Special Session Sp4  26 June 2015

Galaxy studies in the mid-infrared from space and ground

Aims and scope

Mid-infrared (MIR) observations have marked a before and an after for extragalactic astronomy, both at high-redshift and in the local universe. The Spitzer Space Telescope and the Wide-field Infrared Survey Explorer (WISE) have seen through dust clouds in our galaxy and beyond and largely increased our understanding of star formation (SF) and nuclear activity in galaxies. Furthermore, upcoming facilities such as MIRI on the James Webb Space Telescope (JWST) and METIS on the 40 m European Extremely Large Telescope (E-ELT) will be leading extragalactic research during the next decades. This Special Session will bring the MIR extragalactic community together to review some of the most salient observational and theoretical results on galaxy evolution of the last years, and discuss the challenges and opportunities brought by current and upcoming MIR instruments.

Ground-based 8 to 10 m class telescopes currently operating in the MIR are the Gran Telescopio CANARIAS (GTC) and the Subaru Telescope. On the GTC, the MIR instrument CanariCam is fully operational, and the first scientific results are starting to come out. Even smaller spatial scales than those observable with CanariCam have been probed with the MID-infrared Interferometric instrument (MIDI) on the Very Large Telescope Interferometer (VLTI), although restricted to bright and nearby sources. In 2016/17, the new VLTI instrument MATISSE (the Multi AperTure mid-Infrared SpectroScopic Experiment) will offer a more efficient capability for image reconstruction.

Much higher sensitivities are obtained from space, at the cost of lower (diffraction-limited) spatial resolutions. The high sensitivity of Spitzer allowed for the first time to study the IR emission of star-forming galaxies and active galactic nuclei (AGN) at high redshifts, and the all-sky WISE observations provided MIR photometry for a very large sample of galaxies, comparable in size to the Sloan Digital Sky Survey main galaxy sample. The launch of the JWST, planned for 2018, will represent a revolution for extragalactic astronomy, since it will combine extreme sensitivity and sub-arcsecond angular resolution. From the ground, the instrument METIS, mounted on the E-ELT, will also provide unprecedented angular resolution data. This Special Session aims to present a complete MIR view of extragalactic astronomy, focusing on interstellar dust, star formation in galaxies, (ultra-)luminous infrared galaxies and AGN.

Image: The Andromeda Galaxy observed by WISE (12-micron light has been color coded orange, and 22-micron light, red). Credit: NASA/JPL-Caltech/WISE Team.


    Key recent discoveries facilitated by MIR observations that will be discussed include:
    • The tight relation between MIR and bolometric emission from AGN.
    • The correlation between AGN activity and nuclear to galaxy-wide star formation.
    • The IR spectral energy distribution (SED) of high redshift (U)LIRGs, which unlike the mostly merger-driven local (U)LIRGs, are "normal" main sequence galaxies and have SEDs similar to those of normal star-forming galaxies in the local universe.

    Invited speakers

    • Almudena Alonso Herrero (Instituto de Física de Cantabria, Spain)
    • Bernhard Brandl (Leiden Observatory, The Netherlands)
    • Sebastian Hönig (University of Southampton, United Kingdom)
    • Pablo Pérez González (Universidad Complutense de Madrid, Spain)
    • Dimitra Rigopoulou (University of Oxford, United Kingdom)

    Scientific organisers

    • Almudena Alonso-Herrero (Instituto de Física de Cantabria, Spain)
    • Poshak Gandhi (University of Southampton, United Kingdom)
    • Evanthia Hatziminaoglou (European Southern Observatory, Germany)
    • Antonio Hernán Caballero - co-chair (Instituto de Física de Cantabria, Spain)
    • Cristina Ramos Almeida - co-chair (Instituto de Astrofísica de Canarias, Spain)
    • Henrik Spoon (Cornell University, USA)


    Updated on Tue Jun 02 11:55:42 CEST 2015