An Open-source Bayesian Atmospheric Radiative Transfer (BART) Code. I. Design, Tests, and Application to Exoplanet HD 189733b

Autor: Joseph Harrington, Michael D. Himes, Patricio E. Cubillos, Jasmina Blecic, Patricio M. Rojo, Ryan C. Challener, Nate B. Lust, M. Oliver Bowman, Sarah D. Blumenthal, Ian Dobbs-Dixon, Andrew S. D. Foster, Austin J. Foster, M. R. Green, Thomas J. Loredo, Kathleen J. McIntyre, Madison M. Stemm, David C. Wright

Publikováno v: The Planetary Science Journal. 3:80

We present the open-source Bayesian Atmospheric Radiative Transfer (BART) retrieval package, which produces estimates and uncertainties for an atmosphere’s thermal profile and chemical abundances from observations. Several BART components are also

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::f60d39feab9ab3f088cb8abe5d7b6d78
https://doi.org/10.3847/psj/ac3513

A Search for Technosignatures from 14 Planetary Systems in the Kepler Field with the Green Bank Telescope at 1.15–1.73 GHz

Autor: M. Oliver Bowman, Szilard Gyalay, Donald Nguyen, Brittany E. Miles, Akshay Shinde, Adam H. Greenberg, Conor Power, Ryan S. Lynch, Jesse Santana, Rashmi Raviprasad, Pavlo Pinchuk, Callum Fisher, Namrata Ramani, Srinivas Prasad Mn, Willow McKibbin, Yashaswi Alladi, Jean-Luc Margot

Publikováno v: The Astronomical Journal, vol 155, iss 5
ASTRONOMICAL JOURNAL, vol 155, iss 5
Margot, J-L; Greenberg, AH; Pinchuk, P; Shinde, A; Alladi, Y; Prasad, SMN; et al.(2018). A Search for Technosignatures from 14 Planetary Systems in the Kepler Field with the Green Bank Telescope at 1.15-1.73GHz. ASTRONOMICAL JOURNAL, 155(5). doi: 10.3847/1538-3881/aabb03. UCLA: Retrieved from: http://www.escholarship.org/uc/item/2qf7q3f3

Analysis of Kepler mission data suggests that the Milky Way includes billions of Earth-like planets in the habitable zone of their host star. Current technology enables the detection of technosignatures emitted from a large fraction of the Galaxy. We

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4e508cbbe978cc527627c1516dd78dcd
https://escholarship.org/uc/item/2qf7q3f3

Spitzer observations of the thermal emission from WASP-43b

Autor: Jasmina Blecic, Joseph Harrington, Nikku Madhusudhan, Kevin B. Stevenson, Ryan A. Hardy, Patricio E. Cubillos, Matthew Hardin, Oliver Bowman, Sarah Nymeyer, David R. Anderson, Coel Hellier, Alexis M. S. Smith, Andrew Collier Cameron

WASP-43b is one of the closest-orbiting hot Jupiters, with a semimajor axis of a = 0.01526 +/- 0.00018 AU and a period of only 0.81 days. However, it orbits one of the coolest stars with a hot Jupiter (Tstar = 4520 +/- 120 K), giving the planet a mod

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c705bf3c630d8ad307eb27bd4424cf1b

ASPITZERFIVE-BAND ANALYSIS OF THE JUPITER-SIZED PLANET TrES-1

Autor: M. Oliver Bowman, Andrew S. D. Foster, Nikku Madhusudhan, Nate B. Lust, Ryan A. Hardy, Joseph Harrington, Patricio E. Cubillos

Publikováno v: The Astrophysical Journal. 797:42

With an equilibrium temperature of 1200 K, TrES-1 is one of the coolest hot Jupiters observed by Spitzer. It was also the first planet discovered by any transit survey and one of the first exoplanets from which thermal emission was directly observed.

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::d072c57d7d937585ff249b6edcfb899a
https://doi.org/10.1088/0004-637x/797/1/42

A Search for Technosignatures from 14 Planetary Systems in the Kepler Field with the Green Bank Telescope at 1.15–1.73 GHz.

Autor: Jean-Luc Margot, Adam H. Greenberg, Pavlo Pinchuk, Akshay Shinde, Yashaswi Alladi, Srinivas Prasad MN, M. Oliver Bowman, Callum Fisher, Szilard Gyalay, Willow McKibbin, Brittany Miles, Donald Nguyen, Conor Power, Namrata Ramani, Rashmi Raviprasad, Jesse Santana, Ryan S. Lynch

Publikováno v: Astronomical Journal; May2018, Vol. 155 Issue 5, p1-1, 1p