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/

  • Non-refereed
    Optical Linear Polarization in the Case of Two Supernovae Associated to X-ray Flashes: XRF060218/SN2006aj and XRF080109/SN2008D
    We present the polarization monitoring carried out for two SNe associated with GRBs: XRF060218/SN2006aj and XRF080109/SN2008D. For XRF060218/SN2006aj we measured a mean polarization of P˜4% at 2.6-5.6 days after the X-ray event. This is the highest polarization value ever measured for a supernova. We derived the intrinsic polarization of XRF080109
    Gorosabel, J. et al.

    Advertised on:

    11
    2011
    Bibcode
    2011ASPC..449..421G
    Citations
    1
  • Refereed
    Optical novae: the major class of supersoft X-ray sources in M 31
    We searched for X-ray counterparts of optical novae detected in M 31 and M 33. We combined an optical nova catalogue from the WeCAPP survey with optical novae reported in the literature and correlated them with the most recent X-ray catalogues from ROSAT, XMM-Newton, and Chandra, and in addition searched for nova correlations in archival data. We
    Pietsch, W. et al.

    Advertised on:

    11
    2005
    Bibcode
    2005A&A...442..879P
    Citations
    83
  • Refereed
    Optical studies of V404 Cyg, the X-ray transient GS 2023+338. IV. The rotation speed of the companion star.
    Not Available
    Casares, J. et al.

    Advertised on:

    11
    1994
    Bibcode
    1994MNRAS.271L...5C
    Citations
    118
  • Refereed
    Optical variability of the ultracool dwarf TVLM 513-46546: evidence for inhomogeneous dust clouds
    We present multicolour photometry of the M8.5V ultracool dwarf `pulsar' TVLM 513-46546 (hereafter TVLM 513) obtained with the triple-beam photometer ULTRACAM. Data were obtained simultaneously in the Sloan-g' and Sloan-i' bands. The previously reported sinusoidal variability, with a period of 2 h, is recovered here. However, the Sloan-g' and Sloan
    Littlefair, S. P. et al.

    Advertised on:

    11
    2008
    Bibcode
    2008MNRAS.391L..88L
    Citations
    32
  • Refereed
    Orbital periods of cataclysmic variables identified by the SDSS. VI. The 4.5-h period eclipsing system SDSS J100658.40+233724.4
    We present time-resolved spectroscopy and photometry of SDSS J100658.40+233724.4, which we have discovered to be an eclipsing cataclysmic variable with an orbital period of 0.18591324 days (267.71507 min). The observed velocity amplitude of the secondary star is 276 ± 7 km s-1, which an irradiation correction reduces to 258 ± 12 km s-1. Doppler
    Southworth, J. et al.

    Advertised on:

    11
    2009
    Bibcode
    2009A&A...507..929S
    Citations
    29