Showing 1–14 of 14 results
/ Date/ Name
Nov 11, 2025Euclid preparation: LXXXVII. Non-Gaussianity of 2-point statistics likelihood: Precise analysis of the matter power spectrum distributionOct 20, 2025Euclid preparation: The flat-sky approximation for the clustering of Euclid's photometric galaxiesJun 10, 2025Euclid preparation: The NISP spectroscopy channel, on ground performance and calibrationMay 7, 2025Euclid preparation. The impact of redshift interlopers on the two-point correlation function analysisMar 19, 2025Euclid Quick Data Release (Q1), A first look at the fraction of bars in massive galaxies at $z<1$Mar 19, 2025Euclid Quick Data Release (Q1): First visual morphology catalogueJun 17, 2014A comparison of the morphological properties between local and z~1 infrared luminous galaxies. Are local and high-z (U)LIRGs different?Jan 3, 2014Is There a Maximum Star Formation Rate in High-Redshift Galaxies?May 16, 2013A statistical relation between the X-ray spectral index and Eddington ratio of active galactic nuclei in deep surveysAug 30, 2011Dissecting Photometric redshift for Active Galactic Nuclei using XMM- and Chandra-COSMOS samplesOct 3, 2008Chasing highly obscured QSOs in the COSMOS fieldAug 20, 2008Relation Between Stellar Mass and Star Formation Activity in GalaxiesMay 16, 2007Evolution of the Frequency of Luminous (\geq L_V*) Close Galaxy Pairs at z < 1.2 in the COSMOS FieldDec 12, 2006The XMM-Newton wide-field survey in the COSMOS field: I. Survey description