Tipo de publicación: Con árbitro

  • Publicación
    The effect of environment on Type Ia supernovae in the Dark Energy Survey three-year cosmological sample
    Analyses of Type Ia supernovae (SNe Ia) have found puzzling correlations between their standardized luminosities and host galaxy properties: SNe Ia in high-mass...
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    The Effect of Hot Gas in the First-Year Wilkinson Microwave Anisotropy Probe (WMAP) Data
    By cross-correlating templates constructed from the Two Micron All Sky Survey Extended Source Catalog with the first-year data from the Wilkinson Microwave...
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    The Effect of Piston Errors on the Image Quality of Ground-Based Segmented Mirror Telescopes
    The errors associated with a segmented primary mirror limit the image quality obtainable with those astronomical telescopes which employ them. It is necessary...
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    The Effect of Seeing Variations in Time-Series CCD Inner Coma Photometry of Comets: A New Correction Method
    Time series CCD photometry of the inner coma of active comets has been used over the last twenty years to determine the rotation period of their nucleus...
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    The effect of stellar activity on the Li I 6708, Na I 5896 and K I 7699 Å lines. A comparison with the Pleiades, field stars and the Sun
    An analytical model has been developed to empirically study the effects of stellar spots and faculae on the observed equivalent widths of Li i 6708, Na i 5896...
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    The effect of stellar contamination on low-resolution transmission spectroscopy: needs identified by NASA's Exoplanet Exploration Program Study Analysis Group 21
    Study Analysis Group 21 (SAG21) of NASA's Exoplanet Exploration Program Analysis Group was organized to study the effect of stellar contamination on space-based...
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    The Effect of Strong Scattering Processes in the Continuum on the Stellar Emergent Energy Distribution
    The numerical solution of the idealized, but self-consistent, LTE atmosphere problem posed by the authors has been used to introduce the effect of multiple...
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    The effect of temperature fluctuations on the determination of the carbon abundance of planetary nebulae.
    By combining the C III λλ1906+1909 with the C II λ4267 line intensities it is possible to determine T(C++); this temperature is, in general, considerably...
  • Publicación
    The effect of the environment on the stellar mass-size relationship for present-day galaxies
    In order to study how the environment can influence the relationship between the stellar mass and effective radius for nearby galaxies (z 0.12), we use a mass...