Zobrazeno 1 - 10
of 106
pro vyhledávání: '"Dunlop JS"'
Autor:
Koekemoer, Anton M, Foley, RJ, Spergel, DN, Bagley, M, Bezanson, R, Bianco, FB, Bouwens, R, Bradley, L, Brammer, G, Capak, P, Davidzon, I, Rosa, G De, Dickinson, ME, Doré, O, Dunlop, JS, Ellis, RS, Fan, X, Fazio, GG, Ferguson, HC, Filippenko, AV, Finkelstein, S, Frye, B, Gawiser, E, Grogin, NA, Hathi, NP, Hirata, CM, Hounsell, R, Illingworth, GD, Jansen, RA, Jauzac, M, Jha, SW, Kartaltepe, JS, Kim, AG, Kelly, P, Kruk, JW, Larson, R, Lotz, J, Lucas, R, Malhotra, S, Mandel, K, Margutti, R, Marrone, D, McLure, RJ, McQuinn, K, Melchior, P, Mobasher, B, Mould, JR, Moustakas, L, Newman, JA, Papovich, C, Peeples, MS, Perlmutter, S, Pirzkal, N, Rhoads, J, Rhodes, J, Robertson, B, Rubin, D, Ryan, R, Scolnic, D, Shapley, A, Somerville, R, Steinhardt, C, Stiavelli, M, Street, R, Trenti, M, Treu, T, Wang, L, Wang, Y, Whalen, D, Windhorst, RA, Wollack, EJ, Yan, H
Studying the formation and evolution of galaxies at the earliest cosmic times, and their role in reionization, requires the deepest imaging possible. Ultra-deep surveys like the HUDF and HFF have pushed to mag \mAB$\,\sim\,$30, revealing galaxies at
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1ba74d212ef66510584df83bdcfb75cc
Autor:
Willott, CJ, Simpson, C, Almaini, O, Manners, JC, Johnson, O, Lawrence, A, Dunlop, JS, Ivison, RJ, Rawlings, S, Gonzalez-Solares, E, Perez-Fournon, I, Serjeant, S, Oliver, SJ, Roche, ND, Mann, RG, Rowan-Robinson, M
The sources discovered in deep hard X-ray surveys with 2-8 keV fluxes of 10^-14 erg cm^-2 s^-1 make up the bulk of the X-ray background at these energies. We present here detailed multi-wavelength observations of three such sources from the ELAIS Dee
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9bb55f0162bbfe1e1db5ecd7fc372702
https://doi.org/10.1046/j.1365-8711.2003.06192.x
https://doi.org/10.1046/j.1365-8711.2003.06192.x
Autor:
Waddington, I, Windhorst, RA, Cohen, SH, Dunlop, JS, Peacock, JA, Jimenez, R, McLure, RJ, Bunker, AJ, Spinrad, H, Dey, A, Stern, D
Deep spectroscopy of the two Leiden-Berkeley Deep Survey mJy radio galaxies LBDS 53W069 and 53W091 has previously shown them to have old (≳3 Gyr) stellar populations at z ≃ 1.5. Here we present the results of Hubble Space Telescope (HST) observat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::01decb91edcc76ec02f0c706c5f8d64f
https://doi.org/10.1046/j.1365-8711.2002.05870.x
https://doi.org/10.1046/j.1365-8711.2002.05870.x
Autor:
Ono, Y, Ouchi, M, Curtis-Lake, E, Schenker, MA, Ellis, RS, McLure, RJ, Dunlop, JS, Robertson, BE, Koekemoer, AM, Bowler, RAA, Rogers, AB, Schneider, E, Charlot, S, Stark, DP, Shimasaku, K, Furlanetto, SR, Cirasuolo, M
Publikováno v:
Astrophysical Journal, vol 777, iss 2
The Astrophysical Journal, vol 777, iss 2
Ono, Y; Ouchi, M; Curtis-Lake, E; Schenker, MA; Ellis, RS; McLure, RJ; et al.(2013). Evolution of the sizes of galaxies over 7 < z < 12 revealed by the 2012 Hubble ultra deep field campaign. Astrophysical Journal, 777(2). doi: 10.1088/0004-637X/777/2/155. UCLA: Retrieved from: http://www.escholarship.org/uc/item/866830j1
The Astrophysical Journal, vol 777, iss 2
Ono, Y; Ouchi, M; Curtis-Lake, E; Schenker, MA; Ellis, RS; McLure, RJ; et al.(2013). Evolution of the sizes of galaxies over 7 < z < 12 revealed by the 2012 Hubble ultra deep field campaign. Astrophysical Journal, 777(2). doi: 10.1088/0004-637X/777/2/155. UCLA: Retrieved from: http://www.escholarship.org/uc/item/866830j1
We analyze the redshift- and luminosity-dependent sizes of dropout galaxy candidates in the redshift range z ∼ 7-12 using deep images from the 2012 Hubble Ultra Deep Field (UDF12) campaign, which offers two advantages over that used in earlier work
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::3513f3b83f74788f1dbd53dc890e1a82
https://escholarship.org/uc/item/866830j1
https://escholarship.org/uc/item/866830j1
Autor:
Drake, AB, Simpson, C, Collins, CA, James, PA, Baldry, IK, Ouchi, M, Jarvis, MJ, Bonfield, DG, Ono, Y, Best, PN, Dalton, GB, Dunlop, JS, McLure, RJ, Smith, DJB
Publikováno v:
Monthly Notices of the Royal Astronomical Society.
