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Related papers: HELP: The Herschel Extragalactic Legacy Project

200 papers

We present the Spitzer Data Fusion, a database incorporating far-ultraviolet to far-infrared flux measurements as well as photometric and spectroscopic redshifts for 4.4 million IRAC-selected sources detected over 8 extragalactic fields…

Astrophysics of Galaxies · Physics 2016-06-22 Mattia Vaccari

The Arecibo Legacy Fast ALFA (ALFALFA) Survey is a program aimed at obtaining a census of HI-bearing objects over a cosmologically significant volume of the local Universe. It will cover 7074 square degrees of the high latitude sky…

Astrophysics · Physics 2010-11-11 Riccardo Giovanelli

We review the results of HI line surveys of extragalactic sources in the local Universe. In the last two decades major efforts have been made in establishing on firm statistical grounds the properties of the HI source population, the two…

Astrophysics of Galaxies · Physics 2016-01-20 Riccardo Giovanelli , Martha P. Haynes

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…

Contribution of resolved and unresolved extragalactic point sources to the low-frequency sky spectrum is a potentially non-negligible part of the astrophysical foregrounds for cosmic dawn 21-cm experiments. The clustering of such point…

Cosmology and Nongalactic Astrophysics · Physics 2024-10-01 Shikhar Mittal , Girish Kulkarni , Dominic Anstey , Eloy de Lera Acedo

We propose a new method of pushing $Herschel$ to its faintest detection limits using universal trends in the redshift evolution of the far infrared over 24$\mu$m colours in the well-sampled GOODS-North field. An extension to other fields…

The Herschel Lensing Survey (HLS) takes advantage of gravitational lensing by massive galaxy clusters to sample a population of high-redshift galaxies which are too faint to be detected above the confusion limit of current…

We present an overview of the Space Telescope A901/2 Galaxy Evolution Survey (STAGES). STAGES is a multiwavelength project designed to probe physical drivers of galaxy evolution across a wide range of environments and luminosity. A complex…

This is the second data release (DR2) of the INvestigating Stellar Population In RElics (INSPIRE) project, comprising 21 new systems with observations completed before March 2022. For each system, we release four one-dimensional (1D)…

The distribution of stars in the Hertzsprung-Russell diagram narrates their evolutionary history and directly assesses their properties. Placing stars in this diagram however requires the knowledge of their distances and interstellar…

Solar and Stellar Astrophysics · Physics 2014-10-29 N. Castro , L. Fossati , N. Langer , S. Simón-Díaz , F. R. N. Schneider , R. G. Izzard

A detailed map of the distribution of dust at high Galactic latitudes is essential for future cosmic microwave background (CMB) polarization experiments because the dust, while diffuse, remains a significant foreground in these regions. We…

Astrophysics of Galaxies · Physics 2024-10-16 Matthew O'Callaghan , Gerry Gilmore , Kaisey S. Mandel

We use a Minimum Spanning Tree algorithm to characterize the spatial distribution of Galactic Far-IR sources and derive their clustering properties. We aim to reveal the spatial imprint of different types of star forming processes, e.g.…

To exploit synergies between the Herschel Space Observatory and next generation radio facilities, we have extended the semi-empirical extragalactic radio continuum simulation of Wilman et al. (2008) to the mid- and far-infrared. Here we…

Cosmology and Nongalactic Astrophysics · Physics 2017-03-22 R. J. Wilman , M. J. Jarvis , T. Mauch , S. Rawlings , S. Hickey

We present first results from SPICES, the Spectroscopic, Photometric, Infrared-Chosen Extragalactic Survey. SPICES is comprised of four ~30 square arcminute high Galactic latitude fields with deep BRIzJK imaging reaching depths of ~25th…

We present the High-$z$ Evolution of Large and Luminous Objects (HELLO) project, a set of $\sim\!30$ high-resolution cosmological simulations aimed to study Milky Way analogues ($M_\star\sim10^{10-11}$\,\Msun) at high redshift ($z\sim…

