GRB 971227 follow-up work

S. G. Djorgovski, S. R. Kulkarni, A. N. Ramaprakash, (Caltech), and D. Frail (NRAO), on behalf of the Caltech GRB collaboration

Please cite the appropriate GCN messages as needed.


This is the Keck R-band image from UT Dec 30.8, field size = 218 arcsec, centered on the position of the X-ray source 1SAX J1257.3+5924. The center coordinates (J2000) are:

RA = 12 h 57 m 15.0 s

DEC = +59 d 24 ' 02 "

The limiting magnitude is R ~ 25.5.


This image is available in Postscript , and GIF formats.



This is a zoom-in on the same image, field size = 109 arcsec, centered on the position of a detection claimed by Castro-Tirado et al. (IAUC 6800). The center coordinates (J2000) are:

RA = 12 h 57 m 10.6 s

DEC = +59 d 24 ' 43 "


This image is available in Postscript , and GIF formats.



The marked objects have positions (good to 0.4 arcsec, on the basis of USNO A1.0 catalog) and magnitudes (good to 0.2-0.5? mag zero-point, on the basis of APM catalog):

Star A: RA = 12 h 57 m 13.68 s, DEC = +59 h 23 ' 36.7 ", R = 19.1 mag

Star B: RA = 12 h 57 m 11.15 s, DEC = +59 h 24 ' 45.4 ", R = 22.1 mag

Galaxy C: RA = 12 h 57 m 08.74 s, DEC = +59 h 24 ' 35.7 ", R = 20.6 mag

Star D: RA = 12 h 57 m 04.95 s, DEC = +59 h 24 ' 39.2 ", R = 19.4 mag

Galaxy E: RA = 12 h 57 m 08.22 s, DEC = +59 h 24 ' 52.4 ", R = 21.4 mag

Galaxy F: RA = 12 h 57 m 08.30 s, DEC = +59 h 25 ' 00.5 ", R = 21.25 mag

D is the comparison star mentioned by Galama et al. (GCN 31Dec97), and galaxy C is almost certainly the object they propose as the possible identification of the claimed detection by Castro-Tirado et al.


This is the DSS image, 6 arcmin square:


Work on other GRBs