activity
20102014
most citedThe SIRIUS Mixed analog-digital ASIC developed for the LOFT LAD and WFM instruments

2 citations · 2 across the 1 of their papers we have counts for

collaborators

6 papers

astro-ph.IM2014★ 2 cited

The SIRIUS Mixed analog-digital ASIC developed for the LOFT LAD and WFM instruments

A. Cros, D. Rambaud, E. Moutaye +11

We report on the development and characterization of the low-noise, low power, mixed analog-digital SIRIUS ASICs for both the LAD and WFM X-ray instruments of LOFT. The ASICs we de…

astro-ph.IM2012

LOFT: the Large Observatory For X-ray Timing

M. Feroci, J. W. den Herder, E. Bozzo +245

The LOFT mission concept is one of four candidates selected by ESA for the M3 launch opportunity as Medium Size missions of the Cosmic Vision programme. The launch window is curren…

astro-ph.GA2010

The methanol lines and hot core of OMC2-FIR4, an intermediate-mass protostar, with Herschel-HIFI

M. Kama, C. Dominik, S. Maret +61

In contrast with numerous studies on the physical and chemical structure of low- and high-mass protostars, much less is known about their intermediate-mass counterparts, a class of…

astro-ph.SR2010

Ortho-to-para ratio of interstellar heavy water

C. Vastel, C. Ceccarelli, E. Caux +65

Despite the low elemental deuterium abundance in the Galaxy, enhanced molecular D/H ratios have been found in the environments of low-mass star forming regions, and in particular t…

astro-ph.GA2010

Nitrogen hydrides in interstellar gas: Herschel/HIFI observations towards G10.6-0.4 (W31C)

C. M. Persson, J. H. Black, J. Cernicharo +49

The HIFI instrument on board the Herschel Space Observatory has been used to observe interstellar nitrogen hydrides along the sight-line towards G10.6-0.4 in order to improve our u…

astro-ph.GA2010

Strong absorption by interstellar hydrogen fluoride: Herschel/HIFI observations of the sight-line to G10.6-0.4 (W31C)

D. A. Neufeld, P. Sonnentrucker, T. G. Phillips +45

We report the detection of strong absorption by interstellar hydrogen fluoride along the sight-line to the submillimeter continuum source G10.6-0.4 (W31C). We have used Herschel's…