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
    The bright optical afterglow of the long GRB 001007
    We present optical follow up observations of the long GRB 001007 between 6.14 hours and ~468 days after the event. An unusually bright optical afterglow (OA) was seen to decline following a steep power law decay with index α = -2.03 ± 0.11, possibly indicating a break in the light curve at t - t0 3.5 days, as found in other bursts. Upper limits
    Castro Cerón, J. M. et al.

    Advertised on:

    10
    2002
    Bibcode
    2002A&A...393..445C
    Citations
    10
  • Refereed
    The brightest pure-H ultracool white dwarf
    We report the identification of LSR J0745+2627 in the United Kingdom InfraRed Telescope Infrared Deep Sky Survey (UKIDSS) Large Area Survey (LAS) as a cool white dwarf with kinematics and age compatible with the thick-disk/halo population. LSR J0745+2627 has a high proper motion (890 mas/yr) and a high reduced proper motion value in the J band (HJ
    Catalán, S. et al.

    Advertised on:

    10
    2012
    Bibcode
    2012A&A...546L...3C
    Citations
    9
  • Refereed
    The Brightest Young Star Clusters in NGC 5253.
    The nearby dwarf starburst galaxy NGC 5253 hosts a number of young, massive star clusters, the two youngest of which are centrally concentrated and surrounded by thermal radio emission (the “radio nebula”). To investigate the role of these clusters in the starburst energetics, we combine new and archival Hubble Space Telescope images of NGC 5253
    Calzetti, D. et al.

    Advertised on:

    10
    2015
    Bibcode
    2015ApJ...811...75C
    Citations
    63
  • Refereed
    The C+N+O abundances and the splitting of the subgiant branch in the globular cluster NGC 1851
    Among the newly discovered features of multiple stellar populations in globular clusters (GCs), the cluster NGC 1851 harbours a double subgiant branch (SGB), that can be explained in terms of two stellar generations, only slightly differing in age, the younger one having an increased total C+N+O abundance. Thanks to this difference in the chemistry
    Ventura, P. et al.

    Advertised on:

    10
    2009
    Bibcode
    2009MNRAS.399..934V
    Citations
    85