228 citations · 1.7k across the 41 of their papers we have counts for
9 papers · 1 filter
An open-source Bayesian atmospheric radiative transfer (BART) code: III. Initialization, atmospheric profile generator, post-processing routines, and application to exoplanet WASP-43b
Jasmina Blecic, Joseph Harrington, Patricio E. Cubillos +12
This and companion papers by Harrington et al. 2021, submitted and Cubillos et al. 2021, submitted describe an open-source retrieval framework, Bayesian Atmospheric Radiative Trans…
An Open-Source Bayesian Atmospheric Radiative Transfer (BART) Code: I. Design, Tests, and Application to Exoplanet HD 189733 b
Joseph Harrington, Michael D. Himes, Patricio E. Cubillos +14
We present the open-source Bayesian Atmospheric Radiative Transfer (BART) retrieval package, which produces estimates and uncertainties for an atmosphere's thermal profile and chem…
An Open-source Bayesian Atmospheric Radiative Transfer (BART) Code: II. The Transit Radiative-transfer Module and Retrieval of HAT-P-11b
Patricio E. Cubillos, Joseph Harrington, Jasmina Blecic +9
This and companion papers by Harrington et al. and Blecic et al. present the Bayesian Atmospheric Radiative Transfer (BART) code, an open-source, open-development package to charac…
The Atmosphere and Interior Structure of HAT-P-13b from Spitzer Secondary Eclipses
Ryan A. Hardy, Joseph Harrington, Matthew R. Hardin +6
We present {\em Spitzer} secondary-eclipse observations of the hot Jupiter HAT-P-13 b in the 3.6 {\micron} and 4.5 {\micron} bands. HAT-P-13 b inhabits a two-planet system with a c…
On Correlated-noise Analyses Applied To Exoplanet Light Curves
Patricio Cubillos, Joseph Harrington, Thomas J. Loredo +3
Time-correlated noise is a significant source of uncertainty when modeling exoplanet light-curve data. A correct assessment of correlated noise is fundamental to determine the true…
Thermal Emission of WASP-14b Revealed with Three Spitzer Eclipses
Jasmina Blecic, Joseph Harrington, Nikku Madhusudhan +10
Exoplanet WASP-14b is a highly irradiated, transiting hot Jupiter. Joshi et al. calculate an equilibrium temperature Teq of 1866 K for zero albedo and reemission from the entire pl…