The Art of Measuring Physical Parameters in Galaxies: A Critical Assessment of Spectral Energy Distribution Fitting Techniques

The study of galaxy evolution hinges on our ability to interpret multi-wavelength galaxy observations in terms of their physical properties. To do this, we rely on spectral energy distribution (SED) models which allow us to infer physical parameters from spectrophotometric data. In recent years, tha...

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Veröffentlicht in:	arXiv.org 2022-12
Hauptverfasser:	Pacifici, Camilla, Iyer, Kartheik G, Mobasher, Bahram, da Cunha, Elisabete, Acquaviva, Viviana, Burgarella, Denis, Rivera, Gabriela Calistro, Carnall, Adam C, Yu-Yen, Chang, Chartab, Nima, Cooke, Kevin C, Fairhurst, Ciaran, Kartaltepe, Jeyhan, Leja, Joel, Malek, Katarzyna, Salmon, Brett, Torelli, Marianna, Vidal-Garcia, Alba, Boquien, Mederic, Brammer, Gabriel G, Brown, Michael J I, Capak, Peter L, Chevallard, Jacopo, Circosta, Chiara, Croton, Darren, Davidzon, Iary, Dickinson, Mark, Duncan, Kenneth J, Faber, Sandra M, Ferguson, Harry C, Fontana, Adriano, Guo, Yicheng, Haeussler, Boris, Hemmati, Shoubaneh, Jafariyazani, Marziye, Kassin, Susan A, Larson, Rebecca L, Lee, Bomee, Kameswara Bharadwaj Mantha, Marchi, Francesca, Nayyeri, Hooshang, Newman, Jeffrey A, Pandya, Viraj, Pforr, Janine, Reddy, Naveen, Sanders, Ryan, Shah, Ekta, Shahidi, Abtin, Stevans, Matthew L, Triani, Dian Puspita, Tyler, Krystal D, Vanderhoof, Brittany N, de la Vega, Alexander, Wang, Weichen, Weston, Madalyn E
Format:	Artikel
Sprache:	eng
Schlagworte:	Active galactic nuclei Algorithms Astronomical models Attenuation Best practice Dust Galactic evolution Galaxy distribution Parameters Physical properties Physics - Astrophysics of Galaxies Spectral energy distribution Spectrophotometry Star & galaxy formation Star formation rate Stellar mass Uncertainty
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