Dusty Starbursts Masquerading as Ultra-high Redshift Galaxies in JWST CEERS Observations

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

The radius of baryonic collapse in disc galaxy formation

Autor: Kassin, SA, Devriendt, J, Fall, SM, Jong, RSD, Allgood, B, Primack, JR

In the standard picture of disc galaxy formation, baryons and dark matter receive the same tidal torques, and therefore approximately the same initial specific angular momentum. However, observations indicate that disc galaxies typically have only ab

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9ec2baed3f53efad745c1f601cc2c3d7
https://ora.ox.ac.uk/objects/uuid:9f6b03dd-363b-4e47-8f1b-336cbbac10c2

THE EPOCH OF DISK SETTLING: z similar to 1 TO NOW

Autor: Kassin, SA, Weiner, B, Faber, S, Gardner, J, Willmer, C, Coil, A, Cooper, M, Devriendt, J, Dutton, A, Guhathakurta, P, Koo, D, Metevier, A, Noeske, K, Primack, JR

Publikováno v: ASTROPHYSICAL JOURNAL. 758(2)

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::b5aa4d8985cf79ce9cbebd13552f6b6b
http://ora.ox.ac.uk/objects/uuid:1164f81a-d0b4-422f-a016-028f34599568

The angular momentum of baryons and dark matter halos revisited

Autor: Kimm, T, Devriendt, J, Slyz, A, Pichon, C, Kassin, SA, Dubois, Y

Recent theoretical studies have shown that galaxies at high redshift are fed by cold, dense gas filaments, suggesting angular momentum transport by gas differs from that by dark matter. Revisiting this issue using high-resolution cosmological hydrody

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::be88b90cf1c909788aedfb4cf278ac08

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