High cadence near infrared timing observations of extrasolar planets
| Autor: | Elena Mason, Dominique Naef, Fernando Selman, Dante Minniti, Grzegorz Pietrzyński, Valentin D. Ivanov, C. Melo, Claudio Caceres |
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| Rok vydání: | 2009 |
| Předmět: |
Earth and Planetary Astrophysics (astro-ph.EP)
Physics Astrophysics::Instrumentation and Methods for Astrophysics FOS: Physical sciences Astronomy and Astrophysics Astrophysics::Cosmology and Extragalactic Astrophysics Astrophysics Planetary system Ephemeris Gravitational microlensing Exoplanet Stars Space and Planetary Science Planet Astrophysics::Earth and Planetary Astrophysics Transit (astronomy) Hot Neptune Astrophysics - Instrumentation and Methods for Astrophysics Instrumentation and Methods for Astrophysics (astro-ph.IM) Astrophysics::Galaxy Astrophysics Astrophysics - Earth and Planetary Astrophysics |
| Zdroj: | Astronomy & Astrophysics Artículos CONICYT CONICYT Chile instacron:CONICYT |
| ISSN: | 1432-0746 0004-6361 |
| DOI: | 10.1051/0004-6361/200810908 |
| Popis: | Currently the only technique sensitive to Earth mass planets around nearby stars (that are too close for microlensing) is the monitoring of the transit time variations of the transiting extrasolar planets. We search for additional planets in the systems of the hot Neptune GJ 436b, and the hot-Jupiter XO-1b, using high cadence observations in the J and Ks bands. New high-precision transit timing measurements are reported: GJ 436b Tc = 2454238.47898 \pm 0.00046 HJD; XO-1b Tc(A) = 2454218.83331 \pm 0.00114 HJD, Tc(B) = 2454222.77539 \pm 0.00036 HJD, Tc(C) = 2454222.77597 \pm 0.00039 HJD, Tc(D) = 2454226.71769 \pm 0.00034 HJD, and they were used to derive new ephemeris. We also determined depths for these transits. No statistically significant timing deviations were detected. We demonstrate that the high cadence ground based near-infrared observations are successful in constraining the mean transit time to ~30 sec., and are a viable alternative to space missions. 7 pages, 4 figures. To appear in A&A |
| Databáze: | OpenAIRE |
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