cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25919/5bb0f7fc60936
title: Parkes observations for project P892 semester 2016OCTS_BPSR_63

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: 10.25919/5bb0f846c2838
title: Parkes observations for project P892 semester 2016OCTS_BPSR_64

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: 10.25491/072x-1k79
title: GTEX-UPJH-0726-SM-4IHJW

description: Sample ID: GTEX-UPJH-0726-SM-4IHJW
DOI: 10.25491/0bn3-dp10
title: GTEX-PLZ4-0926-SM-2S1OI

description: Sample ID: GTEX-PLZ4-0926-SM-2S1OI
DOI: 10.25491/0tbd-tj30
title: GTEX-PLZ4-2726-SM-3P61A

description: Sample ID: GTEX-PLZ4-2726-SM-3P61A
DOI: 10.25491/1b4e-0f40
title: GTEX-RU72-0011-R10A-SM-2TF6D

description: Sample ID: GTEX-RU72-0011-R10A-SM-2TF6D
DOI: 10.25491/5jkw-k096
title: GTEX-UPIC-1726-SM-4IHKG

description: Sample ID: GTEX-UPIC-1726-SM-4IHKG
DOI: 10.25491/5rt0-2c96
title: GTEX-PLZ4-0126-SM-2S1OG

description: Sample ID: GTEX-PLZ4-0126-SM-2S1OG
DOI: 10.25491/5t6m-jd21
title: GTEX-RU72-0011-R5A-SM-2TF6U

description: Sample ID: GTEX-RU72-0011-R5A-SM-2TF6U
DOI: 10.25491/671g-s502
title: GTEX-PLZ4-1326-SM-2S1O7

description: Sample ID: GTEX-PLZ4-1326-SM-2S1O7
DOI: 10.25491/67an-sn18
title: GTEX-UPJH-0226-SM-3GADV

description: Sample ID: GTEX-UPJH-0226-SM-3GADV
DOI: 10.25491/77rs-7e38
title: GTEX-X5EB-1526-SM-4E3JC

description: Sample ID: GTEX-X5EB-1526-SM-4E3JC
DOI: 10.25491/7by5-8v97
title: GTEX-UPJH-0006-SM-3GACW

description: Sample ID: GTEX-UPJH-0006-SM-3GACW
DOI: 10.25491/87n1-pn78
title: GTEX-ZU9S-0226-SM-5E441

description: Sample ID: GTEX-ZU9S-0226-SM-5E441
DOI: 10.25491/8pe8-wz18
title: GTEX-X5EB-1426-SM-46MVW

description: Sample ID: GTEX-X5EB-1426-SM-46MVW
DOI: 10.25491/8zyj-8v62
title: GTEX-X5EB-1926-SM-4E3IW

description: Sample ID: GTEX-X5EB-1926-SM-4E3IW
DOI: 10.25491/90v9-xh33
title: GTEX-X5EB-2026-SM-4E3KA

description: Sample ID: GTEX-X5EB-2026-SM-4E3KA
DOI: 10.25491/9b8n-0g40
title: GTEX-RU1J-1926-SM-2TF6S

description: Sample ID: GTEX-RU1J-1926-SM-2TF6S
DOI: 10.25491/9jg2-2a49
title: GTEX-YEC4-0126-SM-4W21T

description: Sample ID: GTEX-YEC4-0126-SM-4W21T
DOI: 10.25491/9vvz-e966
title: GTEX-UPJH-0326-SM-3GADU

description: Sample ID: GTEX-UPJH-0326-SM-3GADU
DOI: 10.25491/b5c3-qz69
title: GTEX-YEC4-0426-SM-4W1ZH

description: Sample ID: GTEX-YEC4-0426-SM-4W1ZH
DOI: 10.25491/cha2-cg44
title: GTEX-RU1J-1726-SM-2TF5S

description: Sample ID: GTEX-RU1J-1726-SM-2TF5S
DOI: 10.25491/ec8h-fe42
title: GTEX-ZUA1-0011-R10a-SM-51MT6

