TOPMed: NWD212367.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/q0j8-bk60
title: NWD125790.b38.irc.v1.cram

description: TOPMed: NWD125790.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/q8fa-a941
title: NWD125872.b38.irc.v1.cram

description: TOPMed: NWD125872.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/r05t-2w98
title: NWD212362.b38.irc.v1.cram

description: TOPMed: NWD212362.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/rfcc-dn81
title: NWD125634.b38.irc.v1.cram

description: TOPMed: NWD125634.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/sgab-a474
title: NWD211940.b38.irc.v1.cram

description: TOPMed: NWD211940.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/sq3b-n660
title: NWD382045.b38.irc.v1.cram

description: TOPMed: NWD382045.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/svb9-my89
title: NWD216753.b38.irc.v1.cram

description: TOPMed: NWD216753.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/sxrg-d480
title: NWD212879.b38.irc.v1.cram

description: TOPMed: NWD212879.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/v0td-8s73
title: NWD212476.b38.irc.v1.cram

description: TOPMed: NWD212476.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/v8tx-nj87
title: NWD150626.b38.irc.v1.cram

description: TOPMed: NWD150626.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/vd5p-2r57
title: NWD140620.b38.irc.v1.cram

description: TOPMed: NWD140620.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/w8st-5854
title: NWD381897.b38.irc.v1.cram

description: TOPMed: NWD381897.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/wtpc-pd92
title: NWD382440.b38.irc.v1.cram

description: TOPMed: NWD382440.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/ww57-6165
title: NWD146859.b38.irc.v1.cram

description: TOPMed: NWD146859.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/y97x-cx86
title: NWD144831.b38.irc.v1.cram

description: TOPMed: NWD144831.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.25549/pcra-c14-99691
title: Gouden-schooven-1929_0257
DOI: 10.25549/uschist-c104-178366
title: Summer Trojan, Vol. 164, No. 6, June 25, 2008

description: Summer Trojan, Vol. 164, No. 6, June 25, 2008.
DOI: 10.25549/uschist-c104-179659
title: Daily Trojan, Vol. 166, No. 11, January 29, 2009

description: Daily Trojan, Vol. 166, No. 11, January 29, 2009.
DOI: 10.25549/uschist-c104-181305
title: Daily Trojan, Vol. 168, No. 40, October 21, 2009

description: Daily Trojan, Vol. 168, No. 40, October 21, 2009.
DOI: 10.25549/uschist-c104-182557
title: Daily Trojan, Vol. 169, No. 51, April 07, 2010

description: Daily Trojan, Vol. 169, No. 51, April 07, 2010.
DOI: 10.25549/uschist-c104-195670
title: Daily Trojan, vol. 177, no. 22, Sep 28, 2012

description: Daily Trojan, vol. 177, no. 22, Sep 28, 2012.
DOI: 10.25549/uschist-c104-196734
title: Daily Trojan, vol. 175, no. 10, Jan 25, 2012

description: Daily Trojan, vol. 175, no. 10, Jan 25, 2012.
DOI: 10.25549/uschist-c104-198281
title: Daily Trojan, vol. 174, no. 48, Oct 31, 2011

description: Daily Trojan, vol. 174, no. 48, Oct 31, 2011.
DOI: 10.25549/uschist-c104-199395
title: Daily Trojan, vol. 178, no. 57, Apr 18, 2013

description: Daily Trojan, vol. 178, no. 57, Apr 18, 2013.
DOI: 10.25549/uschist-c104-200653
title: Daily Trojan, vol. 171, no. 63, Nov 22, 2010

description: Daily Trojan, vol. 171, no. 63, Nov 22, 2010.
DOI: 10.25549/uschist-c104-205011
title: Daily Trojan, vol. 180, no. 21, Sep 25, 2013

description: Daily Trojan, vol. 180, no. 21, Sep 25, 2013.
DOI: 10.25549/uschist-c104-206051
title: Daily Trojan, vol. 181, no. 38, Mar 12, 2014

description: Daily Trojan, vol. 181, no. 38, Mar 12, 2014.
DOI: 10.25549/uschist-c104-207772
title: Daily Trojan, vol. 183, no. 51, Nov 06, 2014

description: Daily Trojan, vol. 183, no. 51, Nov 06, 2014.
DOI: 10.25549/uschist-c104-217014
title: Daily Trojan, vol. 184, no. 27, Feb 24, 2015

description: Daily Trojan, vol. 184, no. 27, Feb 24, 2015.
DOI: 10.25549/uschist-c104-252820
title: Summer Trojan, vol. 185, no. 06, Jun 24, 2015

description: Summer Trojan, vol. 185, no. 06, Jun 24, 2015.
DOI: 10.25919/5bb0e55019f00
title: Parkes observations for project P892 semester 2016OCTS

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: 10.25919/5bb0e59c42669
title: Parkes observations for project P892 semester 2016OCTS_BPSR_01

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: 10.25919/5bb0e5e6cee6b
title: Parkes observations for project P892 semester 2016OCTS_BPSR_02

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: 10.25919/5bb0e632a5a92
title: Parkes observations for project P892 semester 2016OCTS_BPSR_03

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: 10.25919/5bb0e67dc8170
title: Parkes observations for project P892 semester 2016OCTS_BPSR_04

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: 10.25919/5bb0e6d141438
title: Parkes observations for project P892 semester 2016OCTS_BPSR_05

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: 10.25919/5bb0e71bde25f
title: Parkes observations for project P892 semester 2016OCTS_BPSR_06

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: 10.23725/0h33-4r79
title: NWD212718.b38.irc.v1.cram

description: TOPMed: NWD212718.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/0jph-cn97
title: NWD126151.b38.irc.v1.cram

description: TOPMed: NWD126151.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/0src-jr13
title: NWD152319.b38.irc.v1.cram

description: TOPMed: NWD152319.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/11ap-tp29
title: NWD382983.b38.irc.v1.cram

description: TOPMed: NWD382983.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/2tbc-j153
title: NWD382511.b38.irc.v1.cram

description: TOPMed: NWD382511.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/3p7d-cs63
title: NWD297709.b38.irc.v1.cram

description: TOPMed: NWD297709.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/3wq5-4k88
title: NWD297751.b38.irc.v1.cram

description: TOPMed: NWD297751.b38.irc.v1.cram <br>File: CRAM file
DOI: 10.23725/3ys1-9y04
title: NWD297953.b38.irc.v1.cram

description: TOPMed: NWD297953.b38.irc.v1.cram <br>File: CRAM file