output
20022009
most citedThe Cosmic Infrared Background Resolved by Spitzer. Contributions of Mid-Infrared Galaxies to the Far-Infrared Background

516 citations

Showing 2009Show all

13 papers · 1 filter

astro-ph.CO200921 cited

Multi-wavelength properties of Spitzer-selected starbursts at z~2

N. Fiolet, A. Omont, M. Polletta +17

A complete sample of 33 sources believed to be starbursts ("5.8micron-peakers") was selected in the (0.5 sq. deg.) J1046+56 field with selection criteria F_(24micron)>400muJy, the…

astro-ph.SR200986 cited

Solar-like oscillations with low amplitude in the CoRoT target HD 181906

R. A. Garcia, C. Regulo, R. Samadi +23

Context: The F8 star HD 181906 (effective temperature ~6300K) was observed for 156 days by the CoRoT satellite during the first long run in the centre direction. Analysis of the da…

astro-ph.CO20096 cited

Simulating the impact of dust cooling on the statistical properties of the intracluster medium

E. Pointecouteau, A. Da Silva, A. Catalano +4

From the first stages of star and galaxy formation, non-gravitational processes such as ram pressure stripping, SNs, galactic winds, AGNs, galaxy-galaxy mergers, etc... lead to the…

astro-ph.SR200971 cited

Solar-like oscillations in a massive star

K. Belkacem, R. Samadi, M. -J. Goupil +15

Seismology of stars provides insight into the physical mechanisms taking place in their interior, with modes of oscillation probing different layers. Low-amplitude acoustic oscilla…

astro-ph.SR20092 cited

HD 50844: the new look of Delta Sct stars from CoRoT space photometry

E. Poretti, E. Michel, R. Garrido +21

It has also been suggested that the detection of a wealth of very low amplitude modes in Delta Sct stars was only a matter of signal--to--noise ratio. Access to this treasure, impo…

astro-ph.SR2009187 cited

Radius determination of solar-type stars using asteroseismology: What to expect from the Kepler mission

D. Stello, W. J. Chaplin, H. Bruntt +22

For distant stars, as observed by the NASA Kepler satellite, parallax information is currently of fairly low quality and is not complete. This limits the precision with which the a…