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Sökning: onr:"swepub:oai:DiVA.org:su-173161" > GROWTH on S190510g :

LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00004326naa a2200673 4500
001oai:DiVA.org:su-173161
003SwePub
008190923s2019 | |||||||||||000 ||eng|
024a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-1731612 URI
024a https://doi.org/10.3847/2041-8213/ab33992 DOI
040 a (SwePub)su
041 a engb eng
042 9 SwePub
072 7a ref2 swepub-contenttype
072 7a art2 swepub-publicationtype
100a Andreoni, Igor4 aut
2451 0a GROWTH on S190510g :b DECam Observation Planning and Follow-up of a Distant Binary Neutron Star Merger Candidate
264 c 2019-08-09
264 1b American Astronomical Society,c 2019
338 a print2 rdacarrier
520 a The first two months of the third Advanced LIGO and Virgo observing run (2019 April-May) showed that distant gravitational-wave (GW) events can now be readily detected. Three candidate mergers containing neutron stars (NS) were reported in a span of 15 days, all likely located more than 100 Mpc away. However, distant events such as the three new NS mergers are likely to be coarsely localized, which highlights the importance of facilities and scheduling systems that enable deep observations over hundreds to thousands of square degrees to detect the electromagnetic counterparts. On 2019 May 10 02: 59:39.292 UT the GW candidate S190510g was discovered and initially classified as a binary neutron star (BNS) merger with 98% probability. The GW event was localized within an area of 3462 deg(2), later refined to 1166 deg(2) (90%) at a distance of 227 +/- 92 Mpc. We triggered Target-of-Opportunity observations with the Dark Energy Camera (DECam), a wide-field optical imager mounted at the prime focus of the 4 m Blanco Telescope at Cerro Tololo Inter-American Observatory in Chile. This Letter describes our DECam observations and our real-time analysis results, focusing in particular on the design and implementation of the observing strategy. Within 24 hr of the merger time, we observed 65% of the total enclosed probability of the final skymap with an observing efficiency of 94%. We identified and publicly announced 13 candidate counterparts. S190510g was reclassified 1.7 days after the merger, after our observations were completed, with a BNS merger probability reduced from 98% to 42% in favor of a terrestrial classification.
650 7a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng
653 a binaries: general
653 a gravitational waves
653 a methods: observational
653 a stars: neutron
653 a supernovae: general
700a Goldstein, Daniel A.4 aut
700a Anand, Shreya4 aut
700a Coughlin, Michael W.4 aut
700a Singer, Leo P.4 aut
700a Ahumada, Tomás4 aut
700a Medford, Michael4 aut
700a Kool, Erik C.u Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)erko1670
700a Webb, Sara4 aut
700a Bulla, Mattiau Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)mbull
700a Bloom, Joshua S.4 aut
700a Kasliwal, Mansi M.4 aut
700a Nugent, Peter E.4 aut
700a Bagdasaryan, Ashot4 aut
700a Barnes, Jennifer4 aut
700a Cook, David O.4 aut
700a Cooke, Jeff4 aut
700a Duev, Dmitry A.4 aut
700a Fremling, U. Christoffer4 aut
700a Gatkine, Pradip4 aut
700a Golkhou, V. Zach4 aut
700a Kong, Albert K. H.4 aut
700a Mahabal, Ashish4 aut
700a Martínez-Palomera, Jorge4 aut
700a Tao, Duo4 aut
700a Zhang, Keming4 aut
710a Stockholms universitetb Institutionen för astronomi4 org
773t Astrophysical Journal Lettersd : American Astronomical Societyg 881:1q 881:1x 2041-8205x 2041-8213
856u https://doi.org/10.3847/2041-8213/ab3399y Fulltext
856u https://authors.library.caltech.edu/96513/2/Andreoni_2019_ApJL_881_L16.pdf
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-173161
8564 8u https://doi.org/10.3847/2041-8213/ab3399

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