[HTML][HTML] From clusters to proto-clusters: the infrared perspective on environmental galaxy evolution
Environment is one of the primary drivers of galaxy evolution; via multiple mechanisms, it
can control the critical process of transforming galaxies from star forming to quiescent …
can control the critical process of transforming galaxies from star forming to quiescent …
Supermassive black holes at high redshift are expected to be obscured by their massive host galaxies' interstellar medium
We combine results from deep ALMA observations of massive (M*> 10 10 M⊙) galaxies at
different redshifts to show that the column density of their interstellar medium (ISM) rapidly …
different redshifts to show that the column density of their interstellar medium (ISM) rapidly …
The ALMA REBELS Survey: dust continuum detections at z > 6.5
H Inami, HSB Algera, S Schouws… - Monthly Notices of …, 2022 - academic.oup.com
We report 18 dust continuum detections (≥ 3.3 σ) at∼ 88 and 158 out of 49 ultraviolet (UV)-
bright galaxies (M UV<− 21.3 mag) at> 6.5, observed by the Cycle-7 Atacama Large …
bright galaxies (M UV<− 21.3 mag) at> 6.5, observed by the Cycle-7 Atacama Large …
EPOCHS VI: the size and shape evolution of galaxies since z ∼ 8 with JWST Observations
We present the results of a size and structural analysis of 1395 galaxies at 0.5≤ z≲ 8 with
stellar masses log (M*/M⊙)> 9.5 within the James Webb Space Telescope Public CEERS …
stellar masses log (M*/M⊙)> 9.5 within the James Webb Space Telescope Public CEERS …
GOODS-ALMA 2.0: Source catalog, number counts, and prevailing compact sizes in 1.1 mm galaxies
Submillimeter/millimeter observations of dusty star-forming galaxies with the Atacama Large
Millimeter/submillimeter Array (ALMA) have shown that dust continuum emission generally …
Millimeter/submillimeter Array (ALMA) have shown that dust continuum emission generally …
The discovery of rest-frame UV colour gradients and a diversity of dust morphologies in bright z ≃ 7 Lyman-break galaxies
RAA Bowler, F Cullen, RJ McLure… - Monthly Notices of …, 2022 - academic.oup.com
We present deep ALMA dust continuum observations for a sample of luminous (M UV<− 22)
star-forming galaxies at z≃ 7. We detect five of the six sources in the far-infrared (FIR) …
star-forming galaxies at z≃ 7. We detect five of the six sources in the far-infrared (FIR) …
Enhanced Subkiloparsec-scale Star Formation: Results from a JWST Size Analysis of 341 Galaxies at 5< z< 14
Enhanced Subkiloparsec-scale Star Formation: Results from a JWST Size Analysis of 341
Galaxies at 5 < z < 14 - IOPscience This site uses cookies. By continuing to use this site you …
Galaxies at 5 < z < 14 - IOPscience This site uses cookies. By continuing to use this site you …
IllustrisTNG in the HSC-SSP: image data release and the major role of mini mergers as drivers of asymmetry and star formation
At fixed galaxy stellar mass, there is a clear observational connection between structural
asymmetry and offset from the star-forming main sequence, ΔSFMS. Herein, we use the …
asymmetry and offset from the star-forming main sequence, ΔSFMS. Herein, we use the …
First Light And Reionisation Epoch Simulations (flares) – IV. The size evolution of galaxies at z ≥ 5
We present the intrinsic and observed sizes of galaxies at z≥ 5 in the First Light And
Reionisation Epoch Simulations (flares). We employ the large effective volume of flares to …
Reionisation Epoch Simulations (flares). We employ the large effective volume of flares to …
Sub-millimetre galaxies with Webb-Near-infrared counterparts and multi-wavelength morphology
We utilised the unprecedented depth and resolution of recent early-release science (ERS)
JWST observations to define the near-infrared counterparts of sub-millimetre galaxies …
JWST observations to define the near-infrared counterparts of sub-millimetre galaxies …