activity
20132026
most citedGaia DR2 unravels incompleteness of nearby cluster population: New open clusters in the direction of Perseus

120 citations · 462 across the 25 of their papers we have counts for

collaborators

25 papers

gr-qc2026

Beyond ΛCDM with the SKA Observatory -- I: Probing Gravity on Cosmological Scales

S. Camera, C. Addis, S. L. Guedezounme +26

General relativity (GR) is currently the best description of the gravitational interaction at our disposal and is one of the foundations of the concordance cosmological model. For…

astro-ph.CO2026

Constraining reionization morphology and source properties with 21cm galaxy cross-correlation surveys

Yannic Pietschke, Anne Hutter, Caroline Heneka

Cross-correlations between 21cm observations and galaxy surveys provide a powerful probe of reionization by providing robustness against foreground contamination while linking ioni…

astro-ph.CO2025★ 3 cited

The 21cm-galaxy cross-correlation: Realistic forecast for 21cm signal detection and reionisation constraints

Anne Hutter, Caroline Heneka

21cm-galaxy cross-correlation will play a key role in confirming the cosmological 21cm signal. We investigate which survey configurations detect the 21cm-LAE cross-correlation sign…

astro-ph.GA2024★ 7 cited

Galaxy Spectra Networks (GaSNet). III. Generative pre-trained network for spectrum reconstruction, redshift estimate and anomaly detection

Fucheng Zhong, Nicola R. Napolitano, Caroline Heneka +11

Classification of spectra (1) and anomaly detection (2) are fundamental steps to guarantee the highest accuracy in redshift measurements (3) in modern all-sky spectroscopic surveys…

astro-ph.CO2023★ 3 cited

Deep Learning 21cm Lightcones in 3D

Caroline Heneka

Interferometric measurements of the 21cm signal are a prime example of the data-driven era in astrophysics we are entering with current and upcoming experiments. We showcase the us…

astro-ph.IM2023★ 10 cited

Galaxy Spectra neural Network (GaSNet). II. Using Deep Learning for Spectral Classification and Redshift Predictions

Fucheng Zhong, Nicola R. Napolitano, Caroline Heneka +25

Large sky spectroscopic surveys have reached the scale of photometric surveys in terms of sample sizes and data complexity. These huge datasets require efficient, accurate, and fle…

astro-ph.CO2023★ 14 cited

On the general nature of 21cm-Lyman- emitters cross-correlations during reionisation

Anne Hutter, Caroline Heneka, Pratika Dayal +4

We explore how the characteristics of the cross-correlation functions between the 21cm emission from the spin-flip transition of neutral hydrogen (HI) and early Lyman- (Ly) r…

astro-ph.CO2022★ 43 cited

Cosmology with one galaxy?

Francisco Villaescusa-Navarro, Jupiter Ding, Shy Genel +10

Galaxies can be characterized by many internal properties such as stellar mass, gas metallicity, and star-formation rate. We quantify the amount of cosmological and astrophysical i…

astro-ph.CO2021★ 21 cited

Optimal survey parameters: Ly and H intensity mapping for synergy with the 21cm signal during reionization

Caroline Heneka, Asantha Cooray

Intensity mapping of multiple emission lines is emerging as a new branch to astronomy, to probe both properties of ionizing sources and the medium between, in particular the interg…

physics.soc-ph2020

Women in academia: a warning on selection bias in gender studies from the astronomical perspective

M. L. L. Dantas, E. Cameron, Rafael S. de Souza +13

The recent paper by AlShebli et al. (2020) investigates the impact of mentorship in young scientists. Among their conclusions, they state that female protégés benefit more from mal…

astro-ph.CO2020★ 17 cited

The spin-temperature dependence of the 21cm -- LAE cross-correlation

Caroline Heneka, Andrei Mesinger

Cross-correlating 21cm with known cosmic signals will be invaluable proof of the cosmic origin of the first 21cm detections. As some of the widest fields available, comprising thou…

astro-ph.CO2019★ 18 cited

Constraining coupled quintessence with the 21cm signal

Xue-Wen Liu, Caroline Heneka, Luca Amendola

The 21cm line probes the evolution of matter perturbations over a wide range of redshifts, from the dark ages down to the completion of reionization. Observing the 21cm cosmologica…

