activity
20192025
most citedSnowmass2021 CMB-HD White Paper

39 citations · 157 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.GA2025

Surveying Galaxy Clusters (in formation) in the Distant Universe

J. M. Pérez-Martínez, H. Dannerbauer, E. van Kampen +8

Present-day galaxy clusters are the largest virialized structures in the Universe, yet their early assembly remains poorly understood. At z2, clusters in formation span tens of…

astro-ph.IM2024

herakoi: a sonification experiment for astronomical data

Michele Ginolfi, Luca Di Mascolo, Anita Zanella

Recent research is revealing data-sonification as a promising complementary approach to vision, benefiting both data perception and interpretation. We present herakoi, a novel open…

astro-ph.IM2024★ 2 cited

AtLAST Science Overview Report

Mark Booth, Pamela Klaassen, Claudia Cicone +81

Submillimeter and millimeter wavelengths provide a unique view of the Universe, from the gas and dust that fills and surrounds galaxies to the chromosphere of our own Sun. Current…

astro-ph.CO2024★ 3 cited

Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: Surveying the distant Universe

Eelco van Kampen, Tom Bakx, Carlos De Breuck +27

During the most active period of star formation in galaxies, which occurs in the redshift range 1<z<3, strong bursts of star formation result in significant quantities of dust, whi…

astro-ph.GA2022★ 33 cited

The 700 ks Chandra Spiderweb Field II: Evidence for inverse-Compton and thermal diffuse emission in the Spiderweb galaxy

P. Tozzi, R. Gilli, A. Liu +22

We present the X-ray imaging and spectral analysis of the diffuse emission around the Spiderweb galaxy at z=2.16 and of its nuclear emission, based on a deep (700 ks) Chandra obser…

astro-ph.CO2022★ 16 cited

The thermal and non-thermal components within and between galaxy clusters Abell 399 and Abell 401

Federico Radiconi, Valentina Vacca, Elia Battistelli +28

We measure the local correlation between radio emission and Compton- signal across two galaxy clusters, Abell~399 and Abell~401, using maps from the Low-Frequency Array (LOFAR)…

astro-ph.CO2022★ 39 cited

Snowmass2021 CMB-HD White Paper

HD Collaboration, Simone Aiola, Yashar Akrami +61

CMB-HD is a proposed millimeter-wave survey over half the sky that would be ultra-deep (0.5 uK-arcmin) and have unprecedented resolution (15 arcseconds at 150 GHz). Such a survey w…

astro-ph.CO2021★ 2 cited

Observations of compact sources in galaxy clusters using MUSTANG2

Simon R. Dicker, Elia S. Battistelli, Tanay Bhandarkar +26

Compact sources can cause scatter in the scaling relationships between the amplitude of the thermal Sunyaev-Zel'dovich Effect (tSZE) in galaxy clusters and cluster mass. Estimates…

astro-ph.GA2021★ 17 cited

Atacama Cosmology Telescope measurements of a large sample of candidates from the Massive and Distant Clusters of WISE Survey: Sunyaev-Zeldovich effect confirmation of MaDCoWS candidates using ACT

John Orlowski-Scherer, Luca Di Mascolo, Tanay Bhandarkar +35

Galaxy clusters are an important tool for cosmology, and their detection and characterization are key goals for current and future surveys. Using data from the Wide-field Infrared…

astro-ph.CO2020★ 26 cited

The Massive and Distant Clusters of WISE Survey X: Initial Results from a Sunyaev-Zeldovich Effect Study of Massive Galaxy Clusters at z>1 using MUSTANG2 on the GBT

Simon R. Dicker, Charles E. Romero, Luca Di Mascolo +17

The properties of galaxy clusters as a function of redshift can be utilized as an important cosmological tool. We present initial results from a program of follow-up observations o…

astro-ph.CO2020★ 14 cited

CMB-HD: Astro2020 RFI Response

Neelima Sehgal, Simone Aiola, Yashar Akrami +45

CMB-HD is a proposed ultra-deep (0.5 uk-arcmin), high-resolution (15 arcseconds) millimeter-wave survey over half the sky that would answer many outstanding questions in both funda…

astro-ph.CO2019★ 5 cited

CMB-HD: An Ultra-Deep, High-Resolution Millimeter-Wave Survey Over Half the Sky

Neelima Sehgal, Simone Aiola, Yashar Akrami +37

A millimeter-wave survey over half the sky, that spans frequencies in the range of 30 to 350 GHz, and that is both an order of magnitude deeper and of higher-resolution than curren…