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20212026
most citedEvidence for strong progenitor age dependence of type Ia supernova luminosity standardization process

18 citations · 18 across the 7 of their papers we have counts for

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5 papers · 1 filter

astro-ph.GA2026

Strong Progenitor Age Bias in Supernova Cosmology. III. Progenitor Age as the Physical Origin of the Type Ia Supernova Magnitude Steps with Host Properties

Seunghyun Park, Young-Wook Lee, Chul Chung +4

The standardized magnitude of a type Ia supernova (SN Ia) correlates with host-galaxy properties, and a host mass-step correction is now routinely included in SN Ia luminosity stan…

astro-ph.GA2026

How Robust is the Cosmic Distance with Tip of Red Giant Branch against Stellar Population Variations?

Chul Chung, Young-Wook Lee, Suk-Jin Yoon +10

The tip of the red giant branch (TRGB) provides a key standard candle for extragalactic distance measurements and for refining the Hubble constant. We test its robustness by quanti…

astro-ph.GA2024

Strong progenitor age bias in supernova cosmology. I. Robust and ubiquitous evidence from a larger sample of host galaxies in a broader redshift range

Chul Chung, Seunghyun Park, Junhyuk Son +2

Type Ia supernovae (SNe Ia) serve as the most crucial standardizable candles in cosmology, providing direct measurements of the universe's expansion history. However, it is well-kn…

astro-ph.GA2023

On the root cause of the host `mass-step' in the Hubble residuals of type Ia supernovae

Chul Chung, Suk-Jin Yoon, Seunghyun Park +4

It is well established that the Hubble residuals of type Ia supernovae (SNe Ia) show the luminosity step with respect to their host galaxy stellar masses. This `mass-step' is taken…

astro-ph.GA2021★ 18 cited

Evidence for strong progenitor age dependence of type Ia supernova luminosity standardization process

Young-Wook Lee, Chul Chung, Pierre Demarque +3

Supernova (SN) cosmology is based on the assumption that the width-luminosity relation (WLR) and the color-luminosity relation (CLR) in the type Ia SN luminosity standardization wo…