Possible Supernova in NGC7537
by Alain Klotz
1. Instrumental design
I observed about 300 galaxies by clear night since 1 feb 2000 with a fully
automatized LX200 telescope (8" diameter). The CCD is an Audine equiped
by an Kaf-401E chip (grade 0 quality). The camera has no shutter. An "unsmearing"
algorithm is used after the dark correction. The flat correction is not
performed. Each image is integrated 60 seconds with a binning 2x2 (sampling
is 4.4 arcsec/pixel). About 300 to 400 fields are recorded each night.
A quick visu software, named SNVisu, was created with the AudeLA platform.
It allows to see the night image (at left) and the reference image (at
right) on the same screen.
The screen copy below indicate the DATE-OBS of the images (UT). North is
up and East is left (no inversion).
Candidate : 2002-10-05T20:49:01.63
Reference : 2000-09-01T00:24:05.02
The possible supernova is located at about 8" N, 34" E from the nucleus
of the galaxy. The magnitude is estimated to 16.7. Bellow, the DSS image
The following image is a coadded 7x60sec images taken near 2002-10-06T20:06.
The image was zoomed 3 times.