A. M. Koekemoer, P. Goudfrooij, L. L. Dressel, Santiago Arribas, Elizabeth Barker, ...
Abstract. We provide an overview of the most important calibration aspects of the NICMOS instrument on board of HST. We describe the performance of the instrument after the installation of the NICMOS...
The 2005 HST Calibration Workshop Space Telescope Science Institute, 2005 (2009)
A. M. Koekemoer, P. Goudfrooij, L. L. Dressel, Santiago Arribas, L. Eddie Bergeron, Roelof De Jong, ...
and 12 (regular) calibration programs executed after the installation of the NICMOS Cooling System (NCS). The special calibrations on Cycle 13 were focussed on a follow up of the spectroscopic...
PMAS integral field spectroscopy of luminous infrared galaxies. I.- The atlas (2009)
Alonso-Herrero, Almudena, Garcia-Marin, Macarena, Monreal-Ibero, Ana, Colina, Luis, Arribas, Santiago, Alfonso-Garzon, Julia, ...
In this paper we present PMAS optical (3800-7200A) IFS of the northern hemisphere portion of a volume-limited sample of 11 LIRGs. The PMAS observations typically cover the central ~5kpc and are...
Shapiro, Kristen L., Genzel, Reinhard, Schreiber, Natascha M. Förster, Tacconi, Linda J., Bouché, Nicolas, Cresci, Giovanni, ...
We present a simple set of kinematic criteria that can distinguish between galaxies dominated by ordered rotational motion and those involved in major merger events. Our criteria are based on the...
Shapiro, Kirsten L., Genzel, Reinhard, Förster Schreiber, Natascha M., Tacconi, Linda J., Bouché, Nicolas, Cresci, Giovanni, ...
Arribas, Santiago, Colina, Luis, Monreal-Ibero, Ana, Alfonso, Julia, García-Marín, Macarena, Alonso-Herrero, Almudena
(Ultra)Luminous Infrared Galaxies [(U)LIRGs] are much more numerous at cosmological distances than locally, and are likely precursors of elliptical galaxies. Our goal is to carry out an integral...
Presentado en el IV Curso de Iniciación a la Investigación en Estructura de la Materia: Desde las partículas subatómicas hasta los compuestos moleculares (Instituto de Estructura de la Materia,...
Integral field spectroscopy of the Luminous Infrared Galaxy Arp299 (IC694+NGC3690) (2006)
Garcia-Marin, Macarena, Colina, Luis, Arribas, Santiago, Alonso-Herrero, Almudena, Mediavilla, Evencio
The luminous infrared galaxy Arp299 (IC694+NGC3690) is studied using optical integral field spectroscopy obtained with the INTEGRAL system, together with archival Hubble Space Telescope WFPC2 and...
De Jong, Roelof S., Arribas, Santiago, Barker, Elizabeth, Bergeron, Louis E., Bohlin, Ralph C., Calzetti, Daniela, ...
We provide an overview of the most important calibration aspects of the NICMOS instrument on board of HST. We describe the performance of the instrument after the installation of the NICMOS Cooling...
Arribas, Santiago, Gilliland, Ronald L., Sparks, William B., Lopez-Martin, Luis, Mediavilla, Evencio, Gomez-Alvarez, Pedro, ...
We explore the use of Integral Field Spectroscopy (IFS) to observe extrasolar planet transits. Although this technique should find its full potential in space observations (e.g. JWST, TPF), we have...
Arribas, Santiago, Bushouse, Howard, Lucas, Ray A., Colina, Luis, Borne, Kirk D.
A sample of 19 low redshift (0.03$
Is a minor-merger driving the nuclear activity in the Seyfert 2 galaxy NGC 2110? (2002)
Delgado, Rosa M. Gonzalez, Arribas, Santiago, Perez, Enrique, Heckman, Timothy
We report on a detailed morphological and kinematic study of the isolated non-barred nearby Seyfert 2 galaxy NGC 2110. We combine Integral Field optical spectroscopy, with long-slit and WFPC2 imaging...
Colina, Luis, Arribas, Santiago, Borne, Kirk D., Monreal, Ana
Integral field optical spectroscopy with the INTEGRAL fiber-fed system and HST optical imaging are used to map the complex stellar and warm ionized gas structure in the ultraluminous infrared galaxy...
Two-Dimensional Line Strength Maps in Three Well-studied Early-Type Galaxies (1999)
Peletier, Reynier F., Vazdekis, Alexandre, Arribas, Santiago, Del Burgo, Carlos, Garcia-Lorenzo, Begona, Gutierrez, Carlos, ...
Integral field spectroscopy has been obtained for the nuclear regions of 3 large, well-studied, early-type galaxies. From these spectra we have obtained line strength maps for about 20 absorption...