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Related papers: The Herschel ATLAS

200 papers

The Herschel Satellite and the Atacama Large Millimeter Array (ALMA) are two very large sub-mm and far infrared (FIR) astronomy projects that are expected to come into operation in this decade. This report contains descriptions of these…

Astrophysics · Physics 2007-05-23 T. L. Wilson , D. Elbaz , eds

The Herschel Space Observatory was the fourth cornerstone mission in the European Space Agency (ESA) science programme with excellent broad band imaging capabilities in the sub-mm and far-infrared part of the spectrum. Although the…

The DustPedia project is capitalising on the legacy of the Herschel Space Observatory, using cutting-edge modelling techniques to study dust in the 875 DustPedia galaxies - representing the vast majority of extended galaxies within 3000 km…

{Submillimetre galaxies (SMGs) are excellent background sources for magnification-bias studies, but the limited sky coverage in the submillimetre (sub-mm) band constrains their statistical power. Beyond H-ATLAS, Herschel produced additional…

Cosmology and Nongalactic Astrophysics · Physics 2025-10-28 R. Fernandez-Fernandez , M. M. Cueli , J. González-Nuevo , L. Bonavera , D. Crespo , E. Goitia , J. M. Casas , J. A. Cano , M. Migliaccio

The European Large Area ISO Survey (ELAIS) has surveyed ~12 square degrees of the sky at 15mu and 90mu and subsets of this area at 6.75mu and 175mu using the Infrared Space Observatory (ISO). This project was the largest single open time…

Astrophysics · Physics 2007-05-23 Seb Oliver

In these proceedings I discuss various extragalactic surveys which will be undertaken over the next few years and which will be complementary to any HI and/or continuum surveys with the SKA-pathfinder telescopes. I concentrate on the…

Astrophysics · Physics 2009-06-23 Matt J. Jarvis

The results of the first extragalactic gamma-ray survey by the High Energy Stereoscopic System (H.E.S.S.) are presented. The survey comprises 2720 hours of very high-energy gamma-ray observations of the extragalactic sky, recorded with…

High Energy Astrophysical Phenomena · Physics 2025-05-01 H. E. S. S. Collaboration , F. Aharonian , F. Ait Benkhali , J. Aschersleben , H. Ashkar , M. Backes , V. Barbosa Martins , R. Batzofin , Y. Becherini , D. Berge , K. Bernlöhr , M. Böttcher , C. Boisson , J. Bolmont , M. de Bony de Lavergne , J. Borowska , M. Bouyahiaoui , F. Bradascio , R. Brose , A. Brown , F. Brun , B. Bruno , T. Bulik , C. Burger-Scheidlin , T. Bylund , S. Casanova , J. Celic , M. Cerruti , T. Chand , S. Chandra , A. Chen , J. Chibueze , O. Chibueze , G. Cotter , P. Cristofari , J. Damascene Mbarubucyeye , I. D. Davids , J. Devin , J. Djuvsland , A. Dmytriiev , K. Egberts , S. Einecke , S. Fegan , G. Fontaine , S. Funk , S. Gabici , J. F. Glicenstein , J. Glombitza , P. Goswami , G. Grolleron , L. Haerer , B. Heß , J. A. Hinton , W. Hofmann , T. L. Holch , M. Holler , D. Horns , Zhiqiu Huang , M. Jamrozy , F. Jankowsky , A. Jardin-Blicq , E. Kasai , K. Katarzyński , R. Khatoon , B. Khélifi , Nu. Komin , K. Kosack , D. Kostunin , A. Kundu , R. G. Lang , S. Le Stum , A. Lemière , M. Lemoine-Goumard , J. -P. Lenain , F. Leuschner , A. Luashvili , J. Mackey , D. Malyshev , V. Marandon , G. Martí-Devesa , R. Marx , A. Mehta , A. Mitchell , R. Moderski , L. Mohrmann , A. Montanari , M. de Naurois , J. Niemiec , P. O'Brien , L. Olivera-Nieto , E. de Ona Wilhelmi , M. Ostrowski , S. Panny , M. Panter , U. Pensec , G. Pühlhofer , M. Punch , A. Quirrenbach , S. Ravikularaman , M. Regeard , A. Reimer , O. Reimer , I. Reis , H. Ren , B. Reville , F. Rieger , G. Rowell , B. Rudak , E. Ruiz-Velasco , V. Sahakian , H. Salzmann , D. A. Sanchez , A. Santangelo , M. Sasaki , J. Schäfer , F. Schüssler , J. N. S. Shapopi , A. Sharma , H. Sol , S. Spencer , Ł. Stawarz , R. Steenkamp , S. Steinmassl , C. Steppa , H. Suzuki , T. Takahashi , T. Tanaka , A. M. Taylor , R. Terrier , A. Thakur , M. Tsirou , C. van Eldik , M. Vecchi , C. Venter , J. Vink , H. J. Völk , T. Wach , S. J. Wagner , A. Wierzcholska , M. Zacharias , A. A. Zdziarski , A. Zech , N. Żywucka

