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Related papers: HerMES: Point source catalogues from Herschel-SPIR…

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We present 3D-Herschel, a new 0.3-350$\mu$m photometric catalog that combines deblended Herschel far-infrared (FIR) imaging with the CANDELS/3D-HST legacy fields to probe the dust-obscured universe. Using the 17-parameter fitting code…

[Abridged] We make use of a semi-analytic cosmological model that includes simple prescriptions for dust attenuation and emission to make predictions for the observable and physical properties of galaxies that may be detected by the…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-03 Sami-Matias Niemi , Rachel S. Somerville , Henry C. Ferguson , Kuang-Han Huang , Jennifer Lotz , Anton M. Koekemoer

SPIRE, the Spectral and Photometric Imaging Receiver, is the Herschel Space Observatory's submillimetre camera and spectrometer. It contains a three-band imaging photometer operating at 250, 350 and 500 {\mu}m, and an imaging Fourier…

The Spectral and Photometric Imaging Receiver (SPIRE), is the Herschel Space Observatory`s submillimetre camera and spectrometer. It contains a three-band imaging photometer operating at 250, 350 and 500 microns, and an imaging Fourier…

Instrumentation and Methods for Astrophysics · Physics 2015-05-19 M. J. Griffin , A. Abergel , A. Abreu , P. A. R. Ade , P. André , J. -L. Augueres , T. Babbedge , Y. Bae , T. Baillie , J. -P. Baluteau , M. J. Barlow , G. Bendo , D. Benielli , J. J. Bock , P. Bonhomme , D. Brisbin , C. Brockley-Blatt , M. Caldwell , C. Cara , N. Castro-Rodriguez , R. Cerulli , P. Chanial , S. Chen , E. Clark , D. L. Clements , L. Clerc , J. Coker , D. Communal , L. Conversi , P. Cox , D. Crumb , C. Cunningham , F. Daly , G. R. Davis , P. De Antoni , J. Delderfield , N. Devin , A. Di Giorgio , I. Didschuns , K. Dohlen , M. Donati , A. Dowell , C. D. Dowell , L. Duband , L. Dumaye , R. J. Emery , M. Ferlet , D. Ferrand , J. Fontignie , M. Fox , A. Franceschini , M. Frerking , T. Fulton , J. Garcia , R. Gastaud , W. K. Gear , J. Glenn , A. Goizel , D. K. Griffin , T. Grundy , S. Guest , L. Guillemet , P. C. Hargrave , M. Harwit , P. Hastings , E. Hatziminaoglou , M. Herman , B. Hinde , V. Hristov , M. Huang , P. Imhof , K. J. Isaak , U. Israelsson , R. J. Ivison , D. Jennings , B. Kiernan , K. J. King , A. E. Lange , W. Latter , G. Laurent , P. Laurent , S. J. Leeks , E. Lellouch , L. Levenson , B. Li , J. Li , J. Lilienthal , T. Lim , J. Liu , N. Lu , S. Madden , G. Mainetti , P. Marliani , D. McKay , K. Mercier , S. Molinari , H. Morris , H. Moseley , J. Mulder , M. Mur , D. A. Naylor , H. Nguyen , B. O'Halloran , S. Oliver , G. Olofsson , H. -G. Olofsson , R. Orfei , M. J. Page , I. Pain , P. Panuzzo , A. Papageorgiou , G. Parks , P. Parr-Burman , A. Pearce , C. Pearson , I. Pérez-Fournon , F. Pinsard , G. Pisano , J. Podosek , M. Pohlen , E. T. Polehampton , D. Pouliquen , D. Rigopoulou , D. Rizzo , I. G. Roseboom , H. Roussel , M. Rowan-Robinson , B. Rownd , P. Saraceno , M. Sauvage , R. Savage , G. Savini , E. Sawyer , C. Scharmberg , D. Schmitt , N. Schneider , B. Schulz , A. Schwartz , R. Shafer , D. L. Shupe , B. Sibthorpe , S. Sidher , A. Smith , A. J. Smith , D. Smith , L. Spencer , B. Stobie , R. Sudiwala , K. Sukhatme , C. Surace , J. A. Stevens , B. M. Swinyard , M. Trichas , T. Tourette , H. Triou , S. Tseng , C. Tucker , A. Turner , M. Vaccari , I. Valtchanov , L. Vigroux , E. Virique , G. Voellmer , H. Walker , R. Ward , T. Waskett , M. Weilert , R. Wesson , G. J. White , N. Whitehouse , C. D. Wilson , B. Winter , A. L. Woodcraft , G. S. Wright , C. K. Xu , A. Zavagno , M. Zemcov , L. Zhang , E. Zonca

We introduce the Serendipitous H-ATLAS-fields Observations of Radio Extragalactic Sources (SHORES) multiple pencil beam survey that observed at 2.1 GHz with the Australia Telescope Compact Array (ATCA) 29 fields in total intensity and…

The HELP project focuses on the data from ESA's Herschel mission, which covered over 1300$deg^2$ and is preparing to publish a multi-wavelength catalogue of millions of objects. Our main goal is to find the best approach to simultaneously…

We present the results of our systematic search for the reddest far-infrared (FIR) and submillimeter (sub-mm) galaxies using the data from the Herschel Multi-tiered Extragalactic Survey (HerMES) and the SCUBA2 Cosmological Legacy Survey…

