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

Autor: Camilla Pacifici, Kartheik G. Iyer, Bahram Mobasher, Elisabete da Cunha, Viviana Acquaviva, Denis Burgarella, Gabriela Calistro Rivera, Adam C. Carnall, Yu-Yen Chang, Nima Chartab, Kevin C. Cooke, Ciaran Fairhurst, Jeyhan Kartaltepe, Joel Leja, Katarzyna Małek, Brett Salmon, Marianna Torelli, Alba Vidal-García, Médéric Boquien, Gabriel G. Brammer, Michael J. I. Brown, Peter L. Capak, Jacopo Chevallard, Chiara Circosta, Darren Croton, Iary Davidzon, Mark Dickinson, Kenneth J. Duncan, Sandra M. Faber, Harry C. Ferguson, Adriano Fontana, Yicheng Guo, Boris Haeussler, Shoubaneh Hemmati, Marziye Jafariyazani, Susan A. Kassin, Rebecca L. Larson, Bomee Lee, Kameswara Bharadwaj Mantha, Francesca Marchi, Hooshang Nayyeri, Jeffrey A. Newman, Viraj Pandya, Janine Pforr, Naveen Reddy, Ryan Sanders, Ekta Shah, Abtin Shahidi, Matthew L. Stevans, Dian Puspita Triani, Krystal D. Tyler, Brittany N. Vanderhoof, Alexander de la Vega, Weichen Wang, Madalyn E. Weston

Publikováno v: Pacifici, C, Iyer, K G, Mobasher, B, da Cunha, E, Acquaviva, V, Burgarella, D, Rivera, G C, Carnall, A C, Chang, Y-Y, Chartab, N, Cooke, K C, Fairhurst, C, Kartaltepe, J, Leja, J, Malek, K, Salmon, B, Torelli, M, Vidal-Garcia, A, Boquien, M, Brammer, G G, Brown, M J I, Capak, P L, Chevallard, J, Circosta, C, Croton, D, Davidzon, I, Dickinson, M, Duncan, K J, Faber, S M, Ferguson, H C, Fontana, A, Guo, Y, Haeussler, B, Hemmati, S, Jafariyazani, M, Kassin, S A, Larson, R L, Lee, B, Mantha, K B, Marchi, F, Nayyeri, H, Newman, J A, Pandya, V, Pforr, J, Reddy, N, Sanders, R, Shah, E, Shahidi, A, Stevans, M L, Triani, D P, Tyler, K D, Vanderhoof, B N, de la Vega, A, Wang, W & Weston, M E 2023, ' The Art of Measuring Physical Parameters in Galaxies : A Critical Assessment of Spectral Energy Distribution Fitting Techniques ', Astrophysical Journal, vol. 944, no. 2, 141 . https://doi.org/10.3847/1538-4357/acacff

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

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::df92440c48a98ef48152b90d914453d0
http://arxiv.org/abs/2212.01915