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The following is a GCN Circular circulated via the AAVSO network.
For an archive and more information on circulars visit:
http://lheawww.gsfc.nasa.gov/docs/gamcosray/legr/bacodine/gcn3_archive.html
TITLE: GCN CIRCULAR
NUMBER: 7657
SUBJECT: GRB 080430 optical observations
DATE: 08/05/01 16:35:47 GMT
FROM: AAVSO GRB Network at AAVSO <matthewt_at_aavso.org>
Arto Oksanen (Muurame, Finland) and Veli-Pekka Hentunen (Varkaus, Finland)
report to the AAVSO High Energy Network the following optical observations
of GRB 080430 (Guidorzi et al., GCN Circular #7647):
Arto Oksanen (Hankasalmi Obs., Hankasalmi, Finland) reports the detection
of the optical counterpart of GRB 080430. Unfiltered observations were
made using a 0.4-meter RC telescope with an SBIG STL-1001E CCD. The
initial Swift XRT position was observed unfiltered with an initial set of
10 60-second exposures having a mid-point time of 2008 April 30, 20:08:54
UT; the afterglow was detected with a magnitude of 18.1 +/- 0.05
calibrated relative to GSC 3450-0639. Astrometry of the initial frames
yields a position of RA 11:01:14.76 , Dec +51:41:08.9 (USNOA2.0 ref, +/-
0.4 arcseconds), which is within the stated uncertainties of the UVOT
position (GCNCirc #7647).
Images taken between April 30.839 and April 30.969 UT were reanalyzed and
calibrated relative to two USNO-B1.0 stars of magnitude ~16.5. Photometry
of combined frames yields a smoothly decaying light curve during the span
of observations:
obs midpoint CR error
2008 April 30.839 17.798 0.088
2008 April 30.849 18.329 0.120
2008 April 30.860 18.484 0.087
2008 April 30.875 18.751 0.076
2008 April 30.893 18.868 0.055
2008 April 30.911 18.956 0.052
2008 April 30.929 19.044 0.067
2008 April 30.949 19.012 0.064
2008 April 30.969 19.156 0.076
A detailed report of the initial observations is available at the
following URL:
ftp://ftp.aavso.org/grb/A.Oksanen_GRB080430_2454587.38588_.txt
A FITS image of this observation is available at the following URL:
ftp://ftp.aavso.org/grb/A.Oksanen_GRB080430_2454587.38588_.fits
Markku Nissinen and Veli-Pekka Hentunen (Taurus Hill Observatory, Varkaus,
Finland) also report the detection of the optical afterglow of GRB 080430.
Observations were made using a Meade LX-200 0.3-meter telescope with an
SBIG ST8-XME CCD; observations were made using both clear and R filters.
A total of six 600-second exposures were obtained having an average
midpoint time of 2008 April 30.943. Photometry of the combined clear and
Rc frames yields magnitudes of CR=19.2+/-0.3 and R=19.5+/-0.5 calibrated
relative to the GSC2.3 star N7JI005540. The observers noted the sky was
not completely dark due to their high latitude and time of year.
The AAVSO thanks the Curry Foundation for their continued support of the
AAVSO International High Energy Network.
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