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LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00005006naa a2200565 4500
001oai:research.chalmers.se:791749ad-d2de-480b-9dc6-fe1e19b0b1de
003SwePub
008180906s2018 | |||||||||||000 ||eng|
024a https://doi.org/10.3847/1538-4357/aad2d72 DOI
024a https://research.chalmers.se/publication/5048312 URI
040 a (SwePub)cth
041 a engb eng
042 9 SwePub
072 7a art2 swepub-publicationtype
072 7a ref2 swepub-contenttype
100a Anderson, Marin M.u California Institute of Technology (Caltech)4 aut
2451 0a Simultaneous Search for Prompt Radio Emission Associated with the Short GRB 170112A Using the All-sky Imaging Capability of the OVRO-LWA
264 c 2018-08-27
264 1b American Astronomical Society,c 2018
338 a electronic2 rdacarrier
520 a We have conducted the most sensitive low-frequency (below 100 MHz) search to date for prompt, low-frequency radio emission associated with short-duration gamma-ray bursts (GRBs), using the Owens Valley Radio Observatory Long Wavelength Array (OVRO-LWA). The OVRO-LWA's nearly full-hemisphere field of view (similar to 20,000 square degrees) allows us to search for low-frequency (sub-100 MHz) counterparts for a large sample of the subset of GRB events for which prompt radio emission has been predicted. Following the detection of short GRB 170112A by Swift, we used all-sky OVRO-LWA images spanning one hour prior to and two hours following the GRB event to search for a transient source coincident with the position of GRB 170112A. We detect no transient source to within a 3 sigma flux density limit of 4.5. Jy at 13 s timescales for frequencies spanning 27-84. MHz. We place constraints on a number of models predicting prompt, low-frequency radio emission accompanying short GRBs and their potential binary neutron star merger progenitors, and place an upper limit of L-radio/L gamma less than or similar to 3.5 x 10(-6) on the fraction of energy released in the prompt radio emission, under the assumptions of negligible scattering of the radio pulse and beaming of emission along the line of sight. These observations serve as a pilot effort for a program targeting a wider sample of both short and long GRBs with the OVRO-LWA, including bursts with confirmed redshift measurements that are critical to placing constraining limits on prompt radio emission models, as well as a program for the follow-up of gravitational wave compact binary coalescence events detected by advanced LIGO and Virgo.
650 7a NATURVETENSKAPx Fysikx Subatomär fysik0 (SwePub)103012 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Subatomic Physics0 (SwePub)103012 hsv//eng
650 7a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng
650 7a NATURVETENSKAPx Fysikx Atom- och molekylfysik och optik0 (SwePub)103022 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Atom and Molecular Physics and Optics0 (SwePub)103022 hsv//eng
653 a radiation mechanisms: non-thermal
653 a radio continuum: general
653 a gamma-ray burst: general
653 a gravitational waves
653 a gamma-ray burst: individual (170112A)
700a Hallinan, Greggu California Institute of Technology (Caltech)4 aut
700a Eastwood, Michael W.u California Institute of Technology (Caltech)4 aut
700a Monroe, Ryan M.u California Institute of Technology (Caltech)4 aut
700a Vedantham, Harish K.u California Institute of Technology (Caltech)4 aut
700a Bourke, Stephen,d 1978u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)bourke
700a Greenhill, Lincoln J.u Harvard-Smithsonian Center for Astrophysics4 aut
700a Kocz, Jonathonu California Institute of Technology (Caltech)4 aut
700a Lazio, T. Joseph W.u California Institute of Technology (Caltech)4 aut
700a Price, Danny C.u Swinburne University of Technology,Harvard-Smithsonian Center for Astrophysics4 aut
700a Schinzel, Frank K.u University of New Mexico,National Radio Astronomy Observatory4 aut
700a Wang, Yuankunu California Institute of Technology (Caltech)4 aut
700a Woody, David P.u California Institute of Technology (Caltech)4 aut
710a California Institute of Technology (Caltech)b Chalmers tekniska högskola4 org
773t Astrophysical Journald : American Astronomical Societyg 864:1q 864:1x 1538-4357x 0004-637X
856u https://research.chalmers.se/publication/504831/file/504831_Fulltext.pdfx primaryx freey FULLTEXT
856u https://research.chalmers.se/publication/504831/file/504831_Fulltext.pdf
8564 8u https://doi.org/10.3847/1538-4357/aad2d7
8564 8u https://research.chalmers.se/publication/504831

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