activity
19972023
most citedThe Transiting Exoplanet Survey Satellite

4.1k citations · 17k across the 170 of their papers we have counts for

collaborators
Showing 2011Show all

8 papers · 1 filter

astro-ph.EP2011★ 80 cited

Warm Spitzer Photometry of XO-4b, HAT-P-6b and HAT-P-8b

Kamen O. Todorov, Drake Deming, Heather A. Knutson +11

We have analyzed Warm Spitzer/IRAC observations of the secondary eclipses of three planets, XO-4b, HAT-P-6b and HAT-P-8b. We measure secondary eclipse amplitudes at 3.6μm and 4.5μm…

astro-ph.EP2011★ 2 cited

Combining Kepler and HARPS Occurrence Rates to Infer the Period-Mass-Radius Distribution of Super-Earths/Sub-Neptunes

A. Wolfgang, G. Laughlin

The ongoing High Accuracy Radial velocity Planet Search (HARPS) has found that 30-50% of GK dwarfs in the solar neighborhood host planets with sub-Neptune masses in orbits of P < 5…

astro-ph.EP2011★ 76 cited

Kepler Exoplanet Candidate Host Stars are Preferentially Metal Rich

Kevin C. Schlaufman, Gregory Laughlin

We find that Kepler exoplanet candidate (EC) host stars are preferentially metal-rich, including the low-mass stellar hosts of small-radius ECs. The last observation confirms a ten…

astro-ph.EP2011★ 140 cited

A Spitzer Transmission Spectrum for the Exoplanet GJ 436b, Evidence for Stellar Variability, and Constraints on Dayside Flux Variations

Heather A. Knutson, Nikku Madhusudhan, Nicolas B. Cowan +10

In this paper we describe a uniform analysis of eight transits and eleven secondary eclipses of the extrasolar planet GJ 436b obtained in the 3.6, 4.5, and 8.0 micron bands using t…

astro-ph.EP2011★ 17 cited

Improved Orbital Parameters and Transit Monitoring for HD 156846b

Stephen R. Kane, Andrew W. Howard, Genady Pilyavsky +10

HD 156846b is a Jovian planet in a highly eccentric orbit (e = 0.85) with a period of 359.55 days. The pericenter passage at a distance of 0.16 AU is nearly aligned to our line of…

astro-ph.EP2011★ 14 cited

Resolving the Sin(I) degeneracy in Low-Mass Multi-Planet Systems

Konstantin Batygin, Gregory Laughlin

Long-term orbital evolution of multi-planet systems under tidal dissipation often converges to a stationary state, known as the tidal fixed point. The fixed point is characterized…