Astrophysics of Galaxies · Physics 2020-07-08 Haojing Yan , Zhiyuan Ma , Jia-Sheng Huang , Lulu Fan

Cosmic magnification is due to the weak gravitational lensing of sources in the distant Universe by foreground large-scale structure leading to coherent changes in the observed number density of the background sources. Depending on the…

The properties of the dust grains (e.g., temperature and mass) can be derived from fitting far-IR SEDs (>100 micron). Only with SPIRE on Herschel has it been possible to get high spatial resolution at 200 to 500 micron that is beyond the…

The HI Parkes All-Sky Survey (HIPASS) Catalogue forms the largest uniform catalogue of HI sources compiled to date, with 4,315 sources identified purely by their HI content. The catalogue data comprise the southern region declination <+2…

We present the Herschel Bright Sources (HerBS) sample, a sample of bright, high-redshift Herschel sources detected in the 616.4 square degree H-ATLAS survey. The HerBS sample contains 209 galaxies, selected with a 500 {\mu}m flux density…

HERMES Pathfinder is an in-orbit demonstration consisting of a constellation of six 3U cubesats hosting simple but innovative X-ray/gamma-ray detectors for the monitoring of cosmic high-energy transients. HERMES-PF, funded by ASI and by the…

We present the results of a gravitational lensing analysis of the bright $\zs=2.957$ sub-millimeter galaxy (SMG), HERMES J105751.1+573027 found in {\it Herschel}/SPIRE Science Demonstration Phase data from the Herschel Multi-tiered…

We present the first results from the science demonstration phase for the Hi-GAL survey, the Herschel key-project that will map the inner Galactic Plane of the Milky Way in 5 bands. We outline our data reduction strategy and present some…

Astrophysics of Galaxies · Physics 2015-05-19 S. Molinari , B. Swinyard , J. Bally , M. Barlow , J. P. Bernard , P. Martin , T. Moore , A. Noriega-Crespo , R. Plume , L. Testi , A. Zavagno , A. Abergel , B. Ali , L. Anderson , P. André , J. P. Baluteau , C. Battersby , M. T. Beltrán , M. Benedettini , N. Billot , J. Blommaert , S. Bontemps , F. Boulanger , J. Brand , C. Brunt , M. Burton , L. Calzoletti , S. Carey , P. Caselli , R. Cesaroni , J. Cernicharo , S. Chakrabarti , A. Chrysostomou , M. Cohen , M. Compiegne , P. de Bernardis , G. de Gasperis , A. M. di Giorgio , D. Elia , F. Faustini , N. Flagey , Y. Fukui , G. A. Fuller , K. Ganga , P. Garcia-Lario , J. Glenn , P. F. Goldsmith , M. J. Griffin , M. Hoare , M. Huang , D. Ikhenaode , C. Joblin , G. Joncas , M. Juvela , J. M. Kirk , G. Lagache , J. Z. Li , T. L. Lim , S. D. Lord , M. Marengo , D. J. Marshall , S. Masi , F. Massi , M. Matsuura , V. Minier , M. A. Miville-Deschenes , L. A. Montier , L. Morgan , F. Motte , J. C. Mottram , T. G. Mueller , P. Natoli , J. Neves , L. Olmi , R. Paladini , D. Paradis , H. Parsons , N. Peretto , M. Pestalozzi , S. Pezzuto , F. Piacentini , L. Piazzo , D. Polychroni , M. Pomarès , C. C. Popescu , W. T. Reach , I. Ristorcelli , J. F. Robitaille , T. Robitaille , J. A. Rodón , A. Roy , P. Royer , D. Russeil , P. Saraceno , M. Sauvage , P. Schilke , E. Schisano , N. Schneider , F. Schuller , B. Schulz , B. Sibthorpe , H. A. Smith , M. D. Smith , L. Spinoglio , D. Stamatellos , F. Strafella , G. S. Stringfellow , E. Sturm , R. Taylor , M. A. Thompson , A. Traficante , R. J. Tuffs , G. Umana , L. Valenziano , R. Vavrek , M. Veneziani , S. Viti , C. Waelkens , D. Ward-Thompson , G. White , L. A. Wilcock , F. Wyrowski , H. W. Yorke , Q. Zhang

Deep far-infrared photometric surveys studying galaxy evolution and the nature of the cosmic infrared background are a key strength of the Herschel mission. We describe the scientific motivation for the PACS Evolutionary Probe (PEP)…

The H.E.S.S. Galactic Plane Survey (HGPS), carried out between 2004 and 2013, is the most extensive survey of our Galaxy at very-high energies that covers the southern sky. Since the first HPGS catalogue release, the new observations…

High Energy Astrophysical Phenomena · Physics 2023-08-21 Q. Remy

We present a multi-band analysis of the six Hubble Frontier Field clusters and their parallel fields, producing catalogs with measurements of source photometry and photometric redshifts. We release these catalogs to the public along with…

Astrophysics of Galaxies · Physics 2021-09-29 A. Pagul , F. J. Sánchez , I. Davidzon , B. Mobasher

A detailed analysis of Herschel-PACS observations at the North Ecliptic Pole is presented. High quality maps, covering an area of 0.44 square degrees, are produced and then used to derive potential candidate source lists. A rigorous quality…

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