astro-ph.GA2019★ 59 cited

Photometry of high-redshift blended galaxies using deep learning

Alexandre Boucaud, Marc Huertas-Company, Caroline Heneka +11

The new generation of deep photometric surveys requires unprecedentedly precise shape and photometry measurements of billions of galaxies to achieve their main science goals. At su…

astro-ph.CO2019★ 7 cited

Tomography of the Cosmic Dawn and Reionization Eras with Multiple Tracers

Tzu-Ching Chang, Angus Beane, Olivier Dore +41

The Cosmic Dawn and Reionization epochs remain a fundamental but challenging frontier of astrophysics and cosmology. We advocate a large-scale, multi-tracer approach to develop a c…

astro-ph.GA2019★ 18 cited

CDIM: Cosmic Dawn Intensity Mapper Final Report

Asantha Cooray, Tzu-Ching Chang, Stephen Unwin +23

The Cosmic Dawn Intensity Mapper (CDIM) will transform our understanding of the era of reionization when the Universe formed the first stars and galaxies, and UV photons ionized th…

astro-ph.GA2019★ 6 cited

Cosmic Dawn and Reionization: Astrophysics in the Final Frontier

Asantha Cooray, James Aguirre, Yacine Ali-Haimoud +71

The cosmic dawn and epoch of reionization mark the time period in the universe when stars, galaxies, and blackhole seeds first formed and the intergalactic medium changed from neut…

astro-ph.CO2018★ 8 cited

Stress testing the dark energy equation of state imprint on supernova data

Ben Moews, Rafael S. de Souza, Emille E. O. Ishida +4

This work determines the degree to which a standard Lambda-CDM analysis based on type Ia supernovae can identify deviations from a cosmological constant in the form of a redshift-d…

astro-ph.GA2018★ 120 cited

Gaia DR2 unravels incompleteness of nearby cluster population: New open clusters in the direction of Perseus

T. Cantat-Gaudin, A. Krone-Martins, N. Sedaghat +13

Open clusters (OCs) are popular tracers of the structure and evolutionary history of the Galactic disk. The OC population is often considered to be complete within 1.8 kpc of the S…

astro-ph.CO2018★ 2 cited

Status of kinematic cosmology with SN Ia: JLA, Pantheon and future constraints with LSST

Caroline Heneka

In this work we derive state-of-the-art model-independent constraints on cosmology from SN Ia by measuring purely kinematical model parameters (where and $…

astro-ph.CO2018★ 1 cited

Constraining General Modifications of Gravity during Reionisation

C. Heneka, L. Amendola

Intensity mapping enables us to test cosmology and fundamental physics during the Epoch of Reionisation, with power spectra of line fluctuations probing a large range of scales and…

astro-ph.CO2018★ 21 cited

General Modified Gravity With 21cm Intensity Mapping: Simulations and Forecast

C. Heneka, L. Amendola

Line intensity mapping opens up a new and exciting window for probing cosmology and fundamental physics during the Epoch of Reionisation, extending to redshifts previously untested…

astro-ph.CO2017★ 19 cited

Cold dark energy constraints from the abundance of galaxy clusters

Caroline Heneka, David Rapetti, Matteo Cataneo +3

We constrain cold dark energy of negligible sound speed using galaxy cluster abundance observations. In contrast to standard quasi-homogeneous dark energy, negligible sound speed i…

astro-ph.CO2016★ 39 cited

Probing the Intergalactic Medium with Ly and 21 cm Fluctuations

Caroline Heneka, Asantha Cooray, Chang Feng

We study 21cm and Ly fluctuations, as well as H, while distinguishing between Ly emission of galactic, diffuse, and scattered intergalactic medium (IG…

astro-ph.CO2014★ 1 cited

Searching for bias and correlations in a Bayesian way

Caroline Heneka, Alexandre Posada, Valerio Marra +1

A range of Bayesian tools has become widely used in cosmological data treatment and parameter inference (see Kunz, Bassett & Hlozek (2007), Trotta (2008), Amendola, Marra & Quartin…