Publications

This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..

It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/

  • Refereed
    Stellar populations of galaxies in the ALHAMBRA survey up to z ̃ 1. IV. Properties of quiescent galaxies on the stellar mass-size plane
    Aims: We perform a comprehensive study of the stellar population properties (formation epoch, age, metallicity, and extinction) of quiescent galaxies as a function of size and stellar mass to constrain the physical mechanism governing the stellar mass assembly and the likely evolutive scenarios that explain their growth in size. Methods: After
    Díaz-García, L. A. et al.

    Advertised on:

    11
    2019
    Bibcode
    2019A&A...631A.158D
    Citations
    19
  • Refereed
    Stellar populations of galaxies in the ALHAMBRA survey up to z ̃ 1. III. The stellar content of the quiescent galaxy population during the last 8 Gyr
    Aims: We aim at constraining the stellar population properties of quiescent galaxies. These properties reveal how these galaxies evolved and assembled since z ̃ 1 up to the present time. Methods: Combining the ALHAMBRA multi-filter photo-spectra with the fitting code for spectral energy distribution MUFFIT (MUlti-Filter FITting), we built a
    Díaz-García, L. A. et al.

    Advertised on:

    11
    2019
    Bibcode
    2019A&A...631A.157D
    Citations
    13
  • Refereed
    Stellar populations of galaxies in the ALHAMBRA survey up to z ̃ 1. II. Stellar content of quiescent galaxies within the dust-corrected stellar mass-colour and the UVJ colour-colour diagrams
    Aims: Our aim is to determine the distribution of stellar population parameters (extinction, age, metallicity, and star formation rates) of quiescent galaxies within the rest-frame stellar mass-colour diagrams and UVJ colour-colour diagrams corrected for extinction up to z ̃ 1. These novel diagrams reduce the contamination in samples of quiescent
    Díaz-García, L. A. et al.

    Advertised on:

    11
    2019
    Bibcode
    2019A&A...631A.156D
    Citations
    33
  • Refereed
    SIGNALS: I. Survey description
    SIGNALS, the Star formation, Ionized Gas, and Nebular Abundances Legacy Survey, is a large observing programme designed to investigate massive star formation and H II regions in a sample of local extended galaxies. The programme will use the imaging Fourier transform spectrograph SITELLE at the Canada-France-Hawaii Telescope. Over 355 h (54.7
    Rousseau-Nepton, L. et al.

    Advertised on:

    11
    2019
    Bibcode
    2019MNRAS.489.5530R
    Citations
    51
  • Refereed
    Secondary Infall in the Seyfert’s Sextet: A Plausible Way Out of the Short Crossing Time Paradox
    We used integral field spectroscopy from CALIFA DR3 and multiwavelength publicly available data to investigate the star formation histories of galaxies in the Seyfert’s Sextet (SS; HCG 79). The galaxies H79a, H79b, H79c, and H79f have low star formation rates despite showing strong signs of interaction. By exploring their individual specific star
    López-Cruz, Omar et al.

    Advertised on:

    11
    2019
    Bibcode
    2019ApJ...886L...2L
    Citations
    2
  • Refereed
    Radial velocity confirmation of K2-100b: a young, highly irradiated, and low-density transiting hot Neptune
    We present a detailed analysis of HARPS-N radial velocity observations of K2-100, a young and active star in the Praesepe cluster, which hosts a transiting planet with a period of 1.7 d. We model the activity-induced radial velocity variations of the host star with a multidimensional Gaussian Process framework and detect a planetary signal of 10.6
    Barragán, O. et al.

    Advertised on:

    11
    2019
    Bibcode
    2019MNRAS.490..698B
    Citations
    64