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Verfasst von: | Street, Rachel [VerfasserIn] ![]() |
Tsapras, Yiannis [VerfasserIn] ![]() | |
Schmidt, Robert W. [VerfasserIn] ![]() | |
Wambsganß, Joachim [VerfasserIn] ![]() | |
Titel: | Spitzer parallax of OGLE-2015-BLG-0966 |
Titelzusatz: | a cold neptune in the galactic disk |
Verf.angabe: | R.A. Street, A. Udalski, S. Calchi Novati, M.P.G. Hundertmark, W. Zhu, A. Gould, J. Yee, Y. Tsapras, D.P. Bennett (The RoboNet Project & MiNDSTEp Consortium), U.G. Jørgensen, M. Dominik, M.I. Andersen, E. Bachelet, V. Bozza, D.M. Bramich, M.J. Burgdorf, A. Cassan, S. Ciceri, G. D’Ago, Subo Dong, D.F. Evans, Sheng-hong Gu, H. Harkonnen, T.C. Hinse, Keith Horne, R. Figuera Jaimes, N. Kains, E. Kerins, H. Korhonen, M. Kuffmeier, L. Mancini, J. Menzies, S. Mao, N. Peixinho, A. Popovas, M. Rabus, S. Rahvar, C. Ranc, R. Tronsgaard Rasmussen, G. Scarpetta, R. Schmidt, J. Skottfelt, C. Snodgrass, J. Southworth, I.A. Steele, J. Surdej, E. Unda-Sanzana, P. Verma, C. von Essen, J. Wambsganss, Yi-Bo Wang, O. Wertz (The OGLE Project), R. Poleski, M. Pawlak, M.K. Szymański, J. Skowron, P. Mróz, S. Kozłowski, Ł Wyrzykowski, P. Pietrukowicz, G. Pietrzyński, I. Soszyński, K. Ulaczyk (The Spitzer Team), C. Beichman, G. Bryden, S. Carey, B.S. Gaudi, C.B. Henderson, R.W. Pogge, Y. Shvartzvald (The MOA Collaboration), F. Abe, Y. Asakura, A. Bhattacharya, I.A. Bond, M. Donachie, M. Freeman, A. Fukui, Y. Hirao, K. Inayama, Y. Itow, N. Koshimoto, M.C.A. Li, C.H. Ling, K. Masuda, Y. Matsubara, Y. Muraki, M. Nagakane, T. Nishioka, K. Ohnishi, H. Oyokawa, N. Rattenbury, To Saito, A. Sharan, D.J. Sullivan, T. Sumi, D. Suzuki, J. Tristram, Y. Wakiyama, A. Yonehara (KMTNet Modeling Team), C. Han, J.-Y. Choi, H. Park, Y. K. Jung, and I.-G. Shin |
Fussnoten: | Gesehen am 08.11.2017 |
Titel Quelle: | Enthalten in: The astrophysical journal / 1 |
Jahr Quelle: | 2016 |
Band/Heft Quelle: | 819(2016,2) Artikel-Nummer 93, 12 Seiten |
ISSN Quelle: | 1538-4357 |
Abstract: | We report the detection of a cold Neptune m planet = 21 ± 2 M ⊕ orbiting a 0.38 M ⊙ M dwarf lying 2.5-3.3 kpc toward the Galactic center as part of a campaign combining ground-based and Spitzer observations to measure the Galactic distribution of planets. This is the first time that the complex real-time protocols described by Yee et al., which aim to maximize planet sensitivity while maintaining sample integrity, have been carried out in practice. Multiple survey and follow up teams successfully combined their efforts within the framework of these protocols to detect this planet. This is the second planet in the Spitzer Galactic distribution sample. Both are in the near to mid-disk and are clearly not in the Galactic bulge. |
DOI: | doi:10.3847/0004-637X/819/2/93 |
URL: | Bitte beachten Sie: Dies ist ein Bibliographieeintrag. Ein Volltextzugriff für Mitglieder der Universität besteht hier nur, falls für die entsprechende Zeitschrift/den entsprechenden Sammelband ein Abonnement besteht oder es sich um einen OpenAccess-Titel handelt. Kostenfrei: Verlag: http://dx.doi.org/10.3847/0004-637X/819/2/93 |
DOI: https://doi.org/10.3847/0004-637X/819/2/93 | |
Datenträger: | Online-Ressource |
Sprache: | eng |
K10plus-PPN: | 1565125452 |
Verknüpfungen: | → Zeitschrift |