Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Rigby, EE"'
Autor:
Smith, DJB, Dunne, L, da Cunha, E, Rowlands, K, Maddox, SJ, Gomez, HL, Bonfield, DG, Charlot, S, Driver, SP, Popescu, CC, Tuffs, RJ, Dunlop, JS, Jarvis, MJ, Seymour, N, Symeonidis, M, Baes, M, Bourne, N, Clements, DL, Cooray, A, De Zotti, G, Dye, S, Eales, S, Scott, D, Verma, A, van der Werf, P, Andrae, E, Auld, R, Buttiglione, S, Cava, A, Dariush, A, Fritz, J, Hopwood, R, Ibar, E, Ivison, RJ, Kelvin, L, Madore, BF, Pohlen, M, Rigby, EE, Robotham, A, Seibert, M, Temi, P
We present a pan-chromatic analysis of an unprecedented sample of 1402 250 μm selected galaxies at z < 0.5 (z-=0.24) from the Herschel-ATLAS survey. We complement our Herschel 100-500μm data with UV-K-band photometry from the Galaxy And Mass Assemb
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::99e0f75a9e25e8b619d1c669d13ee254
http://hdl.handle.net/10044/1/54844
http://hdl.handle.net/10044/1/54844
Autor:
Smith, DJB, Dunne, L, da Cunha, E, Rowlands, K, Maddox, SJ, Gomez, HL, Bonfield, DG, Charlot, S, Driver, SP, Popescu, CC, Tuffs, RJ, Dunlop, JS, Jarvis, MJ, Seymour, N, Symeonidis, M, Baes, Maarten, Bourne, N, Clements, DL, Cooray, A, De Zotti, G, Dye, S, Eales, S, Scott, D, Verma, A, van der Werf, P, Andrae, E, Auld, R, Buttiglione, S, Cava, A, Dariush, A, Fritz, Jacopo, Hopwood, R, Ibar, E, Ivison, RJ, Kelvin, L, Madore, BF, Pohlen, M, Rigby, EE, Robotham, A, Seibert, M, Temi, P
Publikováno v:
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
We present a pan-chromatic analysis of an unprecedented sample of 1402 250 mu m selected galaxies at z < 0.5 ( = 0.24) from the Herschel-ATLAS survey. We complement our Herschel 100-500 mu m data with UV-K-band photometry from the Galaxy And Mass Ass
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______330::07cf67f09d4011c493b75c1dfdd28832
https://hdl.handle.net/1854/LU-3080182
https://hdl.handle.net/1854/LU-3080182
Autor:
Guo, Q, Cole, S, Lacey, CG, Baugh, CM, Frenk, CS, Norberg, P, Auld, R, Baldry, IK, Bamford, SP, Bourne, N, Buttiglione, ES, Cava, A, Cooray, A, Croom, S, Dariush, A, De Zotti, G, Driver, S, Dunne, L, Dye, S, Eales, S, Fritz, J, Hopkins, A, Hopwood, R, Ibar, E, Ivison, RJ, Jarvis, M, Jones, DH, Kelvin, L, Liske, J, Loveday, J, Maddox, SJ, Parkinson, H, Pascale, E, Peacock, JA, Pohlen, M, Prescott, M, Rigby, EE, Robotham, A, Rodighiero, G, Sharp, R, Smith, DJB, Temi, P, van Kampen, E
Publikováno v:
Monthly notices of the Royal Astronomical Society, 2011, Vol.412(4), pp.2277-2285 [Peer Reviewed Journal]
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society
We measure the projected cross-correlation between low-redshift (z < 0.5) far-infrared selected galaxies in the science demonstration phase (SDP) field of the Herschel-ATLAS (H-ATLAS) survey and optically selected galaxies from the Galaxy and Mass As
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::9cd95fb89bd579c5aab078441f28fa03
http://dro.dur.ac.uk/14056/1/14056.pdf
http://dro.dur.ac.uk/14056/1/14056.pdf
Autor:
