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Future high-resolution microwave background measurements hold the promise of detecting galaxy clusters throughout our Hubble volume through their Sunyaev-Zel'dovich (SZ) signature, down to a given limiting flux. The number density of galaxy…

Astrophysics · Physics 2007-05-23 Matthew R. Francis , Rachel Bean , Arthur Kosowsky

We derive physical properties of 10 submillimeter galaxies located in the CANDELS coverage of the GOODS-S field. The galaxies were first identified as submillimeter sources with the LABOCA bolometer and subsequently targeted for 870um…

Context. The XMM-XXL survey uses observations from XMM-Newton to detect clusters of galaxies over a wide range in mass and redshift. The moderate PSF of XMM-Newton means that point sources within or projected onto a cluster may not be…

We discuss the clustering properties of galaxies with signs of ongoing star formation detected by the Spitzer Space Telescope at 24mum band in the SWIRE Lockman Hole field. The sample of mid-IR-selected galaxies includes ~20,000 objects…

Cosmology and Nongalactic Astrophysics · Physics 2012-05-30 S. Starikova , S. Berta , A. Franceschini , L. Marchetti , G. Rodighiero , M. Vaccari , A. Vikhlinin

We present a stacked lensing analysis of 96 galaxy clusters selected by the thermal Sunyaev-Zel'dovich (SZ) effect in maps of the cosmic microwave background (CMB). We select foreground galaxy clusters with a $5\sigma$-level SZ threshold in…

We report our analysis of MACS J0717.5+3745 using 140 and 268 GHz Bolocam data collected at the Caltech Submillimeter Observatory. We detect extended Sunyaev-Zel'dovich (SZ) effect signal at high significance in both Bolocam bands, and we…

We present results from Submillimeter Array (SMA) 860-micron sub-arcsec astrometry and multiwavelength observations of the brightest millimeter (S_1.1mm = 8.4 mJy) source, SSA22-AzTEC1, found near the core of the SSA22 protocluster that is…

We have conducted a submillimetre mapping survey of faint, gravitationally lensed sources, where we have targeted twelve galaxy clusters and additionally the NTT Deep Field. The total area surveyed is 71.5 arcmin^2 in the image plane;…

Astrophysics · Physics 2009-11-13 K. K. Knudsen , P. P. van der Werf , J. -P. Kneib

We have undertaken a deep (sigma~1.1 mJy) 1.1-mm survey of the z=0.54 cluster MS 0451.6-0305 using the AzTEC camera on the James Clerk Maxwell Telescope. We detect 36 sources with S/N>3.5 in the central 0.10 deg^2 and present the AzTEC map,…

We investigate the contamination of the Sunyaev--Zel'dovich (SZ) effect for six galaxy clusters, A1689, A1995, A2142, A2163, A2261, and A2390, observed by the Y. T. Lee Array for Microwave Background Anisotropy during 2007. With the range…

Abridged] We present here new results on the space density of rich, optically-selected, clusters of galaxies at low redshift (z<0.15). These results are based on the application of the matched filter cluster-finding algorithm to 1067 deg2…

Astrophysics · Physics 2009-10-31 D. A. Bramel , R. C. Nichol , A. C. Pope

(abridged) We present the results of a redshift survey of intercluster galaxies in the central region of the Shapley Concentration supercluster, aimed at determining the distribution of galaxies in between obvious overdensities. Our sample…

Astrophysics · Physics 2009-10-31 S. Bardelli , E. Zucca , G. Zamorani , L. Moscardini , R. Scaramella

We present results from JCMT sub-mm observations of sources selected from the {\sl ISO} FIRBACK (Far-IR BACKground) survey, along with UKIRT near-IR imaging of a sub-sample. This gives valuable insight into the brightest $\sim$10% of…

Astrophysics · Physics 2009-11-07 A. Sajina , C. Borys , S. Chapman , H. Dole , M. Halpern , G. Lagache , J. -L. Puget , D. Scott

Determing the nature of the bright sub-mm sources and their role in the process of galaxy formation is likely to be a major focus of extra-galactic research over the next few years. In particular, we would like to know if these sources are…

Astrophysics · Physics 2007-05-23 James S. Dunlop

We present a catalog of 500 galaxy cluster candidates in the SPT-Deep field: a 100 deg$^2$ field that combines data from the SPT-3G and SPTpol surveys to reach noise levels of 3.0, 2.2, and 9.0 $\mu$K-arcmin at 95, 150, and 220 GHz,…

