output
19952026
most citedDigital Twin: Enabling Technologies, Challenges and Open Research

2.9k citations

Showing 2011 · astro-ph.EPShow all

25 papers · 2 filters

astro-ph.EP2011★ 116 cited

EChO - Exoplanet Characterisation Observatory

G. Tinetti, J. P. Beaulieu, T. Henning +131

A dedicated mission to investigate exoplanetary atmospheres represents a major milestone in our quest to understand our place in the universe by placing our Solar System in context…

astro-ph.EP2011★ 59 cited

Thermal emission at 3.6-8 micron from WASP-19b: a hot Jupiter without a stratosphere orbiting an active star

D. R. Anderson, A. M. S. Smith, N. Madhusudhan +12

We report detection of thermal emission from the exoplanet WASP-19b at 3.6, 4.5, 5.8 and 8.0 micron. We used the InfraRed Array Camera on the Spitzer Space Telescope to observe two…

astro-ph.EP2011★ 48 cited

Refined physical properties of the HAT-P-13 planetary system

John Southworth, I. Bruni, L. Mancini +1

We present photometry of four transits of the planetary system HAT-P-13, obtained using defocussed telescopes. We analyse these, plus nine datasets from the literature, in order to…

astro-ph.EP2011★ 74 cited

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…

astro-ph.EP2011★ 47 cited

WASP-36b: A new transiting planet around a metal-poor G-dwarf, and an investigation into analyses based on a single transit light curve

A. M. S. Smith, D. R. Anderson, A. Collier Cameron +16

We report the discovery, from WASP and CORALIE, of a transiting exoplanet in a 1.54-d orbit. The host star, WASP-36, is a magnitude V = 12.7, metal-poor G2 dwarf (Teff = 5959 \pm 1…

astro-ph.EP2011★ 1 cited

Homogeneous studies of transiting planets: an online catalogue

John Southworth

The derived physical properties of the known transiting extrasolar planetary systems come from a variety of sources, and are calculated using a range of different methods so are no…