most citedSpitzer Secondary Eclipses of the Dense, Modestly-irradiated, Giant Exoplanet HAT-P-20b Using Pixel-Level Decorrelation

285 citations · 327 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.EP201624 cited

Spitzer Secondary Eclipse Depths with Multiple Intrapixel Sensitivity Correction Methods: Observations of WASP-13b, WASP-15b, WASP-16b, WASP-62b, and HAT-P-22b

Brian M. Kilpatrick, Nikole K. Lewis, Tiffany Kataria +4

We measure the 4.5 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) o…

astro-ph.EP201613 cited

Spitzer Space Telescope Mid-IR Light Curves of Neptune

J. R. Stauffer, M. S. Marley, J. E. Gizis +9

We have used the Spitzer Space Telescope in February 2016 to obtain high cadence, high signal-to-noise, 17-hour duration light curves of Neptune at 3.6 and 4.5 m. The light curv…

astro-ph.EP2014285 cited

Spitzer Secondary Eclipses of the Dense, Modestly-irradiated, Giant Exoplanet HAT-P-20b Using Pixel-Level Decorrelation

Drake Deming, Heather Knutson, Joshua Kammer +13

HAT-P-20b is a giant exoplanet that orbits a metal-rich star. The planet itself has a high total density, suggesting that it may also have a high metallicity in its atmosphere. We…

astro-ph.GA20145 cited

The pros and cons of the inversion method approach to derive 3D dust emission properties of the ISM: the Hi-GAL field centred on (l,b)=(30,0)

Alessio Traficante, Roberta Paladini, Mathieu Compiegne +13

Herschel FIR continuum data obtained as part of the Hi-GAL survey have been used, together with the GLIMPSE 8 m and MIPSGAL 24 m data, to attempt the first 3D-decomposition o…