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Milagro constraints on very high energy emission from short-duration gamma-ray bursts

Title: Milagro constraints on very high energy emission from short-duration gamma-ray bursts
Authors: Abdo, AA; Allen, BT; Berley, D; Blaufuss, E; Casanova, S; Dingus, BL; Ellsworth, RW; Gonzalez, MM; Goodman, JA; Hays, E; Hoffman, CM; Kolterman, BE; Lansdell, CP; Linnemann, JT; Mcenery, JE; Mincer, AI; Nemethy, P; Noyes, D; Ryan, JM; Samuelson, FW; Saz Parkinson, PM; Shoup, A; Sinnis, G; Smith, AJ; Sullivan, GW; Vasileiou, V; Walker, GP; Williams, DA; Xu, XW; Yodh, GB
Publisher Information: //iopscience.iop.org/2041-8205; United Kingdom
Publication Year: 2007
Collection: University of Hong Kong: HKU Scholars Hub
Subject Terms: Gamma Rays: Bursts; Gamma Rays: Observations
Description: Recent rapid localizations of short, hard gamma-ray bursts (GRBs) by the Swift and HETE satellites have led to the observation of the first afterglows and the measurement of the first redshifts from this type of burst (Fox et al. 2005; Gehrels et al. 2005; Villasenor et al. 2005; Berger et al. 2005; Barthelmy et al. 2005). Detection of >100 GeV counterparts would place powerful constraints on GRB mechanisms. Seventeen short-duration (100 GeV counterparts to these GRBs and find no significant emission correlated with these bursts. Due to the absorption of high-energy gamma rays by the extragalactic background light (EBL), detections are only expected for redshifts less than ∼0.5. While most long-duration GRBs occur at redshifts higher than 0.5, the opposite is thought to be true of short GRBs. Lack of a detected VHE signal thus allows setting meaningful fluence limits. One GRB in the sample (050509b) has a likely association with a galaxy at a redshift of 0.225, while another (051103) has been tentatively linked to the nearby galaxy M81. Fluence limits are corrected for EBL absorption, either using the known measured redshift, or computing the corresponding absorption for a redshift of 0.1 and 0.5, as well as for the case of z = 0. © 2007. The American Astronomical Society. All rights reserved. ; link_to_subscribed_fulltext
Document Type: article in journal/newspaper
Language: English
Relation: Astrophysical Journal Letters; http://www.scopus.com/mlt/select.url?eid=2-s2.0-35348893257&selection=ref&src=s&origin=recordpage; 367; WOS:000249058600034; 1 I; 361; https://hub.hku.hk/handle/10722/188358; 666
DOI: 10.1086/519763
Availability: https://hub.hku.hk/handle/10722/188358; https://doi.org/10.1086/519763
Accession Number: edsbas.C190BFCE
Database: BASE