SILVERRUSH. V. Census of Lyα, [O iii] λ5007, Hα, and [C ii] 158 μm Line Emission with ∼1000 LAEs at z = 4.9–7.0 Revealed with Subaru/HSC

Autor: Harikane, Y, Ouchi, M, Shibuya, T, Kojima, T, Zhang, H, Itoh, R, Ono, Y, Higuchi, R, Inoue, AK, Chevallard, J, Capak, PL, Nagao, T, Onodera, M, Faisst, AL, Martin, CL, Rauch, M, Bruzual, GA, Charlot, S, Davidzon, I, Fujimoto, S, Hilmi, M, Ilbert, O, Lee, CH, Matsuoka, Y, Silverman, JD, Toft, S

Publikováno v: The Astrophysical Journal, vol 859, iss 2
Harikane, Yuichi; Ouchi, Masami; Shibuya, Takatoshi; Kojima, Takashi; Zhang, Haibin; Itoh, Ryohei; et al.(2018). SILVERRUSH. V. Census of Lyα, [O iii] λ5007, Hα, and [C ii] 158 μm Line Emission with ∼1000 LAEs at z = 4.9–7.0 Revealed with Subaru/HSC. The Astrophysical Journal, 859(2), 84-84. doi: 10.3847/1538-4357/aabd80. UC Santa Barbara: Retrieved from: http://www.escholarship.org/uc/item/4rg3p18p
Astrophysical Journal, vol 859, iss 2

We investigate Lyα, [O iii] λ5007, Hα, and [C ii] 158 μm emission from 1124 galaxies at z = 4.9-7.0. Our sample is composed of 1092 Lyα emitters (LAEs) at z = 4.9, 5.7, 6.6, and 7.0 identified by Subaru/Hyper-Suprime-Cam (HSC) narrowband surveys

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::43b6a9790c58ed7ed62ee429f8b64698
https://escholarship.org/uc/item/4rg3p18p

Galaxies at redshifts 5 to 6 with systematically low dust content and high [C II] emission.

Autor: Capak PL; 1] Infrared Processing and Analysis Center (IPAC), 1200 East California Boulevard, Pasadena, California 91125, USA [2] California Institute of Technology, 1200 East California Boulevard, Pasadena, California 91125, USA., Carilli C; 1] National Radio Astronomy Observatory, PO Box 0, Socorro, New Mexico 87801, USA [2] Astrophysics Group, Cavendish Laboratory, J. J. Thomson Avenue, Cambridge CB3 0HE, UK., Jones G; New Mexico Institute of Mining and Technology, 801 Leroy Place, Socorro, New Mexico 87801, USA., Casey CM; Department of Astronomy, The University of Texas at Austin, 2515 Speedway, Stop C1400, Austin, Texas 78712, USA., Riechers D; Department of Astronomy, Cornell University, 220 Space Sciences Building, Ithaca, New York 14853, USA., Sheth K; National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, Virginia 22903, USA., Carollo CM; Institute for Astronomy, ETH Zurich, CH-8093 Zurich, Switzerland., Ilbert O; Aix Marseille Université, CNRS, LAM (Laboratoire d'Astrophysique de Marseille), UMR 7326, 13388 Marseille, France., Karim A; Argelander-Institut für Astronomie, Auf dem Hügel 71, D-53121 Bonn, Germany., LeFevre O; Aix Marseille Université, CNRS, LAM (Laboratoire d'Astrophysique de Marseille), UMR 7326, 13388 Marseille, France., Lilly S; National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, Virginia 22903, USA., Scoville N; California Institute of Technology, 1200 East California Boulevard, Pasadena, California 91125, USA., Smolcic V; Physics Department, University of Zagreb, Bijenička cesta 32, 10002 Zagreb, Croatia., Yan L; 1] Infrared Processing and Analysis Center (IPAC), 1200 East California Boulevard, Pasadena, California 91125, USA [2] California Institute of Technology, 1200 East California Boulevard, Pasadena, California 91125, USA.

Publikováno v: Nature [Nature] 2015 Jun 25; Vol. 522 (7557), pp. 455-8.

An unusually brilliant transient in the galaxy M85.

Autor: Kulkarni SR; Caltech Optical Observatories, California Institute of Technology, California 91125, USA. srk@astro.caltech.edu, Ofek EO, Rau A, Cenko SB, Soderberg AM, Fox DB, Gal-Yam A, Capak PL, Moon DS, Li W, Filippenko AV, Egami E, Kartaltepe J, Sanders DB

Publikováno v: Nature [Nature] 2007 May 24; Vol. 447 (7143), pp. 458-60.