HELP: the Herschel Extragalactic Legacy Project

Monthly Notices of the Royal Astronomical Society Oxford University Press 507:1 (2021) 129-155

Authors:

R Shirley, K Duncan, Mc Campos Varillas, Pd Hurley, K Malek, Y Roehlly, Mwl Smith, H Aussel, T Bakx, V Buat, D Burgarella, N Christopher, S Duivenvoorden, S Eales, A Efstathiou, Ea Gonzalez Solares, M Griffin, M Jarvis, B Lo Faro, L Marchetti, I McCheyne, A Papadopoulos, K Penner, E Pons, M Prescott, E Rigby, H Rottgering, A Saxena, J Scudder, M Vaccari, L Wang, Sj Oliver

Abstract:

We present the Herschel Extragalactic Legacy Project (HELP). This project collates, curates, homogenizes, and creates derived data products for most of the premium multiwavelength extragalactic data sets. The sky boundaries for the first data release cover 1270 deg2 defined by the Herschel SPIRE extragalactic survey fields; notably the Herschel Multi-tiered Extragalactic Survey (HerMES) and the Herschel Atlas survey (H-ATLAS). Here, we describe the motivation and principal elements in the design of the project. Guiding principles are transparent or 'open' methodologies with care for reproducibility and identification of provenance. A key element of the design focuses around the homogenization of calibration, meta data, and the provision of information required to define the selection of the data for statistical analysis. We apply probabilistic methods that extract information directly from the images at long wavelengths, exploiting the prior information available at shorter wavelengths and providing full posterior distributions rather than maximum-likelihood estimates and associated uncertainties as in traditional catalogues. With this project definition paper, we provide full access to the first data release of HELP; Data Release 1 (DR1), including a monolithic map of the largest SPIRE extragalactic field at 385 deg2 and 18 million measurements of PACS and SPIRE fluxes. We also provide tools to access and analyse the full HELP data base. This new data set includes far-infrared photometry, photometric redshifts, and derived physical properties estimated from modelling the spectral energy distributions over the full HELP sky. All the software and data presented is publicly available.

The nature of sub-millimetre galaxies I: a comparison of AGN and star-forming galaxy SED fits

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 505:1 (2021) 1509-1529

Authors:

T Shanks, B Ansarinejad, RM Bielby, I Heywood, N Metcalfe, L Wang

The SAMI Galaxy Survey: the third and final data release

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 505:1 (2021) 991-1016

Authors:

Scott M Croom, Matt S Owers, Nicholas Scott, Henry Poetrodjojo, Brent Groves, Jesse van de Sande, Tania M Barone, Luca Cortese, Francesco D’Eugenio, Joss Bland-Hawthorn, Julia Bryant, Sree Oh, Sarah Brough, James Agostino, Sarah Casura, Barbara Catinella, Matthew Colless, Gerald Cecil, Roger L Davies, Michael J Drinkwater, Simon P Driver, Ignacio Ferreras, Caroline Foster, Amelia Fraser-McKelvie, Jon Lawrence, Sarah K Leslie, Jochen Liske, Ángel R López-Sánchez, Nuria PF Lorente, Rebecca McElroy, Anne M Medling, Danail Obreschkow, Samuel N Richards, Rob Sharp, Sarah M Sweet, Dan S Taranu, Edward N Taylor, Edoardo Tescari, Adam D Thomas, James Tocknell, Sam P Vaughan

A low [CII]/[NII] ratio in the center of a massive galaxy at z = 3.7: Evidence for a transition to quiescence at high redshift? (Corrigendum)

Astronomy & Astrophysics EDP Sciences 650 (2021) c2

Authors:

C Schreiber, K Glazebrook, C Papovich, T Díaz-Santos, A Verma, D Elbaz, GG Kacprzak, T Nanayakkara, P Oesch, M Pannella, L Spitler, C Straatman, K-V Tran, T Wang

Origins space telescope: from first light to life

Experimental Astronomy Springer Nature 51:3 (2021) 595-624

Authors:

MC Wiedner, S Aalto, L Armus, E Bergin, J Birkby, CM Bradford, D Burgarella, P Caselli, V Charmandaris, A Cooray, E De Beck, JM Desert, M Gerin, J Goicoechea, M Griffin, P Hartogh, F Helmich, M Hogerheijde, L Hunt, A Karska, Q Kral, D Leisawitz, G Melnick, M Meixner, M Matsuura, S Milam, C Pearson, DW Pesce, KM Pontoppidan, A Pope, D Rigopoulou, T Roellig, I Sakon, J Staguhn, K Stevenson