Item request has been placed! ×
Item request cannot be made. ×
loading  Processing Request

Fitting spectral energy distributions of FMOS-COSMOS emission-line galaxies at z$\sim$1.6: Star formation rates, dust attenuation, and [OIII]$\lambda$5007 emission-line luminosities

Item request has been placed! ×
Item request cannot be made. ×
loading   Processing Request
اقرأ أكثر حفظ في قائمتي
  • معلومة اضافية
    • Contributors:
      Laboratoire d'Astrophysique de Marseille (LAM); Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS); Institut Universitaire de France (IUF); Ministère de l'Education nationale, de l’Enseignement supérieur et de la Recherche (M.E.N.E.S.R.); Centro de Astronomia [Antofagasta] (CITEVA); Universidad de Antofagasta; Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES)
    • بيانات النشر:
      HAL CCSD, 2021.
    • الموضوع:
      2021
    • نبذة مختصرة :
      We perform SED fitting analysis on a COSMOS sample covering UV-to-FIR wavelengths with emission lines from the FMOS survey. The sample of 182 objects with H$\alpha$ and [OIII]$\lambda5007$ emission spans over a range of $1.40
      Comment: Accepted for publication in A&A, 17 pages, 19 figures
    • ISSN:
      0004-6361
    • الرقم المعرف:
      10.1051/0004-6361/202140890⟩
    • Rights:
      OPEN
    • الرقم المعرف:
      edsair.doi.dedup.....9f490de12943dc30f67ade2a32933189