We present spectroscopic observations with the 3.6m ESO telescope of two emission-line galaxies, J2104-0035 and J0113+0052, selected from the Data Release 4 (DR4) of the Sloan Digital Sky Survey (SDSS). From our data we determine the oxygen abundance of these systems to be respectively 12+logO/H = 7.26+/-0.03 and 7.17+/-0.09, making them the two most metal-deficient galaxies found thus far in the SDSS and placing them among the five most metal-deficient emission-line galaxies ever discovered. Their oxygen abundances are close to those of the two most metal-deficient emission-line galaxies known, SBS0335-052W with 12+logO/H = 7.12+/-0.03 and I Zw 18 with 12+logO/H = 7.17+/-0.01
We present chemical abundances and radial velocities of six H II regions in the extremely metal-poor...
International audienceAims:The goal of this study is to measure parameters of the integrated H I emi...
Context. The most metal-poor stars in the Milky Way witnessed the early phases of formation of the G...
We present spectroscopic observations with the 3.6 m ESO telescope of two emission-line galaxies, J2...
International audienceWe present 6.5-m MMT and 3.5 m APO spectrophotometry of 69 H ii regions in 42 ...
We report the discovery of eight new extremely metal poor galaxies [XMPGs; 12+log(O/H) lt;7.65...
We present a spectroscopic study of eight extremely low-metallicity candidate emission-line galaxies...
We present a spectroscopic study of metal-deficient dwarf galaxy candidates, selected from the SDSS ...
International audienceWe have derived element abundances in 310 emission-line galaxies from the Earl...
We have re-evaluated empirical expressions for the abundance determination of N, O, Ne, S, Cl, Ar an...
We present 3.6 m ESO telescope spectroscopic observations of the system of the two blue compact dwa...
We present new MMT spectroscopic observations of four dwarf galaxies represen-tative of a larger sam...
We present H I spectral-line imaging of the extremely metal-poor galaxy DDO 68. This system has a ne...
Aims: The purpose of this work is to make available new gas-phase oxygen abundance measurements for ...
We present a sample of low-redshift (z < 0.133) candidates for extremely low-metallicity star-formi...
We present chemical abundances and radial velocities of six H II regions in the extremely metal-poor...
International audienceAims:The goal of this study is to measure parameters of the integrated H I emi...
Context. The most metal-poor stars in the Milky Way witnessed the early phases of formation of the G...
We present spectroscopic observations with the 3.6 m ESO telescope of two emission-line galaxies, J2...
International audienceWe present 6.5-m MMT and 3.5 m APO spectrophotometry of 69 H ii regions in 42 ...
We report the discovery of eight new extremely metal poor galaxies [XMPGs; 12+log(O/H) lt;7.65...
We present a spectroscopic study of eight extremely low-metallicity candidate emission-line galaxies...
We present a spectroscopic study of metal-deficient dwarf galaxy candidates, selected from the SDSS ...
International audienceWe have derived element abundances in 310 emission-line galaxies from the Earl...
We have re-evaluated empirical expressions for the abundance determination of N, O, Ne, S, Cl, Ar an...
We present 3.6 m ESO telescope spectroscopic observations of the system of the two blue compact dwa...
We present new MMT spectroscopic observations of four dwarf galaxies represen-tative of a larger sam...
We present H I spectral-line imaging of the extremely metal-poor galaxy DDO 68. This system has a ne...
Aims: The purpose of this work is to make available new gas-phase oxygen abundance measurements for ...
We present a sample of low-redshift (z < 0.133) candidates for extremely low-metallicity star-formi...
We present chemical abundances and radial velocities of six H II regions in the extremely metal-poor...
International audienceAims:The goal of this study is to measure parameters of the integrated H I emi...
Context. The most metal-poor stars in the Milky Way witnessed the early phases of formation of the G...