Astrophotography by Anthony Ayiomamitis

Differential Photometry - Ursa Major

A variable star, as its name suggests, is a star whose magnitude varies intrinsically, in contrast to eclipsing binaries whose magnitude varies as a result of one star in the binary system eclipsing the other. True variables are one of five types, namely Mira stars, semiregular stars, cepheids, eruptive variables and, finally, cataclysmic variables. Minimum to maximum magnitude can range from days to many months with some variables displaying irregular periods.

A popular method for the study of variable stars, particularly short-term variables, is by the use of the technique known as "differential photometry". Rather than measure the (variable) magnitude of a variable star on an absolute scale, measurements are made over time relative to one or more non-variable star(s) and these differences are then plotted so as to study and illustrate the relative or differential change in magnitude. Due to the very large number of variables stars, the field of differential photometry represents one of the key fields in astronomy whereby the amateur astronomer can make a meaningful and long-lasting contribution to both science and astronomy.

More recently, the search for extrasolar planets (over 700 discovered so far) has identified yet another interesting application for the practice of differential photometry whereby the minute drops in magnitude of a star hosting an exoplanet are studied. Further details for the interested party are available here.

Note: The large-amplitude short-period pulsating star GSC 03832-0152 is a fast pulsating variable star with a period of 131.53 minutes and which involves a delta mag of 0.40 (R) magnitudes during this brief time interval. GSC 03832-00152 is a delta Scuti variable first reported by Wils et al in 2009 following identification while searching for RR Lyrae stars from the Northern Sky Variability Survey (NSVS; Wozniak et al., 2004). Further details from the International Variable Star Index are available here whereas an AAVSO finder chart is available here.

Image Details
Light Curve for GSC 03832-00152
Imaging Details
Variable Star:
GSC 3832-0152

Other Designation:
N/A

RA / Dec:
11h 48m 42s /
+54° 43' 07"


Magnitude:
11.7 - 12.1 (R)

Period:
0.09134218 days

Variability:
HADS

Comparison Star:
GSC 3832:0144

Check Star:
GSC 3832:0179


Date:
Jun 03-04, 2012
22:05 - 01:05 UT+3


Location:
Athens, Greece

Equipment:
AP 305/f3.8 Riccardi-Honders
AP 1200GTO GEM
SBIG ST-10XME
SBIG CFW10
SBIG LRGB filters


Integrations:
Lum :  147 x 60 sec
Dark :  010 x 60 sec
Flat :  ~ 22,400 ADU
Binning :  1x1

Temperatures:
Ambient : + 23.0 ° C
CCD Chip : - 15.0 ° C

Software:
CCDSoft V5.00.201
AIP4Win V2.4.0


Processing:
Reduction
Differential Photometry