English
Related papers

Related papers: Revisiting Spitzer transit observations with Indep…

200 papers

Blind source separation techniques are used to reanalyse two exoplanetary transit lightcurves of the exoplanet HD189733b recorded with the IR camera IRAC on board the Spitzer Space Telescope at 3.6$\mu$m during the "cold" era. These…

Earth and Planetary Astrophysics · Physics 2015-06-19 Giuseppe Morello , Ingo P. Waldmann , Giovanna Tinetti , Giovanni Peres , Giuseppina Micela , Ian D. Howarth

We present here a reanalysis of the Spitzer Space Telescope phase curves of the hot Jupiter WASP43 b, using the wavelet pixel-Independent Component Analysis, a blind signal-source separation method. The data analyzed were recorded with the…

Earth and Planetary Astrophysics · Physics 2019-08-28 Giuseppe Morello , Camilla Danielski , Daniel Dicken , Pascal Tremblin , Pierre-Olivier Lagage

The research of effective and reliable detrending methods for Spitzer data is of paramount importance for the characterization of exoplanetary atmospheres. To date, the totality of exoplanetary observations in the mid- and far-infrared, at…

Earth and Planetary Astrophysics · Physics 2016-04-06 Giuseppe Morello , Ingo P. Waldmann , Giovanna Tinetti

In this paper we describe a uniform analysis of eight transits and eleven secondary eclipses of the extrasolar planet GJ 436b obtained in the 3.6, 4.5, and 8.0 micron bands using the IRAC instrument on the Spitzer Space Telescope between UT…

We present a new primary transit observation of the hot-jupiter HD189733b, obtained at 3.6 microns with the Infrared Array Camera (IRAC) onboard the Spitzer Space Telescope. Previous measurements at 3.6 microns suffered from strong…

Earth and Planetary Astrophysics · Physics 2015-05-19 J. -M. Desert , D. Sing , A. Vidal-Madjar , G. Hebrard , D. Ehrenreich , A. Lecavelier des Etangs , V. Parmentier , R. Ferlet , G. W. Henry

We present time series photometry for six partial transits of GJ436b obtained with the Fine Guidance Sensor instrument on the Hubble Space Telescope (HST). Our analysis of these data yields independent estimates of the host star's radius…

The hot Jupiter HD 189733b was observed during its primary transit using the Infrared Array Camera on the Spitzer Space Telescope. The transit depths were measured simultaneously at 3.6 and 5.8 microns. Our analysis yields values of 2.356…

Astrophysics · Physics 2010-03-01 J. P. Beaulieu , S. Carey , I. Ribas , G. Tinetti

We discovered evidence for a possible additional 0.75 R_Earth transiting planet in the NASA EPOXI observations of the known M dwarf exoplanetary system GJ 436. Based on an ephemeris determined from the EPOXI data, we predicted a transit…

We report the results of an analysis of all Spitzer/MIPS 24 micron observations of HD 209458b, one of the touchstone objects in the study of irradiated giant planet atmospheres. Altogether we analyze 2.5 transits, 3 eclipses, and a 58-hour…

Earth and Planetary Astrophysics · Physics 2015-06-04 Ian J. M. Crossfield , Heather Knutson , Jonathan Fortney , Adam P. Showman , Nicolas B. Cowan , Drake Deming

We present observations of seven transits and seven eclipses of the transiting planet system HD 189733 taken with Spitzer IRAC at 8 microns. We use a new correction for the detector ramp variation with a double-exponential function. Our…

Earth and Planetary Astrophysics · Physics 2014-11-21 E. Agol , N. B. Cowan , H. A. Knutson , D. Deming , J. H. Steffen , G. W. Henry , D. Charbonneau

We present an analysis of seven primary transit observations of the hot Neptune GJ436b at 3.6, 4.5 and $8~\mu$m obtained with the Infrared Array Camera (IRAC) on the Spitzer Space Telescope. After correcting for systematic effects, we…

The nearby transiting system GJ 436b offers a unique opportunity to probe the structure and atmosphere of an extra-solar "hot Neptune". In this Letter, we present the main results of observations covering two transit events with the NICMOS…

Astrophysics · Physics 2009-11-13 F. Pont , R. L. Gilliland , H. Knutson , M. Holman , D. Charbonneau

We report the results of infrared (8 micron) transit and secondary eclipse photometry of the hot Neptune exoplanet, GJ436b using Spitzer. The nearly photon-limited precision of these data allow us to measure an improved radius for the…

Context. GJ 436b is one of the few transiting warm Neptunes for which a detailed characterisation of the atmosphere is possible, whereas its non-negligible orbital eccentricity calls for further investigation. Independent analyses of…

We observed the transiting super-Earth exoplanet GJ1214b using Warm Spitzer at 4.5 microns wavelength during a 20-day quasi-continuous sequence in May 2011. The goals of our long observation were to accurately define the infrared transit…

In recent years, a number of observations have been made of the transits of 'Hot Jupiters', such as HD 189733b, which have been modelled to derive atmospheric structure and composition. As measurement techniques improve, the transit spectra…

Earth and Planetary Astrophysics · Physics 2015-06-22 Patrick G. J. Irwin , Joanna K. Barstow , Neil E. Bowles , Leigh N. Fletcher , Suzanne Aigrain , Jae-Min Lee

We present Spitzer Space Telescope infrared photometry of a secondary eclipse of the hot Neptune GJ436b. The observations were obtained using the 8-micron band of the InfraRed Array Camera (IRAC). The data spanning the predicted time of…

We present Spitzer Space Telescope observations of the extrasolar planet HD189733b primary transit, obtained simultaneously at 3.6 and 5.8 microns with the Infrared Array Camera. The system parameters, including planetary radius, stellar…

We report observations of two consecutive transits of the warm super-Earth exoplanet GJ1214b at 3.6 and 4.5 microns with the Infrared Array Camera instrument on-board the Spitzer Space Telescope. The two transit light curves allow for the…

We report on H-band, ground-based observations of a transit of the hot Neptune GJ 436b. Once combined to achieve sampling equivalent to archived observations taken with Spitzer, our measurements reach comparable precision levels. We analyze…

Astrophysics · Physics 2009-11-13 R. Alonso , M. Barbieri , M. Rabus , H. J. Deeg , J. A. Belmonte , J. M. Almenara
‹ Prev 1 2 3 10 Next ›