HSCS J022532-035509 , the SIMBAD biblio

HSCS J022532-035509 , the SIMBAD biblio (20 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST03:05:35

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2004A&A...423...75V 1 8 46 The XMM-LSS survey. First high redshift galaxy clusters: Relaxed and collapsing systems. VALTCHANOV I., PIERRE M., WILLIS J., et al.
2004MNRAS.353..353A 25 32 Galaxy evolution in clusters up to z= 1.0. ANDREON S., WILLIS J., QUINTANA H., et al.
2007MNRAS.382.1289P 16       D               1 37 140 The XMM-LSS survey: the Class 1 cluster sample over the initial 5 deg2 and its cosmological modelling. PACAUD F., PIERRE M., ADAMI C., et al.
2008MNRAS.385..695B 89       D         F     2 23 45 Combined analysis of weak lensing and X-ray blind surveys. BERGE J., PACAUD F., REFREGIER A., et al.
2010MNRAS.401..941A 53       D     X         2 21 6 Luminosity functions of XMM-LSS C1 galaxy clusters. ALSHINO A., KHOSROSHAHI H., PONMAN T., et al.
2010MNRAS.407.2543A 90       D         F     3 30 9 Evolution of the X-ray profiles of poor clusters from the XMM-LSS survey. ALSHINO A., PONMAN T., PACAUD F., et al.
2011A&A...526A..18A 15       D               2 72 57 The XMM-LSS survey: optical assessment and properties of different X-ray selected cluster classes. ADAMI C., MAZURE A., PIERRE M., et al.
2011A&A...535A...4R viz 15       D               1 225 108 Observational constraints on the redshift evolution of X-ray scaling relations of galaxy clusters out to z ∼ 1.5. REICHERT A., BOEHRINGER H., FASSBENDER R., et al.
2012A&A...543A..19R 15       D               1 35 22 Galaxy mass, cluster-centric distance and secular evolution: their role in the evolution of galaxies in clusters in the last 10 gyr. RAICHOOR A. and ANDREON S.
2013A&A...557A..81M viz 15       D               1 4209 16 Classification and environmental properties of X-ray selected point-like sources in the XMM-LSS field. MELNYK O., PLIONIS M., ELYIV A., et al.
2014A&A...566A.140G viz 15       D               1 134 22 Mining the gap: evolution of the magnitude gap in X-ray galaxy groups from the 3-square-degree XMM coverage of CFHTLS. GOZALIASL G., FINOGUENOV A., KHOSROSHAHI H.G., et al.
2014A&A...567A..83K 15       D               1 34 13 X-ray AGN in the XMM-LSS galaxy clusters: no evidence of AGN suppression. KOULOURIDIS E., PLIONIS M., MELNYK O., et al.
2014MNRAS.444.2723C 15       D               1 54 34 The XMM-LSS survey: the Class 1 cluster sample over the extended 11 deg^2 and its spatial distribution. CLERC N., ADAMI C., LIEU M., et al.
2016ApJ...816...98Z viz 16       D               1 109 31 Galaxies in X-ray selected clusters and groups in Dark Energy Survey data. I. Stellar mass growth of bright central galaxies since z∼1.2. ZHANG Y., MILLER C., McKAY T., et al.
2016MNRAS.455.3020L 16       D               1 33 16 The RedGOLD cluster detection algorithm and its cluster candidate catalogue for the CFHT-LS W1. LICITRA R., MEI S., RAICHOOR A., et al.
2018A&A...620A...5A 16       D               1 381 77 The XXL Survey. XX. The 365 cluster catalogue. ADAMI C., GILES P., KOULOURIDIS E., et al.
2018PASJ...70S..20O viz 16       D               1 1922 120 An optically-selected cluster catalog at redshift 0.1 < z < 1.1 from the Hyper Suprime-Cam Subaru Strategic Program S16A data. OGURI M., LIN Y.-T., LIN S.-C., et al.
2019MNRAS.488....1Z 16       D               1 93 ~ Galaxies in X-ray selected clusters and groups in Dark Energy Survey data - II. Hierarchical Bayesian modelling of the red-sequence galaxy luminosity function. ZHANG Y., MILLER C.J., ROONEY P., et al.
2020ApJ...890..148U viz 16       D               2 137 50 Weak-lensing analysis of X-ray-selected XXL galaxy groups and clusters with Subaru HSC data. UMETSU K., SERENO M., LIEU M., et al.
2021ApJ...911...82C viz 17       D               1 388 ~ Cosmological constraints from galaxy cluster sparsity, cluster gas mass fraction, and baryon acoustic oscillation data. CORASANITI P.-S., SERENO M. and ETTORI S.

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