description: Sample ID: GTEX-ZUA1-0011-R10a-SM-51MT6
DOI: 10.25491/eg53-s382
title: GTEX-YEC4-0826-SM-5P9FV

description: Sample ID: GTEX-YEC4-0826-SM-5P9FV
DOI: 10.25491/egf0-db05
title: GTEX-RU72-0011-R11A-SM-5SI8G

description: Sample ID: GTEX-RU72-0011-R11A-SM-5SI8G
DOI: 10.25491/fp24-b524
title: GTEX-PLZ4-0226-SM-2S1NW

description: Sample ID: GTEX-PLZ4-0226-SM-2S1NW
DOI: 10.25491/g9kw-c220
title: GTEX-RU72-0011-R2A-SM-2TF6O

description: Sample ID: GTEX-RU72-0011-R2A-SM-2TF6O
DOI: 10.25491/gfxn-9z41
title: GTEX-RU72-0006-SM-2TF65

description: Sample ID: GTEX-RU72-0006-SM-2TF65
DOI: 10.25491/h1xy-xk61
title: GTEX-YEC4-0226-SM-4W1YG

description: Sample ID: GTEX-YEC4-0226-SM-4W1YG
DOI: 10.25491/h8ws-yy77
title: GTEX-ZUA1-0005-SM-4YCEV

description: Sample ID: GTEX-ZUA1-0005-SM-4YCEV
DOI: 10.25491/hvwk-yd79
title: GTEX-UPJH-0126-SM-4IHLL

description: Sample ID: GTEX-UPJH-0126-SM-4IHLL
DOI: 10.25491/jptk-kk38
title: GTEX-RU72-0011-R11A-SM-2TF6J

description: Sample ID: GTEX-RU72-0011-R11A-SM-2TF6J
DOI: 10.25491/jq51-ad65
title: GTEX-YEC4-0726-SM-5CVLV

description: Sample ID: GTEX-YEC4-0726-SM-5CVLV
DOI: 10.25491/js6q-9r74
title: GTEX-PLZ4-0226-SM-5SI7M

description: Sample ID: GTEX-PLZ4-0226-SM-5SI7M
DOI: 10.25491/k6nj-0z72
title: GTEX-YEC4-0526-SM-4W21U

description: Sample ID: GTEX-YEC4-0526-SM-4W21U
DOI: 10.25491/kcjb-zq21
title: GTEX-UPIC-1826-SM-4IHKC

description: Sample ID: GTEX-UPIC-1826-SM-4IHKC
DOI: 10.25491/kx6x-n575
title: GTEX-YEC4-0326-SM-4W216

description: Sample ID: GTEX-YEC4-0326-SM-4W216
DOI: 10.25491/kynx-d195
title: GTEX-X5EB-1626-SM-4E3IV

description: Sample ID: GTEX-X5EB-1626-SM-4E3IV
DOI: 10.25491/mpnr-2271
title: GTEX-ZUA1-0002-SM-4YCF7

description: Sample ID: GTEX-ZUA1-0002-SM-4YCF7
DOI: 10.25491/nxp0-z145
title: GTEX-PLZ4-0126-SM-5SI8O

description: Sample ID: GTEX-PLZ4-0126-SM-5SI8O
DOI: 10.25491/nyzf-0h41
title: GTEX-UPJH-0526-SM-4IHK8

description: Sample ID: GTEX-UPJH-0526-SM-4IHK8
DOI: 10.25491/re3p-8m28
title: GTEX-ZU9S-1926-SM-5NQBP

description: Sample ID: GTEX-ZU9S-1926-SM-5NQBP
DOI: 10.25491/v5d6-kn50
title: GTEX-X5EB-1126-SM-46MVV

description: Sample ID: GTEX-X5EB-1126-SM-46MVV
DOI: 10.25491/v9t2-ca93
title: GTEX-YEC4-0002-SM-4W1Z6

