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19952026
most citedOverview of the DESI Legacy Imaging Surveys

1.9k citations

Showing 2006 · astro-phShow all

14 papers · 2 filters

astro-ph2006

Asteroseismology of exoplanets-host stars: a link between the two scientific programmes of COROT

Sylvie Vauclair, Matthieu Castro, Stephane Charpinet +5

Studying the internal structure of exoplanets-host stars compared to that of similar stars without detected planets is particularly important for the understanding of planetary for…

astro-ph2006★ 13 cited

X-ray Flashes or soft Gamma-ray Bursts? The case of the likely distant XRF 040912

G. Stratta, S. Basa, N. Butler +49

In this work, we present a multi-wavelength study of XRF 040912, aimed at measuring its distance scale and the intrinsic burst properties. We performed a detailed spectral and temp…

astro-ph2006★ 40 cited

The `666' collaboration on OGLE transits: I. Accurate radius of the planets OGLE-TR-10b and OGLE-TR-56b with VLT deconvolution photometry

Frederic Pont, Claire Moutou, Michael Gillon +14

Transiting planets are essential to study the structure and evolution of extra-solar planets. For that purpose, it is important to measure precisely the radius of these planets. He…

astro-ph2006★ 56 cited

Biomarkers in disk-averaged near-UV to near-IR Earth spectra using Earthshine observations

Slim Hamdani, Luc Arnold, C. Foellmi +6

We analyse the detectability of vegetation on a global scale on Earth's surface. Considering its specific reflectance spectrum showing a sharp edge around 700 nm, vegetation can be…

astro-ph2006★ 302 cited

WASP-1b and WASP-2b: Two new transiting exoplanets detected with SuperWASP and SOPHIE

A. Collier Cameron, F. Bouchy, G. Hebrard +36

We have detected low-amplitude radial-velocity variations in two stars, USNO-B1.0 1219-0005465 (GSC 02265-00107 = WASP-1) and USNO-B1.0 0964-0543604 (GSC 00522-01199 = WASP-2). Bot…

astro-ph2006★ 36 cited

No Expanding Fireball: Resolving the Recurrent Nova RS Ophiuchi with Infrared Interferometry

J. D. Monnier, R. K. Barry, W. A. Traub +17

Following the recent outburst of the recurrent nova RS Oph on 2006 Feb 12, we measured its near-infrared size using the IOTA, Keck, and PTI Interferometers at multiple epochs. The…