English   español  
Please use this identifier to cite or link to this item: http://hdl.handle.net/10261/213930
Share/Impact:
Statistics
logo share SHARE logo core CORE   Add this article to your Mendeley library MendeleyBASE

Visualizar otros formatos: MARC | Dublin Core | RDF | ORE | MODS | METS | DIDL | DATACITE
Exportar a otros formatos:

DC FieldValueLanguage
dc.contributor.authorHo, Anna Y. Q.-
dc.contributor.authorKulkarni, S. R.-
dc.contributor.authorNugent, Peter E.-
dc.contributor.authorZhao, Weijie-
dc.contributor.authorRusu, Florin-
dc.contributor.authorCenko, S. Bradley-
dc.contributor.authorRavi, Vikram-
dc.contributor.authorKasliwal, Mansi M.-
dc.contributor.authorPerley, Daniel A.-
dc.contributor.authorAdams, Scott M.-
dc.contributor.authorBellm, Eric C.-
dc.contributor.authorBrady, Patrick-
dc.contributor.authorFremling, Christoffer-
dc.contributor.authorGal-Yam, Avishay-
dc.contributor.authorKann, David Alexander-
dc.contributor.authorKaplan, David-
dc.contributor.authorLaher, Russ R.-
dc.contributor.authorMasci, Frank-
dc.contributor.authorOfek, Eran O.-
dc.contributor.authorSollerman, Jesper-
dc.contributor.authorUrban, Alex-
dc.date.accessioned2020-06-10T07:08:57Z-
dc.date.available2020-06-10T07:08:57Z-
dc.date.issued2018-
dc.identifierdoi: 10.3847/2041-8213/aaaa62-
dc.identifierissn: 2041-8213-
dc.identifier.citationThe Astrophysical Journal Letters 854(1): L13 (2018)-
dc.identifier.urihttp://hdl.handle.net/10261/213930-
dc.description.abstractThere has been speculation about a class of relativistic explosions with an initial Lorentz factor Γ smaller than that of classical gamma-ray bursts (GRBs). These >dirty fireballs> would lack prompt GRB emission but could be pursued via their optical afterglow, appearing as transients that fade overnight. Here we report a search for such transients (that fade by 5-σ in magnitude overnight) in four years of archival photometric data from the intermediate Palomar Transient Factory (iPTF). Our search criteria yielded 50 candidates. Of these, two were afterglows to GRBs that had been found in dedicated follow-up observations to triggers from the Fermi GRB Monitor. Another (iPTF14yb) was a GRB afterglow discovered serendipitously. Eight were spurious artifacts of reference image subtraction, and one was an asteroid. The remaining 38 candidates have red stellar counterparts in external catalogs. The photometric and spectroscopic properties of the counterparts identify these transients as strong flares from M dwarfs of spectral type M3-M7 at distances of d ≈ 0.15-2.1 kpc; three counterparts were already spectroscopically classified as late-type M stars. With iPTF14yb as the only confirmed relativistic outflow discovered independently of a high-energy trigger, we constrain the all-sky rate of transients that peak at m = 18 and fade by Δm = 2 mag in Δt = 3 hr to be , with a 68% confidence interval of . This implies that the rate of visible dirty fireballs is at most comparable to that of the known population of long-duration GRBs.© 2018. The American Astronomical Society. All rights reserved..-
dc.description.sponsorshipA.Y.Q.H. was supported by a National Science Foundation Graduate Research Fellowship under grant No. DGE1144469. D.A.K. acknowledges support from from the Spanish research project AYA 2014-58381-P and the Juan de la Cierva Incorporacion fellowship IJCI-2015-261. This work was supported by the GROWTH project funded by the National Science Foundation under PIRE grant No. 1545949. The Intermediate Palomar Transient Factory project is a scientific collaboration among the California Institute of Technology, Los Alamos National Laboratory, the University of Wisconsin, Milwaukee, the Oskar Klein Center, the Weizmann Institute of Science, the TANGO Program of the University System of Taiwan, and the Kavli Institute for the Physics and Mathematics of the Universe. This research made use of Astropy, a community-developed core Python package for Astronomy (Astropy Collaboration et al. 2013).-
dc.languageeng-
dc.relationMINECO/ICTI2013-2016/AYA 2014-58381-P-
dc.relationMINECO/ICTI2013-2016/IJCI-2015-261-
dc.relation.isversionofPostprint-
dc.rightsopenAccess-
dc.subjectCatalogs-
dc.subjectCamma-ray burst: general-
dc.subjectStars: activity-
dc.subjectStars: flare-
dc.subjectStars: jets-
dc.subjectSurveys-
dc.titleIPTF Archival Search for Fast Optical Transients-
dc.typeartículo-
dc.identifier.doihttp://dx.doi.org/10.3847/2041-8213/aaaa62-
dc.relation.publisherversionhttp://dx.doi.org/10.3847/2041-8213/aaaa62-
dc.date.updated2020-06-10T07:08:57Z-
dc.contributor.funderNational Science Foundation (US)-
dc.contributor.funderMinisterio de Economía y Competitividad (España)-
dc.contributor.funderEuropean Commission-
dc.relation.csic-
dc.identifier.funderhttp://dx.doi.org/10.13039/100000001es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100003329es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100000780es_ES
Appears in Collections:(IAA) Artículos
Files in This Item:
File Description SizeFormat 
IAA_2018_ApJL_iPTF_Archival.pdf349,84 kBAdobe PDFThumbnail
View/Open
Show simple item record
 


WARNING: Items in Digital.CSIC are protected by copyright, with all rights reserved, unless otherwise indicated.