Spectroscopic Confirmation of Three Red-sequence Selected Galaxy Clusters at z = 0.87, 1.16, and 1.21 from the SpARCS Survey

@article{Demarco2010SpectroscopicCO,
  title={Spectroscopic Confirmation of Three Red-sequence Selected Galaxy Clusters at z = 0.87, 1.16, and 1.21 from the SpARCS Survey},
  author={Ricardo Demarco and Gillian Wilson and Adam Muzzin and Mark Lacy and J. Surace and Howard K. C. Yee and Henk Hoekstra and Kris Blindert and David Gilbank},
  journal={The Astrophysical Journal},
  year={2010},
  volume={711},
  pages={1185-1197}
}
The Spitzer Adaptation of the Red-sequence Cluster Survey (SpARCS) is a z'-passband imaging survey of the 50 deg^2 Spitzer SWIRE Legacy fields, designed with the primary aim of creating the first large, homogeneously selected sample of massive clusters at z > 1. SpARCS uses an infrared adaptation of the two-filter cluster red-sequence technique. In this paper, we report Keck/LRIS spectroscopic confirmation of two new exceptionally rich galaxy clusters, SpARCS J161315+564930 at z = 0.871 ± 0.002… Expand
The Star-Formation History of BCGs to z = 1.8 from the SpARCS/SWIRE Survey: Evidence for significant in-situ star formation at high-redshift
We present the results of a MIPS-24um study of the Brightest Cluster Galaxies (BCGs) of 535 high-redshift galaxy clusters. The clusters are drawn from the Spitzer Adaptation of the Red-SequenceExpand
Candidate Clusters of Galaxies at z > 1.3 Identified in the Spitzer South Pole Telescope Deep Field Survey
We present 279 galaxy cluster candidates at z > 1.3 selected from the 94 deg^2 Spitzer South Pole Telescope Deep Field (SSDF) survey. We use a simple algorithm to select candidate high-redshiftExpand
Discovery of a Rich Cluster at z = 1.63 Using the Rest-frame 1.6 μm ''Stellar Bump Sequence'' Method
We present a new two-color algorithm, the "Stellar Bump Sequence" (SBS), that is optimized for robustly identifying candidate high-redshift galaxy clusters in combined wide-field optical andExpand
A Kinematic Approach to Assessing Environmental Effects : Star-forming Galaxies in a z ~ 0.9 SpARCS Cluster Using Spitzer 24 μm Observations
We present an infrared study of a z = 0.872 cluster, SpARCS J161314+564930, with the primary aim of distinguishing the dynamical histories of spectroscopically confirmed star-forming members toExpand
The x-ray luminous galaxy cluster population at 0.9 < z ≲ 1.6 as revealed by the XMM-Newton Distant Cluster Project*
We present the largest sample to date of spectroscopically confirmed x-ray luminous high-redshift galaxy clusters comprising 22 systems in the range as part of the XMM-Newton Distant Cluster ProjectExpand
The SCUBA-2 Cosmology Legacy Survey: Ultraluminous star-forming galaxies in a z=1.6 cluster
We analyze new SCUBA-2 submillimeter and archival SPIRE far-infrared imaging of a z = 1.62 cluster, Cl 0218.3–0510, which lies in the UKIRT Infrared Deep Sky Survey/Ultra-Deep Survey field of theExpand
An Extreme Starburst in the Core of a Rich Galaxy Cluster at z = 1.7
We have discovered an optically rich galaxy cluster at z = 1.7089 with star formation occurring in close proximity to the central galaxy. The system, SpARCS104922.6+564032.5, was detected within theExpand
The submillimetre view of massive clusters at z ∼ 0.8–1.6
We analyse 850 μm continuum observations of eight massive X-ray detected galaxy clusters at z ∼ 0.8–1.6 taken with SCUBA-2 on the James Clerk Maxwell Telescope. We find an average overdensity of 850Expand
EVIDENCE FOR THE UNIVERSALITY OF PROPERTIES OF RED-SEQUENCE GALAXIES IN X-RAY- AND RED-SEQUENCE-SELECTED CLUSTERS AT z ∼ 1
We study the slope, intercept, and scatter of the color–magnitude and color–mass relations for a sample of 10 infrared red-sequence-selected clusters at z ~ 1. The quiescent galaxies in theseExpand
Stellar mass function of cluster galaxies at z ~ 1.5: Evidence for reduced quenching efficiency at high redshift
We present the stellar mass functions (SMFs) of passive and star-forming galaxies with a limiting mass of 10 10.1 M ⊙ in four spectroscopically confirmed Spitzer Adaptation of the Red-sequenceExpand
...
1
2
3
4
5
...

