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A New Measurement of the Cosmic Microwave Background Radiation Temperature at z = 1.97*

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Jian Ge1, Jill Bechtold1 and John H. Black1

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[1]

Redshift Dependence of the Cosmic Microwave Background Temperature from Sunyaev-Zeldovich Measurements

G. Luzzi et al.  The Astrophysical Journal 2009  705 1122
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Fine-Structure Excitation of O I and C I by Impact with Atomic Hydrogen

E. Abrahamsson et al.  The Astrophysical Journal 2007  654 1171
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Molecular Hydrogen in the Damped Lyα Absorber of Q1331+170

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Atomic and molecular processes in the early Universe

S Lepp et al  Journal of Physics B: Atomic, Molecular and Optical Physics 2002  35 R57
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[5]

H2, C I, Metallicity, and Dust Depletion in the z = 2.34 Damped Lyα Absorption System toward QSO 1232+0815

Jian Ge et al  The Astrophysical Journal Letters 2001  547 L1
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[6]

The Tolman Surface Brightness Test for the Reality of the Expansion. IV. A Measurement of the Tolman Signal and the Luminosity Evolution of Early-Type Galaxies

Lori M. Lubin and Allan Sandage  The Astronomical Journal 2001  122 1084
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[7]

The z = 1.6748 C I Absorber toward PKS 1756+237

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[8]

Molecular Hydrogen Absorption in the z = 1.97 Damped Lyα Absorption System toward Quasi-Stellar Object Q0013–004

Jian Ge and Jill Bechtold  The Astrophysical Journal Letters 1997  477 L73
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[9]

Interstellar Abundances in the Magellanic Clouds. I. GHRS Observations of the Small Magellanic Cloud Star Sk 108

D. E. Welty et al.  The Astrophysical Journal 1997  489 672
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[10]

Spectroscopy of PKS 0528–250: New Limits on CO Absorption and Emission

Jian Ge et al.  The Astrophysical Journal 1997  486 727
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