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A&A 431, 1189-1201 (2005)
DOI: 10.1051/0004-6361:20041684
Variable stars in the dwarf irregular galaxy NGC 6822: The photometric catalogue
L. Baldacci1, 2, L. Rizzi3, 4, G. Clementini1 and E. V. Held31 INAF - Osservatorio Astronomico di Bologna, via Ranzani 1, 40127 Bologna, Italy
e-mail: [lara.baldacci;gisella.clementini]@bo.astro.it
2 Dipartimento di Astronomia, Università di Bologna, via Ranzani 1, 40127 Bologna, Italy
3 INAF - Osservatorio Astronomico di Padova, vicolo dell'Osservatorio 5, 35122 Padova, Italy
e-mail: held@pd.astro.it
4 Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822, USA
e-mail: rizzi@ifa.hawaii.edu (Present address)
(Received 17 July 2004/ Accepted 19 October 2004 )
Abstract
Deep
B,
V time-series photometry obtained with the ESO Very Large Telescope
has been used to identify variable stars in the dwarf irregular galaxy
NGC 6822
.
We surveyed a
arcmin area
of the galaxy and detected a total number of 390 candidate variables
with the optimal image subtraction technique (Alard 2000, A&AS, 144, 363).
Light curves on a magnitude scale were obtained for 262 of these
variables. Differential flux light curves are available for the
remaining sample. In this paper we present the photometric catalogue
of calibrated light curves and time-series data, along with
coordinates and classification of the candidate variables. A
detailed description is provided of the procedures used to identify
the variable stars and calibrate their differential flux light curves
on a magnitude scale.
Key words: galaxies: individual: NGC 6822 -- galaxies: dwarf -- galaxies: irregular -- stars: variables: general -- galaxies: Local Group -- stars: variables: RR Lyr
SIMBAD Objects
Tables at the CDS
© ESO 2005
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