The Herschel Multi-Tiered Extragalactic Survey: source extraction and cross-identifications in confusion-dominated SPIRE images

Autor: Roseboom, IG, Oliver, SJ, Kunz, M, Altieri, B, Amblard, A, Arumugam, V, Auld, R, Aussel, H, Babbedge, T, Bethermin, M, Blain, A, Bock, J, Boselli, A, Brisbin, D, Buat, V, Burgarella, D, Castro-Rodriguez, N, Cava, A, Chanial, P, Chapin, E, Clements, DL, Conley, A, Conversi, L, Cooray, A, Dowell, CD, Dwek, E, Dye, S, Eales, S, Elbaz, D, Farrah, D, Fox, M, Franceschini, A, Gear, W, Glenn, J, Solares, EAG, Griffin, M, Halpern, M, Harwit, M, Hatziminaoglou, E, Huang, J, Ibar, E, Isaak, K, Ivison, RJ, Lagache, G, Levenson, L, Lu, N, Madden, S, Maffei, B, Mainetti, G, Marchetti, L, Marsden, G, Mortier, AMJ, Nguyen, HT, O'Halloran, B, Omont, A, Page, MJ, Panuzzo, P, Papageorgiou, A, Patel, H, Pearson, CP, Perez-Fournon, I, Pohlen, M, Rawlings, JI, Raymond, G, Rigopoulou, D, Rizzo, D, Rowan-Robinson, M, Sanchez Portal, M, Schulz, B, Scott, D, Seymour, N, Shupe, DL, Smith, AJ, Stevens, JA, Symeonidis, M, Trichas, M, Tugwell, KE, Vaccari, M, Valtchanov, I, Vieira, JD, Vigroux, L, Wang, L, Ward, R, Wright, G, Xu, CK, Zemcov, M

Publikováno v: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2010, 409 (1), pp.48--65. ⟨10.1111/j.1365-2966.2010.17634.x⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2010, 409 (1), pp.48--65. ⟨10.1111/j.1365-2966.2010.17634.x⟩

We present the cross-identification and source photometry techniques used to process Herschel SPIRE imaging taken as part of the Herschel Multi-Tiered Extragalactic Survey (HerMES). Cross-identifications are performed in map-space so as to minimise s

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::396629975436990184488f56c812df33
http://doc.rero.ch/record/298163/files/mnras0409-0048.pdf

A POPULATION OF DUST-RICH QUASARS AT z similar to 1.5

Autor: Dai, YS, Bergeron, J, Elvis, M, Omont, A, Huang, J-S, Bock, J, Cooray, A, Fazio, G, Hatziminaoglou, E, Ibar, E, Magdis, GE, Oliver, SJ, Page, MJ, Perez-Fournon, I, Rigopoulou, D, Roseboom, IG, Scott, D, Symeonidis, M, Trichas, M, Vieira, JD, Willmer, CNA, Zemcov, M

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::33d9c4ac9451b219c7fe2bd1a7d9e234
https://ora.ox.ac.uk/objects/uuid:1e1449c5-bee5-49c6-a27c-217a3212925d

HerMES: CANDIDATE HIGH-REDSHIFT GALAXIES DISCOVERED WITH HERSCHEL/SPIRE**http://hermes.sussex.ac.uk.,††Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA

