This project has two lines of fundamental development. First, the application of 3D techniques, in particular of integral field spectroscopy, to the study of extended objects (nuclear activity in galaxies, star formation regions, etc), as well as the participation in the development of new instruments and data analysis procedures related to 3D techniques. In particular, we participate in the development of HARMONI, the first-light high-spatial resolution integral field spectrograph for the ESO Extremely Large Telescope (ELT). Second, the scientific exploitation of the GTC observations of galaxies with active nuclei (AGN) obtained with the infrared instruments CanariCam and EMIR and with ALMA in the sub-mm regime. The data is being used to characterize the dusty torus that obscures local AGN and to study quasar winds in luminous obscured AGN (AGN feedback). Moreover, this project is devoted to get observing time with the JWST as part of the GATOS consortium (Galactic Activity, Torus and Outflow Survey), as well as to exploit on-going ALMA observations of nearby AGN.
Members of the project
Highlights and results
- H2020-ITN-2019 Big Data Applications for Black Hole Evolution Studies (BID4BEST) awarded to our network (PI: F. Sharkar). PhD positions will be advertised in Feb 2020.
- Starting Grant proposal "ChANGE", lead by Cristina Ramos Almeida, was selected for the interview at Brussels, which took place in June 2019.
- Pilot study of the differences between active and non-active twin galaxies on kpc-scales led by Ignacio del Moral Castro published in MNRAS (del Moral Castro, García-Lorenzo, Ramos Almeida et al. 2019).
- Study of the torus properties of an ultra-hard X-ray selected sample of Seyfert galaxies led by Ismael García Bernete published in MNRAS (García-Bernete, Ramos Almeida, Alonso-Herrero et al. 2019).
- First work entirely based on GTC/EMIR data led by Cristina Ramos Almeida published in MNRAS letters (Ramos Almeida, Acosta-Pulido, Tadhunter, et al. 2019). Multiphase outflow properties in the type-2 quasar J1509+0434.
- Cristina Ramos Almeida visiting scholar at the Institute of Astronomy of the University of Cambridge in August 2019. This stay is funded by the Severo Ochoa mobility programme.
- The HARMONI project succesfully completed the Phase B (Preliminary Design) in December 2018.
Investigating the sensitivity of observed spectral energy distributions to clumpy torus properties in Seyfert galaxies
We present nuclear spectral energy distributions (SEDs) from 1 to 18 μm of a small sample of nearby, nearly face-on and undisturbed Seyfert galaxies without prominent nuclear dust lanes. These nuclear SEDs probe the central ˜35 pc of the galaxies, on average, and include photometric and spectroscopic infrared (IR) data. We use these SEDs, theRamos Almeida, C. et al.
CALIFA: a diameter-selected sample for an integral field spectroscopy galaxy survey
We describe and discuss the selection procedure and statistical properties of the galaxy sample used by the Calar Alto Legacy Integral Field Area (CALIFA) survey, a public legacy survey of 600 galaxies using integral field spectroscopy. The CALIFA "mother sample" was selected from the Sloan Digital Sky Survey (SDSS) DR7 photometric catalogue toWalcher, C. J. et al.
Ionized gas kinematics of galaxies in the CALIFA survey. I. Velocity fields, kinematic parameters of the dominant component, and presence of kinematically distinct gaseous systems
Context. Ionized gas kinematics provide important clues to the dynamical structure of galaxies and hold constraints to the processes driving their evolution. Aims: The motivation of this work is to provide an overall characterization of the kinematic behavior of the ionized gas of the galaxies included in the Calar Alto Legacy Integral field AreaGarcía-Lorenzo, B. et al.