The evolution of the low-density H i intergalactic medium from z = 3.6 to 0: Data, transmitted flux and H i column density*†‡,Monthly Notices of the Royal Astronomical Society

当前位置： X-MOL 学术 › Mon. Not. R. Astron. Soc. › 论文详情

Our official English website, www.x-mol.net, welcomes your feedback! (Note: you will need to create a separate account there.)

The evolution of the low-density H i intergalactic medium from z = 3.6 to 0: Data, transmitted flux and H i column density*†‡
Monthly Notices of the Royal Astronomical Society ( IF 4.7 ) Pub Date : 2020-12-14 , DOI: 10.1093/mnras/staa3844
T-S Kim _{1,

2} , B P Wakker ₁ , F Nasir _{3,

4} , R F Carswell ₅ , B D Savage ₁ , J S Bolton ₃ , A J Fox ₆ , M Viel _{2,

7,

8,

9} , M G Haehnelt ₅ , J C Charlton ₁₀ , B E Rosenwasser ₁

Affiliation

Department of Astronomy, University of Wisconsin, 475 North Charter Street, Madison, WI 53706, USA
Osservatorio Astronomico di Trieste, Via G. B. Tiepolo, 11, I-34143 Trieste, Italy
School of Physics and Astronomy, University of Nottingham, University Park, Nottingham NG7 2RD, UK
Department of Physics and Astronomy, University of California, 900 University Avenue, Riverside, CA 92507, USA
Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
AURA for ESA, Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA
SISSA, International School for Advanced Studies, Via Bonomea 265, I-34136 Trieste, Italy
INFN, Sezione di Trieste, Via Valerio 2, I-34127 Trieste, Italy
IFPU, Institute for Fundamental Physics of the Universe, Via Beirut 2, I-34014 Trieste, Italy
Department of Astronomy and Astrophysics, The Pennsylvania State University, 525 Davey Lab, University Park, PA 16802, USA

We present a new, uniform analysis of the HI transmitted flux (F) and HI column density (N(HI)) distribution in the low-density IGM as a function of redshift z for 0

中文翻译：