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Related papers: A Deep Wide-Field Variable Star Catalog of Omega C…

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We present a CCD survey of variable stars in the Draco dwarf spheroidal galaxy. This survey, which has the largest areal coverage since the original variable star survey by Baade & Swope, includes photometry for 270 RR Lyrae stars, 9…

An algorithm, based on Fourier decomposition of light curves, permitted to define a sample of 388 contact binaries with well observed light curves, periods shorter one day and with available V-I colors (the R-sample), from among 933…

Astrophysics · Physics 2009-10-28 Slavek M. Rucinski

We report the results of photometric monitoring of the Melotte 66 field in BVI filters. Ten variables were identified with nine being new discoveries. The sample includes eight eclipsing binaries of which four are W UMa type stars, one star…

Astrophysics · Physics 2009-11-13 K. Zloczewski , J. Kaluzny , W. Krzeminski , A. Olech , I. B. Thompson

We report the discovery of an optical counterpart to a quiescent neutron star in the globular cluster Omega Centauri (NGC 5139). The star was found as part of our wide-field imaging study of Omega Cen using the Advanced Camera for Surveys…

Time-series photometry of the CoRoT field SRa01 was carried out with the Berlin Exoplanet Search Telescope II (BEST II) in 2008/2009. A total of 1,161 variable stars were detected, of which 241 were previously known and 920 are newly found.…

We present a subset of the results of a three season, 124 night, near-infrared monitoring campaign of the dark clouds Lynds 1003 and Lynds 1004 in the Cygnus OB7 star forming region. In this paper, we focus on the field star population.…

Solar and Stellar Astrophysics · Physics 2013-02-08 Scott J. Wolk , Thomas S. Rice , Colin A. Aspin

The field of the globular cluster NGC 6362 was monitored between 1995 and 2009 in a search for variable stars. BV light curves were obtained for 69 periodic variables including 34 known RR Lyr stars, 10 known objects of other types and 25…

Solar and Stellar Astrophysics · Physics 2015-01-22 J. Kaluzny , I. B. Thompson , M. Rozyczka , W. Pych , W. Narloch

We present results of star variability analysis in OGLE II first bulge field. Photometric database was derived by means of image subtraction method (Wozniak 2000) and contains 4597 objects pre-classified as variables. We analyzed all the…

Astrophysics · Physics 2007-05-23 Tomasz Mizerski , Michal Bejger

A photometric survey of three Southern target fields with BEST II yielded the detection of 2,406 previously unknown variable stars and an additional 617 stars with suspected variability. This study presents a catalog including their…

New B, V, I photometry was obtained for a sample of 152 variables (125 RR Lyrae's, 4 anomalous Cepheids, 11 classical Cepheids, 11 eclipsing binaries and a delta Scuti star) in two regions near the bar of the Large Magellanic Cloud (LMC).…

Astrophysics · Physics 2007-05-23 M. Maio , G. Clementini , A. Bragaglia , E. Carretta , R. Gratton , L. Di Fabrizio

We present the results of a search for variable stars in the globular cluster NGC 5286, which has recently been suggested to be associated with the Canis Major dwarf spheroidal galaxy. 57 variable stars were detected, only 19 of which had…

We report 350 pulsating variable stars found in four DECam fields ($\sim 12$ sq. deg.) covering the Antlia 2 satellite galaxy. The sample of variables includes 318 RR Lyrae stars and eight anomalous Cepheids in the galaxy. Reclassification…

Astrophysics of Galaxies · Physics 2021-12-17 Kathy Vivas , Clara Martínez-Vázquez , Alistair Walker , Vasily Belokurov , Ting Li , Denis Erkal

We used archival multi-band Hubble Space Telescope observations obtained with the Wide-Field Camera 3 in the UV-optical channel to present new important observational findings on the color-magnitude diagram (CMD) of the Galactic globular…

Astrophysics of Galaxies · Physics 2015-05-19 Bellini A. , Bedin L. R. , Piotto G. , Milone A. P. , Marino A. F. , Villanova S.

We used the Aladin Virtual Obsrvatory tool and High Resolution Imager ROSAT archival data to search for X-ray variability in scale of days in 23 young stars in the sigma Orionis cluster and a background galaxy. Five stars displayed…

Solar and Stellar Astrophysics · Physics 2015-05-13 J. A. Caballero , J. Lopez-Santiago , E. de Castro , M. Cornide

We initiated digitization of the Moscow collection of astronomical plates using flatbed scanners. Techniques of photographic photometry of the digital images were applied, enabling an effective search for new variable stars. Our search for…

Astrophysics · Physics 2008-10-08 D. M. Kolesnikova , L. A. Sat , K. V. Sokolovsky , S. V. Antipin , N. N. Samus

We have conducted a three band (BVI) variability survey of the globular cluster M3. This is the first three band survey of the cluster using modern image subtraction techniques. Observations were made over 9 nights in 1998 on the 1.2m…

Astrophysics · Physics 2009-11-10 J. D. Hartman , J. Kaluzny , A. Szentgyorgyi , K. Z. Stanek

We report the results of an extensive VLT high-resolution imaging campaign of the central region of the giant globular cluster omega Centauri. More than 100,000 stars have been measured in the inner 9'x 9' region of the cluster. On the…

Astrophysics · Physics 2011-07-18 A. Sollima , F. R. Ferraro , E. Pancino , M. Bellazzini

We made a survey of the variable stars in a $13.2 \times 13.2$ arcmin$^2$ centered on the field of the Galactic bulge cluster NGC 6558. A total of 78 variables was found in the field of the cluster. Many of these variables are included in…

Solar and Stellar Astrophysics · Physics 2024-07-02 A. Arellano Ferro , L. J. Zerpa Guillen , M. A. Yepez , I. H. Bustos Fierro , Z. Prudil , C. E. Pérez Parra

We present the results of a photometric search for variable stars in the core of the Galactic globular cluster M4. The input data are a large and unprecedented set of deep Hubble Space Telescope WFC3 images (large program GO-12911; 120…

We present ~47,000 periodic variables found during the analysis of 5.4 million variable star candidates within a 20,000 square degree region covered by the Catalina Surveys Data Release-1 (CSDR1). Combining these variables with type-ab RR…

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