THE CATALINA SURVEYS PERIODIC VARIABLE STAR CATALOG

Journal Article · Tue Jul 01 00:00:00 EDT 2014 · Astrophysical Journal, Supplement Series

DOI:https://doi.org/10.1088/0067-0049/213/1/9· OSTI ID:22340203

Drake, A. J.; Graham, M. J.; Djorgovski, S. G.; Mahabal, A. A.; Donalek, C.; Williams, R. ^[1]; Catelan, M.; Torrealba, G. ^[2]; García-Álvarez, D. ^[3]; Prieto, J. L.; Beshore, E. ^[4]; Larson, S.; Christen sen, E.; Boattini, A.; Gibbs, A.; Hill, R.; Kowalski, R.; Johnson, J. ^[5]; Belokurov, V.; Koposov, S. E. ^[6] ; others, and

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1. California Institute of Technology, 1200 East California Boulevard, CA 91225 (United States)
2. Pontificia Universidad Católica de Chile, Instituto de Astrofísica, Facultad de Física, Av. Vicuña Mackena 4860, 782-0436 Macul, Santiago (Chile)
3. Instituto de Astrofísica de Canarias, Avenida Vía Láctea, E-38205 La Laguna, Tenerife (Spain)
4. Department of Astronomy, Princeton University, 4 Ivy Ln., Princeton, NJ 08544 (United States)
5. Department of Planetary Sciences, Lunar and Planetary Laboratory, The University of Arizona, 1629 East University Boulevard, Tucson, AZ 85721 (United States)
6. Institute of Astronomy, Madingley Road, Cambridge CB3 0HA (United Kingdom)

We present ∼47,000 periodic variables found during the analysis of 5.4 million variable star candidates within a 20,000 deg{sup 2} region covered by the Catalina Surveys Data Release-1 (CSDR1). Combining these variables with type ab RR Lyrae from our previous work, we produce an online catalog containing periods, amplitudes, and classifications for ∼61,000 periodic variables. By cross-matching these variables with those from prior surveys, we find that >90% of the ∼8000 known periodic variables in the survey region are recovered. For these sources, we find excellent agreement between our catalog and prior values of luminosity, period, and amplitude as well as classification. We investigate the rate of confusion between objects classified as contact binaries and type c RR Lyrae (RRc's) based on periods, colors, amplitudes, metallicities, radial velocities, and surface gravities. We find that no more than a few percent of the variables in these classes are misidentified. By deriving distances for this clean sample of ∼5500 RRc's, we trace the path of the Sagittarius tidal streams within the Galactic halo. Selecting 146 outer-halo RRc's with SDSS radial velocities, we confirm the presence of a coherent halo structure that is inconsistent with current N-body simulations of the Sagittarius tidal stream. We also find numerous long-period variables that are very likely associated within the Sagittarius tidal stream system. Based on the examination of 31,000 contact binary light curves we find evidence for two subgroups exhibiting irregular light curves. One subgroup presents significant variations in mean brightness that are likely due to chromospheric activity. The other subgroup shows stable modulations over more than a thousand days and thereby provides evidence that the O'Connell effect is not due to stellar spots.

• OSTI ID: 22340203
• Journal Information: Astrophysical Journal, Supplement Series, Vol. 213, Issue 1; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 0067-0049
• Country of Publication: United States
• Language: English

Related Subjects

79 ASTROPHYSICS
COSMOLOGY AND ASTRONOMY
AMPLITUDES
BRIGHTNESS
CATALOGS
CHANDRASEKHAR THEORY
CLASSIFICATION
COLOR
GALAXIES
LUMINOSITY
MANY-BODY PROBLEM
METALLICITY
PERIODICITY
RADIAL VELOCITY
STARSPOTS
VARIABLE STARS
VISIBLE RADIATION
X-RAY DETECTION