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LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00004987naa a2200721 4500
001oai:DiVA.org:su-198241
003SwePub
008211104s2021 | |||||||||||000 ||eng|
024a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-1982412 URI
024a https://doi.org/10.3847/1538-4357/ac0bc72 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 Fast-transient Searches in Real Time with ZTFReST :b Identification of Three Optically Discovered Gamma-Ray Burst Afterglows and New Constraints on the Kilonova Rate
264 c 2021-09-08
264 1b American Astronomical Society,c 2021
338 a print2 rdacarrier
520 a The most common way to discover extragalactic fast transients, which fade within a few nights in the optical, is via follow-up of gamma-ray burst and gravitational-wave triggers. However, wide-field surveys have the potential to identify rapidly fading transients independently of such external triggers. The volumetric survey speed of the Zwicky Transient Facility (ZTF) makes it sensitive to objects as faint and fast fading as kilonovae, the optical counterparts to binary neutron star mergers, out to almost 200 Mpc. We introduce an open-source software infrastructure, the ZTF REaltime Search and Triggering, ZTFReST, designed to identify kilonovae and fast transients in ZTF data. Using the ZTF alert stream combined with forced point-spread-function photometry, we have implemented automated candidate ranking based on their photometric evolution and fitting to kilonova models. Automated triggering, with a human in the loop for monitoring, of follow-up systems has also been implemented. In 13 months of science validation, we found several extragalactic fast transients independently of any external trigger, including two supernovae with post-shock cooling emission, two known afterglows with an associated gamma-ray burst (ZTF20abbiixp, ZTF20abwysqy), two known afterglows without any known gamma-ray counterpart (ZTF20aajnksq, ZTF21aaeyldq), and three new fast-declining sources (ZTF20abtxwfx, ZTF20acozryr, ZTF21aagwbjr) that are likely associated with GRB200817A, GRB201103B, and GRB210204A. However, we have not found any objects that appear to be kilonovae. We constrain the rate of GW170817-like kilonovae to R < 900 Gpc(-3) yr(-1) (95% confidence). A framework such as ZTFReST could become a prime tool for kilonova and fast-transient discovery with the Vera Rubin Observatory.
650 7a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng
700a Coughlin, Michael W.4 aut
700a Kool, Erik C.u Stockholms universitet,Oskar Klein-centrum för kosmopartikelfysik (OKC),Institutionen för astronomi4 aut0 (Swepub:su)erko1670
700a Kasliwal, Mansi M.4 aut
700a Kumar, Harsh4 aut
700a Bhalerao, Varun4 aut
700a Carracedo, Ana Saguésu Stockholms universitet,Oskar Klein-centrum för kosmopartikelfysik (OKC),Fysikum4 aut0 (Swepub:su)anca9835
700a Ho, Anna Y. Q.4 aut
700a Pang, Peter T. H.4 aut
700a Saraogi, Divita4 aut
700a Sharma, Kritti4 aut
700a Shenoy, Vedant4 aut
700a Burns, Eric4 aut
700a Ahumada, Tomás4 aut
700a Anand, Shreya4 aut
700a Singer, Leo P.4 aut
700a Perley, Daniel A.4 aut
700a De, Kishalay4 aut
700a Fremling, U. C.4 aut
700a Bellm, Eric C.4 aut
700a Bulla, Mattiau Stockholms universitet,Oskar Klein-centrum för kosmopartikelfysik (OKC),Institutionen för astronomi4 aut0 (Swepub:su)mbull
700a Crellin-Quick, Arien4 aut
700a Dietrich, Tim4 aut
700a Drake, Andrew4 aut
700a Duev, Dmitry A.4 aut
700a Goobar, Arielu Stockholms universitet,Oskar Klein-centrum för kosmopartikelfysik (OKC),Fysikum4 aut0 (Swepub:su)ariel
700a Graham, Matthew J.4 aut
700a Kaplan, David L.4 aut
700a Kulkarni, S. R.4 aut
700a Laher, Russ R.4 aut
700a Mahabal, Ashish A.4 aut
700a Shupe, David L.4 aut
700a Sollerman, Jesperu Stockholms universitet,Oskar Klein-centrum för kosmopartikelfysik (OKC),Institutionen för astronomi4 aut0 (Swepub:su)solle
700a Walters, Richard4 aut
700a Yao, Yuhan4 aut
710a Stockholms universitetb Oskar Klein-centrum för kosmopartikelfysik (OKC)4 org
773t Astrophysical Journald : American Astronomical Societyg 918:2q 918:2x 0004-637Xx 1538-4357
856u https://arxiv.org/abs/2104.06352y arXiv:2104.06352
856u http://arxiv.org/pdf/2104.06352
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-198241
8564 8u https://doi.org/10.3847/1538-4357/ac0bc7

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