References

SHOWING 1-10 OF 54 REFERENCES
SPECTROSCOPIC CONFIRMATION OF A MASSIVE RED-SEQUENCE-SELECTED GALAXY CLUSTER AT z = 1.34 IN THE SpARCS-SOUTH CLUSTER SURVEY
The Spitzer Adaptation of the Red-sequence Cluster Survey (SpARCS) is a z ′ -passband imaging survey, consisting of deep (z ′ ≃ 24 AB) observations made from both hemispheres using the CFHT 3.6m andExpand
A Keck Spectroscopic Survey of MS 1054–03 (z = 0.83): Forming the Red Sequence*
Using a magnitude-limited, spectroscopic survey of the X-ray-luminous galaxy cluster MS 1054-03, we isolate 153 cluster galaxies and measure MS 1054's redshift and velocity dispersion to be z =Expand
A VLT spectroscopic survey of RX J0152.7-1357, a forming cluster of galaxies at z = 0.837
We present the results of an extensive spectroscopic survey of RX J0152.7-1357, one of the most massive dis- tant clusters of galaxies known. Multi-object spectroscopy, carried out with FORS1 andExpand
VLT and ACS observations of RDCS J1252.9-2927: dynamical structure and galaxy populations in a massive cluster at z=1.237
We present results from an extensive spectroscopic survey, carried out with VLT FORS, and from an extensive multiwavelength imaging data set from the HST Advanced Camera for Surveys and ground-basedExpand
The Red-Sequence Cluster Survey. I. The Survey and Cluster Catalogs for Patches RCS 0926+37 and RCS 1327+29
The Red-Sequence Cluster Survey (RCS) is a ~100 deg2, two-filter imaging survey in the RC and z' filters, designed primarily to locate and characterize galaxy clusters to redshifts as high as z =Expand
An IR-selected Galaxy Cluster at z = 1.41
We report the discovery of a galaxy cluster at z = 1.41. ISCS J143809+341419 was found in the Spitzer/IRAC Shallow Survey of the Bootes field in the NOAO Deep Wide-Field Survey carried out usingExpand
The XMM Cluster Survey: A Massive Galaxy Cluster at z = 1.45
We report the discovery of XMMXCS J2215.9-1738, a massive galaxy cluster at z=1.45, which was found in the XMM Cluster Survey. The cluster candidate was initially identified as an extended X-rayExpand
JKCS 041: a colour-detected galaxy cluster at zphot ~ 1.9 with deep potential well as confirmed by X-ray data
We report the discovery of JKCS 041, a massive near-infrared selected cluster of galaxies at zphot ∼ 1.9. The cluster was originally discovered using a modified red-sequence method and also detectedExpand
An JR-Selected Galaxy Cluster at Z = 1.27
We report the discovery of a galaxy cluster at z=1.27. ClG J0848+4453 was found in a near{endash}IR field survey as a high density region of objects with very red J{minus}K colors. OpticalExpand
Galaxy clusters in the IRAC Dark Field. I. Growth of the Red Sequence
Using three newly identified galaxy clusters at z ~ 1 (photometric redshift) we measure the evolution of the galaxies within clusters from high redshift to the present day by studying the growth ofExpand
...
1
2
3
4
5
...