Radio and Optical Follow-up Observations and Improved Interplanetary Network Position of GRB 970111

, , , , , , , , , , , , , , and

©1997. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation T. J. Galama et al 1997 ApJ 486 L5 DOI 10.1086/310822

1538-4357/486/1/L5

Abstract

We report on Westerbork 840 MHz and 1.4 and 5 GHz radio observations of the improved Interplanetary Network Wide Field Camera (IPN WFC) error box of the γ-ray burst GRB 970111, between 26.4 hr and 120 days after the event onset. In the ~13 arcmin2 area defined by the IPN (BATSE and Ulysses) annulus and the published refined BeppoSAX WFC error box, we detected no steady sources brighter than 0.56 mJy (4 σ) and no varying radio emission, down to 1.0 mJy (4 σ). We also report on B-, V-, R-, and I-band observations of the error box with the 4.2 m William Herschel Telescope at La Palma.

Export citation and abstract BibTeX RIS

Please wait… references are loading.
10.1086/310822