Zobrazeno 1 - 10
of 42
pro vyhledávání: '"Grogin, NA"'
Autor:
Zavala, JA, Buat, V, Casey, CM, Finkelstein, SL, Burgarella, D, Bagley, MB, Ciesla, L, Daddi, E, Dickinson, M, Ferguson, HC, Franco, M, Jiménez-Andrade, EF, Kartaltepe, JS, Koekemoer, AM, Bail, AL, Murphy, EJ, Papovich, C, Tacchella, S, Wilkins, SM, Aretxaga, I, Behroozi, P, Champagne, JB, Fontana, A, Giavalisco, M, Grazian, A, Grogin, NA, Kewley, LJ, Kocevski, DD, Kirkpatrick, A, Lotz, JM, Pentericci, L, Pérez-González, PG, Pirzkal, N, Ravindranath, S, Somerville, RS, Trump, Yang, G, Aaron Yung, LY, Almaini, O, Amorín, RO, Annunziatella, M, Haro, PA, Backhaus, BE, Barro, G, Bell, EF, Bhatawdekar, R, Bisigello, L, Buitrago, F, Calabrò, A, Castellano, M, Chávez Ortiz, ÓA, Chworowsky, K, Cleri, NJ, Cohen, SH, Cole, JW, Cooke, KC, Cooper, MC, Cooray, AR, Costantin, L, Cox, IG, Croton, D, Davé, R, Vega, ADL, Dekel, A, Elbaz, D, Estrada-Carpenter, V, Fernández, V, Finkelstein, KD, Freundlich, J, Fujimoto, S, García-Argumánez, Á, Gardner, JP, Gawiser, E, Gómez-Guijarro, C, Guo, Y, Hamilton, TS, Hathi, NP, Holwerda, BW, Hirschmann, M, Huertas-Company, M, Hutchison, TA, Iyer, KG, Jaskot, AE, Jha, SW, Jogee, S, Juneau, S, Jung, I, Kassin, SA, Kurczynski, P, Larson, RL, Leung, GCK, Long, AS, Lucas, RA, Magnelli, B, Mantha, KB, Matharu, J, McGrath, EJ, McIntosh, DH, Medrano, A, Merlin, E
Lyman-break galaxy (LBG) candidates at z ≳ 10 are rapidly being identified in James Webb Space Telescope (JWST)/NIRCam observations. Due to the (redshifted) break produced by neutral hydrogen absorption of rest-frame UV photons, these sources are e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::22103052e44ddcfe90d52766a1afb845
https://www.repository.cam.ac.uk/handle/1810/346866
https://www.repository.cam.ac.uk/handle/1810/346866
Autor:
Finkelstein, SL, Bagley, MB, Haro, PA, Dickinson, M, Ferguson, HC, Kartaltepe, JS, Papovich, C, Burgarella, D, Kocevski, DD, Huertas-Company, M, Iyer, KG, Koekemoer, AM, Larson, RL, Pérez-González, PG, Rose, C, Tacchella, S, Wilkins, SM, Chworowsky, K, Medrano, A, Morales, AM, Somerville, RS, Aaron Yung, LY, Fontana, A, Giavalisco, M, Grazian, A, Grogin, NA, Kewley, LJ, Kirkpatrick, A, Kurczynski, P, Lotz, JM, Pentericci, L, Pirzkal, N, Ravindranath, S, Ryan, RE, Trump, Yang, G, Almaini, O, Amorín, RO, Annunziatella, M, Backhaus, BE, Barro, G, Behroozi, P, Bell, EF, Bhatawdekar, R, Bisigello, L, Bromm, V, Buat, V, Buitrago, F, Calabrò, A, Casey, CM, Castellano, M, Chávez Ortiz, ÓA, Ciesla, L, Cleri, NJ, Cohen, SH, Cole, JW, Cooke, KC, Cooper, MC, Cooray, AR, Costantin, L, Cox, IG, Croton, D, Daddi, E, Davé, R, De La Vega, A, Dekel, A, Elbaz, D, Estrada-Carpenter, V, Faber, SM, Fernández, V, Finkelstein, KD, Freundlich, J, Fujimoto, S, García-Argumánez, Á, Gardner, JP, Gawiser, E, Gómez-Guijarro, C, Guo, Y, Hamblin, K, Hamilton, TS, Hathi, NP, Holwerda, BW, Hirschmann, M, Hutchison, TA, Jaskot, AE, Jha, SW, Jogee, S, Juneau, S, Jung, I, Kassin, SA, Le Bail, A, Leung, GCK, Lucas, RA, Magnelli, B, Mantha, KB, Matharu, J, McGrath, EJ, McIntosh, DH, Merlin, E, Mobasher, B
We report the discovery of a candidate galaxy with a photo-z of z ∼ 12 in the first epoch of the James Webb Space Telescope (JWST) Cosmic Evolution Early Release Science Survey. Following conservative selection criteria, we identify a source with a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b0f56cc3c645208120b26a0226bee36e