We present key results from the Herschel Orion Protostar Survey (HOPS): spectral energy distributions (SEDs) and model fits of 330 young stellar objects, predominantly protostars, in the Orion molecular clouds. This is the largest sample of…

New far-infrared and sub-millimeter photometry from the Herschel Space Observatory is presented for 61 nearby galaxies from the Key Insights on Nearby Galaxies: A Far-Infrared Survey with Herschel (KINGFISH) sample. The spatially-integrated…

A public release of slitless spectra, obtained with ACS/WFC and the G800L grism, is presented. Spectra were automatically extracted in a uniform way from 153 archival fields (or "associations") distributed across the two Galactic caps,…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-27 M. Kuemmel , P. Rosati , R. Fosbury , J. Haase , R. N. Hook , H. Kuntschner , M. Lombardi , A. Micol , K. K. Nilsson , F. Stoehr , J. R. Walsh

While the selection of strongly lensed galaxies with 500{\mu}m flux density S_500>100 mJy has proven to be rather straightforward (Negrello et al. 2010), for many applications it is important to analyze samples larger than the ones obtained…

SPHERE (Beuzit et al,. 2019) has now been in operation at the VLT for more than 5 years, demonstrating a high level of performance. SPHERE has produced outstanding results using a variety of operating modes, primarily in the field of direct…

Earth and Planetary Astrophysics · Physics 2020-03-16 A. Boccaletti , G. Chauvin , D. Mouillet , O. Absil , F. Allard , S. Antoniucci , J. -C. Augereau , P. Barge , A. Baruffolo , J. -L. Baudino , P. Baudoz , M. Beaulieu , M. Benisty , J. -L. Beuzit , A. Bianco , B. Biller , B. Bonavita , M. Bonnefoy , S. Bos , J. -C. Bouret , W. Brandner , N. Buchschache , B. Carry , F. Cantalloube , E. Cascone , A. Carlotti , B. Charnay , A. Chiavassa , E. Choquet , Y. Clenet , A. Crida , J. De Boer , V. De Caprio , S. Desidera , J. -M. Desert , J. -B. Delisle , P. Delorme , K. Dohlen , D. Doelman , C. Dominik , V. D Orazi , C. Dougados , S. Doute , D. Fedele , M. Feldt , F. Ferreira , C. Fontanive , T. Fusco , R. Galicher , A. Garufi , E. Gendron , A. Ghedina , C. Ginski , J. -F. Gonzalez , D. Gratadour , R. Gratton , T. Guillot , S. Haffert , J. Hagelberg , T. Henning , E. Huby , M. Janson , I. Kamp , C. Keller , M. Kenworthy , P. Kervella , Q. Kral , J. Kuhn , E. Lagadec , G. Laibe , M. Langlois , A. -M. Lagrange , R. Launhardt , L. Leboulleux , H. Le Coroller , G. Li Causi , M. Loupias , A. L. Maire , G. Marleau , F. Martinache , P. Martinez , D. Mary , M. Mattioli , J. Mazoyer , H. Meheut , F. Menard , D. Mesa , N. Meunier , Y. Miguel , J. Milli , M. Min , P. Molliere , C. Mordasini , G. Moretto , L. Mugnier , G. Muro Arena , N. Nardetto , M. N Diaye , N. Nesvadba , F. Pedichini , P. Pinilla , E. Por , A. Potier , S. Quanz , J. Rameau , R. Roelfsema , D. Rouan , E. Rigliaco , B. Salasnich , M. Samland , J. -F. Sauvage , H. -M. Schmid , D. Segransan , I. Snellen , F. Snik , F. Soulez , E. Stadler , D. Stam , M. Tallon , P. Thebault , E. Thiebaut , C. Tschudi , S. Udry , R. van Holstein , P. Vernazza , F. Vidal , A. Vigan , R. Waters , F. Wildi , M. Willson , A. Zanutta , A. Zavagno , A. Zurlo
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