CONSTRAINING THE WARM DARK MATTER PARTICLE MASS THROUGH ULTRA-DEEP UV LUMINOSITY FUNCTIONS AT z = 2 - Observatoire de Paris
Journal Articles The Astrophysical Journal Year : 2016

CONSTRAINING THE WARM DARK MATTER PARTICLE MASS THROUGH ULTRA-DEEP UV LUMINOSITY FUNCTIONS AT z = 2

N. Menci
  • Function : Author
INAF - Osservatorio Astronomico di Roma
N. Sanchez
  • Function : Author
M. Castellano
INAF - Osservatorio Astronomico di Roma
A. Grazian
  • Function : Author
INAF - Osservatorio Astronomico di Roma

Domains

Sciences of the Universe [physics] Astrophysics [astro-ph] Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] Galactic Astrophysics [astro-ph.GA]

Norma G. Sanchez  : Connect in order to contact the contributor

https://hal-obspm.ccsd.cnrs.fr/obspm-02542416

Submitted on : Tuesday, April 14, 2020-4:42:11 PM

Last modification on : Friday, February 9, 2024-1:54:21 PM

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Dates and versions

obspm-02542416 , version 1 (14-04-2020)

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N. Menci, N. Sanchez, M. Castellano, A. Grazian. CONSTRAINING THE WARM DARK MATTER PARTICLE MASS THROUGH ULTRA-DEEP UV LUMINOSITY FUNCTIONS AT z = 2. The Astrophysical Journal, 2016, 818 (1), pp.90. ⟨10.3847/0004-637x/818/1/90⟩. ⟨obspm-02542416⟩

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