MAGPHYS+photo-z: Constraining the Physical Properties of Galaxies with Unknown Redshifts
Résumé
We present an enhanced version of the multiwavelength spectral modeling code MAGPHYS that allows the estimation of galaxy photometric redshift and physical properties (e.g., stellar mass, star formation rate, dust attenuation) simultaneously, together with robust characterization of their uncertainties. The self-consistent modeling over ultraviolet to radio wavelengths in MAGPHYS+photo-z is unique compared to standard photometric redshift codes. The broader wavelength consideration is particularly useful for breaking certain degeneracies in color vs. redshift for dusty galaxies with limited observer-frame ultraviolet and optical data (or upper limits). We demonstrate the success of the code in estimating redshifts and physical properties for over 4,000 infrared-detected galaxies at 0.4
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Astrophysique [astro-ph]INSPIRE HEP : Connectez-vous pour contacter le contributeur
https://hal.science/hal-02290785
Soumis le : mardi 17 septembre 2019-23:39:14
Dernière modification le : vendredi 24 mars 2023-14:53:12
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Identifiants
- HAL Id : hal-02290785 , version 1
- ARXIV : 1908.00771
- DOI : 10.3847/1538-4357/ab345d
- INSPIRE : 1747807
Citer
A.J. Battisti, E. da Cunha, K. Grasha, M. Salvato, E. Daddi, et al.. MAGPHYS+photo-z: Constraining the Physical Properties of Galaxies with Unknown Redshifts. Astrophys.J., 2019, 882, pp.61. ⟨10.3847/1538-4357/ab345d⟩. ⟨hal-02290785⟩
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