2XLSSd J022258.4-040709 , the SIMBAD biblio

2XLSSd J022258.4-040709 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST00:55:59


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Title First 3 Authors
2006MNRAS.365..915A 1 10 40 The Butcher-Oemler effect at z∼ 0.35: a change in perspective. ANDREON S., QUINTANA H., TAJER M., et al.
2010MNRAS.401..294S viz 15       D               1 471 28 Optical identification of XMM sources in the Canada-France-Hawaii telescope legacy survey. STALIN C.S., PETITJEAN P., SRIANAND R., et al.
2011A&A...526A..18A 15       D               1 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.
2012MNRAS.423.3561C viz 15       D               1 424 44 The cosmological analysis of X-ray cluster surveys – II. Application of the CR–HR method to the XMM archive. CLERC N., SADIBEKOVA T., PIERRE M., et al.
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.
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.
2018A&A...620A..15G viz 11 8 The XXL Survey. XXX. Characterisation of the XLSSsC N01 supercluster and analysis of the galaxy stellar populations. GUGLIELMO V., POGGIANTI B.M., VULCANI B., 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.
2021A&A...652A..12K viz 17       D               1 1564 14 The X-CLASS survey: A catalogue of 1646 X-ray-selected galaxy clusters up to z ∼ 1.5. KOULOURIDIS E., CLERC N., SADIBEKOVA T., et al.

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