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  MAGPHYS+photo-z: constraining the physical properties of galaxies with unknown redshifts

Battisti, A. J., da Cunha, E., Grasha, K., Salvato, M., Daddi, E., Davies, L., et al. (2019). MAGPHYS+photo-z: constraining the physical properties of galaxies with unknown redshifts. The Astrophysical Journal, 882(2): 61. doi:10.3847/1538-4357/ab345d.

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Item Permalink: http://hdl.handle.net/21.11116/0000-0005-4ACC-3 Version Permalink: http://hdl.handle.net/21.11116/0000-0005-4ACD-2
Genre: Journal Article

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MAGPHYS+photo-z Constraining the Physical Properties of Galaxies with Unknown Redshifts.pdf (Any fulltext), 5MB
 
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 Creators:
Battisti, A. J., Author
da Cunha, E., Author
Grasha, K., Author
Salvato, M.1, Author              
Daddi, E., Author
Davies, L., Author
Jin, S., Author
Liu, D., Author
Schinnerer, E., Author
Vaccari, M., Author
Affiliations:
1High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society, ou_159890              

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 Abstract: 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<z<6.0 in the COSMOS field with robust spectroscopic redshifts. We achieve high photo-z precision (σΔz/(1+zspec) ≲0.04), high accuracy (i.e., minimal offset biases; median(Δz/(1+zspec))≲0.02), and low catastrophic failure rates (η≃4%) over all redshifts. Interestingly, we find that a weak 2175A absorption feature in the attenuation curve models is required to remove a subtle systematic photo-z offset (zphot−zspec≃−0.03) that occurs when this feature is not included. As expected, the accuracy of derived physical properties in MAGPHYS+photo-z decreases strongly as redshift uncertainty increases. The all-in-one treatment of uncertainties afforded with this code is beneficial for accurately interpreting physical properties of galaxies in large photometric datasets. Finally, we emphasize that MAGPHYS+photo-z is not intended to replace existing photo-z codes, but rather offer flexibility to robustly interpret physical properties when spectroscopic redshifts are unavailable. The MAGPHYS+photo-z code is publicly available online.

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 Dates: 2019-09-04
 Publication Status: Published online
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 Identifiers: DOI: 10.3847/1538-4357/ab345d
Other: LOCALID: 3180083
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Title: The Astrophysical Journal
Source Genre: Journal
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Publ. Info: Bristol; Vienna : IOP Publishing; IAEA
Pages: - Volume / Issue: 882 (2) Sequence Number: 61 Start / End Page: - Identifier: ISSN: 0004-637X
CoNE: https://pure.mpg.de/cone/journals/resource/954922828215_3