activity
20032020
most citedGHASP : An Halpha kinematic survey of spiral and irregular galaxies - VI. New Halpha data cubes for 108 galaxies

177 citations · 859 across the 11 of their papers we have counts for

collaborators

10 papers

astro-ph.IM2020★ 172 cited

SPIRou: nIR velocimetry & spectropolarimetry at the CFHT

J. -F. Donati, D. Kouach, C. Moutou +63

This paper presents an overview of SPIRou, the new-generation near-infrared spectropolarimeter / precision velocimeter recently installed on the 3.6-m Canada-France-Hawaii Telescop…

astro-ph.SR2010★ 10 cited

The kinematics of the quadrupolar nebula M1-75 and the identification of its central star

M. Santander-García, P. Rodríguez-Gil, O. Hernandez +9

The link between the shaping of bipolar planetary nebulae and their central stars is still poorly understood. The kinematics and shaping of the multipolar nebula M 1-75 are hereby…

astro-ph2008★ 177 cited

GHASP : An Halpha kinematic survey of spiral and irregular galaxies - VI. New Halpha data cubes for 108 galaxies

B. Epinat, P. Amram, M. Marcelin +7

We present the Fabry-Perot observations obtained for a new set of 108 galaxies that completes the GHASP survey (Gassendi HAlpha survey of SPirals). The GHASP survey consists of 3D…

astro-ph2008

GH FaS : Galaxy H-alpha Fabry-Perot System for the WHT

O. Hernandez, K. Fathi, C. Carignan +11

GHFaS a new Fabry-Perot system, is now available at the William Herschel Telescope. It was mounted, for the first time, at the Nasmyth focus of the 4.2 meter WHT on La Palma in…

astro-ph2008★ 78 cited

H-alpha Kinematics of the SINGS Nearby Galaxies Survey. II

I. Dicaire, C. Carignan, P. Amram +8

This is the second part of an H-alpha kinematics follow-up survey of the Spitzer Infrared Nearby Galaxies Survey (SINGS) sample. The aim of this program is to shed new light on the…

astro-ph2007★ 3 cited

AMBER on the VLTI: data processing and calibration issues

Florentin Millour, Romain Petrov, Fabien Malbet +7

We present here the current performances of the AMBER / VLTI instrument for standard use and compare these with the offered modes of the instrument. We show that the instrument is…