J/ApJ/916/89     85 short GRB kilonovae opt. & NIR obs.      (Rastinejad+, 2021)

Probing kilonova ejecta properties using a catalog of short gamma-ray burst observations. Rastinejad J.C., Fong W., Kilpatrick C.D., Paterson K., Tanvir N.R., Levan A.J., Metzger B.D., Berger E., Chornock R., Cobb B.E., Laskar T., Milne P., Nugent A.E., Smith N. <Astrophys. J., 916, 89 (2021)> =2021ApJ...916...89R 2021ApJ...916...89R
ADC_Keywords: GRB; Redshifts; Photometry, ugriz; References Keywords: Gamma-ray bursts ; Neutron stars Abstract: The discovery of GW170817 and GRB 170817A in tandem with AT 2017gfo cemented the connection between neutron star mergers, short gamma-ray bursts (GRBs), and kilonovae. To investigate short GRB observations in the context of diverse kilonova behavior, we present a comprehensive optical and near-IR catalog of 85 bursts discovered over 2005-2020 on timescales of ≲12days. The sample includes previously unpublished observations of 23 bursts and encompasses both detections and deep upper limits. We identify 11.8% and 15.3% of short GRBs in our catalog with upper limits that probe luminosities lower than those of AT2017gfo and a fiducial neutron star-black hole kilonova model (for pole-on orientations), respectively. We quantify the ejecta masses allowed by the deepest limits in our catalog, constraining blue and "extremely blue" kilonova components of 14.1% of bursts to Mej≲0.01-0.1M. The sample of short GRBs is not particularly constraining for red kilonova components. Motivated by the large catalog, as well as model predictions of diverse kilonova behavior, we investigate modified search strategies for future follow-up to short GRBs. We find that ground-based optical and near-IR observations on timescales of ≳2days can play a significant role in constraining more diverse outcomes. We expect future short GRB follow-up efforts, such as from the James Webb Space Telescope, to expand the reach of kilonova detectability to redshifts of z∼1. Description: We present optical and NIR observations of 85 bursts discovered from 2005 to 2020 in an updated catalog of short GRB observations that probe kilonova emission properties. We primarily draw from short GRBs (T90≲2s or classified by the Swift Burst Alert Telescope (BAT) catalog; Lien+ 2016, J/ApJ/829/7) detected by BAT on board Swift. We draw optical and NIR observations from three sources: (i) unpublished observations that mainly comprise deep upper limits (Section 2.2), (ii) deep upper limits from GCN circulars (searched between 2013 and 2020) that have not been otherwise published in the literature (Section 2.3), and (iii) published observations (or reanalyses of published observations) of past short GRBs, some of which have also been included in previous samples (Section 2.4). Notably, this work introduces 55 unpublished observations and over 40 deep upper limits from GCNs. In total, we include observations of 85 bursts. We obtained new observations of 23 bursts with the 8m twin Gemini-North and Gemini-South telescopes, the 6.5m MMT, the 6.5m Magellan/Baade and Clay telescopes, the 4.2m William Herschel Telescope (WHT), and the 3.8m United Kingdom Infrared Telescope (UKIRT). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tablea1.dat 86 261 Catalog of short GRB kilonovae observations refs.dat 57 84 References -------------------------------------------------------------------------------- See also: I/284 : The USNO-B1.0 Catalog (Monet+ 2003) VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006) V/147 : The SDSS Photometric Catalogue, Release 12 (Alam+, 2015) J/MNRAS/397/1177 : Swift-XRT observations of GRBs (Evans+, 2009) J/ApJ/829/7 : 3rd Swift/BAT GRB catalog (past ∼11yrs) (BAT3) (Lien+, 2016) J/ApJ/848/L29 : Opt. follow-up of GW170817 counterpart (Diaz+, 2017) J/ApJ/848/L16 : Counterpart of GW170817. I. DECam (Soares-Santos+, 2017) J/ApJ/851/L21 : UV-NIR compilation of GW170817 counterpart (Villar+, 2017) J/ApJ/884/L55 : Opt. follow-up of gal. within S190814bv reg. (Gomez+, 2019) J/A+A/643/A113 : iz photometry of S190814bv ctp candidates (Ackley+, 2020) J/ApJ/890/131 : Follow-up of counterparts of S190814bv (Andreoni+, 2020) J/ApJ/896/L20 : Swift BAT gamma-ray burst durations (Jespersen+, 2020) Byte-by-byte Description of file: tablea1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 A7 --- Name GRB name 9- 11 A3 --- f_Name Flag on Name (1) 13- 18 F6.4 --- z [0.11/2.22] Known redshift or z=0.5 20 A1 --- f_z [d] Flag on z (2) 22- 44 A23 --- Tel Telescope and Instrument name 46- 51 F6.3 d dt [0.003/11.92] Time since burst 53- 57 A5 --- Band Filter/Band name 59- 62 F4.1 mag mag [20.8/27.7] 3-sigma limit or detection AB magnitude in Band 64- 67 F4.1 mag e_mag [0.1/0.6]? Error in mag 69- 71 F3.1 --- f_mag [0/1] Detection flag in mag; 1=Detection 73- 80 E8.2 10-7W nuLnu [1e+40/2.6e+44] Luminosity of observation; in erg/s 82- 86 A5 --- Ref Reference code(s) (see refs.dat file) -------------------------------------------------------------------------------- Note (1): Flag as follows: * = kilonova candidate; a = Burst does not have an X-ray afterglow found by Swift-XRT. b = Burst detected by INTEGRAL-IBIS/ISGRI, not detected by Swift-BAT. c = Burst detected by Fermi-GBM, Fermi-LAT and by Suzaku-WAM, not detected by Swift-BAT. d = Limit applies to partial coverage of BAT localization. e = We present a separate analysis of observations published in O'Connor+ 2021MNRAS.502.1279O 2021MNRAS.502.1279O (68) finding upper limits deeper by 0.2-0.3 magnitudes. Note (2): Flag as follows: d = Redshift unknown, z=0.5 taken as fiducial value in analysis, except for GRB 180418A which is assumed to be z=1.0 (c.f., Rouco Escorial+ 2021ApJ...912...95R 2021ApJ...912...95R). -------------------------------------------------------------------------------- Byte-by-byte Description of file: refs.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- Ref Reference code 4- 22 A19 --- BibCode Bibcode of the reference 24- 47 A24 --- Auth First author's name(s) 49- 57 A9 --- Comm Comment -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 30-Dec-2022
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