Near-Infrared Variability in the 2MASS Calibration Fields: A Search for Planetary Transit Candidates

The Two Micron All Sky Survey (2MASS) photometric calibration observations cover ~6 square degrees on the sky in 35 "calibration fields", each sampled in nominal photometric conditions between 562 and 3692 times during the 4 years of the 2MASS mission. We compile a catalog of variables from the calibration observations to search for M dwarfs transited by extrasolar planets. We present our methods for measuring periodic and nonperiodic flux variability. From 7554 sources with apparent K_s magnitudes between 5.6 and 16.1, we identify 247 variables, including extragalactic variables and 23 periodic variables. We have discovered three M dwarf eclipsing systems, including two candidates for transiting extrasolar planets.

[1]  The Large Bright Quasar Survey. VII. The LBQS and FIRST Surveys , 2001, astro-ph/0105124.

[2]  R. D. Mathieu,et al.  Photometric variability in the old open cluster M 67 - II. General survey , 2001, astro-ph/0112189.

[3]  J. Carpenter Color Transformations for the 2MASS Second Incremental Data Release , 2001, astro-ph/0101463.

[4]  J. Elias,et al.  Bolometric luminosities and infrared properties of carbon stars in the Magellanic Clouds and the galaxy. , 1981 .

[5]  O. Szewczyk,et al.  Discovery of a cool planet of 5.5 Earth masses through gravitational microlensing , 2006, Nature.

[6]  R. Stellingwerf Period determination using phase dispersion minimization , 1978 .

[7]  S. Strom,et al.  Are wide pre-main-sequence binaries coeval? , 1994 .

[8]  Slavek M. Rucinski,et al.  The shortest-period m-dwarf eclipsing system bw3 v38 , 1997 .

[9]  J. Scargle Studies in astronomical time series analysis. II - Statistical aspects of spectral analysis of unevenly spaced data , 1982 .

[10]  J. Liske,et al.  The Millennium Galaxy Catalogue: 16 ⩽ BMGC < 24 galaxy counts and the calibration of the local galaxy luminosity function , 2002 .

[11]  S. Maddox,et al.  The APM galaxy survey. I - APM measurements and star-galaxy separation , 1990 .

[12]  E. Greisen,et al.  The NRAO VLA Sky Survey , 1996 .

[13]  A Long‐Period Jupiter‐Mass Planet Orbiting the Nearby M Dwarf GJ 849 , 2006, astro-ph/0610179.

[14]  G. Neugebauer,et al.  The near-infrared variability of a sample of optically selected quasars , 1989 .

[15]  M. Dworetsky A period-finding method for sparse randomly spaced observations or “How long is a piece of string?” , 1983 .

[16]  G. Kov'acs,et al.  A box-fitting algorithm in the search for periodic transits , 2002, astro-ph/0206099.

[17]  W. Cochran,et al.  Exploring the Frequency of Close-in Jovian Planets around M Dwarfs , 2006, astro-ph/0606121.

[18]  Mercedes Lopez-Morales,et al.  On the Correlation between the Magnetic Activity Levels, Metallicities, and Radii of Low-Mass Stars , 2007, astro-ph/0701702.

[19]  Laird M. Close,et al.  Discovery of a Tight Brown Dwarf Companion to theLow-Mass Star LHS 2397a , 2003 .

[20]  All‐Sky Automated Survey eclipsing binaries with observed high period change rates , 2007, astro-ph/0703705.

[21]  B. Peterson,et al.  JHK′ Imaging Photometry of Seyfert 1 Active Galactic Nuclei and Quasars. III. Variability of Radio-Quiet and Radio-Loud Active Galactic Nuclei , 2002, astro-ph/0204011.

[22]  Near-Infrared Photometric Variability of Stars toward the Orion A Molecular Cloud , 2001, astro-ph/0102446.

[23]  J. Lissauer,et al.  A ~7.5 M⊕ Planet Orbiting the Nearby Star, GJ 876* , 2005, astro-ph/0510508.

