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A Cold Neptune-Mass Planet OGLE-2007-BLG-368Lb: Cold Neptunes are Common
journal contribution
posted on 2023-05-17, 02:34 authored by Sumi, T, Bennett, DP, Bond, IA, Udalski, A, Batista, V, Dominik, M, Fouque, P, Kubas, D, Gould, A, Macintosh, B, Cook, K, Dong, S, Skuljan, L, Cassan, A, Abe, F, Botzler, CS, Fukui, A, Furusawa, K, Hearnshaw, JB, Itow, Y, Kamiya, K, Kilmartin, PM, Korpela, A, Lin, W, Ling, CH, Masuda, K, Matsubara, Y, Miyake, N, Muraki, Y, Nagaya, M, Nagayama, T, Ohnishi, K, Okumura, T, Perrott, YC, Rattenbury, N, Saito, T, Sako, T, Sullivan, DJ, Sweatman, WL, Tristram, PJ, Yock, PCM, Beaulieu, JP, Andrew ColeAndrew Cole, Coutures, C, Duran, MF, Greenhill, J, Jablonski, F, Marboeuf, U, Martioli, E, Pedretti, E, Pejcha, O, Rojo, P, Albrow, MD, Brilliant, S, Bode, M, Bramich, DM, Burgdorf, MJ, Caldwell, JAR, Calitz, H, Corrales, E, Dieters, S, Dominis Prester, D, Donatowicz, J, Kym HillKym Hill, Hoffman, M, Horne, K, Jorgensen, UG, Kains, N, Kane, S, Marquette, JB, Martin, R, Meintjes, P, Menzies, J, Pollard, KR, Sahu, KC, Snodgrass, C, Steele, I, Street, R, Tsapras, Y, Wambsganss, J, Williams, A, Zub, M, Szymanski, MK, Kubiak, M, Pietrzynski, G, Soszynski, I, Szewczyk, O, Wyrzykowski, L, Ulaczyk, K, Allen, W, Christie, GW, DePoy, DL, Gaudi, BS, Han, C, Janczak, J, Lee, CU, McCormick, J, Mallia, F, Monard, B, Natusch, T, Park, BG, Pogge, RW, Santallo, RWe present the discovery of a Neptune-mass planet OGLE-2007-BLG-368Lb with a planet Cstar 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 -0.26M andDl = 5.9+0.9 -1.4 kpc, respectively, so themass and separation of the planet areMp = 20+7 -8M 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 dNpl/d log q q -0.70.2 with a 95% confidence level upper limit of n < -0.35 (where dNpl/d log q 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.
History
Publication title
Astrophysical JournalVolume
710Pagination
1641-1653ISSN
0004-637XDepartment/School
School of Natural SciencesPublisher
Univ Chicago PressPlace of publication
1427 E 60Th St, Chicago, USA, Il, 60637-2954Rights statement
© 2010, American Astronomical SocietyRepository Status
- Restricted