Hardcastle, MJ, Virdee, JS, Jarvis, MJ, Bonfield, DG, Dunne, L, Rawlings, S, Stevens, JA, Christopher, NM, Heywood, I, Mauch, T, Rigopoulou, D, Verma, A, Baldry, IK, Bamford, SP, Buttiglione, S, Cava, A, Clements, DL, Cooray, A, Croom, SM, Dariush, A, De Zotti, G, Eales, S, Fritz, J, Hill, DT, Hughes, D, Hopwood, R, Ibar, E, Ivison, RJ, Jones, DH, Loveday, J, Maddox, SJ, Michalowski, MJ, Negrello, M, Norberg, P, Pohlen, M, Prescott, M, Rigby, EE, Robotham, ASG, Rodighiero, G, Scott, D, Sharp, R, Smith, DJB, Temi, P, Van Kampen, E
We use the Herschel-ATLAS science demonstration data to investigate the star-formation properties of radio-selected galaxies in the GAMA-9h field as a function of radio luminosity and redshift. Radio selection at the lowest radio luminosities, as exp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8e4a373c068ee7b7453903add2c9f866
http://arxiv.org/abs/1009.5866
http://arxiv.org/abs/1009.5866
Autor:
Eales, SA, Smith, MWL, Wilson, CD, Bendo, GJ, Cortese, L, Pohlen, M, Boselli, A, Gomez, HL, Auld, R, Baes, Maarten, Barlow, MJ, Bock, JJ, Bradford, M, Buat, V, Castro-Rodriguez, N, Chanial, P, Charlot, S, Ciesla, L, Clements, DL, Cooray, A, Cormier, D, Davies, JI, Dwek, E, Elbaz, D, Galametz, M, Galliano, F, Gear, WK, Glenn, J, Griffin, M, Hony, S, Isaak, KG, Levenson, LR, Lu, N, Madden, S, O'Halloran, B, Okumura, K, Oliver, S, Page, MJ, Panuzzo, P, Papageorgiou, A, Parkin, TJ, Perez-Fournon, I, Rangwala, N, Rigby, EE, Roussel, H, Rykala, A, Sacchi, N, Sauvage, M, Schulz, B, Schirm, MRP, Spinoglio, L, Srinivasan, S, Stevens, JA, Symeonidis, M, Trichas, M, Vaccari, M, Vigroux, L, Wozniak, H, Wright, GS, Zeilinger, WW
Publikováno v:
ASTRONOMY & ASTROPHYSICS
The standard method of mapping the interstellar medium in a galaxy, by observing the molecular gas in the CO 1-0 line and the atomic gas in the 21-cm line, is largely limited with current telescopes to galaxies in the nearby universe. In this letter,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______330::4ed9b8f74f6dd51b57a18803eeb86948
https://hdl.handle.net/1854/LU-1237016
https://hdl.handle.net/1854/LU-1237016
Autor:
Negrello M; Department of Physics and Astronomy, The Open University, Walton Hall, Milton Keynes, MK7 6AA, UK. m.negrello@open.ac.uk, Hopwood R, De Zotti G, Cooray A, Verma A, Bock J, Frayer DT, Gurwell MA, Omont A, Neri R, Dannerbauer H, Leeuw LL, Barton E, Cooke J, Kim S, da Cunha E, Rodighiero G, Cox P, Bonfield DG, Jarvis MJ, Serjeant S, Ivison RJ, Dye S, Aretxaga I, Hughes DH, Ibar E, Bertoldi F, Valtchanov I, Eales S, Dunne L, Driver SP, Auld R, Buttiglione S, Cava A, Grady CA, Clements DL, Dariush A, Fritz J, Hill D, Hornbeck JB, Kelvin L, Lagache G, Lopez-Caniego M, Gonzalez-Nuevo J, Maddox S, Pascale E, Pohlen M, Rigby EE, Robotham A, Simpson C, Smith DJ, Temi P, Thompson MA, Woodgate BE, York DG, Aguirre JE, Beelen A, Blain A, Baker AJ, Birkinshaw M, Blundell R, Bradford CM, Burgarella D, Danese L, Dunlop JS, Fleuren S, Glenn J, Harris AI, Kamenetzky J, Lupu RE, Maddalena RJ, Madore BF, Maloney PR, Matsuhara H, Michaowski MJ, Murphy EJ, Naylor BJ, Nguyen H, Popescu C, Rawlings S, Rigopoulou D, Scott D, Scott KS, Seibert M, Smail I, Tuffs RJ, Vieira JD, van der Werf PP, Zmuidzinas J
Publikováno v:
Science (New York, N.Y.) [Science] 2010 Nov 05; Vol. 330 (6005), pp. 800-4.
