Showing 1–18 of 18 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 catalogueFeb 28, 2025COSMOS Spectroscopic Redshift Compilation (First Data Release): 488k Redshifts Encompassing Two Decades of SpectroscopyFeb 28, 2017A Herschel Space Observatory Spectral Line Survey of Local Luminous Infrared Galaxies from 194 to 671 MicronsJun 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 samplesApr 6, 2010The Great Observatories All-Sky LIRG Survey: Comparison of Ultraviolet and Far-Infrared PropertiesOct 3, 2008Chasing highly obscured QSOs in the COSMOS fieldAug 20, 2008Relation Between Stellar Mass and Star Formation Activity in GalaxiesJul 23, 2007Tracing PAHs and Warm Dust Emission in the Seyfert Galaxy NGC 1068May 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