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WASP-12b is one of the most well-studied transiting exoplanets, as its highly-inflated radius and its 1.1 day orbit around a G0-type star make it an excellent target for atmospheric categorisation through observation during its secondary…

We present photometry of the extrasolar planet WASP-5b in the 3.6 and 4.5 micron bands taken with the Spitzer Space Telescope's Infrared Array Camera as part of the extended warm mission. By examining the depth of the planet's secondary…

We demonstrate a path to hitherto unachievable differential photometric precisions from the ground, both in the optical and near-infrared (NIR), using custom-fabricated beam-shaping diffusers produced using specialized nanofabrication…

After observing WASP-12 in the second year of the primary mission, the Transiting Exoplanet Survey Satellite (TESS) revisited the system in late 2021 during its extended mission. In this paper, we incorporate the new TESS photometry into a…

地球与行星天体物理 · 物理学 2022-03-22 Ian Wong , Avi Shporer , Shreyas Vissapragada , Michael Greklek-McKeon , Heather A. Knutson , Joshua N. Winn , Björn Benneke

We present four new secondary eclipse observations for the ultrahot Jupiter WASP-121b acquired using the Hubble Space Telescope Wide Field Camera 3. The eclipse depth is measured to a median precision of 60ppm across 28 spectroscopic…

We report a new detection of the H-band thermal emission of CoRoT-1b and two confirmation detections of the Ks-band thermal emission of WASP-12b at secondary eclipses. The H-band measurement of CoRoT-1b shows an eclipse depth of…

地球与行星天体物理 · 物理学 2015-05-30 Ming Zhao , John D. Monnier , Mark R. Swain , Travis Barman , Sasha Hinkley

[Abridged] We report Warm Spitzer full-orbit phase observations of WASP-12b at 3.6 and 4.5 micron. We are able to measure the transit depths, eclipse depths, thermal and ellipsoidal phase variations at both wavelengths. The large amplitude…

地球与行星天体物理 · 物理学 2015-06-03 N. B. Cowan , P. Machalek , B. Croll , L. M. Shekhtman , A. Burrows , D. Deming , T. Greene , J. L. Hora

WASP-10b, a non-inflated hot Jupiter, was discovered around a K-dwarf in a near circular orbit ($\sim $$0.06$). Since its discovery in 2009, different published parameters for this system have led to a discussion about the size, density,…

We observed two secondary eclipses of the exoplanet WASP-12b using the Infrared Array Camera on the Spitzer Space Telescope. The close proximity of WASP-12b to its G-type star results in extreme tidal forces capable of inducing apsidal…

We report the detection of thermal emission from the hot Jupiter WASP-3b in the KS band, using a newly developed guiding scheme for the WIRC instrument at the Palomar Hale 200in telescope. Our new guiding scheme has improved the telescope…

地球与行星天体物理 · 物理学 2015-06-04 Ming Zhao , Jennifer Milburn , Travis Barman , Sasha Hinkley , Mark R. Swain , Jason Wright , John D. Monnier

We present Ks, H & J-band photometry of the very highly irradiated hot Jupiter WASP-12b using the Wide-field Infrared Camera on the Canada-France-Hawaii telescope. Our photometry brackets the secondary eclipse of WASP-12b in the Ks and…

地球与行星天体物理 · 物理学 2015-05-19 Bryce Croll , David Lafreniere , Loic Albert , Ray Jayawardhana , Jonathan J. Fortney , Norman Murray

We present H and Ks-band photometry bracketing the secondary eclipse of the hot Jupiter TrES-3b using the Wide-field Infrared Camera on the Canada-France-Hawaii Telescope. We detect the secondary eclipse of TrES-3b with a depth of…

地球与行星天体物理 · 物理学 2015-05-19 Bryce Croll , Ray Jayawardhana , Jonathan J. Fortney , Loic Albert , David Lafrenière

WASP-121b is a transiting gas giant exoplanet orbiting close to its Roche limit, with an inflated radius nearly double that of Jupiter and a dayside temperature comparable to a late M dwarf photosphere. Secondary eclipse observations…

We measure the 4.5 $\mu$m thermal emission of five transiting hot Jupiters, WASP-13b, WASP-15b, WASP-16b, WASP-62b and HAT-P-22b using channel 2 of the Infrared Array Camera (IRAC) on the {\sl Spitzer Space Telescope}. Significant…

We present the results of a ground-based search for the secondary eclipse of the 3.3 Mjup transiting planet CoRoT-2b. We performed near infrared photometry using the LIRIS instrument on the 4.2 m William Herschel Telescope, in the H and K_s…

地球与行星天体物理 · 物理学 2015-05-18 R. Alonso , H. J. Deeg , P. Kabath , M. Rabus

From its discovery, the low density transiting Neptune HAT-P-26b showed a 2.1-sigma detection drift in its spectroscopic data, while photometric data showed a weak curvature in the timing residuals that required further follow-up…

地球与行星天体物理 · 物理学 2019-08-21 C. von Essen , S. Wedemeyer , M. S. Sosa , M. Hjorth , V. Parkash , J. Freudenthal , M. Mallonn , R. G. Miculan , L. Zibecchi , S. Cellone , A. F. Torres

We report new Ks band secondary eclipse observations for the hot-Jupiters WASP-19b and WASP-43b. Using the IRIS2 infrared camera on the Anglo-Australian Telescope (AAT), we measured significant secondary eclipses for both planets, with…

地球与行星天体物理 · 物理学 2015-06-22 G. Zhou , D. D. R. Bayliss , L. Kedziora-Chudczer , G. Salter , C. G. Tinney , J. Bailey

We report detections and constraints for the near infrared Ks band secondary eclipses of seven hot-Jupiters using the IRIS2 infrared camera on the Anglo-Australian Telescope. Eclipses in the Ks band for WASP-18b and WASP-36b have been…

地球与行星天体物理 · 物理学 2015-10-28 G. Zhou , D. Bayliss , L. Kedziora-Chudczer , C. G. Tinney , J. Bailey , G. Salter , J. Rodriguez

We present z'-band secondary eclipse photometry of the highly irradiated hot Jupiter WASP-12b using ULTRACAM on the 4.2m William Herschel Telescope. We measure a decrease in flux of \delta = 0.130+/-0.013% during the passage of the planet…

地球与行星天体物理 · 物理学 2015-06-16 D. Föhring , V. S. Dhillon , Nikku Madhusudhan , T. R. Marsh , C. M. Copperwheat , S. P. Littlefair , Richard W. Wilson

Transmission spectroscopy has been successfully used from both the ground and in space to characterise the atmospheres of transiting exoplanets. This technique is challenging from the ground because ground-based spectrographs tend not to be…

地球与行星天体物理 · 物理学 2015-06-16 C. M. Copperwheat , P. J. Wheatley , J. Southworth , J. Bento , T. R. Marsh , V. S. Dhillon , J. J. Fortney , S. P. Littlefair , R. Hickman
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