Millimagnitude photometry for transiting extrasolar planetary candidates. III. Accurate radius and period for OGLE-TR-111-b1

We present accurate V-band photometry for a planetary transit of OGLE-TR-111 acquired with VIMOS at the ESO Very Large Telescope. The measurement of this transit allows us to refine the planetary radius, obtaining R p = 1.01 ± 0.06 RJ. Given the mass of Mp = 0.53 MJ previously measured from radial v...

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Autores principales: Minniti, D., Fernández, J.M., Díaz, R.F., Udalski, A., Pietrzynski, G., Gieren, W., Rojo, P., Ruíz, M.T., Zoccali, M.
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_0004637X_v660_n1I_p858_Minniti
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spelling todo:paper_0004637X_v660_n1I_p858_Minniti2023-10-03T14:02:05Z Millimagnitude photometry for transiting extrasolar planetary candidates. III. Accurate radius and period for OGLE-TR-111-b1 Minniti, D. Fernández, J.M. Díaz, R.F. Udalski, A. Pietrzynski, G. Gieren, W. Rojo, P. Ruíz, M.T. Zoccali, M. Planetary systems Stars: individual (OGLE-TR-111) We present accurate V-band photometry for a planetary transit of OGLE-TR-111 acquired with VIMOS at the ESO Very Large Telescope. The measurement of this transit allows us to refine the planetary radius, obtaining R p = 1.01 ± 0.06 RJ. Given the mass of Mp = 0.53 MJ previously measured from radial velocities, we confirm that the density is ρp = 0.6 ± 0.2 g cm-3. We also revise the ephemeris for OGLE-TR-111-b, obtaining an accurate orbital period P = 4.014484 ± 0.000014 days and predicting that the next observable transits would occur around December 2006, and after that only in mid-2008. Even though this period is different from previously published values, we cannot yet rule out a constant period. © 2007. The American Astronomical Society. All rights reserved. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_0004637X_v660_n1I_p858_Minniti
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic Planetary systems
Stars: individual (OGLE-TR-111)
spellingShingle Planetary systems
Stars: individual (OGLE-TR-111)
Minniti, D.
Fernández, J.M.
Díaz, R.F.
Udalski, A.
Pietrzynski, G.
Gieren, W.
Rojo, P.
Ruíz, M.T.
Zoccali, M.
Millimagnitude photometry for transiting extrasolar planetary candidates. III. Accurate radius and period for OGLE-TR-111-b1
topic_facet Planetary systems
Stars: individual (OGLE-TR-111)
description We present accurate V-band photometry for a planetary transit of OGLE-TR-111 acquired with VIMOS at the ESO Very Large Telescope. The measurement of this transit allows us to refine the planetary radius, obtaining R p = 1.01 ± 0.06 RJ. Given the mass of Mp = 0.53 MJ previously measured from radial velocities, we confirm that the density is ρp = 0.6 ± 0.2 g cm-3. We also revise the ephemeris for OGLE-TR-111-b, obtaining an accurate orbital period P = 4.014484 ± 0.000014 days and predicting that the next observable transits would occur around December 2006, and after that only in mid-2008. Even though this period is different from previously published values, we cannot yet rule out a constant period. © 2007. The American Astronomical Society. All rights reserved.
format JOUR
author Minniti, D.
Fernández, J.M.
Díaz, R.F.
Udalski, A.
Pietrzynski, G.
Gieren, W.
Rojo, P.
Ruíz, M.T.
Zoccali, M.
author_facet Minniti, D.
Fernández, J.M.
Díaz, R.F.
Udalski, A.
Pietrzynski, G.
Gieren, W.
Rojo, P.
Ruíz, M.T.
Zoccali, M.
author_sort Minniti, D.
title Millimagnitude photometry for transiting extrasolar planetary candidates. III. Accurate radius and period for OGLE-TR-111-b1
title_short Millimagnitude photometry for transiting extrasolar planetary candidates. III. Accurate radius and period for OGLE-TR-111-b1
title_full Millimagnitude photometry for transiting extrasolar planetary candidates. III. Accurate radius and period for OGLE-TR-111-b1
title_fullStr Millimagnitude photometry for transiting extrasolar planetary candidates. III. Accurate radius and period for OGLE-TR-111-b1
title_full_unstemmed Millimagnitude photometry for transiting extrasolar planetary candidates. III. Accurate radius and period for OGLE-TR-111-b1
title_sort millimagnitude photometry for transiting extrasolar planetary candidates. iii. accurate radius and period for ogle-tr-111-b1
url http://hdl.handle.net/20.500.12110/paper_0004637X_v660_n1I_p858_Minniti
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