description: Sample ID: GTEX-YEC4-0002-SM-4W1Z6
DOI: 10.25491/vg1v-y241
title: GTEX-ZU9S-1826-SM-5NQ9E

description: Sample ID: GTEX-ZU9S-1826-SM-5NQ9E
DOI: 10.25491/w0rt-a949
title: GTEX-PLZ4-0726-SM-2TC6Q

description: Sample ID: GTEX-PLZ4-0726-SM-2TC6Q
DOI: 10.25491/wqtq-j458
title: GTEX-ZTX8-1826-SM-5N9E5

description: Sample ID: GTEX-ZTX8-1826-SM-5N9E5
DOI: 10.25491/wzjc-x802
title: GTEX-RU72-0008-SM-46MV8

description: Sample ID: GTEX-RU72-0008-SM-46MV8
DOI: 10.25491/x8t0-2v95
title: GTEX-X5EB-1826-SM-4E3K8

description: Sample ID: GTEX-X5EB-1826-SM-4E3K8
DOI: 10.25491/x8te-nw74
title: GTEX-ZU9S-1626-SM-5E452

description: Sample ID: GTEX-ZU9S-1626-SM-5E452
DOI: 10.25491/xhm0-by94
title: GTEX-PLZ4-1226-SM-2I5FE

description: Sample ID: GTEX-PLZ4-1226-SM-2I5FE
DOI: 10.25491/xxht-h450
title: GTEX-X5EB-1726-SM-4E3J7

description: Sample ID: GTEX-X5EB-1726-SM-4E3J7
DOI: 10.25919/5bb0f89503604
title: Parkes observations for project P892 semester 2016OCTS_BPSR_65

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: 10.25919/5bb0f92b78d0c
title: Parkes observations for project P574 semester 2016OCTS_BPSR_01

description: We request time to observe 260 pulsars on a regular basis in order to provide the accurate ephemerides necessary for the detection and characterisation of gamma-ray pulsars with the Fermi satellite. The main science goals are to increase the number of known gamma-ray pulsars (both radio loud and radio quiet), to determine accurate pulse profiles, and to characterise their high energy (phase-resolved) spectra. In the radio, the observations will also allow us to find glitches, characterise timing noise, investigate dispersion and rotation measure variability, and enhance our knowledge of single pulse phenomenology. To date, we
are (co-)authors on 50 papers arising from the collaboration and P574 data. The data have contributed to the PhD theses of students from the Bordeaux group and Stanford and are remain in active use (detailed within).
DOI: 10.25919/5bb0f97cdf846
title: Parkes observations for project P880 semester 2016OCTS

description: XSS J1227-4859 is the second "Transitional" pulsar binary system discovered in the galactic field. We plan to continue our campaign of observations at 20cm with the aims of: (i) discriminating the various proposed mechanisms responsible for the orbital variations seen in the system; (ii) keeping the phase coherence of the timing solution in order to investigate the nature of the gamma-ray emission from the binary; (iii) determining the critical X-ray luminosity above which the pulsed radio emission disappears;  (iv) constraining the geometry of the emission from the system in the radio, X-ray and gamma-ray bands through (quasi) simultaneous multiwavelength observations..
DOI: 10.25919/5bb0f9ce33e4e
title: Parkes observations for project P880 semester 2016OCTS_BPSR_01

description: XSS J1227-4859 is the second "Transitional" pulsar binary system discovered in the galactic field. We plan to continue our campaign of observations at 20cm with the aims of: (i) discriminating the various proposed mechanisms responsible for the orbital variations seen in the system; (ii) keeping the phase coherence of the timing solution in order to investigate the nature of the gamma-ray emission from the binary; (iii) determining the critical X-ray luminosity above which the pulsed radio emission disappears;  (iv) constraining the geometry of the emission from the system in the radio, X-ray and gamma-ray bands through (quasi) simultaneous multiwavelength observations..
DOI: 10.25919/5bb0fa191c314
title: Parkes observations for project P871 semester 2016OCTS

