Atomic carbon at redshift ~2.5
A&A, 429 2 (2005) L25-L28
Published online: 2004-12-17
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SERENDIPITOUS ALMA DETECTION OF A DISTANT CO-EMITTING X-RAY BRIGHT GALAXY
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Herschel-ATLAS and ALMA
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Physical conditions of molecular gas in the Circinus galaxy Multi-JCO and Ci3PP0observations
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Atomic carbon as a powerful tracer of molecular gas in the high-redshift Universe: perspectives for ALMA
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Using [C i] to probe the interstellar medium in z ∼ 2.5 sub-millimeter galaxies★
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VERY LARGE ARRAY MAPPING OF THE CO(1-0) LINE IN SMM J14011+0252
Chelsea E. Sharon, Andrew J. Baker, Andrew I. Harris and Alasdair P. ThomsonThe Astrophysical Journal 765 (1) 6 (2013)
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HIGH-RESOLUTION NEAR-INFRARED IMAGING OF SUBMILLIMETER GALAXIES
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The preferentially magnified active nucleus in IRAS F10214+4724 – II. Spatially resolved cold molecular gas
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Cool Gas in High-Redshift Galaxies
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A brightz= 5.2 lensed submillimeter galaxy in the field of Abell 773
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BR1202–0725: an extreme multiple merger atz= 4.7
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CI, [CII] and CO observations towards TNJ 1338–1942: Probing the ISM in a massive proto-cluster galaxy at z = 4.11
S König, T R Greve, N Seymour, et al.Journal of Physics: Conference Series 372 012064 (2012)
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Pre-ALMA observations of GRBs in the mm/submm range
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Gas and dust in az= 2.8 obscured quasar★
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GAS AND DUST IN A SUBMILLIMETER GALAXY ATz= 4.24 FROM THEHERSCHELATLAS
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A search for gravitationally lensed water masers in dusty quasars and star-forming galaxies
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A SURVEY OF ATOMIC CARBON AT HIGH REDSHIFT
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Tracing the molecular gas in distant submillimetre galaxies via CO(1-0) imaging with the Expanded Very Large Array
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Measuring space-time variation of the fundamental constants with redshifted submillimetre transitions of neutral carbon
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The properties of the interstellar medium within a star-forming galaxy at z= 2.3
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Discovery of an extremely bright submillimeter galaxy atz = 3.93
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A search for neutral carbon towards twoz= 4.05 submillimetre galaxies, GN���20 and GN���20.2
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CONTINUUM OBSERVATIONS AT 350 MICRONS OF HIGH-REDSHIFT MOLECULAR EMISSION LINE GALAXIES
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THE WARM MOLECULAR GAS AROUND THE CLOVERLEAF QUASAR
C. M. Bradford, J. E. Aguirre, R. Aikin, et al.The Astrophysical Journal 705 (1) 112 (2009)
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IMAGING ATOMIC AND HIGHLY EXCITED MOLECULAR GAS IN az= 6.42 QUASAR HOST GALAXY: COPIOUS FUEL FOR AN EDDINGTON-LIMITED STARBURST AT THE END OF COSMIC REIONIZATION
Dominik A. Riechers, Fabian Walter, Frank Bertoldi, et al.The Astrophysical Journal 703 (2) 1338 (2009)
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Mid- and far-infrared fine-structure-line sensitivities to hypothetical variability of the fine-structure constant
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Prospects for AGN studies with ALMA
R. MaiolinoNew Astronomy Reviews 52 (6) 339 (2008)
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The CO line SED and atomic carbon in IRAS F10214+4724
Y. Ao, A. Weiß, D. Downes, et al.Astronomy & Astrophysics 491 (3) 747 (2008)
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A new approach for testing variations of fundamental constants over cosmic epochs using FIR fine-structure lines
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Detection of Emission from the CN Radical in the Cloverleaf Quasar at \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $z=2.56$ \end{document}
Dominik A. Riechers, Fabian Walter, Pierre Cox, et al.The Astrophysical Journal 666 (2) 778 (2007)
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Rapid Star Formation in the Presence of Active Galactic Nuclei
Chris Lintott and Serena VitiThe Astrophysical Journal 646 (1) L37 (2006)
https://doi.org/10.1086/506524
First Detection of HCO + Emission at High Redshift
Dominik A. Riechers, Fabian Walter, Christopher L. Carilli, et al.The Astrophysical Journal 645 (1) L13 (2006)
https://doi.org/10.1086/505908
Atomic Carbon in APM 08279+5255 atz= 3.91
J. Wagg, D. J. Wilner, R. Neri, D. Downes and T. WiklindThe Astrophysical Journal 651 (1) 46 (2006)
https://doi.org/10.1086/507677