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/

  • 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
    Citations
    55
  • The Rest-Frame Optical Luminosity Density, Color, and Stellar Mass Density of the Universe from z = 0 to z = 3
    We present the evolution of the rest-frame optical luminosity density jrestλ, the integrated rest-frame optical color, and the stellar mass density, ρ*, for a sample of Ks band-selected galaxies in the Hubble Deep Field-South (HDF-S). We derived jrestλ in the rest-frame U, B, and V bands and found that jrestλ increases by a factor of 1.9+/-0.4, 2.9
    Rudnick, Gregory et al.

    Advertised on:

    12
    2003
    Citations
    252
  • The MAGIC telescope for gamma-ray astronomy above 30 GeV
    The MAGIC telescope, presently at its commissioning phase, will become fully operative by the end of 2003. Placed at the Roque de los Muchachos Observatory (ORM) on the island of La Palma, MAGIC is the largest among new generation ground-based gamma ray telescopes, and will reach an energy threshold as low as 30 GeV. The range of the
    Moralejo, A. et al.

    Advertised on:

    12
    2003
    Citations
    1
  • The Line Emission Region in III Zw 2: Kinematics and Variability
    We have studied the Lyα, Hβ, Hα, and Mg II λ2798 line profiles of the Seyfert 1 galaxy III Zw 2. The shapes of these broad emission lines show evidence of a multicomponent origin and also features that may be identified as the peaks due to a rotating disk. We have proposed a two-component broad-line region (BLR) model consisting of an inner
    Popović, L. Č. et al.

    Advertised on:

    12
    2003
    Citations
    29
  • The Kinematic Signature of the Sagittarius Dwarf Galaxy Tidal Debris from SDSS-DR1
    Recent results from the Sloan Digital Sky Survey (SDSS) and the 2MASS All-Sky Survey have clearly revealed the extent of the spatial distribution of stars affiliated with the tidal debris tail of the Sagittarius Dwarf Galaxy (Sgr). Although these surveys help to constrain the shape of the Sgr orbit, kinematics of the tidal tail stars are crucial in
    Wilhelm, R. et al.

    Advertised on:

    12
    2003
    Citations
    0
  • The evolution of the Light Elements, Be and B (also Li), in the Galaxy
    We consider the evolution of the light elements, especially beryllium and boron but also lithium, in the Galaxy as derived from observations within 1 kpc of the Sun. The interest in Li has much to do with the evaluation of the universal baryon abundance via primordial nucleosynthesis, but the difficulties of interpretation have led to the need to
    Beckman, J. E. et al.

    Advertised on:

    12
    2003
    Citations
    0