¡Nos trasladamos! E-Prints cerrará el 7 de junio.

En las próximas semanas vamos a migrar nuestro repositorio a una nueva plataforma con muchas funcionalidades nuevas. En esta migración las fechas clave del proceso son las siguientes:

7 de junio: congelación de E-Prints. A partir de este momento, no se podrá hacer ningún depósito ni cambio, modificación o edición.
12 al 30 de junio: migración de E-Prints a Docta Complutense, comprobación y visto bueno de la migración
3 de julio: entrada en producción de Docta Complutense

Es muy importante que cualquier depósito se realice en E-Prints Complutense antes del 7 de junio. En caso de urgencia para realizar un depósito, se puede comunicar a docta@ucm.es.

Spanish | Contactar

Stellar kinematics across the Hubble sequence in the CALIFA survey: general properties and aperture corrections

Impacto

Downloads

Downloads per month over past year

View download statistics for this eprint

Altmetric

>> Ir a Scopus

Buscar en Google Scholar™

Marino, Raffaella Anna and otros, ... (2017) Stellar kinematics across the Hubble sequence in the CALIFA survey: general properties and aperture corrections. Astronomy & Astrophysics, 597 . ISSN 1432-0746

Preview

PDF
14MB

Official URL: http://dx.doi.org/10.1051/0004-6361/201628625

==>>> Export to other formats

Abstract

We present the stellar kinematic maps of a large sample of galaxies from the integral-field spectroscopic survey CALIFA. The sample comprises 300 galaxies displaying a wide range of morphologies across the Hubble sequence, from ellipticals to late-type spirals. This dataset allows us to homogeneously extract stellar kinematics up to several effective radii. In this paper, we describe the level of completeness of this subset of galaxies with respect to the full CALIFA sample, as well as the virtues and limitations of the kinematic extraction compared to other well-known integral-field surveys. In addition, we provide averaged integrated velocity dispersion radial profiles for different galaxy types, which are particularly useful to apply aperture corrections for single aperture measurements or poorly resolved stellar kinematics of high-redshift sources. The work presented in this paper sets the basis for the study of more general properties of galaxies that will be explored in subsequent papers of the survey.

Item Type:	Article
Additional Information:	© ESO, 2016. Artículo firmado por 34 autores. J.F.-B. from grant AYA2013-48226-C3-1-P from the Spanish Ministry of Economy and Competitiveness (MINECO). J.F.-B. and G.v.d.V. from the FP7 Marie Curie Actions of the European Commission, via the Initial Training Network DAGAL under REA grant agreement number 289313. J.M.-A. and V.W. acknowledge support from the European Research Council Starting Grant (SEDMorph P.I. V. Wild). P.S.-B. acknowledge financial support from the BASAL CATA Center for Astrophysics and Associated Technologies through grant PFB-06. R.M.G.D. from grant AYA2014-57490-P. R.G.-B, R.M.G.D. and E.P. acknowledge support from the project JA-FQM-2828. C.J.W. acknowledges support through the Marie Curie Career Integration Grant 303912. L.G. from the Ministry of Economy, Development, and Tourism's Millennium Science Initiative through grant IC120009 awarded to The Millennium Institute of Astrophysics (MAS), and CONICYT through FONDECYT grant 3140566. I.M. from grant AYA2013-42227-P.
Uncontrolled Keywords:	Early-type galaxies; Field area survey; Potsdam multiaperture spectrophotometer; Sight velocity distributions; Emission-line kinematics; Public data release; Digital sky survey; Sauron project; Elliptic galaxies; Lenticular galaxies
Subjects:	Sciences > Physics > Astrophysics Sciences > Physics > Astronomy
ID Code:	42264
Deposited On:	26 Apr 2017 09:30
Last Modified:	10 Dec 2018 15:04

Origin of downloads

Repository Staff Only: item control page