output
20022013
most citedObservations of the Crab Nebula with H.E.S.S

863 citations

Showing 2010Show all

39 papers · 1 filter

astro-ph.CO2010137 cited

Vibrationally Excited HCN in the Luminous Infrared Galaxy NGC 4418

Kazushi Sakamoto, Susanne Aalto, Aaron S. Evans +2

Infrared pumping and its effect on the excitation of HCN molecules can be important when using rotational lines of HCN to probe dense molecular gas in galaxy nuclei. We report the…

astro-ph.CO2010

Evolution of intermediate mass galaxies up to z~0.7 and studies of SNe Ia hosts

Myriam Rodrigues

In the first part of this manuscript, I present the results on the properties of the interstellar medium and the stellar content of galaxies at z=0.6, from a representative sample…

astro-ph.SR20104 cited

Constraints of a pulsation frequency on stellar parameters in the eclipsing spectroscopic binary system: V577 Oph

O. L. Creevey, J. Telting, J. A. Blemonte +7

We present a preliminary spectroscopic analysis of the binary system V577Oph, observed during the summer of 2007 on the 2.6m NOT telescope on La Palma. We have obtained time series…

quant-ph201028 cited

Dynamical Casimir-Polder force on a partially dressed atom near a conducting wall

Riccardo Messina, Ruggero Vasile, Roberto Passante

We study the time evolution of the Casimir-Polder force acting on a neutral atom in front of a perfectly conducting plate, when the system starts its unitary evolution from a parti…

astro-ph.EP201012 cited

Possible detection of phase changes from the non-transiting planet HD 46375b by CoRoT

P. Gaulme, M. Vannier, T. Guillot +19

The present work deals with the detection of phase changes in an exoplanetary system. HD 46375 is a solar analog known to host a non-transiting Saturn-mass exoplanet with a 3.0236…

astro-ph.EP201012 cited

Venus wind map at cloud top level with the MTR/THEMIS visible spectrometer. I. Instrumental performance and first results

P. Gaulme, F. -X Schmider, C. Grec +3

Solar light gets scattered at cloud top level in Venus' atmosphere, in the visible range, which corresponds to the altitude of 67 km. We present Doppler velocity measurements perfo…