TY  - JOUR
AU  - Ramón-Pérez, Marina
AU  - Bongiovanni, Ángel
AU  - Pérez García, Ana María
AU  - Cepa, Jordi
AU  - Nadolny, Jakup
AU  - Pintos-Castro, Irene
AU  - Lara-López, Maritza A.
AU  - Alfaro, Emilio J.
AU  - Castañeda, Héctor O.
AU  - Cerviño, Miguel
AU  - Diego, José A.
AU  - Fernández-Lorenzo, Mirian
AU  - Gallego Maestro, Jesús
AU  - González, J. Jesús
AU  - González-Serrano, J. Ignacio
AU  - Oteo Gómez, Iván
AU  - Pérez Martínez, Ricardo
AU  - Povic, Mirjana
AU  - Sánchez-Portal, Miguel
PY  - 2019
DO  - 10.1051/0004-6361/201833295
SN  - 0004-6361
UR  - https://hdl.handle.net/20.500.14352/12460
T2  - Astronomy & Astrophysics
AB  - Aims. We take advantage of the capability of the OTELO survey to obtain the Hα luminosity function (LF) at z ∼ 0.40. Because of the deepest coverage of OTELO, we are able to determine the faint end of the LF, and thus better constrain the star...
LA  - eng
PB  - EDP Sciencies
KW  - Star-formation rate
KW  - Cosmic vaiance
KW  - Line galaxies
KW  - Stellar-mass
KW  - Evolution
KW  - Hizels
KW  - Emitters
KW  - AGN
KW  - Redshifts
KW  - Z=2.23
TI  - The OTELO survey II. The faint-end of the Hα luminosity function at z ∼ 0.40
TY  - journal article
VL  - 631
ER  -