We present SPECULATOR - a fast, accurate, and flexible framework for emulating stellar population synthesis (SPS) models for predicting galaxy spectra and photometry. For emulating spectra, we use principal component analysis to construct a set of basis functions, and neural networks to learn the basis coefficients as a function of the SPS model parameters. For photometry, we parameterize the magnitudes (for the filters of interest) as a function of SPS parameters by a neural network. The resulting emulators are able to predict spectra and photometry under both simple and complicated SPS model parameterizations to percent-level accuracy, giving a factor of $10^3$-$10^4$ speed up over direct SPS computation. They have readily-computable deri...
The PRObabilistic Value-added Bright Galaxy Survey (PROVABGS) catalog will provide measurements of g...
A fundamental challenge for wide-field imaging surveys is obtaining follow-up spectroscopic obser-va...
A fundamental challenge for wide-field imaging surveys is obtaining follow-up spectroscopic observat...
We present \textsc{speculator} -- a fast, accurate, and flexible framework for emulating stellar pop...
We present SPECULATOR - a fast, accurate, and flexible framework for emulating stellar population sy...
We present a Bayesian hierarchical framework to analyze photometric galaxy survey data with stellar ...
Galaxy spectra are a useful diagnostic tool that can be used to reveal the intrinsic properties of g...
We implement a sample-efficient method for rapid and accurate emulation of semi-analytical galaxy fo...
We present a new method for inferring galaxy star formation histories (SFH) using machine learning m...
State-of-the-art cosmological hydrodynamical simulations have star particles with a typical mass bet...
With current and upcoming experiments such as WFIRST, Euclid and LSST, we can observe up to billions...
Current surveys from modern astronomical observatories contain a huge amount of data; in particular,...
Aims. We present an optimized library of synthetic galaxy spectra that are to be used for the Gaia s...
A fundamental challenge for wide-field imaging surveys is obtaining follow-up spectroscopic observat...
We present our methods for generating a catalogue of 7000 synthetic images and 40 000 integrated spe...
The PRObabilistic Value-added Bright Galaxy Survey (PROVABGS) catalog will provide measurements of g...
A fundamental challenge for wide-field imaging surveys is obtaining follow-up spectroscopic obser-va...
A fundamental challenge for wide-field imaging surveys is obtaining follow-up spectroscopic observat...
We present \textsc{speculator} -- a fast, accurate, and flexible framework for emulating stellar pop...
We present SPECULATOR - a fast, accurate, and flexible framework for emulating stellar population sy...
We present a Bayesian hierarchical framework to analyze photometric galaxy survey data with stellar ...
Galaxy spectra are a useful diagnostic tool that can be used to reveal the intrinsic properties of g...
We implement a sample-efficient method for rapid and accurate emulation of semi-analytical galaxy fo...
We present a new method for inferring galaxy star formation histories (SFH) using machine learning m...
State-of-the-art cosmological hydrodynamical simulations have star particles with a typical mass bet...
With current and upcoming experiments such as WFIRST, Euclid and LSST, we can observe up to billions...
Current surveys from modern astronomical observatories contain a huge amount of data; in particular,...
Aims. We present an optimized library of synthetic galaxy spectra that are to be used for the Gaia s...
A fundamental challenge for wide-field imaging surveys is obtaining follow-up spectroscopic observat...
We present our methods for generating a catalogue of 7000 synthetic images and 40 000 integrated spe...
The PRObabilistic Value-added Bright Galaxy Survey (PROVABGS) catalog will provide measurements of g...
A fundamental challenge for wide-field imaging surveys is obtaining follow-up spectroscopic obser-va...
A fundamental challenge for wide-field imaging surveys is obtaining follow-up spectroscopic observat...