We present a spectroscopic study of eight extremely low-metallicity candidate emission-line galaxies with oxygen abundances possibly below 12 + log O/H = 7.35. These galaxies were selected from data release 10 of the Sloan Digital Sky Survey/Baryon Oscillation Spectroscopic Survey (SDSS/BOSS DR10). We will call these extremely metal-deficient (XMD) galaxies. The electron temperature-sensitive emission line [O ii
We present a sample of low-redshift (z < 0.133) candidates for extremely low-metallicity star-formi...
International audienceUltraviolet (UV) observations of local star-forming galaxies have begun to est...
The goal of this study is to measure parameters of the integrated HI emission for twenty-two dwarf g...
We present a spectroscopic study of metal-deficient dwarf galaxy candidates, selected from the SDSS ...
We report the discovery of eight new extremely metal poor galaxies [XMPGs; 12+log(O/H) lt;7.65...
We present spectroscopic observations with the 3.6m ESO telescope of two emission-line galaxies, J21...
International audienceWe present 6.5-m MMT and 3.5 m APO spectrophotometry of 69 H ii regions in 42 ...
We present spectroscopic observations with the 3.6 m ESO telescope of two emission-line galaxies, J2...
Context. Extremely metal-deficient [ 12 + log(O/H) $\la$ 7.6] emission-line galaxies in the nearby ...
We have re-evaluated empirical expressions for the abundance determination of N, O, Ne, S, Cl, Ar an...
We have derived element abundances in 310 emission-line galaxies from the Early Data Release of the ...
International audienceAims:The goal of this study is to measure parameters of the integrated H I emi...
We demonstrate a successful strategy for identifying extremely metal-poor galaxies. Our preliminary ...
We summarize the progress in identifying and observational study of extremely metal-deficient (...
Using deep narrow-band (NB) imaging and optical spectroscopy from the Keck telescope and MMT, we ide...
We present a sample of low-redshift (z < 0.133) candidates for extremely low-metallicity star-formi...
International audienceUltraviolet (UV) observations of local star-forming galaxies have begun to est...
The goal of this study is to measure parameters of the integrated HI emission for twenty-two dwarf g...
We present a spectroscopic study of metal-deficient dwarf galaxy candidates, selected from the SDSS ...
We report the discovery of eight new extremely metal poor galaxies [XMPGs; 12+log(O/H) lt;7.65...
We present spectroscopic observations with the 3.6m ESO telescope of two emission-line galaxies, J21...
International audienceWe present 6.5-m MMT and 3.5 m APO spectrophotometry of 69 H ii regions in 42 ...
We present spectroscopic observations with the 3.6 m ESO telescope of two emission-line galaxies, J2...
Context. Extremely metal-deficient [ 12 + log(O/H) $\la$ 7.6] emission-line galaxies in the nearby ...
We have re-evaluated empirical expressions for the abundance determination of N, O, Ne, S, Cl, Ar an...
We have derived element abundances in 310 emission-line galaxies from the Early Data Release of the ...
International audienceAims:The goal of this study is to measure parameters of the integrated H I emi...
We demonstrate a successful strategy for identifying extremely metal-poor galaxies. Our preliminary ...
We summarize the progress in identifying and observational study of extremely metal-deficient (...
Using deep narrow-band (NB) imaging and optical spectroscopy from the Keck telescope and MMT, we ide...
We present a sample of low-redshift (z < 0.133) candidates for extremely low-metallicity star-formi...
International audienceUltraviolet (UV) observations of local star-forming galaxies have begun to est...
The goal of this study is to measure parameters of the integrated HI emission for twenty-two dwarf g...