description: Fast Radio Bursts (FRBs) are bright, millisecond-duration radio pulses hypothesized to originate at cosmological distances. To date, one FRB has been seen to repeat but their origins remain a puzzling mystery. Some have proposed FRBs come from Crab-like pulsar giant pulses or periods of high activity of distant magnetars. Both mechanisms would generate observable subsequent FRB-like events. In this proposal we directly test this hypothesis by monitoring the fields of two known FRBs to search for repeating pulses that may explain their progenitors. We target two sources with existing multi-wavelength archival images of the field and small DM-derived distances.
DOI: 10.25919/5bb0fa6476ee5
title: Parkes observations for project P885 semester 2016OCTS

description: We propose to observe 1E 1547.0-5408 weekly, one of two magnetars
known to currently emit radio pulsations, to track its rotation,
flux density, and polarisation. Less frequently we will monitor
PSR J1622-4950 and XTE J1810-197, which used to emit radio pulsations,
to be on the lookout for their revival. After years with unsteady
radio emission, 1E 1547.0-5408 is now detected 100% of the time,
allowing us to obtain a continuous record of its torque which
illuminates the continued release of magnetic energy in the neutron
star. Our broader aims are to develop a better understanding of
the dynamical behaviour of magnetar magnetospheres, and to establish
the conditions under which radio emission takes place therein, in
addition to characterising their variable radio emission in order
to place constraints on the emission mechanisms, which in at least
some respects differ from those of ordinary pulsars.
DOI: 10.25919/5bb0faaf74510
title: Parkes observations for project P895 semester 2016OCTS

description: Since the year 2005, the Parkes Pulsar Timing Array (PPTA) project has been placing ever more stringent constraints on the amplitude of a gravitational wave background signal.  Our most recent constraints rule out the standard models for galaxy formation and black hole evolution.  It is essential for the PPTA project, its Northern Hemisphere counterparts and key science projects on MeerKAT and the SKA to know the amplitude of the expected gravitational wave signal. We therefore propose to observe our most precisely timed pulsar, PSR J1909-3744, regularly in order to either obtain the lowest bound possible before MeerKAT and the SKA are commissioned or to identify the characteristic gravitational wave signal in the data set for this single pulsar.
DOI: 10.25919/5bb0fafa45e8c
title: Parkes observations for project P897 semester 2016OCTS

description: Modulation of pulse times of arrival (TOAs) from pulsars often heralds excitement: planetary companions, neutron star free precession, and the poorly understood but crucially important process of magnetospheric state switching can all produce quasi-periodic TOA modulation.  In a sample of 150 young pulsars, we have detected periodic modulation in six pulsars.  We propose to obtain multi-epoch, deep, well-calibrated 10 cm pulse profiles to search for profile variability, particularly variability correlated with TOA modulation.  The absence of such variation may lend credence to a planet interpretation, while detection will help characterize the magnetospheric states and determine if free precession plays a role.  Because the pulsars are largely southern sky objects, and because the 10cm band is largely free from RFI and scattering, Parkes is uniquely capable to deliver this science.
DOI: 10.25919/5bb0fb449e70f
title: Parkes observations for project P898 semester 2016OCTS

description: Our initial Parkes study of the 5.4-day eclipsing millisecond pulsar
(MSP) J1417-4402 shows it to be the first system identified in the
Galaxy on a standard evolutionary track that will end as a typical
binary MSP with a low-mass white dwarf companion. With the requested
timing observations we seek to characterize the late phase in the
formation of a typical MSP binary, until now unobserved. In particular,
we aim to measure the pulsar spin-down luminosity, the orbital
eccentricity, and to search for gamma-ray pulsations.
DOI: 10.25491/049h-tt34
title: GTEX-RU72-0126-SM-2TF6Z

