activity
20182026
most citedThe PAU Survey: Early demonstration of photometric redshift performance in the COSMOS field

69 citations · 538 across the 43 of their papers we have counts for

collaborators
Showing 2024Show all

8 papers · 1 filter

astro-ph.CO2024★ 2 cited

galsbi: A Python package for the GalSBI galaxy population model

Silvan Fischbacher, Beatrice Moser, Tomasz Kacprzak +5

Large-scale structure surveys measure the shapes and positions of millions of galaxies in order to constrain the cosmological model with high precision. The resulting large data vo…

astro-ph.IM2024★ 3 cited

UFig v1: The ultra-fast image generator

Silvan Fischbacher, Beatrice Moser, Tomasz Kacprzak +8

With the rise of simulation-based inference (SBI) methods, simulations need to be fast as well as realistic. is a public Python package that simulates astronomic…

astro-ph.CO2024

GalSBI: Phenomenological galaxy population model for cosmology using simulation-based inference

Silvan Fischbacher, Tomasz Kacprzak, Luca Tortorelli +4

We present GalSBI, a phenomenological model of the galaxy population for cosmological applications using simulation-based inference. The model is based on analytical parametrizatio…

astro-ph.CO2024★ 12 cited

Impact of stellar population synthesis choices on forward modelling-based redshift distribution estimates

Luca Tortorelli, Jamie McCullough, Daniel Gruen

The forward modelling of galaxy surveys has recently gathered interest as one of the primary methods to achieve the required precision on the estimate of the redshift distributions…

astro-ph.GA2024★ 8 cited

The PAU Survey: galaxy stellar population properties estimates with narrowband data

Benjamin Csizi, Luca Tortorelli, Małgorzata Siudek +17

Narrowband galaxy surveys have recently gained interest as a promising method to achieve the necessary accuracy on the photometric redshift estimate of individual galaxies for stag…

astro-ph.GA2024★ 6 cited

Emission Line Predictions for Mock Galaxy Catalogues: a New Differentiable and Empirical Mapping from DESI

Ashod Khederlarian, Jeffrey A. Newman, Brett H. Andrews +43

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…

astro-ph.CO2024★ 5 cited

The powerful lens galaxy cluster PLCK G287.0+32.9 ()

Maurizio D'Addona, Amata Mercurio, Piero Rosati +17

We present a new high-precision strong lensing model of PLCK G287.032.9, a massive lens galaxy cluster at , with the aim to get an accurate estimation of its effective…

astro-ph.CO2024★ 13 cited

Simulation-based inference of deep fields: galaxy population model and redshift distributions

Beatrice Moser, Tomasz Kacprzak, Silvan Fischbacher +3

Accurate redshift calibration is required to obtain unbiased cosmological information from large-scale galaxy surveys. In a forward modelling approach, the redshift distribution n(…