Millimagnitude photometry for transiting extrasolar planetary candidates-V. Follow-up of 30 OGLE transits. New candidates

Aims: We used VLT/VIMOS images in the V band to obtain light curves of the extrasolar planetary transits OGLE-TR-111 and OGLE-TR-113 and the candidate planetary transits: OGLE-TR-82, OGLE-TR-86, OGLE-TR-91, OGLE-TR-106, OGLE-TR-109, OGLE-TR-110, OGLE-TR-159, OGLE-TR-167, OGLE-TR-170, OGLE-TR-171. Me...

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Autores principales: Pietrukowicz, P., Minniti, D., Díaz, R.F., Fernández, J.M., Zoccali, M., Gieren, W., Pietrzyński, G., Ruíz, M.T., Udalski, A., Szeifert, T., Hempel, M.
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00046361_v509_n1_p_Pietrukowicz
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spelling todo:paper_00046361_v509_n1_p_Pietrukowicz2023-10-03T14:00:30Z Millimagnitude photometry for transiting extrasolar planetary candidates-V. Follow-up of 30 OGLE transits. New candidates Pietrukowicz, P. Minniti, D. Díaz, R.F. Fernández, J.M. Zoccali, M. Gieren, W. Pietrzyński, G. Ruíz, M.T. Udalski, A. Szeifert, T. Hempel, M. Eclipsing Individual OGLE-TR-109 OGLE-TR-111 OGLE-TR-113 - Planetary systems - Binaries Stars Photometers Photometry Data points Difference imaging Eclipsing Eclipsing binaries Extrasolar Geometrical parameters Light curves Multiple systems Observed samples Planetary system Stars Aims: We used VLT/VIMOS images in the V band to obtain light curves of the extrasolar planetary transits OGLE-TR-111 and OGLE-TR-113 and the candidate planetary transits: OGLE-TR-82, OGLE-TR-86, OGLE-TR-91, OGLE-TR-106, OGLE-TR-109, OGLE-TR-110, OGLE-TR-159, OGLE-TR-167, OGLE-TR-170, OGLE-TR-171. Methods: Using difference imaging photometry, we were able to achieve millimagnitude errors in the individual data points. We present the analysis of the data and the light curves by measuring transit amplitudes and ephemerides and by calculating geometrical parameters for some of the systems. Results: We observed nine OGLE objects at the predicted transit moments. Two other transits were shifted in time by a few hours. For another seven objects we expected to observe transits during the VIMOS run, but they were not detected. Conclusions: The stars OGLE-TR-111 and OGLE-TR-113 are probably the only OGLE objects in the observed sample to host planets, with the other objects being very likely eclipsing binaries or multiple systems. In this paper we also report on four new transiting candidates which we have found in the data. © 2010 ESO. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_00046361_v509_n1_p_Pietrukowicz
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic Eclipsing
Individual
OGLE-TR-109
OGLE-TR-111
OGLE-TR-113 - Planetary systems - Binaries
Stars
Photometers
Photometry
Data points
Difference imaging
Eclipsing
Eclipsing binaries
Extrasolar
Geometrical parameters
Light curves
Multiple systems
Observed samples
Planetary system
Stars
spellingShingle Eclipsing
Individual
OGLE-TR-109
OGLE-TR-111
OGLE-TR-113 - Planetary systems - Binaries
Stars
Photometers
Photometry
Data points
Difference imaging
Eclipsing
Eclipsing binaries
Extrasolar
Geometrical parameters
Light curves
Multiple systems
Observed samples
Planetary system
Stars
Pietrukowicz, P.
Minniti, D.
Díaz, R.F.
Fernández, J.M.
Zoccali, M.
Gieren, W.
Pietrzyński, G.
Ruíz, M.T.
Udalski, A.
Szeifert, T.
Hempel, M.
Millimagnitude photometry for transiting extrasolar planetary candidates-V. Follow-up of 30 OGLE transits. New candidates
topic_facet Eclipsing
Individual
OGLE-TR-109
OGLE-TR-111
OGLE-TR-113 - Planetary systems - Binaries
Stars
Photometers
Photometry
Data points
Difference imaging
Eclipsing
Eclipsing binaries
Extrasolar
Geometrical parameters
Light curves
Multiple systems
Observed samples
Planetary system
Stars
description Aims: We used VLT/VIMOS images in the V band to obtain light curves of the extrasolar planetary transits OGLE-TR-111 and OGLE-TR-113 and the candidate planetary transits: OGLE-TR-82, OGLE-TR-86, OGLE-TR-91, OGLE-TR-106, OGLE-TR-109, OGLE-TR-110, OGLE-TR-159, OGLE-TR-167, OGLE-TR-170, OGLE-TR-171. Methods: Using difference imaging photometry, we were able to achieve millimagnitude errors in the individual data points. We present the analysis of the data and the light curves by measuring transit amplitudes and ephemerides and by calculating geometrical parameters for some of the systems. Results: We observed nine OGLE objects at the predicted transit moments. Two other transits were shifted in time by a few hours. For another seven objects we expected to observe transits during the VIMOS run, but they were not detected. Conclusions: The stars OGLE-TR-111 and OGLE-TR-113 are probably the only OGLE objects in the observed sample to host planets, with the other objects being very likely eclipsing binaries or multiple systems. In this paper we also report on four new transiting candidates which we have found in the data. © 2010 ESO.
format JOUR
author Pietrukowicz, P.
Minniti, D.
Díaz, R.F.
Fernández, J.M.
Zoccali, M.
Gieren, W.
Pietrzyński, G.
Ruíz, M.T.
Udalski, A.
Szeifert, T.
Hempel, M.
author_facet Pietrukowicz, P.
Minniti, D.
Díaz, R.F.
Fernández, J.M.
Zoccali, M.
Gieren, W.
Pietrzyński, G.
Ruíz, M.T.
Udalski, A.
Szeifert, T.
Hempel, M.
author_sort Pietrukowicz, P.
title Millimagnitude photometry for transiting extrasolar planetary candidates-V. Follow-up of 30 OGLE transits. New candidates
title_short Millimagnitude photometry for transiting extrasolar planetary candidates-V. Follow-up of 30 OGLE transits. New candidates
title_full Millimagnitude photometry for transiting extrasolar planetary candidates-V. Follow-up of 30 OGLE transits. New candidates
title_fullStr Millimagnitude photometry for transiting extrasolar planetary candidates-V. Follow-up of 30 OGLE transits. New candidates
title_full_unstemmed Millimagnitude photometry for transiting extrasolar planetary candidates-V. Follow-up of 30 OGLE transits. New candidates
title_sort millimagnitude photometry for transiting extrasolar planetary candidates-v. follow-up of 30 ogle transits. new candidates
url http://hdl.handle.net/20.500.12110/paper_00046361_v509_n1_p_Pietrukowicz
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