@article{35aada4ee1db43e1920a4d036e772538,
title = "BIMA observations of gamma-ray bursters GRB 970111 and GRB 970228",
abstract = "The Satellite per Astronomia X (BeppoSAX) is successfully producing small error boxes to gamma-ray bursts, permitting rapid follow-up multiwavelength searches for fading and quiescent counterparts. For GRB 970228 this led to the discovery of the first convincing fading counterpart. However, no counterpart was found for GRB 970111. In this Letter, we present our observations approximately 1 week after GRB 970228 and 1 month after GRB 970111 using the Berkeley-Illinois-Maryland Association (BIMA) array at 3.5 mm. No fading millimeter-wave sources were detected, but we demonstrate that BIMA is well suited for performing future searches.",
keywords = "Gamma rays: bursts, Radio continuum: general",
author = "Smith, {I. A.} and Gruendl, {R. A.} and Liang, {E. P.} and Lo, {K. Y.}",
note = "Funding Information: The BIMA Hat Creek Interferometer is operated under a joint agreement between the University of California, Berkeley, the University of Illinois, and the University of Maryland with support from the NSF: we are particularly grateful to the directors for granting us the Target of Opportunity time. We would like to thank Dale Frail for providing us with radio information and Kevin Hurley for the smaller gamma-ray error box to GRB 970111 than was available in the IAU Circulars at the time of our observations. We are also grateful to Rene Hudec for making several helpful suggestions. This work was supported by NASA grants NAG 5-1515 and NAG 5-3824 at Rice University. Research at the Laboratory for Astronomical Imaging is supported by NSF grants AST9320239 and AST9613999 and by the University of Illinois.",
year = "1997",
doi = "10.1086/310861",
language = "English (US)",
volume = "487",
pages = "L5--L7",
journal = "Astrophysical Journal",
issn = "0004-637X",
publisher = "American Astronomical Society",
number = "1 PART II",
}