SPT-CL J2040-4451 , the SIMBAD biblio

SPT-CL J2040-4451 , the SIMBAD biblio (20 results) C.D.S. - SIMBAD4 rel 1.7 - 2020.07.09CEST22:57:07


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Title First 3 Authors
2020ApJ...893...10F 100           X         2 12 ~ Constraining the mass of the emerging galaxy cluster SpARCS1049+56 at z = 1.71 with infrared weak lensing. FINNER K., JEE M.J., WEBB T., et al.
2019A&A...622A.117S 65       D     X         2 10 ~ Galaxy populations in the most distant SPT-SZ clusters. I. Environmental quenching in massive clusters at 1.4 ≤ z ≤ 1.7. STRAZZULLO V., PANNELLA M., MOHR J.J., et al.
2019ApJ...870....7K 112       D     X         3 11 ~ Spectroscopic confirmation of five galaxy clusters at z > 1.25 in the 2500 deg2 SPT-SZ survey. KHULLAR G., BLEEM L.E., BAYLISS M.B., et al.
2019ApJ...871...50B 19       D               2 63 ~ X-ray properties of SPT-selected galaxy clusters at 0.2 < z < 1.5 observed with XMM-Newton. BULBUL E., CHIU I.-N., MOHR J.J., et al.
2018ApJ...867...12R viz 18       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.
2018MNRAS.479.3563F 197       D       C F     6 42 3 The rate of Type-Ia supernovae in galaxy clusters and the delay-time distribution out to redshift 1.75. FRIEDMANN M. and MAOZ D.
2017ApJ...843...28M 105       D     X         3 15 26 The remarkable similarity of massive galaxy clusters from z ∼ 0 to z ∼ 1.9. McDONALD M., ALLEN S.W., BAYLISS M., et al.
2017ApJ...847..117J 2481 T K A D     X C       56 12 4 First weak-lensing results from See change": quantifying dark matter in the two z >= 1.5 high-redshift galaxy clusters
SPT-CL J2040-4451 and IDCS J1426+3508.
JEE M.J., KO J., PERLMUTTER S., et al.
2016A&A...593A...2A viz 281     A     X C       6 174 12 Size growth of red-sequence early-type galaxies in clusters in the last 10 Gyr. ANDREON S., DONG H. and RAICHOOR A.
2016A&ARv..24...14O 44           X         1 19 36 The realm of the galaxy protoclusters. OVERZIER R.A.
2016ApJ...817..122B 45           X         1 6 16 IDCS J1426.5+3508: the most massive galaxy cluster at z > 1.5. BRODWIN M., McDONALD M., GONZALEZ A.H., et al.
2015ApJ...814...21S 43           X         1 9 13 A multi-wavelength mass analysis of RCS2 J232727.6-020437, a ∼3x1015 M galaxy cluster at z = 0.7. SHARON K., GLADDERS M.D., MARRONE D.P., et al.
2015ApJS..216...27B viz 184       D     X C       4 701 328 Galaxy clusters discovered via the Sunyaev-Zel'dovich effect in the 2500-square-degree SPT-SZ survey. BLEEM L.E., STALDER B., DE HAAN T., et al.
2015MNRAS.450.3675S viz 17       D               1 570 26 CoMaLit - IV. Evolution and self-similarity of scaling relations with the galaxy cluster mass. SERENO M. and ETTORI S.
2014A&A...568A...5F viz 43           X         1 15 31 Galaxy population properties of the massive X-ray luminous galaxy cluster XDCP J0044.0-2033 at z = 1.58 . Red-sequence formation, massive galaxy assembly, and central star formation activity. FASSBENDER R., NASTASI A., SANTOS J.S., et al.
2014ApJ...792...45R viz 222       D     X C       5 2162 58 Optical spectroscopy and velocity dispersions of galaxy clusters from the SPT-SZ survey. RUEL J., BAZIN G., BAYLISS M., et al.
2014ApJ...794...12B 2331 T   A     X C       55 24 37
SPT-CL J2040-4451: an SZ-selected galaxy cluster at z = 1.478 with significant ongoing star formation.
BAYLISS M.B., ASHBY M.L.N., RUEL J., et al.
2013ApJ...763..127R viz 16       D               1 233 226 Galaxy clusters discovered via the Sunyaev-Zel'dovich effect in the first 720 square degrees of the South Pole Telescope survey. REICHARDT C.L., STALDER B., BLEEM L.E., et al.
2013ApJ...779..138B 43           X         1 48 113 The era of star formation in galaxy clusters. BRODWIN M., STANFORD S.A., GONZALEZ A.H., et al.
2012ApJ...761...22S viz 16       D               1 228 71 Redshifts, sample purity, and BCG positions for the galaxy cluster catalog from the first 720 square degrees of the South Pole Telescope survey. SONG J., ZENTENO A., STALDER B., et al.

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2020.07.09-22:57:07

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