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The clustering properties of SCUBA-selected galaxies are investigated within the framework of a unifying scheme relating the formation of QSOs and spheroids. The theoretical angular correlation function is derived for different bias…

Astrophysics · Physics 2007-05-23 M. Magliocchetti , L. Moscardini , G. de Zotti , G. L. Granato , L. Danese

Various data analyses of the Cosmic Microwave Background (CMB) provide observational hints of statistical isotropy breaking. Some of these features can be studied within the framework of primordial vector fields in inflationary theories…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-28 N. Bartolo , E. Dimastrogiovanni , M. Liguori , S. Matarrese , A. Riotto

In this paper we analyze the biasing effect of point sources, either thermal Sunyaev-Zeldovich clusters or standard radio sources, on the estimated strength of the non-Gaussianity in the Cosmic Microwave Background (CMB). We show that the…

Astrophysics · Physics 2008-11-26 Daniel Babich , Elena Pierpaoli

We present an 11 X 11 arcminute map centred on the Hubble Deep Field taken at 850 microns with the SCUBA camera on the JCMT. The map has an average one-sigma sensitivity to point sources of about 2.3 mJy and thus probes the brighter end of…

Astrophysics · Physics 2017-08-23 Colin Borys , Scott Chapman , Mark Halpern , Douglas Scott

In the presence of strong clustering, low-resolution surveys measure the summed contributions of groups of sources within the beam. The counts of bright intensity peaks are therefore shifted to higher flux levels compared to the counts of…

We report cosmic microwave background (CMB) power spectrum measurements from the first 100 sq. deg. field observed by the South Pole Telescope (SPT) at 150 and 220 GHz. On angular scales where the primary CMB anisotropy is dominant, ell ~<…

We present the results of a multi-wavelength study of the 19 most significant sub-mm sources detected in the SCUBA 8-mJy survey. As described in Scott et al. (2001), this survey covers ~260 arcmin^2 using the sub-millimetre camera SCUBA, to…

Herschel and Planck are surveying the sky at unprecedented angular scales and sensitivities over large areas. But both experiments are limited by source confusion in the submillimeter. The high confusion noise in particular restricts the…

Cosmology and Nongalactic Astrophysics · Physics 2015-03-13 N. Fernandez-Conde , G. Lagache , J-L. Puget , H. Dole

We present the first results of a sub-millimeter survey of distant clusters using the new Sub-mm Common-User Bolometer Array (SCUBA) on the James Clerk Maxwell Telescope. We have mapped fields in two massive, concentrated clusters, A370 at…

Astrophysics · Physics 2009-10-30 Ian Smail , R. J. Ivison , A. W. Blain

We present maps, source lists, and number counts from the largest, unbiassed, extragalactic sub-mm survey so far undertaken with the SCUBA camera on the JCMT. Our maps cover 260 sq. arcmin, to a noise level S(850)=2.5 mJy/beam. We have…

We present measurements of a population of matched radio sources at 1.4 and 5 GHz down to a flux limit of 1.5 mJy in 7 sq. degs. of the NOAO Deep Field South. We find a significant fraction of sources with inverted spectral indices that all…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-04 Michael D. Schneider , Robert H. Becker , Willem de Vries , Richard L. White

The Atacama Cosmology Telescope has measured the angular power spectra of microwave fluctuations to arcminute scales at frequencies of 148 and 218 GHz, from three seasons of data. At small scales the fluctuations in the primordial Cosmic…

Using the 850 micron SCUBA camera on the JCMT and a scanning technique different from other sub-mm surveys, we have obtained a 125 square arcminute map centered on the Hubble Deep Field. The one-sigma sensitivity to point sources is roughly…

Astrophysics · Physics 2009-11-06 Colin Borys , Scott Chapman , Mark Halpern , Douglas Scott

The SZ effect from clusters of galaxies is a dominant source of secondary CMB anisotropy in the low-redshift universe. We present analytic predictions for the CMB power spectrum from massive halos arising from the SZ effect. Since halos are…

The presence of a dipolar statistical anisotropy in the spectrum of cosmic microwave background (CMB) fluctuations was reported by the Wilkinson Microwave Anisotropy Probe (WMAP), and has recently been confirmed in the Planck 2013 analysis…

Cosmology and Nongalactic Astrophysics · Physics 2014-04-29 Sugumi Kanno , Misao Sasaki , Takahiro Tanaka

We investigate the extent to which foreground cleaned CMB maps can be used to estimate the cosmological parameters at small scales. We use the SMICA method, a blind separation technique which works directly at the spectral level. In this…

Cosmology and Nongalactic Astrophysics · Physics 2019-04-17 C. Umiltà , J. F. Cardoso , K. Benabed , M. Le Jeune

