189 citations · 461 across the 13 of their papers we have counts for
13 papers
ACOSMOS: The dust content of massive quiescent galaxies and its evolution with cosmic time
Sylvia Adscheid, Benjamin Magnelli, Laure Ciesla +3
We study the dust content of massive () quiescent galaxies (QGs) at redshifts to place constraints on the evolution of their cold interstella…
[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…
A 100 Mpc structure traced by hyperluminous galaxies around a massive = 2.85 protocluster
George C. P. Wang, Scott C. Chapman, Nikolaus Sulzenauer +9
We present wide-field mapping at 850 m and 450 m of the = 2.85 protocluster in the HS154919 field using the Submillimetre Common User Bolometer Array 2 (SCUBA-2). Spec…
ACOSMOS and AGOODSS: Continuum Source Catalogues and Multi-band Number Counts
Sylvia Adscheid, Benjamin Magnelli, Daizhong Liu +7
Galaxy submillimetre number counts are a fundamental measurement in our understanding of galaxy evolution models. Most early measurements are obtained via single-dish telescopes wi…
[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…
The kinematics of massive high-redshift dusty star-forming galaxies
A. Amvrosiadis, J. L. Wardlow, J. E. Birkin +18
We present a new method for modelling the kinematics of galaxies from interferometric observations by performing the optimization of the kinematic model parameters directly in visi…
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…
[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…
Starburst to quiescent from HST/ALMA: Stars and dust unveil minor mergers in submillimeter galaxies at
C. Gómez-Guijarro, S. Toft, A. Karim +32
Dust-enshrouded, starbursting, submillimeter galaxies (SMGs) at have been proposed as progenitors of compact quiescent galaxies (cQGs). To test this connectio…
Total Molecular Gas Masses of Planck - Herschel Selected Strongly Lensed Hyper Luminous Infrared Galaxies
K. C. Harrington, M. S. Yun, B. Magnelli +8
We report the detection of CO(1 - 0) line emission from seven Planck and Herschel selected hyper luminous (LIR(8-1000um) > 10^13Lsun) infrared galaxies with the Green Bank Telescop…
Molecular gas in AzTEC/C159: a star-forming disk galaxy 1.3Gyr after the Big Bang
E. F. Jiménez-Andrade, B. Magnelli, A. Karim +23
We studied the molecular gas properties of AzTEC/C159, a star-forming disk galaxy at . We secured CO molecular line detections for the and trans…
The far-infrared/radio correlation and radio spectral index of galaxies in the SFR-M* plane up to z 2
B. Magnelli, R. J. Ivison, D. Lutz +21
[Abridged] We study the evolution of the radio spectral index and far-infrared/radio correlation (FRC) across the star-formation rate-stellar masse (i.e. SFR-M*) plane up to z 2. W…
Varying [CII]/[NII] line ratios in the interacting system BR1202-0725 at z=4.7
R. Decarli, F. Walter, C. Carilli +8
We study the properties of the interstellar medium in the interacting system BR1202-0725 at z=4.7 via its [NII] and [CII] fine-structure line emission. This system consists of a QS…