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Emission line predictions for mock galaxy catalogues: a new differentiable and empirical mapping from DESI


Abstract We present a simple, differentiable method for predicting emission line strengths from rest-frame optical continua using an empirically-determined mapping. Extensive work has been done to develop mock galaxy catalogues that include robust predictions for galaxy photometry, but reliably predicting the strengths of emission lines has remained challenging. Our new mapping is a simple neural network implemented using the JAX Python automatic differentiation library. It is trained on Dark Energy Spectroscopic Instrument Early Release data to predict the equivalent widths (EWs) of the eight brightest optical emission lines (including Hα, Hβ, [O II], and [O III]) from a galaxy’s rest-frame optical continuum. The predicted EW distributions are consistent with the observed ones when noise is accounted for, and we find Spearman’s rank correlation coefficient ρs > 0.87 between predictions and observations for most lines. Using a non-linear dimensionality reduction technique (UMAP), we show that this is true for galaxies across the full range of observed spectral energy distributions. In addition, we find that adding measurement uncertainties to the predicted line strengths is essential for reproducing the distribution of observed line-ratios in the BPT diagram. Our trained network can easily be incorporated into a differentiable stellar population synthesis pipeline without hindering differentiability or scalability with GPUs. A synthetic catalogue generated with such a pipeline can be used to characterise and account for biases in the spectroscopic training sets used for training and calibration of photo-z’s, improving the modelling of systematic incompleteness for the Rubin Observatory LSST and other surveys.
Authors Ashod Khederlarian ORCID , Jeffrey A. Newman ORCID , Brett H. Andrews ORCID , Biprateep Dey ORCID , John Moustakas ORCID , Andrew P. Hearin ORCID , S. Juneau ORCID , Luca Tortorelli ORCID , David Gruen ORCID , ChangHoon Hahn ORCID , Rebecca Canning ORCID , Jessica Nicole Aguilar ORCID , S. P. Ahlen ORCID , David H. Brooks ORCID , Todd Claybaugh , Axel de la Macorra ORCID , P. Doel ORCID , Kevin Fanning ORCID , Simone Ferraro ORCID , Jaime E. Forero-Romero ORCID , E. Gaztañaga ORCID , Satya Gontcho A Gontcho ORCID , R. Kehoe ORCID , T. S. Kisner ORCID , Anthony Kremin ORCID , Andrew Lambert , Martin Landriau ORCID , Marc Manera ORCID , Aaron M. Meisner ORCID , R. Miquel ORCID , Eva-Maria Mueller ORCID , A. Muñoz-Gutiérrez ORCID , Adam D. Myers University of Wyoming , Jun Nie ORCID , Claire Poppett , Francisco Prada ORCID , Mehdi Rezaie ORCID , Graziano Rossi , E. Sánchez ORCID , M. Schubnell ORCID , Joseph H. Silber , David Sprayberry ORCID , G. Tarlé ORCID , B. A. Weaver , Zhimin Zhang ORCID , Hu Zou ORCID
Journal Info Oxford University Press | Monthly Notices of the Royal Astronomical Society
Publication Date 5/6/2024
ISSN 0035-8711
TypeKeyword Image article
Open Access hybrid Hybrid Access
DOI https://doi.org/10.1093/mnras/stae1189
KeywordsKeyword Image Principal Component Analysis (Score: 0.489319)