Citation notice #3920 · 2026-07-11 03:19:04.563639+00:00
Galaxy Zoo Bar Lengths: A Catalogue of Measurements from Hubble Space Telescope Images and the Evolution of Galactic Bar Structure at z < 1
Correction
Crossref
Open
cites 10.1017/pasa.2019.23, which carries a correction notice dated 2024-03-25. One-hop deterministic notice: the citation edge exists in the Pith bibliography graph; no model judged whether the citation was load-bearing.
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01Evidence
Raw extraction · citation context · bibliography index 41
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-
02Event
- Type
- Correction
- Source
- Crossref
- Original DOI
- 10.1017/pasa.2019.23
- Notice DOI
- 10.1017/pasa.2024.17
- Date
- 2024-03-25
- Title
- Re. I. Understanding galaxy sizes, associated luminosity densities, and the artificial division of the early-type galaxy population – CORRIGENDUM
- Reasons
- ['Correction']
- Work
- - (2019) Publications of the Astronomical Society of Australia
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