Index of /noao/staff/mbrown/grb011121

[ICO]NameLast modifiedSizeDescription

[DIR]Parent Directory   -  
[IMG]grb011121.jpg 29-Nov-2001 16:54 197K 
[TXT]obj474_2.fits 26-Nov-2001 13:12 33M 
[TXT]obj475_2.fits 26-Nov-2001 13:13 33M 
[TXT]obj476_2.fits 26-Nov-2001 13:14 33M 
[TXT]obj477_2.fits 26-Nov-2001 13:15 33M 

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Acknowledgement
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The following images can not be used without permission and when permission
is granted Brown et al. (GCN 1158) must be cited.

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Images
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README this file
grb.jpg BRI composite (North up East left) 
obj474_2.fits 600 second R-band exposure (North right East up)
obj475_2.fits 600 second B-band exposure
obj476_2.fits 900 second U-band exposure
obj477_2.fits 300 second I-band exposure 

The GRB optical transient is located near pixels 1055, 2643 in the fits
images.

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Zeropoints
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1 ADU in image obj474_2 is equivalent to R magnitude 32.395 (airmass=0)
1 ADU in image obj475_2 is equivalent to B magnitude 31.836 (airmass=0)
1 ADU in image obj476_2 is equivalent to U magnitude 30.047 (airmass=0)
1 ADU in image obj477_2 is equivalent to I magnitude 30.814 (airmass=0)

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GCN 1158 Text
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M. Brown, R. Schommer, K. Olsen, B. Jannuzi, A. Dey (NOAO), A. Fruchter,
J. Rhoads (STSci) and the NOAO Deep Wide Field Survey Team. 

The GRB011121 optical transient (Wyrzykowski et al. GCN 1150) was imaged
with the CTIO Blanco 4m with Chip2 of Mosaic-II in UBRI between 7:32 and
8:21 23 Nov 2001 UT. 

Two objects within 2" of each other were detected near the position
reported in GCN 1150.  The brighter object (located at 11:34:29.66
-76:01:41.49 J2000) is the optical transient while the fainter object
(located at 11:34:30.15 -76:01:42.26 J2000) could be the host or a
companion galaxy.

Aperture photometry of the optical transient, candidate host/companion and
Star A from GCN 1150 is provided below. The photometry is in the
Johnson-Kron-Cousins system and has been calibrated with Landolt (1992)
standards from regions SA113 and SA95.  The photometry has been corrected
for atmospheric extinction (to airmass 0) but has not been corrected for
galactic extinction where the Schlegel et al. (1998) dust maps predict
dust reddening of E(B-V)=0.496 magnitudes. 

The 1" aperture photometry misses approximately 0.6 magnitudes of the total
flux while 3" aperture photometry of the candidate host/companion galaxy
suffers from contamination from the optical transient.  Star A is ~0.8
magnitudes fainter in R-band than originally reported in the USNO
catalogue (and GCN 1150) and estimates of the fading of the optical
transient should be corrected accordingly.

Object  Band  Seeing   UT       1" radius    2" radius     3" radius
              (arcsec) (23 Nov) ap. mag.     ap. mag       ap mag.

OT      U     1.95     7:59     23.6 +/- 0.2  22.4 +/- 0.1  22.1 +/- 0.1
OT      B     1.45     7:45     23.3 +/- 0.1  22.6 +/- 0.1  22.4 +/- 0.1
OT      R     1.45     7:32     21.8 +/- 0.1  21.1 +/- 0.1  20.8 +/- 0.1
OT      I     1.50     8:16     21.2 +/- 0.1  20.3 +/- 0.1  20.0 +/- 0.1

Host?   U     1.95     7:59     24.6 +/- 0.4  23.4 +/- 0.3  22.6 +/- 0.2
Host?   B     1.45     7:45     24.4 +/- 0.1  23.1 +/- 0.1  22.5 +/- 0.1
Host?   R     1.45     7:32     22.2 +/- 0.1  21.2 +/- 0.1  20.9 +/- 0.1
Host?   I     1.50     8:16     21.3 +/- 0.1  20.3 +/- 0.1  20.0 +/- 0.1

Star A  U     1.95     7:59     21.7 +/- 0.1  20.9 +/- 0.1  20.7 +/- 0.1
Star A  B     1.45     7:45     20.5 +/- 0.1  20.0 +/- 0.1  20.0 +/- 0.1
Star A  R     1.45     7:32     18.7 +/- 0.1  18.3 +/- 0.1  18.2 +/- 0.1
Star A  I     1.50     8:16     17.6 +/- 0.1  17.6 +/- 0.1  17.5 +/- 0.1

The reduced images are available from the 1st author upon request.

This message can be cited.