SPIRE, the Spectral and Photometric Imaging Receiver, is one of three instruments to fly on ESA's Herschel Space Observatory. It contains a three-band imaging photometer operating at 250, 360 and 520 microns, and an imaging Fourier…

Data from the Herschel Space Observatory is freely available to the public but no uniformly processed catalogue of the observations has been published so far. To date, the Herschel Science Archive does not contain the exact sky coverage…

Instrumentation and Methods for Astrophysics · Physics 2016-07-13 László Dobos , Erika Varga-Verebélyi , Eva Verdugo , David Teyssier , Katrina Exter , Ivan Valtchanov , Tamás Budavári , Csaba Kiss

The number of extragalactic sources detected at very hight energy (VHE, E$>$100GeV) has dramatically increased during the past years to reach more than fifty. The High Energy Stereoscopic System (H.E.S.S.) had observed the sky for more than…

High Energy Astrophysical Phenomena · Physics 2019-08-14 D. A. Sanchez

The proposed VLA Sky Survey (VLASS) comprises two distinct S-band (2--4 GHz) surveys: (1) All-Sky covering the sky north of -40 deg with rms noise 69 microJy/beam = 1.5 K in the 2.5 arcsec beam and (2) Deep covering 10 square deg with rms…

Instrumentation and Methods for Astrophysics · Physics 2015-02-24 Jim Condon

As first data release of a pilot extragalactic HI survey with Five-hundred-meter Aperture Spherical radio Telescope (FAST),we extracted 544 extragalaxies from three-dimensional(3D) spectral data to perform interactive searching and…

Astrophysics of Galaxies · Physics 2025-04-08 Jiangang Kang , Ming Zhu , Mei Ai , Haiyang Yu , Chun Sun

Opening up a new window of millimeter-wave observations that span frequency bands in the range of 30 to 500 GHz, survey half the sky, and are both an order of magnitude deeper (about 0.5 uK-arcmin) and of higher-resolution (about 10…

We report the detection of a significant excess in the surface density of far-infrared sources from the Herschel-Astrophysical Terahertz Large Area Survey (H-ATLAS) within ~1 Mpc of the centres of 66 optically-selected clusters of galaxies…

The Balloon-borne Large-Aperture Sub-millimetre Telescope (BLAST) will operate on a Long Duration Balloon platform with large format bolometer arrays at 250, 350 and 500 microns, initially using a 2m mirror, with plans to increase to 2.5m.…

Astrophysics · Physics 2007-05-23 Douglas Scott , the BLAST Team

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

Context. In the current era of multi-wavelength and multi-messenger astronomy, international organisations are actively working on the definition of new standards for the publication of astronomical data, and substantial effort is devoted…

Instrumentation and Methods for Astrophysics · Physics 2025-10-13 Fabrizio Giordano , Yago Ascasibar , Luca Cortese , Ivan Valtchanov , Bruno Merín

The Cosmic Lens All-Sky Survey (CLASS) is an international collaborative program which has obtained high-resolution radio images of over 10000 flat-spectrum radio sources in order to create the largest and best studied statistical sample of…

We have determined the mass-density radial profiles of the first five strong gravitational lens systems discovered by the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS). We present an enhancement of the semi-linear lens…