ClG 1821+6827 , the SIMBAD biblio

ClG 1821+6827 , the SIMBAD biblio (31 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST08:11:18


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Title First 3 Authors
2003ApJS..149...29G viz 477 58 The ROSAT north ecliptic pole survey: the optical identifications. GIOIA I.M., HENRY J.P., MULLIS C.R., et al.
2004A&A...428..867G 111 T K                 25 12
RXJ1821.6+6827: A cool cluster at z=0.81 from the ROSAT NEP survey.
GIOIA I.M., WOLTER A., MULLIS C.R., et al.
2006A&A...446...97B viz 25 20 The radio luminosity function of the NEP distant cluster radio galaxies. BRANCHESI M., GIOIA I.M., FANTI C., et al.
2008MNRAS.383..102A 15       D               1 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.
2009AJ....137.4867L 5154 T   A D S   X C       134 23 48 The observations of redshift evolution in large-scale environments (ORELSE) survey. I. The survey design and first results on CL 0023+0423 at z = 0.84 and

RX
J1821
.6+6827
at z = 0.82.
LUBIN L.M., GAL R.R., LEMAUX B.C., et al.
2010ApJ...716..970L 2250     A D S   X C F     57 34 56 The origin of [O II] in post-starburst and red-sequence galaxies in high-redshift clusters. LEMAUX B.C., LUBIN L.M., SHAPLEY A., et al.
2011A&A...534A.109P viz 15       D               1 1770 422 The MCXC: a meta-catalogue of X-ray detected clusters of galaxies. PIFFARETTI R., ARNAUD M., PRATT G.W., 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.
2012ApJ...746..155R 2066       D S   X C       52 44 15 The evolution and environments of X-ray emitting active galactic nuclei in high-redshift large-scale structures. RUMBAUGH N., KOCEVSKI D.D., GAL R.R., 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.
2012MNRAS.425..477N viz 15       D               1 1763 27 γ-rays from annihilating dark matter in galaxy clusters: stacking versus single source analysis. NEZRI E., WHITE R., COMBET C., et al.
2013ApJ...763..124R 1264       D S   X C       31 22 13 The X-Ray-Optical relations for nine clusters at z = 0.7-1.1 from the ORELSE survey. RUMBAUGH N., KOCEVSKI D.D., GAL R.R., et al.
2013A&A...558A.100P 39           X         1 44 10 Multi-wavelength landscape of the young galaxy cluster RX J1257.2+4738 at z = 0.866. I. The infrared view. PINTOS-CASTRO I., SANCHEZ-PORTAL M., CEPA J., et al.
2014A&A...564A..17N 16       D               1 26 6 Kinematic analysis of a sample of X-ray luminous distant galaxy clusters. The LX - σv relation in the z > 0.6 universe. NASTASI A., BOEHRINGER H., FASSBENDER R., et al.
2015MNRAS.450.2261M viz 16       D               1 321 30 The galaxy cluster outskirts probed by Chandra. MORANDI A., SUN M., FORMAN W., et al.
2016A&A...592A.108P viz 8 ~ Multi-wavelength landscape of the young galaxy cluster RXJ 1257.2+4738 at z = 0.866. II. Morphological properties. PINTOS-CASTRO I., POVIC M., SANCHEZ-PORTAL M., et al.
2016MNRAS.463..413W 136       D     X C       3 72 2 The XMM Cluster Survey: evolution of the velocity dispersion-temperature relation over half a Hubble time. WILSON S., HILTON M., ROONEY P.J., et al.
2017MNRAS.466..496R 991       D     X         25 80 8 X-ray-emitting active galactic nuclei from z = 0.6 to 1.3 in the intermediate- and high-density environments of the ORELSE survey. RUMBAUGH N., LEMAUX B.C., TOMCZAK A., et al.
2017MNRAS.468.3322S viz 16       D               1 28168 37 CoMaLit - V. Mass forecasting with proxies: method and application to weak lensing calibrated samples. SERENO M. and ETTORI S.
2017MNRAS.472.3512T 180       D       C F     4 11 18 Glimpsing the imprint of local environment on the galaxy stellar mass function. TOMCZAK A.R., LEMAUX B.C., LUBIN L.M., et al.
2017MNRAS.472..419L 43           X         1 7 20 Chronos and KAIROS: MOSFIRE observations of post-starburst galaxies in z ∼ 1 clusters and groups. LEMAUX B.C., TOMCZAK A.R., LUBIN L.M., et al.
2017MNRAS.472..998S 951       D S   X C       22 8 11 The properties of radio galaxies and the effect of environment in large-scale structures at z ∼ 1. SHEN L., MILLER N.A., LEMAUX B.C., et al.
2018MNRAS.478.1403R 469       D     X C       11 20 6 Evaluating tests of virialization and substructure using galaxy clusters in the ORELSE survey. RUMBAUGH N., LEMAUX B.C., TOMCZAK A.R., et al.
2018ApJ...867...12R viz 16       D               1 113 3 Mass-richness relations for X-ray and SZE-selected clusters at 0.4 < z < 2.0 as seen by Spitzer at 4.5 µm. RETTURA A., CHARY R., KRICK J., et al.
2019MNRAS.484.2433S 435       D     X C       10 11 5 Possible evidence of the radio AGN quenching of neighbouring galaxies at z ∼ 1. SHEN L., TOMCZAK A.R., LEMAUX B.C., et al.
2019MNRAS.484.4695T 100       D     X         3 12 8 Conditional quenching: a detailed look at the SFR-density relation at z ∼ 0.9 from ORELSE. TOMCZAK A.R., LEMAUX B.C., LUBIN L.M., et al.
2019A&A...626A...7T viz 17       D               1 2352 1 ComPRASS: a Combined Planck-RASS catalogue of X-ray-SZ clusters. TARRIO P., MELIN J.-B. and ARNAUD M.
2019MNRAS.490.1231L 61       D     X         2 20 45 Persistence of the colour-density relation and efficient environmental quenching to z ∼ 1.4. LEMAUX B.C., TOMCZAK A.R., LUBIN L.M., et al.
2020ApJ...890..156P 17       D               1 76 ~ SZ scaling relations of galaxy groups and clusters near the North Ecliptic Pole. PRATT C.T. and BREGMAN J.N.
2020MNRAS.494.5374S 145       D     X         4 8 ~ The properties of radio and mid-infrared detected galaxies and the effect of environment on the co-evolution of AGN and star formation at z ∼ 1. SHEN L., LEMAUX B.C., LUBIN L.M., 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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