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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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 |
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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 |
work_keys_str_mv |
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1807316891832680448 |