Z. Butcher
YOU?
Author Swipe
View article: Searching in HI for Massive Low Surface Brightness Galaxies: Samples from HyperLeda and the UGC
Searching in HI for Massive Low Surface Brightness Galaxies: Samples from HyperLeda and the UGC Open
A search has been made for 21 cm HI line emission in a total of 350 unique galaxies from two samples whose optical properties indicate they may be massive The first consists of 241 low surface brightness (LSB) galaxies of morphological typ…
View article: Searching in H i for Massive Low Surface Brightness Galaxies: Samples from HyperLeda and the UGC
Searching in H i for Massive Low Surface Brightness Galaxies: Samples from HyperLeda and the UGC Open
A search has been made for 21 cm H i line emission in a total of 350 unique galaxies from two samples whose optical properties indicate they may be massive. The first consists of 241 low surface brightness (LSB) galaxies of morphological t…
View article: The NIBLES bivariate luminosity–H I mass distribution function revised using Arecibo follow-up observations
The NIBLES bivariate luminosity–H I mass distribution function revised using Arecibo follow-up observations Open
We present a modified optical luminosity–H I mass bivariate luminosity function based on H I line observations from the Nançay Interstellar Baryons Legacy Extragalactic Survey (NIBLES), including data from our new, four times more sensitiv…
View article: The Bivariate Luminosity-HI Distribution Function of Galaxies
The Bivariate Luminosity-HI Distribution Function of Galaxies Open
To investigate the correlation between optical luminosity and Hi mass, we obtained 21cm Hi line observations from the 100m class Nanç ay Radio Telescope of 2600 galaxies in the local universe (900 ≤ cz ≤ 12000 km s−1 ). We first present th…
View article: hiss, a new tool for H i stacking: application to NIBLES spectra
hiss, a new tool for H i stacking: application to NIBLES spectra Open
H i stacking has proven to be a highly effective tool to statistically analyse average H i properties for samples of galaxies which may or may not be directly detected. With the plethora of H i data expected from the various upcoming H i s…
View article: Bivariate luminosity-HI mass distribution function of galaxies based on the NIBLES survey
Bivariate luminosity-HI mass distribution function of galaxies based on the NIBLES survey Open
We present a new optical luminosity-HI mass bivariate luminosity function (BLF) based on HI line observations from the Nancay Interstellar Baryons Legacy Extragalactic Survey (NIBLES). NIBLES sources lie within the local universe (900 $\le…
View article: NIBLES - an HI census of stellar mass selected SDSS galaxies: II. Arecibo follow-up HI observations
NIBLES - an HI census of stellar mass selected SDSS galaxies: II. Arecibo follow-up HI observations Open
We obtained Arecibo HI line follow-up observations of 154 of the 2600 galaxies in the Nançay Interstellar Baryons Legacy Extragalactic Survey (NIBLES) sample. These observations are on average four times more sensitive than the original ob…
View article: NIBLES – an HI census of stellar mass selected SDSS galaxies
NIBLES – an HI census of stellar mass selected SDSS galaxies Open
International audience
View article: NIBLES: an H I census of stellar mass selected SDSS galaxies
NIBLES: an H I census of stellar mass selected SDSS galaxies Open
To 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 …