activity
20172026
most citedEuclid. I. Overview of the Euclid mission

550 citations · 2.5k across the 71 of their papers we have counts for

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Showing 2021Show all

9 papers · 1 filter

astro-ph.IM2021★ 12 cited

Degree-Scale Galactic Radio Emission at 122 MHz around the North Celestial Pole with LOFAR-AARTFAAC

B. K. Gehlot, L. V. E. Koopmans, A. R. Offringa +11

Aims: Contamination from bright diffuse Galactic thermal and non-thermal radio emission poses crucial challenges in experiments aiming to measure the 21-cm signal of neutral hydrog…

astro-ph.CO2021★ 30 cited

A numerical study of 21-cm signal suppression and noise increase in direction-dependent calibration of LOFAR data

M. Mevius, F. Mertens, L. V. E. Koopmans +14

We investigate systematic effects in direction dependent gain calibration in the context of the Low-Frequency Array (LOFAR) 21-cm Epoch of Reionization (EoR) experiment. The LOFAR…

astro-ph.CO2021★ 19 cited

The large-scale 21-cm power spectrum from reionization

Ivelin Georgiev, Garrelt Mellema, Sambit K. Giri +1

Radio interferometers, such as the Low-Frequency Array and the future Square Kilometre Array, are attempting to measure the spherically averaged 21-cm power spectrum from the Epoch…

astro-ph.CO2021★ 52 cited

Constraining baryonic feedback and cosmology with weak-lensing, X-ray, and kinematic Sunyaev-Zeldovich observations

Aurel Schneider, Sambit K. Giri, Stefania Amodeo +1

Modern weak-lensing observations are becoming increasingly sensitive to baryonic feedback processes which are still poorly understood. So far, this challenge has been faced either…

astro-ph.CO2021★ 88 cited

Emulation of baryonic effects on the matter power spectrum and constraints from galaxy cluster data

Sambit K. Giri, Aurel Schneider

Baryonic feedback effects consist of a major systematic for upcoming weak-lensing and galaxy-clustering surveys. In this paper, we present an emulator for the baryonic suppression…

astro-ph.CO2021★ 35 cited

Mixed dark matter: matter power spectrum and halo mass function

G. Parimbelli, G. Scelfo, S. K. Giri +4

We investigate and quantify the impact of mixed (cold and warm) dark matter models on large-scale structure observables. In this scenario, dark matter comes in two phases, a cold o…

astro-ph.CO2021★ 1 cited

Decaying Dark Matter: Simulations and Weak-Lensing Forecast

Jonathan Hubert, Aurel Schneider, Doug Potter +2

Despite evidence for the existence of dark matter (DM) from very high and low redshifts, a moderate amount of DM particle decay remains a valid possibility. This includes both mode…

astro-ph.CO2021★ 60 cited

Constraining the state of the intergalactic medium during the Epoch of Reionization using MWA 21-cm signal observations

Raghunath Ghara, Sambit K. Giri, Benedetta Ciardi +2

The Murchison Widefield Array (MWA) team has derived new upper limits on the spherically averaged power spectrum of the 21-cm signal at six redshifts in the range $z \approx 6.5-8.…

astro-ph.IM2021★ 37 cited

Deep learning approach for identification of HII regions during reionization in 21-cm observations

Michele Bianco, Sambit. K. Giri, Ilian T. Iliev +1

The upcoming Square Kilometre Array (SKA-Low) will map the distribution of neutral hydrogen during reionization, and produce a tremendous amount of 3D tomographic data. These image…