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 Very Red Afterglow of GRB 000418: Further Evidence for Dust Extinction in a Gamma-Ray Burst Host Galaxy
    We report near-infrared and optical follow-up observations of the afterglow of the GRB 000418 starting 2.5 days after the occurrence of the burst and extending over nearly 7 weeks. GRB 000418 represents the second case for which the afterglow was initially identified by observations in the near-infrared. During the first 10 days its R-band
    Klose, S. et al.

    Advertised on:

    12
    2000
    Bibcode
    2000ApJ...545..271K
    Citations
    59
  • Refereed
    The visible spectra of three B stars - Pi Cet, 36 Lyn, and 134 Tau
    An identification list is presented for the visible spectra of Pi Cet (B7 V), 36 Lyn (B8 IIIp), and 134 Tau (B9 IV). Equivalent widths are measured on medium dispersion plates of 7.0 and 12.4 A/mm, and the photographic plates are digitized using a PDS 1010A microdensiometer. The effective temperature and gravity of the three stars are estimated
    Crivellari, L. et al.

    Advertised on:

    12
    1981
    Bibcode
    1981Ap&SS..80..425C
    Citations
    0
  • Refereed
    The VLT-FLAMES Tarantula Survey. XII. Rotational velocities of the single O-type stars
    Context. The 30 Doradus (30 Dor) region of the Large Magellanic Cloud, also known as the Tarantula nebula, is the nearest starburst region. It contains the richest population of massive stars in the Local Group, and it is thus the best possible laboratory to investigate open questions on the formation and evolution of massive stars. Aims: Using
    Sana, H. et al.

    Advertised on:

    12
    2013
    Bibcode
    2013A&A...560A..29R
    Citations
    187
  • Non-refereed
    The Warm-Hot Intergalactic Medium as seen by Constellation-X
    We present detailed simulations of the Warm-Hot Intergalactic Medium (WHIM) with the gratings of Constellation-X. Simulations are based on the extrapolation of the expected number density of OVII WHIM systems from hydrodynamical simulations of the local Universe, up to redshift of z=1 and down to an OVII column density of 1014 cm-2, and assume
    Nicastro, F. et al.

    Advertised on:

    12
    2005
    Bibcode
    2005AAS...207.1607N
    Citations
    0
  • Refereed
    The Wendelstein Calar Alto Pixellensing Project (WeCAPP): First MACHO Candidates
    We report the detection of the first two microlensing candidates from the Wendelstein Calar Alto Pixellensing Project (WeCAPP). Both are detected with a high signal-to-noise ratio and were filtered out from 4.5 million pixel light curves using a variety of selection criteria. Here we only consider well-sampled events with timescales of 1 day
    Riffeser, Arno et al.

    Advertised on:

    12
    2003
    Bibcode
    2003ApJ...599L..17R
    Citations
    55
  • Refereed
    The white dwarf binary pathways survey - II. Radial velocities of 1453 FGK stars with white dwarf companions from LAMOST DR 4
    We present the second paper of a series of publications aiming at obtaining a better understanding regarding the nature of type Ia supernovae (SN Ia) progenitors by studying a large sample of detached F, G and K main-sequence stars in close orbits with white dwarf companions (i.e. WD+FGK binaries). We employ the Large Sky Area Multi-Object Fibre
    Rebassa-Mansergas, A. et al.

    Advertised on:

    12
    2017
    Bibcode
    2017MNRAS.472.4193R
    Citations
    33