description: Sample ID: GTEX-RU72-0126-SM-2TF6Z
DOI: 10.25491/11ec-hg31
title: GTEX-YEC4-1126-SM-5CVLW

description: Sample ID: GTEX-YEC4-1126-SM-5CVLW
DOI: 10.25491/1b0e-wg43
title: GTEX-UPK5-0008-SM-4IHJD

description: Sample ID: GTEX-UPK5-0008-SM-4IHJD
DOI: 10.25491/26tj-6p79
title: GTEX-YEC4-1426-SM-5IFHS

description: Sample ID: GTEX-YEC4-1426-SM-5IFHS
DOI: 10.25491/2jrs-ay56
title: GTEX-X5EB-2526-SM-4E3HY

description: Sample ID: GTEX-X5EB-2526-SM-4E3HY
DOI: 10.25491/2vag-6585
title: GTEX-RU72-0726-SM-46MUW

description: Sample ID: GTEX-RU72-0726-SM-46MUW
DOI: 10.25491/379g-ss65
title: GTEX-X62O-0005-SM-46MV1

description: Sample ID: GTEX-X62O-0005-SM-46MV1
DOI: 10.25491/3ge1-2c97
title: GTEX-ZUA1-0011-R1a-SM-4YCE2

description: Sample ID: GTEX-ZUA1-0011-R1a-SM-4YCE2
DOI: 10.25491/3wym-p827
title: GTEX-PLZ4-1626-SM-3P618

description: Sample ID: GTEX-PLZ4-1626-SM-3P618
DOI: 10.25491/555n-7k57
title: GTEX-RU72-0326-SM-2TF5T

description: Sample ID: GTEX-RU72-0326-SM-2TF5T
DOI: 10.25491/56jp-e352
title: GTEX-ZUA1-0011-R8b-SM-51MST

description: Sample ID: GTEX-ZUA1-0011-R8b-SM-51MST
DOI: 10.25491/5e15-r696
title: GTEX-X638-0003-SM-47JZ1

description: Sample ID: GTEX-X638-0003-SM-47JZ1
DOI: 10.25491/5g1n-5t08
title: GTEX-PLZ5-0626-SM-2I5F8

description: Sample ID: GTEX-PLZ5-0626-SM-2I5F8
DOI: 10.25491/6m59-5r71
title: GTEX-ZUA1-0011-R11b-SM-51MTI

description: Sample ID: GTEX-ZUA1-0011-R11b-SM-51MTI
DOI: 10.25491/7t5a-3s93
title: GTEX-PLZ5-0826-SM-4E3JR

description: Sample ID: GTEX-PLZ5-0826-SM-4E3JR
DOI: 10.25491/7tyv-6319
title: GTEX-RU72-0011-R6A-SM-2TF71

description: Sample ID: GTEX-RU72-0011-R6A-SM-2TF71
DOI: 10.25491/7x1h-ds57
title: GTEX-YEC4-1226-SM-5CVLX

description: Sample ID: GTEX-YEC4-1226-SM-5CVLX
DOI: 10.25491/7xjt-pm26
title: GTEX-PLZ5-0826-SM-3P5ZW

description: Sample ID: GTEX-PLZ5-0826-SM-3P5ZW
DOI: 10.25491/89pz-mx60
title: GTEX-X62O-0126-SM-4E3JN

description: Sample ID: GTEX-X62O-0126-SM-4E3JN
DOI: 10.25491/9pn5-ch41
title: GTEX-PLZ5-0426-SM-3P612

description: Sample ID: GTEX-PLZ5-0426-SM-3P612
DOI: 10.25491/9qqa-3e97
title: GTEX-ZUA1-0011-R7b-SM-4YCDP

description: Sample ID: GTEX-ZUA1-0011-R7b-SM-4YCDP
DOI: 10.25491/acmb-bh73
title: GTEX-X5EB-2326-SM-46MW5