[24]  O. Franz,et al.  Interferometric Astrometry of the Low-Mass Binary Gl 791.2 (= HU Del) Using HUBBLE SPACE TELESCOPE Fine Guidance Sensor 3: Parallax and Component Masses , 2000, astro-ph/0005026.

[25]  Leslie Hebb,et al.  Photometric Monitoring of Open Clusters. II. A New M Dwarf Eclipsing Binary System in the Open Cluster NGC 1647 , 2006 .

[26]  M. Skrutskie,et al.  The Two Micron All Sky Survey (2MASS) , 2006 .

[27]  I. Ribas,et al.  GU Bootis: A New 0.6 M☉ Detached Eclipsing Binary , 2005, astro-ph/0505001.

[28]  L. Bildsten,et al.  Classical Novae as a Probe of the Cataclysmic Variable Population , 2005, astro-ph/0503556.

[29]  Richard L. White,et al.  A Catalog of 1.4 GHz Radio Sources from the FIRST Survey , 1997 .

[30]  J. Kirkpatrick,et al.  Low Mass Companions to Nearby Stars: Spectral Classification and its Relation to the Stellar/Substellar Break , 1994 .

[31]  E. al.,et al.  The Sloan Digital Sky Survey: Technical summary , 2000, astro-ph/0006396.

[32]  Peter B. Stetson,et al.  ON THE AUTOMATIC DETERMINATION OF LIGHT-CURVE PARAMETERS FOR CEPHEID VARIABLES , 1996 .

[33]  G. Rieke,et al.  Variability and the nature of QSO optical-infrared continua , 1985 .

[34]  O. Lahav,et al.  The 2dF Galaxy Redshift Survey: the population of nearby radio galaxies at the 1-mJy level , 2001, astro-ph/0106430.

[35]  Suzanne L. Hawley,et al.  The Palomar/MSU Nearby Star Spectroscopic Survey. IV. The Luminosity Function in the Solar Neighborhood and M Dwarf Kinematics , 2002 .

[36]  T. M. Brown,et al.  A New Detached M Dwarf Eclipsing Binary , 2005, astro-ph/0504490.

[37]  Debra A. Fischer,et al.  A Neptune-Mass Planet Orbiting the Nearby M Dwarf GJ 436 , 2004 .

[38]  I. Ribas,et al.  The 0.4-$M_{\odot}$ eclipsing binary CU Cancri - Absolute dimensions, comparison with evolutionary models and possible evidence for a circumstellar dust disk , 2002, astro-ph/0211086.

[39]  Xiaohui Fan,et al.  Deep wide-field spectrophotometry of the open cluster M67 , 1996, astro-ph/9604178.

[40]  D. Schlegel,et al.  Maps of Dust Infrared Emission for Use in Estimation of Reddening and Cosmic Microwave Background Radiation Foregrounds , 1998 .

[41]  K. Zebrun,et al.  OGLE 2003-BLG-235/MOA 2003-BLG-53: A Planetary Microlensing Event , 2004 .

[42]  D. Queloz,et al.  The HARPS search for southern extra-solar planets - VI. A Neptune-mass planet around the nearby M dwarf Gl 581 , 2005 .

[43]  D. Schlegel,et al.  Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds , 1997, astro-ph/9710327.

[44]  M. Skrutskie,et al.  Near-Infrared Photometric Variability of Stars toward the Chamaeleon I Molecular Cloud , 2002, astro-ph/0204430.

[45]  P. Teuben,et al.  A Near-Infrared Imaging Survey of the ρ Ophiuchi Cloud Core , 1997 .

[46]  GU Boo : A New 0 . 6 M ⊙ Detached Eclipsing Binary , 2005 .

[47]  C. Tout,et al.  Stellar evolution models for Z = 0.0001 to 0.03 (Pols+ 1998) , 1998 .

[48]  Oxford,et al.  The 2dF QSO Redshift Survey – XII. The spectroscopic catalogue and luminosity function , 2004, astro-ph/0403040.