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Differential attenuation in star-forming galaxies at 0.3 ≲ z ≲ 1.5 in the SHARDS/CANDELS field

Autor: L Rodríguez-Muñoz, G Rodighiero, P G Pérez-González, M Talia, I Baronchelli, L Morselli, A Renzini, A Puglisi, A Grazian, A Zanella, C Mancini, A Feltre, M Romano, A Vidal García, A Franceschini, B Alcalde Pampliega, P Cassata, L Costantin, H Domínguez Sánchez, N Espino-Briones, E Iani, A Koekemoer, A Lumbreras-Calle, J M Rodríguez-Espinosa

Publikováno v: Monthly notices of the Royal Astronomical Society, 2022, Vol.510(2), pp.2061-2083 [Peer Reviewed Journal]
Digital.CSIC. Repositorio Institucional del CSIC
instname
Monthly Notices of the Royal Astronomical Society, 510(2), 2061-2083. Oxford University Press

We use a sample of 706 galaxies, selected as [O ii]λ3727 ([O ii]) emitters in the Survey for High-z Absorption Red and Dead Sources (SHARDS) on the CANDELS/GOODS-N field, to study the differential attenuation of the nebular emission with respect to

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3b7a3d189ea9f06fcc654530c122389d
https://doi.org/10.1093/mnras/stab3558

Differences and similarities of stellar populations in LAEs and LBGs at z ∼ 3.4−6.8

Autor: David Sobral, Médéric Boquien, B. Alcalde Pampliega, P. Arrabal Haro, Antonio Hernán-Caballero, L. Rodríguez-Muñoz, Casiana Muñoz-Tuñón, A. Lumbreras-Calle, J. M. Rodríguez Espinosa

Publikováno v: E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
E-Prints Complutense. Archivo Institucional de la UCM
instname

The differences between the inherent stellar populations (SPs) of LAEs and LBGs are a key factor in understanding early galaxy formation and evolution. We have run a set of SP burst-like models for a sample of 1,558 sources at $3.4
Comment: Acce

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4c990a2c24ca6683bc6b763802ff4a7a
https://eprints.ucm.es/id/eprint/62049/1/Alcaldepampliega03libre.pdf

Star-forming galaxies at low-redshift in the SHARDS survey

Autor: H. Domínguez Sánchez, Lucia Rodríguez-Muñoz, P. Arrabal Haro, M. C. Eliche-Moral, Anton M. Koekemoer, Antonio Hernán-Caballero, B. Alcalde Pampliega, A. Lumbreras-Calle, J. M. Mas-Hesse, Jairo Méndez-Abreu, Pablo G. Pérez-González, Casiana Muñoz-Tuñón, Almudena Alonso-Herrero, Alejandro Borlaff, Antonio Cava, Jesús Gallego

Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 621, pp.A52. ⟨10.1051/0004-6361/201731670⟩
E-Prints Complutense. Archivo Institucional de la UCM
instname
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid

The physical processes driving the evolution of star formation (SF) in galaxies over cosmic time still present many open questions. Recent galaxy surveys allow now to study these processes in great detail at intermediate redshift. In this work, we bu

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::69be070cf89bba082b9ecb72f5a10828
https://hal.archives-ouvertes.fr/hal-03108898/file/aa31670-17.pdf

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