description: Sample ID: GTEX-X5EB-2326-SM-46MW5
DOI: 10.25491/asmg-s840
title: GTEX-ZUA1-0226-SM-5NQ9Q

description: Sample ID: GTEX-ZUA1-0226-SM-5NQ9Q
DOI: 10.25491/bbt8-ka63
title: GTEX-YEC4-1526-SM-4W1YU

description: Sample ID: GTEX-YEC4-1526-SM-4W1YU
DOI: 10.25491/bxkb-nv87
title: GTEX-UPJH-0826-SM-4WKFD

description: Sample ID: GTEX-UPJH-0826-SM-4WKFD
DOI: 10.25491/cjps-q305
title: GTEX-UPK5-0226-SM-3GAEV

description: Sample ID: GTEX-UPK5-0226-SM-3GAEV
DOI: 10.25491/dq4n-rx05
title: GTEX-ZUA1-0011-R3a-SM-4YCEE

description: Sample ID: GTEX-ZUA1-0011-R3a-SM-4YCEE
DOI: 10.25491/ea5d-0v25
title: GTEX-X5EB-2626-SM-4E3HZ

description: Sample ID: GTEX-X5EB-2626-SM-4E3HZ
DOI: 10.25491/fkqk-2h95
title: GTEX-X5EB-2426-SM-4E3HX

description: Sample ID: GTEX-X5EB-2426-SM-4E3HX
DOI: 10.25491/h4kt-hw76
title: GTEX-RU72-0011-R7A-SM-2TF5U

description: Sample ID: GTEX-RU72-0011-R7A-SM-2TF5U
DOI: 10.25491/hsym-jw04
title: GTEX-YEC4-1026-101814-SM-5P9FX

description: Sample ID: GTEX-YEC4-1026-101814-SM-5P9FX
DOI: 10.25491/hzqc-1h54
title: GTEX-YEC4-1026-SM-5P9FW

description: Sample ID: GTEX-YEC4-1026-SM-5P9FW
DOI: 10.25491/j2h8-9f47
title: GTEX-RU72-0226-SM-46MUD

description: Sample ID: GTEX-RU72-0226-SM-46MUD
DOI: 10.25491/jxkw-2g08
title: GTEX-ZUA1-0011-R6b-SM-4YCDD

description: Sample ID: GTEX-ZUA1-0011-R6b-SM-4YCDD
DOI: 10.25491/jxt1-sf33
title: GTEX-UPK5-0003-SM-3NMDI

description: Sample ID: GTEX-UPK5-0003-SM-3NMDI
DOI: 10.25491/k3fd-d039
title: GTEX-RU72-0011-R8A-SM-2TF61

description: Sample ID: GTEX-RU72-0011-R8A-SM-2TF61
DOI: 10.25491/kd9w-6y15
title: GTEX-PLZ5-0006-SM-2S1NZ

description: Sample ID: GTEX-PLZ5-0006-SM-2S1NZ
DOI: 10.25491/m1ct-ya31
title: GTEX-UPK5-0126-SM-3GADM

description: Sample ID: GTEX-UPK5-0126-SM-3GADM
DOI: 10.25491/psq2-c904
title: GTEX-UPK5-0326-SM-3GAF3

description: Sample ID: GTEX-UPK5-0326-SM-3GAF3
DOI: 10.25491/q2r3-yx80
title: GTEX-ZUA1-0011-R5b-SM-51MTG

description: Sample ID: GTEX-ZUA1-0011-R5b-SM-51MTG
DOI: 10.25491/q9k4-h372
title: GTEX-RU72-0526-SM-2TF5Z

description: Sample ID: GTEX-RU72-0526-SM-2TF5Z
DOI: 10.25491/qrh7-gn26
title: GTEX-X5EB-2226-SM-46MW4

description: Sample ID: GTEX-X5EB-2226-SM-46MW4
DOI: 10.25491/r39w-v821
title: GTEX-YEC4-0926-SM-5PNXY