We present new results on the cosmic star formation history in the Subaru/XMM–Newton Deep Survey (SXDS)–Ultra Deep Survey (UDS) field out to z = 1.6. We compile narrowband\ud data from the Subaru Telescope and the Visible and Infrared Survey Tele
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::492869e8cb3cf785dde1baa38155d7ec
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:
van Kampen, E, Smith, DJB, Maddox, S, Hopkins, AM, Valtchanov, I, Peacock, JA, Michalowski, Michal, Norberg, P, Eales, S, Dunne, L, Liske, J, Baes, Maarten, Scott, D, Rigby, E, Robotham, A, van der Werf, P, Ibar, E, Jarvis, MJ, Loveday, J, Auld, R, Baldry, IK, Bamford, S, Cameron, E, Croom, S, Buttiglione, S, Cava, A, Cooray, A, Driver, S, Dunlop, JS, Dariush, A, Fritz, Jacopo, Ivison, RJ, Pascale, E, Pohlen, M, Rodighiero, G, Temi, P, Bonfield, DG, Hill, D, Jones, DH, Kelvin, L, Parkinson, H, Prescott, M, Sharp, R, de Zotti, G, Serjeant, S, Popescu, CC, Tuffs, RJ
Publikováno v:
Monthly notices of the Royal Astronomical Society, 2012, Vol.426(4), pp.3455-3463 [Peer Reviewed Journal]
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
We have measured the clustering properties of low-redshift (z < 0.3) submm galaxies detected at 250 mu m in the Herschel-ATLAS science demonstration phase field. We selected a sample for which we have high-quality spectroscopic redshifts, obtained fr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::ca7db1c8e3ed331c48360e9cd0b73bd1
http://hdl.handle.net/11573/961472
http://hdl.handle.net/11573/961472
Autor:
Bruce, VA, Dunlop, JS, Cirasuolo, M, McLure, RJ, Targett, TA, Bell, EF, Croton, DJ, Dekel, A, Faber, SM, Ferguson, HC, Grogin, NA, Kocevski, DD, Koekemoer, AM, Koo, DC, Lai, K, Lotz, JM, McGrath, EJ, Newman, JA, van der Wel, Arjen
Publikováno v:
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
We have used high-resolution, Hubble Space Telescope, near-infrared imaging to conduct a detailed analysis of the morphological properties of the most massive galaxies at high redshift, modelling the WFC3/IR H-160-band images of the similar or equal
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______330::d978cacda6b7d5113b7c5fa84c7b6d9b
https://hdl.handle.net/1854/LU-8573756
https://hdl.handle.net/1854/LU-8573756
Autor:
Caputi, KI, Dole, H, Lagache, G, McLure, RJ, Puget, JL, Rieke, GH, Dunlop, JS, Le Floc'h, E, Papovich, C, Perez-Gonzalez, PG
Publikováno v:
The Astrophysical Journal, 637(2), 727-740. IOP PUBLISHING LTD
We present deep K-s 83 mu Jy ( the similar to 80% completeness limit of the Spitzer/GTO 24 mu m catalog); 36% of our galaxies have spectroscopic redshifts ( mostly at z 10(12) L-circle dot) at redshifts z less than or similar to 2-3. Massive star-for
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=narcis______::d2b36e6ddb7660cbba0eb97514150867
https://research.rug.nl/en/publications/6c64d516-17a6-4fcf-aaab-9aef71b509d8
https://research.rug.nl/en/publications/6c64d516-17a6-4fcf-aaab-9aef71b509d8