The Herschel ATLAS

By S. Eales, L. Dunne, D. Clements, A. Cooray, G. Zotti, S. Dye, R. Ivison, M. Jarvis, G. Lagache, S. Maddox and 87 more. 2009

469 citations recorded by the source corpus.

The Herschel ATLAS is the largest open-time key project that will be carried out on the Herschel Space Observatory. It will survey 570 deg2 of the extragalactic sky, 4 times larger than all the other Herschel extragalactic surveys combined, in five far-infrared and submillimeter bands. We describe the survey, the complementary multiwavelength data sets that will be combined with the Herschel data, and the six major science programs we are undertaking. Using new models based on a previous submillimeter survey of galaxies, we present predictions of the properties of the ATLAS sources in other wave bands.

Subfields: Astronomy and Astrophysics, Computational Mechanics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/9e1e2bf74e0c6acac017c5e1d70f13b674fbcae5

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Citations in the corpus

A MEASUREMENT OF THE COSMIC MICROWAVE BACKGROUND B-MODE POLARIZATION POWER SPECTRUM AT SUB-DEGREE SCALES WITH POLARBEAR (2014, background): “5 and RA23 to overlap with quiet observations (Eales et al. 2010; quiet Collaboration 2012).”
HerMES: CANDIDATE GRAVITATIONALLY LENSED GALAXIES AND LENSING STATISTICS AT SUBMILLIMETER WAVELENGTHS (2012, methodology): “The first systematic Herschel survey for lensed SMGs was undertaken with Herschel-Astrophysical Terahertz Large Area Survey (H-ATLAS; Eales et al. (2010)) Science Demonstration Phase (SDP) data.”
EFFICIENT THREE-DIMENSIONAL NLTE DUST RADIATIVE TRANSFER WITH SKIRT (2011, methodology): “This galaxy was one of the first large edge-on galaxies to be observed with the Herschel Space Observatory as part of the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS, Eales et al. 2010) science demonstration phase observations.”
STELLAR MASSES AND STAR FORMATION RATES FOR 1 M GALAXIES FROM SDSS+WISE (2015, methodology): “Herschel-ATLAS provides PACS and SPIRE photometry over the wavelength range 100-500µm.”
Modelling the spectral energy distribution of galaxies - V. The dust and PAH emission SEDs of disk galaxies (2010, background): “…range of mass, morphology and environment for which, thanks to facilities such as GALEX, WISE, Spitzer, AKARI and Herschel (e.g. Driver et al. 2009, Eales et al. 2010, Martin 2010) integrated photometry is nowfor the first time becoming routinely available across the full UVsubmm range.3 In…”
An Extreme Protocluster of Luminous Dusty Starbursts in the Early Universe (2017, background): “…of our systematic search for ultrared DSFGs (sources whose SPIRE flux densities increase from 250 to 500 μm—Ivison et al. 2016) in the H-ATLAS survey (Eales et al. 2010), we discovered one system with exactly those characteristics, which is therefore the ideal observational model of the early…”
Planck2013 results. XXVIII. ThePlanckCatalogue of Compact Sources (2013, methodology): “We also thank Steve Eales and the H-ATLAS team (Eales et al, 2010 PASP 122 499E) for sharing their SPIRE catalogs prior to publication, allowing a comparison of flux densities between HFI and SPIRE.”
ALMA REDSHIFTS OF MILLIMETER-SELECTED GALAXIES FROM THE SPT SURVEY: THE REDSHIFT DISTRIBUTION OF DUSTY STAR-FORMING GALAXIES (2013, background): “This has changed dramatically over the past years with the advent of large area surveys from Herschel (specifically H-ATLAS and HerMES Eales et al. 2010; Oliver et al. 2010) and the South Pole Telescope (SPT-SZ, Carlstrom et al. 2011).”
The VISTA deep extragalactic observations (VIDEO) survey (2012, methodology): “The Herschel Space Observatory is now opening up our view of the Universe with both wide-field (e.g. Eales et al. 2010) and deep-field (e.g. Oliver et al. 2012) surveys, which together probe sufficient volume over a large fraction of cosmic time to determine the full spectral energy distribution…”
The Herschel Multi-tiered Extragalactic Survey: HerMES (2012, background): “…at 250, 350 and 500 µm together with a total IR (8–1000 µm) function, finding a local luminosity density of 1.3+0.2−0.2 × 108 L Mpc−3 (Vaccari et al. 2010) and showing that the 250 µm function evolves strongly to z ∼ 1 (Eales et al. 2010b), similarly to earlier studies at shorter wavelengths.”
Herschel-ATLAS: rapid evolution of dust in galaxies over the last 5 billion years (2010, methodology): “Many surveys of dust emission from 24 to 850 μm (Saunders et al. 1990; Blain et al. 1999; Le Floc’h et al. 2005; Dye et al. 2010; Eales et al. 2010b; Gruppioni et al. 2010) have noted the very strong evolution present in these bands and this is usually ascribed to a decrease in the SFR density over…”
THE HERSCHEL REFERENCE SURVEY: DUST IN EARLY-TYPE GALAXIES AND ACROSS THE HUBBLE SEQUENCE (2011, unknown): “The HRS is a study of dust in nearby galaxies, crucial for calibrating blind surveys of galaxies with Herschel at high redshifts, e.g., HerMES (Oliver et al. 2010) and the Herschel-ATLAS (H-ATLAS; Eales et al. 2010).”
Dust spectral energy distributions of nearby galaxies: an insight from the Herschel Reference Survey (2014, methodology): “Finally, Smith et al. (2012a) used a sample of galaxies selected at 250 µm from the H-ATLAS field (Eales et al. 2010).”
The Herschel census of infrared SEDs through cosmic time (2013, background): “…Oliver et al. 2012), the PACS Evolutionary Probe (PEP; Lutz et al. 2011) and the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS; Eales et al. 2010a), confirmed previous findings on the diversity of IR-luminous galaxy properties at high redshift, as well as the existence of…”
Characterization of Scuba-2 450 μm and 850 μm selected galaxies in the COSMOS field (2013, background): “Herschel has mapped hundreds of square degrees at 250–500µm(Eales et al. 2010; Oliver et al. 2012).”
HERSCHEL-ATLAS GALAXY COUNTS AND HIGH-REDSHIFT LUMINOSITY FUNCTIONS: THE FORMATION OF MASSIVE EARLY-TYPE GALAXIES (2011, methodology): “Once we replace their K−correction with ours, the LF estimates by Eales et al. (2010b) are found to be in good agreement with ours (see Fig.”