description: Sample ID: GTEX-YEC4-0926-SM-5PNXY
DOI: 10.25491/r9ag-2v83
title: GTEX-PLZ5-0326-SM-3P614

description: Sample ID: GTEX-PLZ5-0326-SM-3P614
DOI: 10.25491/t4tt-a488
title: GTEX-ZUA1-0008-SM-4YCEW

description: Sample ID: GTEX-ZUA1-0008-SM-4YCEW
DOI: 10.25491/t9km-0594
title: GTEX-PLZ5-0006-SM-5S2W5

description: Sample ID: GTEX-PLZ5-0006-SM-5S2W5
DOI: 10.25491/vtcm-1x24
title: GTEX-UPK5-0006-SM-3GAD8

description: Sample ID: GTEX-UPK5-0006-SM-3GAD8
DOI: 10.25491/xhsc-7e16
title: GTEX-X62O-0226-SM-4E3JB

description: Sample ID: GTEX-X62O-0226-SM-4E3JB
DOI: 10.25491/xqgt-qv41
title: GTEX-UPJH-0626-SM-4IHJN

description: Sample ID: GTEX-UPJH-0626-SM-4IHJN
DOI: 10.25491/xzz3-cr66
title: GTEX-X62O-0826-SM-46MW8

description: Sample ID: GTEX-X62O-0826-SM-46MW8
DOI: 10.25491/y67a-gw24
title: GTEX-PLZ4-2826-SM-3P617

description: Sample ID: GTEX-PLZ4-2826-SM-3P617
DOI: 10.25491/y9x3-0h78
title: GTEX-RU72-0011-R9A-SM-2TF67

description: Sample ID: GTEX-RU72-0011-R9A-SM-2TF67
DOI: 10.25491/yk5d-r646
title: GTEX-X62O-0008-SM-46MU5

description: Sample ID: GTEX-X62O-0008-SM-46MU5
DOI: 10.25491/ym5j-yw31
title: GTEX-UPJH-0926-SM-4IHKA

description: Sample ID: GTEX-UPJH-0926-SM-4IHKA
DOI: 10.25491/yrb8-6a90
title: GTEX-YEC4-0626-SM-5CVLU

description: Sample ID: GTEX-YEC4-0626-SM-5CVLU
DOI: 10.25549/uschist-dt-m176960
title: The Daily Southern Californian, Vol. 10, No. 3, February 13, 1913

description: The Daily Southern Californian, Vol. 10, No. 3, February 13, 1913.
DOI: 10.25549/uschist-dt-m183727
title: The Daily Southern Californian, Vol. 4, No. 36, April 21, 1914

description: The Daily Southern Californian, Vol. 4, No. 36, April 21, 1914.
DOI: 10.25549/uschist-dt-m185031
title: Daily Trojan, Vol. 36, No. 17, November 30, 1944

description: Daily Trojan, Vol. 36, No. 17, November 30, 1944.
DOI: 10.25549/uschist-dt-m187059
title: Daily Trojan, Vol. 26, No. 20, October 18, 1934

description: Daily Trojan, Vol. 26, No. 20, October 18, 1934.
DOI: 10.25549/uschist-dt-m190311
title: Daily Trojan, Vol. 90, No. 52, April 30, 1981

description: Daily Trojan, Vol. 90, No. 52, April 30, 1981.
DOI: 10.25919/5bb0fb907a7b7
title: Parkes observations for project P914 semester 2016OCTS

description: Murchison Widefield Array (MWA) observations have led to the discovery of bright, point sources that have steep spectral indices and no optical or infrared counterparts.  A sample of these sources were observed last semester using the Australia Telescope Compact Array providing measurements (or constraints) on the spectral indices of these sources and, for the detected sources, accurate positions.  Here, we propose to use the Parkes telescope to confirm whether or not these sources are pulsars.  We obtained some time for this project last semester at 700 MHz. Here we refocus the proposal on a smaller sample of objects at a wavelength of 20 cm.