IQ Eri: a cataclysmic in outburst
Observed: 27, 28 Dec 2008
Michel Bonnardeau
28 Dec 2008
Updated 29, 31 Dec 2008
Abstract
Time series for this cataclysmic variable in outburst are presented.
Introduction
IQ Eri (=1RXS J025538.2-224655) was detected in outburst by Monard (2008).
This is the first outburst since the discovery of
this cataclysmic system in 2002.
Observations
The observations were carried out with a 203mm f/6.3 SC telescope, a
Clear filter and a SBIG ST7E camera (KAF401E CCD). 361 images were obtained,
each with an exposure duration of 60s.
For the differential photometry, the comparison star is GSC 6437-00137
with an assumed unfiltered magnitude of 11.8. The check star is GSC 6437-00013
with a measured average magnitude of 13.063, an average 1-sigma statistical
uncertainty of 0.027 and a standard deviation of 0.040.
The resulting light curves:
Session 27 Dec 2008
Red: IQ Eri, blue: the check star shifted by +0.3mag. The error bars
are +/- the 1-sigma statistical uncertainties. The average 1-sigma statistical uncertainty
of the check star is 0.027, the standard deviation 0.037.
It looks like there is a pulsation with a period around 18mn, but this
is not confirmed the night that follows.
IQ Eri is low over my horizon (it is at DEC=-22° and I am at 45°N).
However the sky was fairly good:
The photometry zero point as a function of the airmass.
The blue dot line is a linear fit, the green line is 0.1mag below.
There are a few measurements that are not too good (below the green line)
but I did not filter out any data.
Red: the air mass, blue: the photometry zero point
shifted by -20 mag.
Session 28 Dec 2008
The average 1-sigma statistical uncertainty of the K is 0.027, the
SD is 0.042.
3 images were discarded because of the extra losses (much below the
green line).
Reference
Monard L.A.G. (2008) IAU CBET 1633.
Technical notes
Telescope and camera configuration.
Computer and software configuration.
Data processing.