Autor: Dowell, C Darren, Conley, A, Glenn, J, Arumugam, V, Asboth, V, Aussel, H, Bertoldi, F, Béthermin, M, Bock, J, Boselli, A, Bridge, C, Buat, V, Burgarella, D, Cabrera-Lavers, A, Casey, CM, Chapman, SC, Clements, DL, Conversi, L, Cooray, A, Dannerbauer, H, De Bernardis, F, Ellsworth-Bowers, TP, Farrah, D, Franceschini, A, Griffin, M, Gurwell, MA, Halpern, M, Hatziminaoglou, E, Heinis, S, Ibar, E, Ivison, RJ, Laporte, N, Marchetti, L, Martínez-Navajas, P, Marsden, G, Morrison, GE, Nguyen, HT, O'Halloran, B, Oliver, SJ, Omont, A, Page, MJ, Papageorgiou, A, Pearson, CP, Petitpas, G, Pérez-Fournon, I, Pohlen, M, Riechers, D, Rigopoulou, D, Roseboom, IG, Rowan-Robinson, M, Sayers, J, Schulz, B, Scott, Douglas, Seymour, N, Shupe, DL, Smith, AJ, Streblyanska, A, Symeonidis, M, Vaccari, M, Valtchanov, I, Vieira, JD, Viero, M, Wang, L, Wardlow, J, Xu, CK, Zemcov, M

Publikováno v: The Astrophysical Journal, vol 780, iss 1

We present a method for selecting z > 4 dusty, star-forming galaxies (DSFGs) using Herschel/Spectral and Photometric Imaging Receiver 250/350/500 μm flux densities to search for red sources. We apply this method to 21 deg2 of data from the HerMES su

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=od_______325::b6d7e2bb8dc8046d1d69be342deeaf4e
https://escholarship.org/uc/item/45g8n6nz

GRAVITATIONAL LENS MODELS BASED ON SUBMILLIMETER ARRAY**The Submillimeter Array is a joint project between the Smithsonian Astrophysical Observatory and the Academia Sinica Institute of Astronomy and Astrophysics and is funded by the Smithsonian Institution and the Academia Sinica. IMAGING OF HERSCHEL††Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA.-SELECTED STRONGLY LENSED SUB-MILLIMETER GALAXIES AT z > 1.5

Autor: Bussmann, RS, Pérez-Fournon, I, Amber, S, Calanog, J, Gurwell, MA, Dannerbauer, H, De Bernardis, F, Fu, Hai, Harris, AI, Krips, M, Lapi, A, Maiolino, R, Omont, A, Riechers, D, Wardlow, J, Baker, AJ, Birkinshaw, M, Bock, J, Bourne, N, Clements, DL, Cooray, A, De Zotti, G, Dunne, L, Dye, S, Eales, S, Farrah, D, Gavazzi, R, Nuevo, J González, Hopwood, R, Ibar, E, Ivison, RJ, Laporte, N, Maddox, S, Martínez-Navajas, P, Michalowski, M, Negrello, M, Oliver, SJ, Roseboom, IG, Scott, Douglas, Serjeant, S, Smith, AJ, Smith, Matthew, Streblyanska, A, Valiante, E, van der Werf, P, Verma, A, Vieira, JD, Wang, L, Wilner, D

Publikováno v: The Astrophysical Journal, vol 779, iss 1

Strong gravitational lenses are now being routinely discovered in wide-field surveys at (sub-)millimeter wavelengths. We present Submillimeter Array (SMA) high-spatial resolution imaging and Gemini-South and Multiple Mirror Telescope optical spectros

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=od_______325::095e65ae4dc7605fa340fa74ab606101
https://escholarship.org/uc/item/4810f874

The contribution of very massive high-redshift SWIRE galaxies to the stellar mass function RID C-5880-2009

Autor: Berta S, Lonsdale CJ, Polletta M, Savage RS, Franceschini A, Buttery H, Cimatti A, Dias J, Feruglio C, Fiore F, Held EV, Maiolino R, Marconi A, Matute I, Oliver SJ, Ricciardelli E, Rubele S, Sacchi N, Shupe D, Surace J., LA FRANCA, Fabio

In the last couple of years a population of very massive (M(*) > 10(11) M(circle dot)), high-redshift (z >= 2) galaxies has been identified, but its role in galaxy evolution has not yet been fully understood. Aims. It is necessary to perform a system

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=od______3668::ef4a291adde2f18d7fe26c4c4ff1dc9f
https://hdl.handle.net/11590/154678