An Ultra Deep Field survey with WFIRST

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

Evolution of the sizes of galaxies over 7 < z < 12 revealed by the 2012 Hubble ultra deep field campaign

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

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

The morphologies of massive galaxies at 1 < z < 3 in the CANDELS-UDS field : compact bulges, and the rise and fall of massive discs

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

Linking stellar mass and star formation in Spitzer MIPS 24 mu m galaxies

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

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