activity
19982008
most citedWASP-3b: a strongly-irradiated transiting gas-giant planet

245 citations · 716 across the 11 of their papers we have counts for

collaborators
Showing 2008Show all

6 papers · 1 filter

astro-ph200831 cited

The unusual pre-main-sequence star V718 Per (HMW 15)

V. Grinin, H. C. Stempels, G. F. Gahm +4

The remarkable pre-main-sequence object V718 Per (HMW 15, H187) in the young cluster IC 348 periodically undergoes long-lasting eclipses caused by variable amounts of circumstellar…

astro-ph200893 cited

WASP-10b: a 3M_J, gas-giant planet transiting a late-type K star

D. J. Christian, N. P. Gibson, E. K. Simpson +37

We report the discovery of WASP-10b, a new transiting extrasolar planet (ESP) discovered by the WASP Consortium and confirmed using NOT FIES and SOPHIE radial velocity data. A 3.09…

astro-ph2008104 cited

WASP-14b: 7.3 Mj transiting planet in an eccentric orbit

Y. C. Joshi, D. Pollacco, A. Collier Cameron +38

We report the discovery of a 7.3 Mjup exoplanet WASP-14b, one of the most massive transiting exoplanets observed to date. The planet orbits the tenth-magnitude F5V star USNO-B1 111…

astro-ph200856 cited

Unveiling extremely veiled T Tauri stars

G. F. Gahm, F. M. Walter, H. C. Stempels +2

Photospheric absorption lines in classical T Tauri stars (CTTS) are weak compared to normal stars. This so-called veiling is normally identified with an excess continuous emission…

astro-ph200829 cited

The first magnetic maps of a pre-main sequence binary star system - HD 155555

N. J. Dunstone, G. A. J. Hussain, A. Collier Cameron +5

We present the first maps of the surface magnetic fields of a pre-main sequence binary system. Spectropolarimetric observations of the young, 18 Myr, HD 155555 (V824 Ara, G5IV + K0…

astro-ph200832 cited

The Pre-Main-Sequence Eclipsing Binary ASAS J052821+0338.5

H. C. Stempels, L. Hebb, K. G. Stassun +4

In this paper we present the first results of a detailed spectroscopic and photometric analysis of the V = 11.7m eclipsing binary ASAS J052821+0338.5. With the FIES spectrograph at…