75 citations · 135 across the 12 of their papers we have counts for
14 papers
ALMA2040: Mapping the Spatially Resolved Dust and Star Formation Physics Driving High-z Galaxy Assembly
Daizhong Liu, Gergö Popping, Pierre Cox +19
Interstellar dust reprocesses approximately half of the starlight emitted across cosmic history. However, dust temperature, which is essential to convert continuum flux into dust m…
Do Submillimeter Galaxies Trace Megaparsec Large-scale Structures? -- An Overdensity Analysis of 449 Submillimeter Galaxies in COSMOS
Canze Deng, Daizhong Liu, Helmut Dannerbauer +19
We present an environmental analysis and overdensity catalog for a large sample of submillimeter galaxies (SMGs) in the COSMOS field in order to understand whether SMGs are signpos…
Strong environmental AGN enhancement among DSFGs in z > 2 protoclusters
Monica Natalia Isla Llave, Fabio Vito, Alberto Traina +17
Galaxy protoclusters (PCs) at z > 2 are dense regions in which cold gas availability and elevated galaxy interaction rates trigger intense, often dust-obscured, star formation. The…
The observed total star formation rate function up to z \sim 6: complementary UV and IR contributions and comparison with state-of-the-art galaxy formation models
A. Traina, C. Gruppioni, I. Delvecchio +21
We investigate how the obscured IR-derived and the dust-corrected UV star formation rate functions (SFRFs) compare with each other, and with predictions from state-of-the-art theor…
An almost NIRCam-dark dusty star-forming galaxy at z=6.63
Longji Bing, Seb Oliver, Mengyuan Xiao +28
We present AC-2168, an almost NIRCam-dark, millimetre-bright galaxy in the COSMOS field. The source was identified blindly in ALMA Band-4 continuum data and remains undetected in t…
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…
Dust emission from the bulk of galaxies at the Epoch of Reionization
L. Ciesla, S. Adscheid, B. Magnelli +6
[Abridged] Our view of dust in primordial galaxies is limited towards a few tens of z~7 galaxies, pre-selected from UV-optical observations, and are thus not necessarily representa…
In-Situ Spheroid Formation in Distant Submillimeter-Bright Galaxies
Qing-Hua Tan, Emanuele Daddi, Benjamin Magnelli +14
The majority of stars in today's Universe reside within spheroids, which are bulges of spiral galaxies and elliptical galaxies. Their formation is still an unsolved problem. Infrar…
ACOSMOS: Measuring the cosmic dust-attenuated star formation rate density at
Benjamin Magnelli, Sylvia Adscheid, Tsan-Ming Wang +14
[Abridged] In recent years, conflicting results have provided an uncertain view of the dust-attenuated properties of star-forming galaxies (SFGs). To solve this, we used the…
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…
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…
ACOSMOS: the infrared luminosity function and dust-obscured star formation rate density at
A. Traina, C. Gruppioni, I. Delvecchio +16
Aims: We leverage the largest available Atacama Large Millimetre/submillimetre Array (ALMA) survey from the archive (ACOSMOS) to study to study infrared luminosity function and…
The Gas Mass Reservoir of Quiescent Galaxies at Cosmic Noon
David Blánquez-Sesé, C. Gómez-Guijarro, G. E. Magdis +14
We present a 1.1mm stacking analysis of moderately massive (log(/) = 10.7 0.2) quiescent galaxies (QGs) at , searching for cold du…
Effects of close binary evolution on the main-sequence morphology of young star clusters
Chen Wang, Norbert Langer, Abel Schootemeijer +4
Star clusters are the building blocks of galaxies. They are composed of stars of nearly equal age and chemical composition, allowing us to use them as chronometers and as testbeds…