Astrofísicas: Función de luminosidad

  • Publicación
    The OTELO survey. II. The faint-end of the Hα luminosity function at z ̃ 0.40
    Aims: We take advantage of the capability of the OTELO survey to obtain the Hα luminosity function (LF) at z ̃ 0.40. Because of the deepest coverage of OTELO...
  • Publicación
    The OTELO survey. Revealing a population of low-luminosity active star-forming galaxies at z ∼ 0.9
    Aims: We study a sample of Hβ emission line sources at z ∼ 0.9 to identify the star-forming galaxies sample and characterise them in terms of line luminosity...
  • Publicación
    The OTELO Survey: The Star Formation Rate Evolution of Low-mass Galaxies
    We present the analysis of a sample of Hα, Hβ, and [O II] emission line galaxies from the OTELO survey, with masses typically below $\mathrm{log}({M}_{* }/{M}_{...
  • Publicación
    The photometric properties of isolated early-type galaxies
    Isolated galaxies are important because they probe the lowest density regimes inhabited by galaxies. We define a sample of 36 nearby isolated early-type...
  • Charla
    The quest for axions
    We introduce the strong CP problem and the existence of the Axion as a possible solution. We discuss the possibility that axions are the dark matter of the...
  • Publicación
    The red giant branch phase transition: Implications for the RGB luminosity function bump and detections of Li-rich red clump stars
    We performed a detailed study of the evolution of the luminosity of He-ignition stage and of the red giant branch bump luminosity during the red giant branch...
  • Publicación
    The relation between the most-massive star and its parental star cluster mass
    We present a thorough literature study of the most-massive star, mmax, in several young star clusters in order to assess whether or not star clusters are...
  • Publicación
    The SDSS-III Baryon Oscillation Spectroscopic Survey: The Quasar Luminosity Function from Data Release Nine
    We present a new measurement of the optical quasar luminosity function (QLF), using data from the Sloan Digital Sky Survey-III: Baryon Oscillation Spectroscopic...
  • Publicación
    The sub-stellar birth rate from UKIDSS
    We present a new sample of mid-L to mid-T dwarfs with effective temperatures of 1100-1700 K selected from the UKIDSS Large Area Survey (LAS) and confirmed with...