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Astrophysical: Photometry

  • Publication
    K[s] number counts in the Groth and Coppi fields
    The COSMOS Survey is currently mapping 0.5 deg2 of sky in optical and near-IR bands to definesamples of compact galaxies at high redshift for spectroscopic...
  • Publication
    LeMMINGs. V. Nuclear activity and bulge properties: A detailed multi-component decomposition of e-MERLIN Palomar galaxies with HST
    We used high-resolution HST imaging and e-MERLIN 1.5-GHz observations of galaxy cores from the LeMMINGs survey to investigate the relation between optical...
  • Publication
    LeMMINGs. VI. Connecting nuclear activity to bulge properties of active and inactive galaxies: radio scaling relations and galaxy environment
    Multiwavelength studies indicate that nuclear activity and bulge properties are closely related, but the details remain unclear. To study this further, we...
  • Publication
    Light curve of HD 172189 (Costa+, 2007)
    The reduced photometric data of HD 172189 are provided. The original data were obtained from the XIII STEPHI campaign carried out between 7-28 June 2004 by...
  • Publication
    Light curves of SDSS J100658.40+233724.4 (Southworth+, 2009)
    We present the discovery and follow-up observations of eclipses of the cataclysmic variable star SDSS J100658.40+233724.4, fom which we determine the orbital...
  • Publication
    Lightcurve analysis of near-Earth objects from the IMPACTON project: Evidence of binary systems and cohesion strength
    Rotations of asteroids have been set and altered by several processes since their formation. In the case of the near-Earth objects (NEOs), the rotational states...
  • Publication
    LIGHTS: A robust technique to identify galaxy edges
    The LIGHTS survey is imaging galaxies at a depth and spatial resolution comparable to what the Legacy Survey of Space and Time (LSST) will produce in 10 years...
  • Publication
    Lithium depletion in CABs (Barrado y Navascues+ 1997)
    We included 2 tables containing photometric data, together equivalent width of LiI6708 A, for a sample of dwarf components of Chromospherically Active Binaries...
  • Publication
    Local Cosmology from Isolated Dwarfs: the derivation of star formation histories.
    The color-magnitude diagram (CMD) is the most powerful tool to derive quantitative star formation histories (SFHs) of complex stellar systems which host...