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Adélie Gorce
Adélie Gorce
Postdoctoral researcher @ McGill University
Verified email at mail.mcgill.ca - Homepage
Title
Cited by
Cited by
Year
Improved constraints on the 21 cm EoR power spectrum and the x-ray heating of the IGM with HERA phase I observations
T Adams, JE Aguirre, P Alexander, ZS Ali, R Baartman, Y Balfour, ...
The Astrophysical Journal 945 (2), 124, 2023
572023
Observational constraints on key-parameters of cosmic reionisation history
A Gorce, M Douspis, N Aghanim, M Langer
Astronomy & Astrophysics 616, A113, 2018
332018
Studying the morphology of reionization with the triangle correlation function of phases
A Gorce, JR Pritchard
Monthly Notices of the Royal Astronomical Society 489 (1), 1321-1337, 2019
232019
Improved constraints on reionisation from CMB observations: A parameterisation of the kSZ effect
A Gorce, S Ilić, M Douspis, D Aubert, M Langer
Astronomy & Astrophysics 640, A90, 2020
182020
Retrieving cosmological information from small-scale CMB foregrounds-II. The kinetic Sunyaev Zel’dovich effect
A Gorce, M Douspis, L Salvati
Astronomy & Astrophysics 662, A122, 2022
162022
Retrieving cosmological information from small-scale CMB foregrounds-I. The thermal Sunyaev Zel’dovich effect
M Douspis, L Salvati, A Gorce, N Aghanim
Astronomy & Astrophysics 659, A99, 2022
102022
Impact of survey geometry and super-sample covariance on future photometric galaxy surveys
SG Beauchamps, F Lacasa, I Tutusaus, M Aubert, P Baratta, A Gorce, ...
Astronomy & Astrophysics 659, A128, 2022
102022
Joint constraints on reionization: A framework for combining the global 21 cm signal and the kinetic Sunyaev-Zel’dovich effect
JM Bégin, A Liu, A Gorce
Physical Review D 105 (8), 083503, 2022
92022
Using the sample variance of 21 cm maps as a tracer of the ionisation topology
A Gorce, A Hutter, JR Pritchard
Astronomy & Astrophysics 653, A58, 2021
72021
Prospects for 21 cm Galaxy Cross-correlations with HERA and the Roman High-latitude Survey
P La Plante, J Mirocha, A Gorce, A Lidz, A Parsons
The Astrophysical Journal 944 (1), 59, 2023
62023
Impact of instrument and data characteristics in the interferometric reconstruction of the 21 cm power spectrum
A Gorce, S Ganjam, A Liu, SG Murray, Z Abdurashidova, T Adams, ...
Monthly Notices of the Royal Astronomical Society 520 (1), 375-391, 2023
52023
Efficient computation of the super-sample covariance for stage IV galaxy surveys
F Lacasa, M Aubert, P Baratta, J Carron, A Gorce, SG Beauchamps, ...
Astronomy & Astrophysics 671, A115, 2023
42023
Inferring reionization and galaxy properties from the patchy kinetic Sunyaev–Zel’dovich signal
I Nikolić, A Mesinger, Y Qin, A Gorce
Monthly Notices of the Royal Astronomical Society 526 (2), 3170-3183, 2023
22023
Constraining cosmic reionization by combining the kinetic Sunyaev–Zel’dovich and the 21 cm power spectra
I Georgiev, A Gorce, G Mellema
Monthly Notices of the Royal Astronomical Society 528 (4), 7218-7235, 2024
12024
CMB at small scales: Cosmology from tSZ power spectrum
M Douspis, L Salvati, A Gorce, N Aghanim
EPJ Web of Conferences 257, 00014, 2022
12022
Hydrogen Epoch of Reionization Array (HERA) Phase II Deployment and Commissioning
LM Berkhout, DC Jacobs, Z Abdurashidova, T Adams, JE Aguirre, ...
Publications of the Astronomical Society of the Pacific 136 (4), 045002, 2024
2024
A demonstration of the effect of fringe-rate filtering in the Hydrogen Epoch of Reionization Array delay power spectrum pipeline
H Garsden, P Bull, M Wilensky, Z Abdurashidova, T Adams, JE Aguirre, ...
arXiv preprint arXiv:2402.08659, 2024
2024
Small-scale CMB cosmological information
M Douspis, A Gorce, L Salvati
EPJ Web of Conferences 293, 00015, 2024
2024
matvis: A matrix-based visibility simulator for fast forward modelling of many-element 21 cm arrays
P Kittiwisit, SG Murray, H Garsden, P Bull, C Cain, AR Parsons, J Sipple, ...
arXiv preprint arXiv:2312.09763, 2023
2023
matvis: Fast matrix-based visibility simulator
P Kittiwisit, SG Murray, H Garsden, P Bull, C Cain, AR Parsons, J Sipple, ...
Astrophysics Source Code Library, ascl: 2312.030, 2023
2023
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