2XLSSd J022738.1-031802 , the SIMBAD biblio

2XLSSd J022738.1-031802 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.7 - 2020.07.02CEST12:09:26


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Title First 3 Authors
2019ApJ...875...63M 65       D     X         2 8 ~ Weak-lensing mass calibration of ACTPol Sunyaev-Zel'dovich clusters with the Hyper Suprime-Cam Survey. MIYATAKE H., BATTAGLIA N., HILTON M., et al.
2016A&A...592A...1P viz 17       D               1 4500 113 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 17       D               2 118 67 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 17       D               2 108 33 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 61       D     X         2 23 28 The XXL Survey. XIII. Baryon content of the bright cluster sample. ECKERT D., ETTORI S., COUPON J., et al.
2016MNRAS.462.4141L viz 17       D               2 86 5 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.
2015A&A...578A..30S viz 17       D               1 169 3 GLACE survey: OSIRIS/GTC tuneable filter Hα imaging of the rich galaxy cluster Zw Cl0024.0+1652 at z=0.395. I. Survey presentation, TF data reduction techniques, and catalogue. SANCHEZ-PORTAL M., PINTOS-CASTRO I., PEREZ-MARTINEZ R., et al.
2015MNRAS.452.1171W viz 17       D               1 119 43 The XMM Cluster Survey: testing chameleon gravity using the profiles of clusters. WILCOX H., BACON D., NICHOL R.C., et al.
2014A&A...567A..83K 181       D     X C       4 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 53 29 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.
2013A&A...557A..81M viz 16       D               1 4208 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.
2012MNRAS.423.1024M viz 16       D               1 505 98 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 16       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.
2011A&A...526A..18A 16       D               2 71 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 16       D               1 225 72 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.
2010MNRAS.407.2543A 94       D         F     3 29 9 Evolution of the X-ray profiles of poor clusters from the XMM-LSS survey. ALSHINO A., PONMAN T., PACAUD F., et al.
2008MNRAS.383..102A 93       D       C       3 35 20 Scaling relations of the colour-detected cluster RzCS 052 at z = 1.016 and some other high-redshift clusters. ANDREON S., DE PROPRIS R., PUDDU E., et al.
2007MNRAS.382.1289P 16       D               1 36 96 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.
2005MNRAS.359.1250A 1 11 36 Batch discovery of nine z∼ 1 clusters using X-ray and K or R, z' images. ANDREON S., VALTCHANOV I., JONES L.R., et al.
2004A&A...423...75V 2 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.

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2020.07.02-12:09:26

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