activity
20112025
most citedDetecting the integrated Sachs-Wolfe effect with stacked voids

89 citations · 127 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2025★ 1 cited

Combining CMB datasets with consistent foreground modelling

M. Tristram, M. Douspis, A. Gorce +7

We present a joint cosmological analysis combining data from the Planck satellite, the Atacama Cosmology Telescope, and the South Pole Telescope. We construct a unified likelihood…

astro-ph.CO2024★ 4 cited

YOLO-CL cluster detection in the Rubin/LSST DC2 simulation

Kirill Grishin, Simona Mei, Stephane Ilic +4

LSST will provide galaxy cluster catalogs up to z1 that can be used to constrain cosmological models once their selection function is well-understood. We have applied the dee…

astro-ph.CO2024

Cosmological measurement of the gravitational constant using the CMB, the BAO and the BBN

Brahim Lamine, Yacob Ozdalkiran, Louis Mirouze +5

Recent cosmological observations have provided numerous new observations with increasing precision that have led to the era of precision cosmology. The exquisite quality of these o…

astro-ph.CO2023★ 19 cited

YOLO-CL: Galaxy cluster detection in the SDSS with deep machine learning

Kirill Grishin, Simona Mei, Stéphane Ilic

(Abridged) Galaxy clusters are a powerful probe of cosmological models. Next generation large-scale optical and infrared surveys will reach unprecedented depths over large areas an…

astro-ph.CO2013★ 89 cited

Detecting the integrated Sachs-Wolfe effect with stacked voids

S. Ilic, M. Langer, M. Douspis

The stacking of cosmic microwave background (CMB) patches has been recently used to detect the integrated Sachs-Wolfe effect (iSW). When focusing on the locations of superstructure…

astro-ph.CO2011★ 14 cited

Cross-correlation between the cosmic microwave and infrared backgrounds for integrated Sachs-Wolfe detection

S. Ilic, M. Douspis, M. Langer +2

We investigate the cross-correlation between the cosmic infrared background (CIB) and cosmic microwave background (CMB) anisotropies due to the integrated Sachs-Wolfe (ISW) effect.…