activity
20192026
most citedCCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on the Fred Young Submillimeter Telescope

101 citations · 226 across the 10 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

8 papers · 1 filter

astro-ph.GA2026

Spectral Data-cube Cleaning for CCAT Deep Spectroscopic Survey. I. Effect of correlated noise and filtering on the power spectrum

A. Dev, C. Karoumpis, Y. Okada +8

The Epoch of Reionization Spectrometer (EoR-Spec) on the Fred Young Submillimeter Telescope (FYST) will conduct the CCAT Deep Spectroscopic Survey (DSS) to perform line-intensity m…

astro-ph.GA2026

Testing masking effectiveness using multi-line image cubes based on COSMOS2020 for [CII] line intensity mapping at

J. Clarke, C. Karoumpis, A. Dev +5

We created line intensity mapping intensity cubes for CO and [CII] emission lines using the COSMOS2020 galaxy catalogue, forming predictions based on empirical data, for observatio…

astro-ph.GA2024

[CII] line intensity mapping the epoch of reionization with the Prime-Cam on FYST II. CO foreground masking based on an external catalog

C. Karoumpis, B. Magnelli, E. Romano-Díaz +7

Context. The Fred Young Submillimeter Telescope (FYST) line intensity mapping (LIM) survey will measure the power spectrum (PS) of the singly ionized carbon 158 m fine-struc…

astro-ph.GA2024★ 3 cited

[CII] luminosity models and large-scale image cubes based on COSMOS 2020 and ALPINE-ALMA [CII] data back to the epoch of reionisation

J. Clarke, C. Karoumpis, D. Riechers +5

We have implemented a novel method to create simulated [CII] emission line intensity mapping (LIM) data cubes using COSMOS 2020 galaxy catalogue data. It allows us to provide solid…

astro-ph.GA2023

ACOSMOS: Dissecting the gas content of star-forming galaxies across the main sequence at 1.2 < 1.6

Tsan-Ming Wang, Benjamin Magnelli, Eva Schinnerer +5

We aim to understand the physical mechanisms that drive star formation in a sample of mass-complete (>10) star-forming galaxies (SFGs) at 1.2 < 1.6. We se…

astro-ph.GA2022★ 49 cited

ACOSMOS: A census on the molecular gas mass and extent of main-sequence galaxies across cosmic time

Tsan-Ming Wang, Benjamin Magnelli, Eva Schinnerer +6

To constrain for the first time the mean mass and extent of the molecular gas of a mass-complete sample of M main-sequence (MS) galaxies at . We appl…

astro-ph.GA2021★ 32 cited

[CII] line intensity mapping the epoch of reionization with the Prime-Cam on FYST

C. Karoumpis, B. Magnelli, E. Romano-Díaz +2

We predict the three-dimensional intensity power spectrum (PS) of the [CII] 158m line throughout the epoch of (and post) reionization at redshifts from 3.5 to 8. We…

astro-ph.GA2019★ 41 cited

Radio continuum size evolution of star-forming galaxies over 0.35 < z < 2.25

E. F. Jiménez-Andrade, B. Magnelli, A. Karim +18

We present the first systematic study of the radio continuum size evolution of star-forming galaxies (SFGs) over the redshift range . We use the VLA COSMOS 3GHz map (n…