A new derivation of the Hubble constant from γ-ray attenuation using improved optical depths for the Fermi and CTA era

Research output: Contribution to journalJournal articleResearchpeer-review

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A new derivation of the Hubble constant from γ-ray attenuation using improved optical depths for the Fermi and CTA era. / Domínguez, A; Østergaard kirkeberg, P; Wojtak, R; Saldana-lopez, A; Desai, A; Primack, J R; Finke, J; Ajello, M; Pérez-gonzález, P G; Paliya, V S; Hartmann, D.

In: Monthly Notices of the Royal Astronomical Society, Vol. 527, No. 3, 02.01.2024, p. 4632-4642.

Research output: Contribution to journalJournal articleResearchpeer-review

Harvard

Domínguez, A, Østergaard kirkeberg, P, Wojtak, R, Saldana-lopez, A, Desai, A, Primack, JR, Finke, J, Ajello, M, Pérez-gonzález, PG, Paliya, VS & Hartmann, D 2024, 'A new derivation of the Hubble constant from γ-ray attenuation using improved optical depths for the Fermi and CTA era', Monthly Notices of the Royal Astronomical Society, vol. 527, no. 3, pp. 4632-4642. https://doi.org/10.1093/mnras/stad3425

APA

Domínguez, A., Østergaard kirkeberg, P., Wojtak, R., Saldana-lopez, A., Desai, A., Primack, J. R., Finke, J., Ajello, M., Pérez-gonzález, P. G., Paliya, V. S., & Hartmann, D. (2024). A new derivation of the Hubble constant from γ-ray attenuation using improved optical depths for the Fermi and CTA era. Monthly Notices of the Royal Astronomical Society, 527(3), 4632-4642. https://doi.org/10.1093/mnras/stad3425

Vancouver

Domínguez A, Østergaard kirkeberg P, Wojtak R, Saldana-lopez A, Desai A, Primack JR et al. A new derivation of the Hubble constant from γ-ray attenuation using improved optical depths for the Fermi and CTA era. Monthly Notices of the Royal Astronomical Society. 2024 Jan 2;527(3):4632-4642. https://doi.org/10.1093/mnras/stad3425

Author

Domínguez, A ; Østergaard kirkeberg, P ; Wojtak, R ; Saldana-lopez, A ; Desai, A ; Primack, J R ; Finke, J ; Ajello, M ; Pérez-gonzález, P G ; Paliya, V S ; Hartmann, D. / A new derivation of the Hubble constant from γ-ray attenuation using improved optical depths for the Fermi and CTA era. In: Monthly Notices of the Royal Astronomical Society. 2024 ; Vol. 527, No. 3. pp. 4632-4642.

Bibtex

@article{4e2232c85fe040a6b0a72652e11e1ece,
title = "A new derivation of the Hubble constant from γ-ray attenuation using improved optical depths for the Fermi and CTA era",
author = "A Dom{\'i}nguez and P {\O}stergaard kirkeberg and R Wojtak and A Saldana-lopez and A Desai and Primack, {J R} and J Finke and M Ajello and P{\'e}rez-gonz{\'a}lez, {P G} and Paliya, {V S} and D Hartmann",
year = "2024",
month = jan,
day = "2",
doi = "10.1093/mnras/stad3425",
language = "English",
volume = "527",
pages = "4632--4642",
journal = "Royal Astronomical Society. Monthly Notices",
issn = "0035-8711",
publisher = "Oxford University Press",
number = "3",

}

RIS

TY - JOUR

T1 - A new derivation of the Hubble constant from γ-ray attenuation using improved optical depths for the Fermi and CTA era

AU - Domínguez, A

AU - Østergaard kirkeberg, P

AU - Wojtak, R

AU - Saldana-lopez, A

AU - Desai, A

AU - Primack, J R

AU - Finke, J

AU - Ajello, M

AU - Pérez-gonzález, P G

AU - Paliya, V S

AU - Hartmann, D

PY - 2024/1/2

Y1 - 2024/1/2

U2 - 10.1093/mnras/stad3425

DO - 10.1093/mnras/stad3425

M3 - Journal article

VL - 527

SP - 4632

EP - 4642

JO - Royal Astronomical Society. Monthly Notices

JF - Royal Astronomical Society. Monthly Notices

SN - 0035-8711

IS - 3

ER -

ID: 388784832