Astrophysical: Galaxies

  • Publication
    Mid-FIR Properties of ELAIS Sources
    We present the properties of all the galaxies detected by ISO at 7, 15 and 90 microns in ELAIS northern fields. The spectral energy distribution (SED) of those...
  • Publication
    Mid-infrared Galaxy Morphology from the Spitzer Survey of Stellar Structure in Galaxies (S4G): The Imprint of the De Vaucouleurs Revised Hubble-Sandage Classification System at 3.6 μm
    Spitzer Space Telescope Infrared Array Camera imaging provides an opportunity to study all known morphological types of galaxies in the mid-IR at a depth...
  • Publication
    Mid-infrared imaging- and spectro-polarimetric subarcsecond observations of NGC 1068
    We present subarcsecond 7.5-13 μm imaging- and spectro-polarimetric observations of NGC 1068 using CanariCam on the 10.4-m Gran Telescopio CANARIAS. At all...
  • Publication
    Mid-infrared sources in the ELAIS Deep X-ray Survey
    We present a cross-correlation of the European Large Area Infrared Space Observatory (ISO) survey (ELAIS) with the ELAIS Deep X-ray Survey of the N1 and N2...
  • Publication
    Mid-infrared spectroscopy of infrared-luminous galaxies at z ~ 0.5-3
    We present results on low-resolution mid-infrared (MIR) spectra of 70 IR-luminous galaxies obtained with the infrared spectrograph (IRS) onboard Spitzer. We...
  • Publication
    Mid-IR cosmological spectrophotometric surveys from space: Measuring AGN and star formation at the cosmic noon with a SPICA-like mission
    We use the SPace Infrared telescope for Cosmology and Astrophysics (SPICA) project as a template to demonstrate how deep spectrophotometric surveys covering...
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    Mid-IR galaxy morphology from S4G (Buta+,
    The goals of the S4G project are described by Sheth et al. (2010, submitted). (1 data file).
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    MIGHTEE-H I: H I galaxy properties in the large-scale structure environment at z 0.37 from a stacking experiment
    We present the first measurement of H I mass of star-forming galaxies in different large scale structure environments from a blind survey at z ~ 0.37. In...
  • Publication
    MIGHTEE-H I: possible interactions with the galaxy NGC 895
    The transformation and evolution of a galaxy is strongly influenced by interactions with its environment. Neutral hydrogen (H I) is an excellent way to trace...