Status Report

NASA Swift: GRB 060427: Swift detection of a burst

By SpaceRef Editor
April 30, 2006
Filed under , ,
NASA Swift: GRB 060427: Swift detection of a burst
http://images.spaceref.com/news/swift.jpg

TITLE: GCN GRB OBSERVATION REPORT
NUMBER: 5006
SUBJECT: GRB 060427: Swift detection of a burst
DATE: 06/04/27 12:06:37 GMT
FROM: Scott Barthelmy at NASA/GSFC Scott@lheamail.gsfc.nasa.gov

V. Mangano (INAF-IASFPA), S. D. Barthelmy (GSFC), S. Campana (INAF-OAB), J. R. Cummings (NASA/ORAU), J. A. Kennea (PSU), H. A. Krimm (GSFC/USRA), F. E. Marshall (NASA/GSFC), K. L. Page (U Leicester), D. M. Palmer (LANL), P. Romano (INAF-OAB) and D. E. Vanden Berk (PSU) report on behalf of the Swift Team:

At 11:43:10 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRB 060427 (trigger=207281). Swift slewed immediately to the burst. The BAT on-board calculated location is RA,Dec 124.303, +62.617 {08h 17m 13s, +62d 37′ 02″} (J2000) with an uncertainty of 3 arcmin (radius, 90% containment, including systematic uncertainty). This was an image trigger so the TDRSS lightcurve does not show any significant activity.

The XRT began observing the field at 11:45:20 UT, 130 seconds after the BAT trigger. XRT found a fading, uncatalogued X-ray source located at RA(J2000) = 08h 17m 04.5s, Dec(J2000) = +62d 40′ 17.4″, with an estimated uncertainty of 5.4 arcseconds (90% confidence radius). This location is 204 arcseconds from the BAT on-board position, outside the BAT error circle. The initial flux in the 2.5s image was 9.6e-10 erg/cm2/s (0.2-10 keV).

UVOT took a finding chart exposure of 400 seconds with the V filter starting 133 seconds after the BAT trigger. No afterglow candidate has been found in the initial data products. The 2.7’x2.7′ sub-image covers 100% of the XRT error circle. The typical 3-sigma upper limit has been about 18.5 mag. The 8’x8′ region for the list of sources generated on-board covers 100% of the XRT error circle. The list of sources has an upper limit of 19.2 mag. No correction has been made for the expected extinction of about 0.2 magnitudes.

SpaceRef staff editor.