Astrophysical: Surveys

  • Publication
    Massive Stars in the SDSS-IV/APOGEE SURVEY. I. OB Stars
    In this work, we make use of DR14 APOGEE spectroscopic data to study a sample of 92 known OB stars. We developed a near-infrared semi-empirical spectral...
  • Publication
    Measuring brown dwarf properties from deep surveys .
    We discuss brown dwarf properties that can be measured from current and future deep surveys, and how fundamental parameters, such as the mass function and...
  • Publication
    Mid-FIR Properties of ELAIS Sources
    We present the properties of all the galaxies detected by ISO at 7, 15 and 90 microns in ELAIS northern fields. The spectral energy distribution (SED) of those...
  • Publication
    Mid-infrared sources in the ELAIS Deep X-ray Survey
    We present a cross-correlation of the European Large Area Infrared Space Observatory (ISO) survey (ELAIS) with the ELAIS Deep X-ray Survey of the N1 and N2...
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    Molecular Line Survey of CRL 618 from 80 to 276 GHz and Complete Model
    We present the complete data set, model, and line identification of a survey of the emission from the C-rich proto-planetary nebula CRL 618 performed with the...
  • Publication
    Most Hard-X-Ray-Selected Quasars in the Chandra Deep Fields are Obscured
    Measuring the population of obscured quasars is one of the key issues in understanding the evolution of active galactic nuclei (AGNs). With a redshift...
  • Publication
    Multiwavelength Study of two Unidentified γ-ray Sources
    Most counterparts of the identified low-latitude γ-ray sources are isolated neutron stars (INSs). Since INSs are characterized by an extremely high value of f X...
  • Publication
    Near-Infrared Galaxy Counts and Evolution from the Wide-Field ALHAMBRA Survey
    The ALHAMBRA survey aims to cover 4 deg2 using a system of 20 contiguous, equal width, medium-band filters spanning the range 3500 Å-9700 Å plus the standard...
  • Publication
    Near-ultraviolet absorption distribution of primitive asteroids from photometric surveys: II. Collisional families
    Context. Primitive asteroids consisting of mainly phyllosilicates and opaque minerals have great variation at near-ultraviolet (NUV) wavelengths (0.35–0.5 μm)...