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
    X-ray spectroscopy of faint X-ray background sources.
    We present results on the X-ray spectral analysis of the XMM-Newton deep surveys on the Lockman Hole and Chandra Deep Field South fields. Using the results of optical identification of sources in both fields, we have derived statistical properties of the faint X-ray population. Using the subsample with known redshifts we examine evidences of
    Streblyanska, A. et al.

    Advertised on:

    0
    2004
    Bibcode
    2004cosp...35..314S
    Citations
    0
  • Non-refereed
    Wide Field Optical Photometry of the Carina Dwarf Spheroidal Galaxy
    We present optical photometry of the Carina Dwarf Spheroidal (dSph) Galaxy. Data have been collected with CCD mosaic cameras available at the 2.2m ESO/MPI and at the 4m CTIO Blanco telescopes. Our current (V,B-V) Color-Magnitude diagram (CMD) confirms the occurrence of an old (˜ 11 Gyr) and an intermediate-age (˜ 5 Gyr ) population. Furthermore, we
    Monelli, M. et al.

    Advertised on:

    0
    2004
    Bibcode
    2004MmSAI..75..114M
    Citations
    5
  • Non-refereed
    Vestoids and V-type asteroids: A Mineralogical Characterization.
    Asteroid (4) Vesta is known as the unique large object of the main belt showing a basaltic crust and is a target of the NASA Dawn Mission. Vesta composition is also similar to that of basaltic achondrite meteorites, specifically the Eucrites, Diogenites and Howardites (HED). On the other hand, in recent taxonomies, asteroids showing a spectrum
    Duffard, R. et al.

    Advertised on:

    0
    2004
    Bibcode
    2004cosp...35..408D
    Citations
    0
  • Refereed
    The Transition from Outburst to Low Level Activity in the Low-Mass X-Ray Binary SAX J1747.0-2853
    SAX J1747.0-2853 is an X-ray transient which exhibited several outbursts between 1998 and 2001 and most probably in 1976. The outburst of 2000 was the longest and brightest. We have analyzed X-ray data sets that focus on times around the 2000 outburst and were obtained with l BeppoSAX, XMM-Newton and l RXTE.
    Werner, N. et al.

    Advertised on:

    0
    2004
    Bibcode
    2004BaltA..13..163W
    Citations
    1