Although the primary goal of ESA's Planck mission is to produce high resolution maps of the temperature and polarization anisotropies of the Cosmic Microwave Background (CMB), its high-sensitivity all-sky surveys of extragalactic sources at…

Astrophysics · Physics 2007-05-23 G. De Zotti , C. Burigana , M. Negrello , S. Tinti , R. Ricci , L. Silva , J. Gonzalez-Nuevo , L. Toffolatti

We present the first release of the data and compact-source catalogue for the JCMT Large Program SCUBA-2 Continuum Observations of Pre-protostellar Evolution (SCOPE). SCOPE consists of 850-um continuum observations of 1235 Planck Galactic…

Astrophysics of Galaxies · Physics 2019-03-06 D. J. Eden , Tie Liu , Kee-Tae Kim , S. -Y. Liu , K. Tatematsu , J. Di Francesco , K. Wang , Y. Wu , M. A. Thompson , G. A. Fuller , Di Li , I. Ristorcelli , Sung-ju Kang , N. Hirano , D. Johnstone , Y. Lin , J. H. He , P. M. Koch , Patricio Sanhueza , S. -L. Qin , Q. Zhang , P. F. Goldsmith , N. J. Evans , J. Yuan , C. -P. Zhang , G. J. White , Minho Choi , Chang Won Lee , L. V. Toth , S. Mairs , H. -W. Yi , M. Tang , A. Soam , N. Peretto , M. R. Samal , M. Fich , H. Parsons , J. Malinen , G. J. Bendo , A. Rivera-Ingraham , H. -L. Liu , J. Wouterloot , P. S. Li , L. Qian , J. Rawlings , M. G. Rawlings , S. Feng , B. Wang , Dalei Li , M. Liu , G. Luo , A. P. Marston , K. M. Pattle , V. -M. Pelkonen , A. J. Rigby , S. Zahorecz , G. Zhang , R. Bogner , Y. Aikawa , S. Akhter , D. Alina , G. Bell , J. -P. Bernard , A. Blain , L. Bronfman , D. -Y. Byun , S. Chapman , H. -R. Chen , M. Chen , W. -P. Chen , X. Chen , Xuepeng Chen , A. Chrysostomou , Y. -H. Chu , E. J. Chung , D. Cornu , G. Cosentino , M. R. Cunningham , K. Demyk , E. Drabek-Maunder , Y. Doi , C. Eswaraiah , E. Falgarone , O. Feher , H. Fraser , P. Friberg , G. Garay , J. X. Ge , W. K. Gear , J. Greaves , X. Guan , L. Harvey-Smith , T. Hasegawa , Y. He , C. Henkel , T. Hirota , W. Holland , A. Hughes , E. Jarken , T. -G. Ji , I. Jimenez-Serra , Miju Kang , K. S. Kawabata , Gwanjeong Kim , Jungha Kim , Jongsoo Kim , S. Kim , B. -C. Koo , Woojin Kwon , Y. -J. Kuan , K. M. Lacaille , S. -P. Lai , C. F. Lee , J. E. Lee , Y. -U. Lee , H. Li , N. Lo , J. A. P. Lopez , X. Lu , A. -R. Lyo , D. Mardones , P. McGehee , F. Meng , L. Montier , J. Montillaud , T. J. T. Moore , O. Morata , G. H. Moriarty-Schieven , S. Ohashi , S. Pak , Geumsook Park , R. Paladini , G. Pech , K. Qiu , Z. -Y. Ren , J. Richer , T. Sakai , H. Shang , H. Shinnaga , D. Stamatellos , Y. -W. Tang , A. Traficante , C. Vastel , S. Viti , A. Walsh , H. Wang , J. Wang , D. Ward-Thompson , A. Whitworth , C. D. Wilson , Y. Xu , J. Yang , Y. -L. Yuan , L. Yuan , A. Zavagno , C. Zhang , G. Zhang , H. -W. Zhang , C. Zhou , J. Zhou. L. Zhu , P. Zuo

We have used multi-frequency follow-up observations of a sample of extragalactic sources from the 9C survey at 15 GHz to make deductions about the expected source population at higher radio frequencies, such as those in the lower frequency…

Astrophysics · Physics 2008-11-26 E. M. Waldram , R. C. Bolton , G. G. Pooley , J. M. Riley

The study of Cosmic Microwave Background (CMB) anisotropies represents one of the most powerful Cosmological tools. After the great success of the two NASA's satellite missions COBE and WMAP, Planck represents the third generation of…

Astrophysics · Physics 2009-11-07 M. Sandri , F. Villa , R. Nesti , C. Burigana , M. Bersanelli , N. Mandolesi