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:
Grazian, A, Giallongo, E, Paris, D, Boutsia, K, Dickinson, M, Santini, P, Windhorst, RA, Jansen, RA, Cohen, SH, Ashcraft, TA, Scarlata, C, Rutkowski, MJ, Vanzella, E, Cusano, F, Cristiani, S, Giavalisco, M, Ferguson, HC, Koekemoer, A, Grogin, NA, Castellano, M, Fiore, F, Fontana, A, Marchi, F, Pedichini, F, Pentericci, L, Amorín, R, Barro, G, Bonchi, A, Bongiorno, A, Faber, SM, Fumana, M, Galametz, A, Guaita, L, Kocevski, DD, Merlin, E, Nonino, M, O'Connell, RW, Pilo, S, Ryan, RE, Sani, E, Speziali, R, Testa, V, Weiner, B, Yan, H
The reionization of the Universe is one of the most important topics of present day astrophysical research. The most plausible candidates for the reionization process are star-forming galaxies, which according to the predictions of the majority of th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3e90e95a7efc9e714219eea5cba41af9
Autor:
Lani, C, Almaini, O, Hartley, WG, Mortlock, A, Häußler, B, Chuter, RW, Simpson, C, Van der Wel, A, Grützbauch, R, Conselice, CJ, Bradshaw, EJ, Cooper, MC, Faber, SM, Grogin, NA, Kocevski, DD, Koekemoer, AM, Lai, K
Publikováno v:
Monthly Notices of the Royal Astronomical Society, vol 435, iss 1
Lani, C; Almaini, O; Hartley, WG; Mortlock, A; Häußler, B; Chuter, RW; et al.(2013). Evidence for a correlation between the sizes of quiescent galaxies and local environment to z~2. Monthly Notices of the Royal Astronomical Society, 435(1), 207-221. doi: 10.1093/mnras/stt1275. UC Irvine: Retrieved from: http://www.escholarship.org/uc/item/9q2829nm
Lani, C; Almaini, O; Hartley, WG; Mortlock, A; Häußler, B; Chuter, RW; et al.(2013). Evidence for a correlation between the sizes of quiescent galaxies and local environment to z~2. Monthly Notices of the Royal Astronomical Society, 435(1), 207-221. doi: 10.1093/mnras/stt1275. UC Irvine: Retrieved from: http://www.escholarship.org/uc/item/9q2829nm
We present evidence for a strong relationship between galaxy size and environment for the quiescent population in the redshift range 1 < z < 2. Environments were measured using projected galaxy overdensities on a scale of 400 kpc, as determined from
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::5dac25ee2e26b4fbe45ead19d955d525
https://escholarship.org/uc/item/9q2829nm
https://escholarship.org/uc/item/9q2829nm
Autor:
Kartaltepe, JS, Dickinson, M, Alexander, DM, Bell, EF, Dahlen, T, Elbaz, D, Faber, SM, Lotz, J, McIntosh, DH, Wiklind, T, Altieri, B, Aussel, H, Bethermin, M, Bournaud, F, Charmandaris, V, Conselice, CJ, Cooray, A, Dannerbauer, H, Dave, R, Dunlop, J, Dekel, A, Ferguson, HC, Grogin, NA, Hwang, HS, Ivison, R, Kocevski, D, Koekemoer, A, Koo, DC, Lai, K, Leiton, R, Lucas, RA, Lutz, D, Magdis, G, Magnelli, B, Morrison, G, Mozena, M, Mullaney, J, Newman, JA, Pope, A, Popesso, P, van der Wel, A, Weiner, B, Wuyts, S
Publikováno v:
ASTROPHYSICAL JOURNAL. 757(1)
Using deep 100 and 160 μm observations in GOODS-South from GOODS-Herschel, combined with high-resolution HST/WFC3 near-infrared imaging from CANDELS, we present the first detailed morphological analysis of a complete, far-infrared (FIR) selected sam
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
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