Back to Search
Start Over
The evolution of the low-density HI intergalactic medium from z=3.6 to 0: Data, transmitted flux and HI column density
- Publication Year :
- 2020
- Publisher :
- arXiv, 2020.
-
Abstract
- 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<br />Comment: 24 pages, 17 figures, 8 tables, accepted for publication to MNRAS, 5 supplementary online-only tables
- Subjects :
- Voigt profile
Physics
Cosmology and Nongalactic Astrophysics (astro-ph.CO)
010308 nuclear & particles physics
Flux
FOS: Physical sciences
Probability density function
Astronomy and Astrophysics
Astrophysics
Astrophysics::Cosmology and Extragalactic Astrophysics
01 natural sciences
Spectral line
Redshift
quasars: absorption lines
Distribution (mathematics)
Settore FIS/05 - Astronomia e Astrofisica
Space and Planetary Science
cosmology: observations
Intergalactic medium
0103 physical sciences
Low density
intergalactic medium
010303 astronomy & astrophysics
Astrophysics - Cosmology and Nongalactic Astrophysics
Subjects
Details
- ISSN :
- 00358711 and 13652966
- Database :
- OpenAIRE
- Accession number :
- edsair.doi.dedup.....025f5e1b31ab22ca8439fd141a784d72
- Full Text :
- https://doi.org/10.48550/arxiv.2012.05861