Showing 1–20 of 116 results
/ Date/ Name
Jan 9, 2023On the correlation between dark matter, intracluster light and globular cluster distribution in SMACS0723Dec 13, 2021Understanding the "Feeble Giant" Crater II with tidally stretched Wave Dark MatterMar 29, 2011The Cluster Lensing and Supernova Survey with Hubble (CLASH): Strong Lensing Analysis of Abell 383 from 16-Band HST WFC3/ACS ImagingAug 10, 2010Herschel FIR counterparts of selected Ly-alpha emitters at z~2.2. Fast evolution since z~3 or missed obscured AGNs?Feb 13, 2009Near-IR Galaxy Counts and Evolution from the Wide-Field ALHAMBRA surveyFeb 15, 2012Quasi-stellar objects in the ALHAMBRA survey. I. Photometric redshift accuracy based on a 23 optical-NIR filter photometryNov 9, 2012A Census of Star-Forming Galaxies in the z~9-10 Universe based on HST+Spitzer Observations Over 19 CLASH clusters: Three Candidate z~9-10 Galaxies and Improved Constraints on the Star Formation Rate Density at z~9Feb 25, 2014Young Galaxy Candidates in the Hubble Frontier Fields. I. Abell 2744Nov 13, 2013The ALHAMBRA survey: evolution of galaxy clustering since $z \sim 1$Mar 13, 2018Unveiling the dynamical state of massive clusters through the ICL fractionApr 11, 2005The K20 survey. VII. The spectroscopic catalogue: spectral properties and evolution of the galaxy populationMay 4, 2004The K20 survey. VI. The Distribution of the Stellar Masses in Galaxies up to z~2Feb 23, 1999The redshift of the gravitationally lensed radio source PKS1830-211Jul 19, 2013The ALHAMBRA survey: Discovery of a faint QSO at z = 5.41Jul 22, 2013CLASH-VLT: The mass, velocity-anisotropy, and pseudo-phase-space density profiles of the z=0.44 galaxy cluster MACS 1206.2-0847Jan 20, 2014The ALHAMBRA survey: an empirical estimation of the cosmic variance for merger fraction studies based on close pairsApr 4, 2014The MUSIC of CLASH: predictions on the concentration-mass relationJul 18, 2001The Spatial Clustering of Distant, z~1, Early-Type GalaxiesNov 28, 2017Stellar populations of galaxies in the ALHAMBRA survey up to $z \sim 1$. II. Stellar content of quiescent galaxies within the dust-corrected stellar mass$-$colour and the $UVJ$ colour$-$colour diagramsSep 3, 2014The ALHAMBRA survey: Accurate merger fractions by PDF analysis of photometric close pairs