Showing 21–40 of 72 results
/ Date/ Name
Jan 14, 2016The ALHAMBRA survey: evolution of galaxy spectral segregationJul 25, 2017The ALHAMBRA survey: 2-D analysis of the stellar populations in massive early-type galaxies at z < 0.3Sep 24, 1998The Ultraviolet Luminosity Density of the Universe from Photometric Redshifts of Galaxies in the Hubble Deep FieldMar 9, 1998High-Redshift Galaxies: The HDF and MoreSep 15, 1997The Compared Number Density of High-Redshift Galaxies and Lyman αCloudsSep 7, 2000Morphological Number Counts and Redshift Distributions to I = 25 from the Hubble Deep Fields: Constraints on Cosmological Models from Early Type GalaxiesMay 12, 2005XMM-Newton and VLT observations of the afterglow of GRB040827Oct 12, 2005Multiband Photometry of the Blazar PKS 0537-441: A Major Active State in December 2004 - March 2005Apr 4, 2016Are LGRBs biased tracers of star formation? Clues from the host galaxies of the Swift/BAT6 complete sample of bright LGRBs. II: star formation rates and metallicities at z < 1Aug 14, 2013The ALHAMBRA survey: reliable morphological catalogue of 22,051 early- and late-type galaxiesFeb 10, 2013Lyman break and UV-selected galaxies at $z \sim 1$ I. Stellar populations from ALHAMBRA surveyJun 18, 2008The ALHAMBRA Project: A large area multi medium-band optical and NIR photometric surveyDec 18, 2008Optimal filter systems for photometric redshift estimationJan 19, 2010The ALHAMBRA photometric systemMar 31, 2008Radio Observations of the Hubble Deep Field South Region IV: Optical Properties of the Faint Radio PopulationSep 24, 1998The Gaseous Extent of Galaxies and The Origin of QSO Absorption Line SystemsDec 4, 2017High redshift galaxies in the ALHAMBRA survey: II. strengthening the evidence of bright-end excess in UV luminosity functions at 2.5 <= z <= 4.5 by PDF analysisSep 17, 2003z-ph-REM: A photometric redshift code for the REM telescopeOct 7, 2010Spectrophotometric Redshifts. A New Approach to the Reduction of Noisy Spectra and its Application to GRB090423Jun 20, 2013The ALHAMBRA Survey: Bayesian Photometric Redshifts with 23 bands for 3 squared degrees