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

Expectations of the size evolution of massive galaxies at $3 \leq z \leq 6$ from the TNG50 simulation: the CEERS/JWST view

Autor: Costantin, L, Pérez-González, PG, Vega-Ferrero, J, Huertas-Company, M, Bisigello, L, Buitrago, F, Bagley, MB, Cleri, NJ, Cooper, MC, Finkelstein, SL, Holwerda, BW, Kartaltepe, JS, Koekemoer, AM, Nelson, D, Papovich, C, Pillepich, A, Pirzkal, N, Tacchella, S, Yung, LYA

We present a catalog of about 25,000 images of massive ($M_{\star} \ge 10^9 M_{\odot}$) galaxies at redshift $3 \leq z \leq 6$ from the TNG50 cosmological simulation, tailored for observations at multiple wavelengths carried out with JWST. The synthe

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cca0e75e7e854f2a2321ea8721c991c8
http://arxiv.org/abs/2208.00007

Confirmation and refutation of very luminous galaxies in the early Universe.

Autor: Arrabal Haro P; NSF's National Optical-Infrared Astronomy Research Laboratory, Tucson, AZ, USA. parrabalh@gmail.com., Dickinson M; NSF's National Optical-Infrared Astronomy Research Laboratory, Tucson, AZ, USA., Finkelstein SL; Department of Astronomy, The University of Texas at Austin, Austin, TX, USA., Kartaltepe JS; Laboratory for Multiwavelength Astrophysics, School of Physics and Astronomy, Rochester Institute of Technology, Rochester, NY, USA., Donnan CT; Institute for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh, UK., Burgarella D; Aix Marseille Univ, CNRS, CNES, LAM Marseille, Marseille, France., Carnall AC; Institute for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh, UK., Cullen F; Institute for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh, UK., Dunlop JS; Institute for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh, UK., Fernández V; Instituto de Investigación Multidisciplinar en Ciencia y Tecnología, Universidad de La Serena, La Serena, Chile., Fujimoto S; Department of Astronomy, The University of Texas at Austin, Austin, TX, USA.; Cosmic Dawn Center (DAWN), Copenhagen, Denmark.; Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark., Jung I; Space Telescope Science Institute, Baltimore, MD, USA., Krips M; IRAM, Domaine Universitaire, Saint-Martin-d'Hères, France., Larson RL; Department of Astronomy, The University of Texas at Austin, Austin, TX, USA.; Laboratory for Multiwavelength Astrophysics, School of Physics and Astronomy, Rochester Institute of Technology, Rochester, NY, USA., Papovich C; Department of Physics and Astronomy, Texas A&M University, College Station, TX, USA.; George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, TX, USA., Pérez-González PG; Centro de Astrobiología (CAB), CSIC-INTA, Madrid, Spain., Amorín RO; Instituto de Investigación Multidisciplinar en Ciencia y Tecnología, Universidad de La Serena, La Serena, Chile.; Departamento de Astronomía, Universidad de La Serena, La Serena, Chile., Bagley MB; Department of Astronomy, The University of Texas at Austin, Austin, TX, USA., Buat V; Aix Marseille Univ, CNRS, CNES, LAM Marseille, Marseille, France., Casey CM; Department of Astronomy, The University of Texas at Austin, Austin, TX, USA., Chworowsky K; Department of Astronomy, The University of Texas at Austin, Austin, TX, USA., Cohen SH; School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA., Ferguson HC; Space Telescope Science Institute, Baltimore, MD, USA., Giavalisco M; University of Massachusetts Amherst, Amherst, MA, USA., Huertas-Company M; Instituto de Astrofísica de Canarias, La Laguna, Spain.; Universidad de la Laguna, La Laguna, Spain.; Université Paris-Cité, LERMA - Observatoire de Paris, PSL, Paris, France., Hutchison TA; Astrophysics Science Division, NASA Goddard Space Flight Center, Greenbelt, MD, USA., Kocevski DD; Department of Physics and Astronomy, Colby College, Waterville, ME, USA., Koekemoer AM; Space Telescope Science Institute, Baltimore, MD, USA., Lucas RA; Space Telescope Science Institute, Baltimore, MD, USA., McLeod DJ; Institute for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh, UK., McLure RJ; Institute for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh, UK., Pirzkal N; Space Telescope Science Institute, Baltimore, MD, USA., Seillé LM; Aix Marseille Univ, CNRS, CNES, LAM Marseille, Marseille, France., Trump JR; Department of Physics, University of Connecticut, Storrs, CT, USA., Weiner BJ; MMT/Steward Observatory, University of Arizona, Tucson, AZ, USA., Wilkins SM; Astronomy Centre, University of Sussex, Brighton, UK.; Institute of Space Sciences and Astronomy, University of Malta, Msida, Malta., Zavala JA; National Astronomical Observatory of Japan, Tokyo, Japan.

Publikováno v: Nature [Nature] 2023 Oct; Vol. 622 (7984), pp. 707-711. Date of Electronic Publication: 2023 Aug 14.

First Data Release of the COSMOS Lyα Mapping and Tomography Observations: 3D Lyα Forest Tomography at 2.05 < z < 2.55

Autor: Lee, KG, Krolewski, A, White, M, Schlegel, D, Nugent, PE, Hennawi, JF, Müller, T, Pan, R, Prochaska, JX, Font-Ribera, A, Suzuki, N, Glazebrook, K, Kacprzak, GG, Kartaltepe, JS, Koekemoer, AM, Le Fèvre, O, Lemaux, BC, Maier, C, Nanayakkara, T, Rich, RM, Sanders, DB, Salvato, M, Tasca, L, Tran, KVH

Publikováno v: Lee, KG; Krolewski, A; White, M; Schlegel, D; Nugent, PE; Hennawi, JF; et al.(2018). First Data Release of the COSMOS Lyα Mapping and Tomography Observations: 3D Lyα Forest Tomography at 2.05 < z < 2.55. Astrophysical Journal, Supplement Series, 237(2), 2. doi: 10.3847/1538-4365/aace58. Lawrence Berkeley National Laboratory: Retrieved from: http://www.escholarship.org/uc/item/20v490mw
The Astrophysical Journal Supplement Series, vol 237, iss 2
The Astrophysical Journal Supplement Series
Astrophysical Journal, Supplement Series, vol 237, iss 2

Faint star-forming galaxies at z ̃ 2-3 can be used as alternative background sources to probe the Lyα forest in addition to quasars, yielding high sightline densities that enable 3D tomographic reconstruction of the foreground absorption field. Her

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::65c90314ea7361d754aca3642c7110ac
http://www.escholarship.org/uc/item/20v490mw

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