activity
20172020
most citedFast Point Spread Function Modeling with Deep Learning

51 citations · 240 across the 10 of their papers we have counts for

collaborators

11 papers

astro-ph.CO2020★ 18 cited

Fast Lightcones for Combined Cosmological Probes

Raphael Sgier, Janis Fluri, Jörg Herbel +4

The combination of different cosmological probes offers stringent tests of the CDM model and enhanced control of systematics. For this purpose, we present an extension of the li…

astro-ph.CO2020

Predicting Cosmological Observables with PyCosmo

F. Tarsitano, U. Schmitt, A. Refregier +7

Current and upcoming cosmological experiments open a new era of precision cosmology, thus demanding accurate theoretical predictions for cosmological observables. Because of the co…

astro-ph.GA2020★ 15 cited

Spectro-Imaging Forward Model of Red and Blue Galaxies

Martina Fagioli, Luca Tortorelli, Jörg Herbel +3

For the next generation of spectroscopic galaxy surveys, it is important to forecast their performances and to accurately interpret their large data sets. For this purpose, it is n…

astro-ph.GA2020★ 29 cited

Measurement of the B-band Galaxy Luminosity Function with Approximate Bayesian Computation

Luca Tortorelli, Martina Fagioli, Jörg Herbel +3

The galaxy Luminosity Function (LF) is a key observable for galaxy formation, evolution studies and for cosmology. In this work, we propose a novel technique to forward model wide-…

astro-ph.CO2019★ 26 cited

Monte Carlo Control Loops for cosmic shear cosmology with DES Year 1

T. Kacprzak, J. Herbel, A. Nicola +52

Weak lensing by large-scale structure is a powerful probe of cosmology and of the dark universe. This cosmic shear technique relies on the accurate measurement of the shapes and re…

astro-ph.GA2018★ 17 cited

The PAU Survey: A Forward Modeling Approach for Narrow-band Imaging

Luca Tortorelli, Lorenza Della Bruna, Jörg Herbel +15

Weak gravitational lensing is a powerful probe of the dark sector, once measurement systematic errors can be controlled. In Refregier & Amara (2014), a calibration method based on…

astro-ph.GA2018★ 16 cited

Forward Modeling of Spectroscopic Galaxy Surveys: Application to SDSS

Martina Fagioli, Julian Riebartsch, Andrina Nicola +6

Galaxy spectra are essential to probe the spatial distribution of galaxies in our Universe. To better interpret current and future spectroscopic galaxy redshift surveys, it is impo…

astro-ph.IM2018★ 51 cited

Fast Point Spread Function Modeling with Deep Learning

Jörg Herbel, Tomasz Kacprzak, Adam Amara +2

Modeling the Point Spread Function (PSF) of wide-field surveys is vital for many astrophysical applications and cosmological probes including weak gravitational lensing. The PSF sm…

astro-ph.CO2017★ 26 cited

Accelerating Approximate Bayesian Computation with Quantile Regression: Application to Cosmological Redshift Distributions

Tomasz Kacprzak, Jörg Herbel, Adam Amara +1

Approximate Bayesian Computation (ABC) is a method to obtain a posterior distribution without a likelihood function, using simulations and a set of distance metrics. For that reaso…

astro-ph.CO2017★ 9 cited

Cosmic shear calibration with forward modeling

Claudio Bruderer, Andrina Nicola, Adam Amara +3

Weak Gravitational Lensing is a powerful probe of the dark sector of the Universe. One of the main challenges for this technique is the treatment of systematics in the measurement…

astro-ph.CO2017★ 33 cited

The redshift distribution of cosmological samples: a forward modeling approach

Jörg Herbel, Tomasz Kacprzak, Adam Amara +3

Determining the redshift distribution of galaxy samples is essential for several cosmological probes including weak lensing. For imaging surveys, this is usually done using…