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

Quasars Probing Galaxies. I. Signatures of Gas Accretion at Redshift z ≈ 0.2

Autor: Ho, SH, Martin, CL, Kacprzak, GG, Churchill, CW

Publikováno v: Astrophysical Journal, vol 835, iss 2

We describe the kinematics of circumgalactic gas near the galactic plane, combining new measurements of galaxy rotation curves and spectroscopy of background quasars. The sightlines pass within 19-93 kpc of the target galaxy and generally detect Mg i

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=od_______325::6165ec203c4450bfcd498001d94b1eb2
https://escholarship.org/uc/item/00p5p8r0

A massive galaxy that formed its stars at z ≈ 11.

Autor: Glazebrook K; Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, Victoria, Australia. kglazebrook@swin.edu.au., Nanayakkara T; Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, Victoria, Australia., Schreiber C; IBEX Innovations, Stockton-on-Tees, UK., Lagos C; Cosmic DAWN Center, Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark.; ARC Centre for Excellence in All-Sky Astrophysics in 3D, Canberra, Australian Capital Territory, Australia.; International Centre for Radio Astronomy Research, University of Western Australia, Crawley, Western Australia, Australia., Kawinwanichakij L; Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, Victoria, Australia., Jacobs C; Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, Victoria, Australia., Chittenden H; Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, Victoria, Australia., Brammer G; Cosmic DAWN Center, Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark., Kacprzak GG; Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, Victoria, Australia., Labbe I; Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, Victoria, Australia., Marchesini D; Physics and Astronomy Department, Tufts University, Medford, MA, USA., Marsan ZC; Department of Physics and Astronomy, York University, Toronto, Ontario, Canada., Oesch PA; Cosmic DAWN Center, Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark.; Department of Astronomy, University of Geneva, Versoix, Switzerland., Papovich C; Department of Physics and Astronomy, and George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, TX, USA., Remus RS; Universitäts-Sternwarte, Fakultät für Physik, Ludwig-Maximilians-Universität München, Munich, Germany., Tran KH; ARC Centre for Excellence in All-Sky Astrophysics in 3D, Canberra, Australian Capital Territory, Australia.; School of Physics, University of New South Wales, Kensington, New South Wales, Australia.; Center for Astrophysics, Harvard & Smithsonian, Cambridge, MA, USA., Esdaile J; Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, Victoria, Australia., Chandro-Gomez A; International Centre for Radio Astronomy Research, University of Western Australia, Crawley, Western Australia, Australia.

Publikováno v: Nature [Nature] 2024 Apr; Vol. 628 (8007), pp. 277-281. Date of Electronic Publication: 2024 Feb 14.

A massive, quiescent galaxy at a redshift of 3.717.

Autor: Glazebrook K; Centre for Astrophysics and Supercomputing, Swinburne University of Technology, PO Box 218, Hawthorn, Victoria 3122, Australia., Schreiber C; Leiden Observatory, Leiden University, PO Box 9513, 2300 RA Leiden, The Netherlands., Labbé I; Leiden Observatory, Leiden University, PO Box 9513, 2300 RA Leiden, The Netherlands., Nanayakkara T; Centre for Astrophysics and Supercomputing, Swinburne University of Technology, PO Box 218, Hawthorn, Victoria 3122, Australia., Kacprzak GG; Centre for Astrophysics and Supercomputing, Swinburne University of Technology, PO Box 218, Hawthorn, Victoria 3122, Australia., Oesch PA; Geneva Observatory, University of Geneva, Chemin des Maillettes 51, 1290 Versoix, Switzerland., Papovich C; George P. and Cynthia W. Mitchell Institute for Fundamental Physics and Astronomy, Department of Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA., Spitler LR; Macquarie Research Centre for Astronomy, Astrophysics and Astrophotonics, Macquarie University, Sydney, New South Wales 2109, Australia.; Australian Astronomical Observatory, PO Box 915, North Ryde, New South Wales 1670, Australia., Straatman CM; Max Planck Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany., Tran KH; George P. and Cynthia W. Mitchell Institute for Fundamental Physics and Astronomy, Department of Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA., Yuan T; Research School of Astronomy and Astrophysics, The Australian National University, Cotter Road, Weston Creek, Australian Capital Territory 2611, Australia.

Publikováno v: Nature [Nature] 2017 Apr 05; Vol. 544 (7648), pp. 71-74.

Astronomy. The pristine universe.

Autor: Kacprzak GG; Center for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, Victoria 3122, Australia. gkacprzak@astro.swin.edu.au

Publikováno v: Science (New York, N.Y.) [Science] 2011 Dec 02; Vol. 334 (6060), pp. 1216-7.