Cosmology and Nongalactic Astrophysics · Physics 2025-03-24 K. Kornoelje , L. E. Bleem , E. S. Rykoff , T. M. C. Abbott , P. A. R. Ade , M. Aguena , O. Alves , A. J. Anderson , F. Andrade-Oliveira , B. Ansarinejad , M. Archipley , M. L. N. Ashby , J. E. Austermann , D. Bacon , L. Balkenhol , J. A. Beall , K. Benabed , A. N. Bender , B. A. Benson , F. Bianchini , S. Bocquet , F. R. Bouchet , D. Brooks , D. L. Burke , M. Calzadilla , E. Camphuis , J. E. Carlstrom , A. Carnero Rosell , J. Carretero , C. L. Chang , P. Chaubal , H. C. Chiang , P. M. Chichura , A. Chokshi , T. -L. Chou , R. Citron , A. Coerver , C. Corbett Moran , M. Costanzi , T. M. Crawford , A. T. Crites , L. N. da Costa , C. Daley , T. de Haan , J. De Vicente , S. Desai , K. R. Dibert , M. A. Dobbs , P. Doel , M. Doohan , A. Doussot , D. Dutcher , W. Everett , S. Everett , C. Feng , K. R. Ferguson , I. Ferrero , K. Fichman , B. Flaugher , B. Floyd , A. Foster , D. Friedel , J. Frieman , S. Galli , J. Gallicchio , A. E. Gambrel , J. Garc'ia-Bellido , R. W. Gardner , R. Gassis , M. Gatti , F. Ge , E. M. George , G. Giannini , N. Goeckner-Wald , S. Grandis , D. Gruen , R. A. Gruendl , R. Gualtieri , F. Guidi , Guillaume Mahler , S. Guns , N. Gupta , G. Gutierrez , N. W. Halverson , S. R. Hinton , E. Hivon , G. P. Holder , D. L. Hollowood , W. L. Holzapfel , K. Honscheid , J. C. Hood , J. D. Hrubes , A. Hryciuk , N. Huang , J. Hubmayr , K. D. Irwin , J. Mena-Fernández , D. J. James , F. Kéruzoré , A. R. Khalife , M. Klein , L. Knox , M. Korman , K. Kuehn , C. -L. Kuo , O. Lahav , A. T. Lee , S. Lee , K. Levy , D. Li , M. Lima , A. E. Lowitz , A. Lowitz , C. Lu , A. Maniyar , J. L. Marshal , J. L. Marshall , E. S. Martsen , Matthew B. Bayliss , M. McDonald , J. J. McMahon , F. Menanteau , M. Millea , R. Miquel , J. J. Mohr , J. Montgomery , J. Myles , Y. Nakato , T. Natoli , J. P. Nibarger , G. I. Noble , V. Novosad , R. L. C. Ogando , Y. Omori , A. Ouellette , S. Padin , Z. Pan , S. Patil , M. E. S. Pereira , K. A. Phadke , A. Pieres , A. A. Plazas Malag'on , A. W. Pollak , K. Prabhu , C. Pryke , W. Quan , S. Raghunathan , M. Rahimi , A. Rahlin , C. L. Reichardt , M. Rodr'iguez-Monroy , A. K. Romer , M. Rouble , J. E. Ruhl , B. R. Saliwanchik , L. Salvati , S. Samuroff , E. Sanchez , A. Saro , K. K. Schaffer , E. Schiappucci , T. Schrabback , I. Sevilla-Noarbe , C. Sievers , G. Smecher , M. Smith , J. A. Sobrin , T. Somboonpanyakul , B. Stalder , A. A. Stark , E. Suchyta , M. E. C. Swanson , C. Tandoi , G. Tarle , B. Thorne , C. To , C. Trendafilova , C. Tucker , C. Umilta , T. Veach , J. D. Vieira , M. Vincenzi , A. Vitrier , Y. Wan , G. Wang , N. Weaverdyck , J. Weller , N. Whitehorn , P. Wiseman , W. L. K. Wu , V. Yefremenko , M. R. Young , J. A. Zebrowski , Y. Zhang

Interferometric observations of the Sunyaev-Zel'dovich Effect (SZE) toward clusters of galaxies provide sensitive cosmological probes. We present results from 1 cm observations (at BIMA and OVRO) of a large, intermediate redshift cluster…

We present observations of the Sunyaev-Zel'dovich effect (SZE) in the Bullet cluster (1E 0657--56) using the APEX-SZ instrument at 150 GHz with a resolution of 1 arcmin. The main results are maps of the SZE in this massive, merging galaxy…

We present the first results from an on-going survey to characterize the circumgalactic medium (CGM) of the massive high-redshift galaxies detected as submillimeter galaxies (SMGs). We constructed a parent sample of 163 SMG-QSO pairs with…

Submillimetre (sub-mm) galaxies have very high infrared (IR) luminosities and are thousands of times more numerous at z~2 than local ultra-luminous IR galaxies. They therefore represent a key phase in galaxy evolution which can be missed in…

Astrophysics · Physics 2007-05-23 Alexandra Pope , Ranga-Ram Chary , Mark Dickinson , Douglas Scott
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