Quick search Find article
Quick search
Find article

A COLD NEPTUNE-MASS PLANET OGLE-2007-BLG-368Lb: COLD NEPTUNES ARE COMMON

FREE ISSUE

T. Sumi1,51, D. P. Bennett2,51,52, I. A. Bond3,51, A. Udalski4,53, V. Batista3,5,52,54, M. Dominik6,52,55, P. Fouqué7,52, D. Kubas5,8,52,54, A. Gould9,56, B. Macintosh10, K. Cook10, S. Dong11,56, L. Skuljan3,51, A. Cassan5,12,52,54, F. Abe1, C. S. Botzler13, A. Fukui1, K. Furusawa1, J. B. Hearnshaw14, Y. Itow1, K. Kamiya1, P. M. Kilmartin15, A. Korpela16, W. Lin3, C. H. Ling3, K. Masuda1, Y. Matsubara1, N. Miyake1, Y. Muraki17, M. Nagaya1, T. Nagayama18, K. Ohnishi19, T. Okumura1, Y. C. Perrott13, N. Rattenbury13, To. Saito20, T. Sako1, D. J. Sullivan16, W. L. Sweatman3, P. J. Tristram15, P. C. M. Yock13 (The MOA Collaboration), J. P. Beaulieu5,54, A. Cole21, Ch. Coutures9,54, M. F. Duran22, J. Greenhill21, F. Jablonski23, U. Marboeuf24, E. Martioli23, E. Pedretti6, O. Pejcha9, P. Rojo22, M. D. Albrow14, S. Brillant56, M. Bode25, D. M. Bramich26, M. J. Burgdorf27,28, J. A. R. Caldwell29, H. Calitz30, E. Corrales5,54, S. Dieters5,21,54, D. Dominis Prester31, J. Donatowicz32,54, K. Hill5,21, M. Hoffman30, K. Horne6, U. G. Jørgensen33, N. Kains6, S. Kane34, J. B. Marquette5,54, R. Martin35, P. Meintjes30, J. Menzies36, K. R. Pollard14, K. C. Sahu37, C. Snodgrass56, I. Steele25, R. Street38, Y. Tsapras38, J. Wambsganss12, A. Williams35, M. Zub12 (The PLANET Collaboration), M. K. Szymański4, M. Kubiak4, G. Pietrzyński4,39, I. Soszyński4, O. Szewczyk39, Ł Wyrzykowski41, K. Ulaczyk4 (The OGLE Collaboration), W. Allen41, G. W. Christie42, D. L. DePoy43, B. S. Gaudi9, C. Han44, J. Janczak9, C.-U. Lee45, J. McCormick46, F. Mallia47, B. Monard48, T. Natusch49, B.-G. Park45, R. W. Pogge9 and R. Santallo50 (The μFUN Collaboration)

Show affiliations


We present the discovery of a Neptune-mass planet OGLE-2007-BLG-368Lb with a planet-star mass ratio of q = [9.5 ± 2.1] × 10–5 via gravitational microlensing. The planetary deviation was detected in real-time thanks to the high cadence of the Microlensing Observations in Astrophysics survey, real-time light-curve monitoring and intensive follow-up observations. A Bayesian analysis returns the stellar mass and distance at Ml = 0.64+0.21 –0.26 M and Dl = 5.9+0.9 –1.4 kpc, respectively, so the mass and separation of the planet are Mp = 20+7 –8 M and a = 3.3+1.4 –0.8 AU, respectively. This discovery adds another cold Neptune-mass planet to the planetary sample discovered by microlensing, which now comprises four cold Neptune/super-Earths, five gas giant planets, and another sub-Saturn mass planet whose nature is unclear. The discovery of these 10 cold exoplanets by the microlensing method implies that the mass ratio function of cold exoplanets scales as dN pl/dlog q vprop q –0.7±0.2 with a 95% confidence level upper limit of n < –0.35 (where dN pl/dlog q vprop qn ). As microlensing is most sensitive to planets beyond the snow-line, this implies that Neptune-mass planets are at least three times more common than Jupiters in this region at the 95% confidence level.


Keywords

gravitational lensing: micro; planetary systems


Dates

Issue 2 (2010 February 20)

Received 2009 December 7, accepted for publication 2010 January 4

Published 2010 February 2



  1. A Cold Neptune-Mass Planet OGLE-2007-BLG-368Lb: Cold Neptunes Are Common

    T. Sumi et al. 2010 ApJ 710 1641

  2. Flux networks in metabolic graphs

    P B Warren et al 2009 Phys. Biol. 6 046006

  3. Wide Field Planetary Camera 2 Observations of Leo A: A Predominantly Young Galaxy within the Local Group

    Eline Tolstoy et al. 1998 The Astronomical Journal 116 1244

  4. Typing Supernova Remnants Using X-Ray Line Emission Morphologies

    L. A. Lopez et al 2009 ApJ 706 L106

  5. Simultaneous Multiwavelength and Optical Microvariability Observations of CTA 102 (PKS J2232+1143)

    Angela Osterman Meyer et al. 2009 The Astronomical Journal 138 1902

  6. Curvature and torsion in growing actin networks

    Joshua W Shaevitz and Daniel A Fletcher 2008 Phys. Biol. 5 026006

  7. The Fast Declining Type Ia Supernova 2003gs, and Evidence for a Significant Dispersion in Near-Infrared Absolute Magnitudes of Fast Decliners at Maximum Light

    Kevin Krisciunas et al. 2009 The Astronomical Journal 138 1584

  8. Transcendentality and crossing

    Niklas Beisert et al J. Stat. Mech. (2007) P01021

  9. 37 GHz Observations of a Large Sample of BL Lacertae Objects

    Elina Nieppola et al. 2007 The Astronomical Journal 133 1947

  10. Microlensing Event MOA-2007-BLG-400: Exhuming the Buried Signature of a Cool, Jovian-Mass Planet

    Subo Dong et al. 2009 ApJ 698 1826

View by subject




Export








Please login to access our web services, or create an account if you don't yet have one.

You must have cookies enabled in your web browser to be able to login.

Username
Password

Forgotten your password? Get a new one here.