Add to ORKGWe present the first results of an ongoing spectroscopic survey of galaxies selected in the rest-frame ultraviolet. The source catalogue was constructed from a flux-limited sample of stars, galaxies and QSOs imaged at 2000 Å with the FOCA balloon-borne camera (Milliard et al. 1992). The redshift distribution obtained for 45 galaxies spans 0<z<0.3 and a high fraction of the spectra show intense nebular emission lines and ultraviolet-optical colors considerably bluer than can be accounted for via normal Hubble sequence galaxies. From the rest-frame ultraviolet galaxy luminosity function, and adopting a normal IMF, we use the integrated UV light to our survey limit to estimate the local volume averaged star formation rate. We find a value sign...
We provide a systematic measurement of the rest-frame UV continuum slope β over a wide range in reds...
We report on the properties of a sample of ultraviolet-luminous galaxies (UVLGs) selected by matchin...
We present new results on the cosmic star formation history in the Subaru/XMM–Newton Deep Survey (SX...
We present the first results of an ongoing spectroscopic survey of galaxies selected in the rest-fra...
We present panoramic u′ and optical ground‐based imaging observations of a complete sample of low‐re...
Using a sample of galaxies from the Sloan Digital Sky Survey spectroscopic catalog with measured sta...
Using Hα spectra of 114 rest-frame UV-selected galaxies at z ~ 2, we compare inferred star formation...
We use the UV-optical color magnitude diagram in combination with spectroscopic and photometric meas...
The acquisition of deep Near-IR imaging with Wide Field Camera 3 on the Hubble Space Telescope has p...
We use deep Swift UV/Optical Telescope (UVOT) near-ultraviolet (1600A to 4000A) imaging of the Chand...
We present new results on the cosmic star formation history in the SXDS-UDS field out to z = 1.6. W...
We measure star formation rates (SFRs) of ≈50,000 optically selected galaxies in the local universe ...
We present the first measurements of the angular correlation function of galaxies selected in the fa...
We present new results on the cosmic star formation history in the Subaru/XMM-Newton Deep Survey (SX...
We provide a systematic measurement of the rest-frame UV continuum slope β over a wide range in reds...
We provide a systematic measurement of the rest-frame UV continuum slope β over a wide range in reds...
We report on the properties of a sample of ultraviolet-luminous galaxies (UVLGs) selected by matchin...
We present new results on the cosmic star formation history in the Subaru/XMM–Newton Deep Survey (SX...
We present the first results of an ongoing spectroscopic survey of galaxies selected in the rest-fra...
We present panoramic u′ and optical ground‐based imaging observations of a complete sample of low‐re...
Using a sample of galaxies from the Sloan Digital Sky Survey spectroscopic catalog with measured sta...
Using Hα spectra of 114 rest-frame UV-selected galaxies at z ~ 2, we compare inferred star formation...
We use the UV-optical color magnitude diagram in combination with spectroscopic and photometric meas...
The acquisition of deep Near-IR imaging with Wide Field Camera 3 on the Hubble Space Telescope has p...
We use deep Swift UV/Optical Telescope (UVOT) near-ultraviolet (1600A to 4000A) imaging of the Chand...
We present new results on the cosmic star formation history in the SXDS-UDS field out to z = 1.6. W...
We measure star formation rates (SFRs) of ≈50,000 optically selected galaxies in the local universe ...
We present the first measurements of the angular correlation function of galaxies selected in the fa...
We present new results on the cosmic star formation history in the Subaru/XMM-Newton Deep Survey (SX...
We provide a systematic measurement of the rest-frame UV continuum slope β over a wide range in reds...
We provide a systematic measurement of the rest-frame UV continuum slope β over a wide range in reds...
We report on the properties of a sample of ultraviolet-luminous galaxies (UVLGs) selected by matchin...
We present new results on the cosmic star formation history in the Subaru/XMM–Newton Deep Survey (SX...