RT Book, Section
T1 Spectrophotometric study in the near-ir of a sample of MIPS selected galaxies at Z~2
A1 Sánchez De Miguel, Alejandro
A1 Gallego Maestro, Jesús
A1 Pérez González, Pablo Guillermo
A1 Cardiel López, Nicolás
A1 Zamorano Calvo, Jaime
A1 Guzmán, R.
A1 González, A.
A1 Gruel, N.
AB Our main objective is to determine what kind of galaxies dominate the cosmic SFR density at z~2. Our sample consists of 24 galaxies in Chandra Deep Field South, a unique field for the study of galaxy evolution (12 observed with GNIRS/GEMINI and 12 with ISAAC/VLT). We use H alpha together with the already merged X-ray, ultraviolet, optical, near and mid-infrared imaging data to obtain estimations of SFRs, metallicities, stellar and dynamical masses, AGN activity, and extinction properties. We have obtained 15 Hα detections, 4 rotation curves, and SFR relationship for 7 galaxies. The metallicities obtained for 8 galaxies of the sample are compatible with the metallicities of local galaxies.
PB Universidad Nacional Autónoma Mexico, Instituto Astronomía
SN 978-607-02-4281-6
YR 2013
FD 2013
LK https://hdl.handle.net/20.500.14352/45643
UL https://hdl.handle.net/20.500.14352/45643
LA eng
NO © 2013 Instituto de Astronomía, UNAM. Science with the GTC Meeting (4º. 2011. Santa Cruz La Palma, España).
DS Docta Complutense
RD 21 abr 2025