2XLSSd J022206.8-030314 , the SIMBAD biblio

2XLSSd J022206.8-030314 , the SIMBAD biblio (20 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST01:12:21

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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
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.
2010MNRAS.407.2543A 92       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.
2011MNRAS.418...14L 16       D               1 31 73 The XMM cluster survey: X-ray analysis methodology. LLOYD-DAVIES E.J., ROMER A.K., MEHRTENS N., et al.
2012MNRAS.423.1024M viz 15       D               1 505 138 The XMM Cluster Survey: optical analysis methodology and the first data release. MEHRTENS N., ROMER A.K., HILTON M., et al.
2012MNRAS.424.2086H viz 15       D               1 211 20 The XMM cluster survey: evidence for energy injection at high redshift from evolution of the X-ray luminosity-temperature relation. HILTON M., ROMER A.K., KAY S.T., et al.
2013A&A...557A..81M viz 16       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...567A..83K 16       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 16       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.
2016A&A...592A...1P viz 16       D               1 5977 212 The XXL Survey. I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programme. PIERRE M., PACAUD F., ADAMI C., et al.
2016A&A...592A...2P viz 16       D               2 117 112 The XXL Survey. II. The bright cluster sample: catalogue and luminosity function. PACAUD F., CLERC N., GILES P.A., et al.
2016A&A...592A...3G 16       D               2 108 82 The XXL Survey. III. Luminosity-temperature relation of the bright cluster sample. GILES P.A., MAUGHAN B.J., PACAUD F., et al.
2016A&A...592A..12E 16       D               1 106 73 The XXL Survey. XIII. Baryon content of the bright cluster sample. ECKERT D., ETTORI S., COUPON J., et al.
2016MNRAS.462.4141L viz 16       D               2 170 12 The XXL survey XV: evidence for dry merger driven BCG growth in XXL-100-GC X-ray clusters. LAVOIE S., WILLIS J.P., DEMOCLES J., et al.
2016MNRAS.463.1929M viz 16       D               1 174 3 The XMM Cluster Survey: the halo occupation number of BOSS galaxies in X-ray clusters. MEHRTENS N., ROMER A.K., NICHOL R.C., et al.
2018A&A...620A...5A 16       D               1 307 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.
2020ApJ...890..148U viz 17       D               1 92 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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