TheNançay Radio Astronomy Station is operated as part of the Paris Observatory,in association with the Centre National de la Recherche Scientifique (CNRS)and partially supported by the Région Centre in FranceInternational audienceTo investigate galaxy properties as a function of their total stellar mass, we obtained 21cm HI line observations at the 100-m class Nan\c{c}ay Radio Telescope of 2839 galaxies from the Sloan Digital Sky Survey (SDSS) in the Local Volume (900<cz<12,000 km/s), dubbed the Nan\c{c}ay Interstellar Baryons Legacy Extragalactic Survey (NIBLES) sample. They were selected evenly over their entire range of absolute SDSS z-band magnitudes (-13.5 to -24 mag), which were used as a proxy for their stellar masses. Here, a first,...
Fundamental to a complete understanding of galaxy properties, formation, and evolution is a thorough...
Aims. This paper presents 828 new 21 cm neutral hydrogen line measurements carried out with the FORT...
The H I mass function (HIMF) for galaxies in the local universe is constructed from the results of t...
TheNançay Radio Astronomy Station is operated as part of the Paris Observatory,in association with t...
To investigate galaxy properties as a function of their total stellar mass, we obtained 21 cm H i li...
To investigate galaxy properties as a function of their total stellar mass, we obtained 21 cm H I li...
To investigate galaxy properties as a function of their total stellar mass, we obtained 21 cm H i li...
International audienceWe obtained Arecibo Hi line follow-up observations of 154 of the 2600 galaxies...
International audienceImproving our knowledge of the H I Universe will improve our readiness to use ...
To investigate galaxy properties as a function of their total stellar mass, we obtained 21 cm H
VizieR online Data Catalogue associated with article published in journal Astronomy & Astrophysi...
International audienceWe present a new optical luminosity-HI mass bivariate luminosity function (BLF...
To investigate the correlation between optical luminosity and Hi mass, we obtained 21cm Hi line obse...
We introduce a new photometric estimator of the HI mass fraction (M_HI/M_*) in local galaxies, which...
Fundamental to a complete understanding of galaxy properties, formation, and evolution is a thorough...
Aims. This paper presents 828 new 21 cm neutral hydrogen line measurements carried out with the FORT...
The H I mass function (HIMF) for galaxies in the local universe is constructed from the results of t...
TheNançay Radio Astronomy Station is operated as part of the Paris Observatory,in association with t...
To investigate galaxy properties as a function of their total stellar mass, we obtained 21 cm H i li...
To investigate galaxy properties as a function of their total stellar mass, we obtained 21 cm H I li...
To investigate galaxy properties as a function of their total stellar mass, we obtained 21 cm H i li...
International audienceWe obtained Arecibo Hi line follow-up observations of 154 of the 2600 galaxies...
International audienceImproving our knowledge of the H I Universe will improve our readiness to use ...
To investigate galaxy properties as a function of their total stellar mass, we obtained 21 cm H
VizieR online Data Catalogue associated with article published in journal Astronomy & Astrophysi...
International audienceWe present a new optical luminosity-HI mass bivariate luminosity function (BLF...
To investigate the correlation between optical luminosity and Hi mass, we obtained 21cm Hi line obse...
We introduce a new photometric estimator of the HI mass fraction (M_HI/M_*) in local galaxies, which...
Fundamental to a complete understanding of galaxy properties, formation, and evolution is a thorough...
Aims. This paper presents 828 new 21 cm neutral hydrogen line measurements carried out with the FORT...
The H I mass function (HIMF) for galaxies in the local universe is constructed from the results of t...