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Reference changes · DOI

Re. I. Understanding galaxy sizes, associated luminosity densities, and the artificial division of the early-type galaxy population – CORRIGENDUM

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Correction Crossref 2 open · 2 total · 0 disputed
DOI
10.1017/pasa.2019.23
Notice DOI
10.1017/pasa.2024.17
Event date
2024-03-25
Machine twin
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01One-hop citing occurrences

Correction Open
Galaxy Zoo Bar Lengths: A Catalogue of Measurements from Hubble Space Telescope Images and the Evolution of Galactic Bar Structure at z < 1

ref [41] · 2604.27100 · notice #3920 · dispute

Raw extraction · citation context

relative bar width (ω rel) as a fraction of disk size, ℓrel ≡ Lbar 2×r 90 andω rel ≡ Wbar 2×r 90 (1) wherer 90 is the 90%F814Wflux radius (A. Leauthaud et al. 2007) of the galaxy. This flux radius encompasses most of the disk and is far less influenced by fluctu- ations in central concentration (e.g.,due to bulges or bars) than radii which only consider smaller fractions of the galaxy light (A. W. Graham 2019). Choosing r90 over the more commonly-used half-light radius thus 13 considerably reduces the possibility of introducing a cor- relation between relative bar size and other galaxy prop- erties which also correlate with bulge strength (such as star-forming properties). Secondly, we seek a parameter which quantifies a galaxy's star-forming status compared to the popula-
Correction Open
Galaxy morphology dependent (black hole mass)-(velocity dispersion) relations: implications for gravitational wave forecasts and cosmological simulations

ref [110] · 2606.05808 · notice #3921 · dispute

Raw extraction · bibliography line

R _ e . I. Understanding galaxy sizes, associated luminosity densities, and the artificial division of the early-type galaxy population. , keywords =. doi:10.1017/pasa.2019.23 , archivePrefix =. 1909.04867 , primaryClass =

Parser render (TeX stripped for reading; raw above is the evidence)

R _ e . I. Understanding galaxy sizes, associated luminosity densities, and the artificial division of the early-type galaxy population., keywords =. doi:10.1017/pasa.2019.23, archivePrefix =. 1909.04867, primaryClass =

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