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Main Authors: Rojas-Bravo, César, Sun, Ning-Chen, Smith, Mathew, Chen, Chun, Chen, Xiaohan, Niu, Zexi, Wang, Anyu, Wang, Zi-Yang, Zhao, Yi-Han, Liu, Jifeng
Format: Preprint
Published: 2026
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Online Access:https://arxiv.org/abs/2605.14437
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author Rojas-Bravo, César
Sun, Ning-Chen
Smith, Mathew
Chen, Chun
Chen, Xiaohan
Niu, Zexi
Wang, Anyu
Wang, Zi-Yang
Zhao, Yi-Han
Liu, Jifeng
author_facet Rojas-Bravo, César
Sun, Ning-Chen
Smith, Mathew
Chen, Chun
Chen, Xiaohan
Niu, Zexi
Wang, Anyu
Wang, Zi-Yang
Zhao, Yi-Han
Liu, Jifeng
contents Early-time flux excesses in Type Ia supernovae (SNe~Ia) offer a unique insight into their progenitor systems and explosion mechanisms. Although individual early-excess events and larger searches have been reported, demographic studies remain limited by sample size. We present a systematic search for early-time excess emission in a volume-limited sample ($z<0.06$) of SNe~Ia based on the Zwicky Transient Facility Data Release 2 (ZTF DR2). Using ZTF $g$- and $r$-band light curves, we identify candidates showing early-excesses shortly after the explosion time, and we apply conservative coverage and quality requirements to build reliable ``excess'' and ``no-excess'' bump and no-bump catalogs. From an initial sample of 1547 SNe~Ia, our final catalogs contain 42 early-excess and 110 no-excess events. We compare the two populations using SN and host environment parameters from ZTF DR2 and quantify the differences using two-sample statistical tests. We find the strongest differences are in SN light-curve properties: early-excess events have larger SALT2 stretch $x_1$ ($7.91σ$) and larger $r$-band secondary-maximum flux $\mathcal{F}_{r_2}$ ($6.25σ$), while differences in SALT2 color $c$ are weak ($0.57σ$). Early-excess events also favor bluer $(g-z)_{\rm local}$ ($3.41σ$) and lower $\log_{10} (M_*/M_\odot)_{\rm local}$ ($2.73σ$). Our results connect early excesses with SNe~Ia diversity, and motivate further analyses of upcoming larger samples.
format Preprint
id arxiv_https___arxiv_org_abs_2605_14437
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Not All Who Wander Are Lost: Early Excess Demographics in the Volume-limited ZTF DR2 SN Ia Sample
Rojas-Bravo, César
Sun, Ning-Chen
Smith, Mathew
Chen, Chun
Chen, Xiaohan
Niu, Zexi
Wang, Anyu
Wang, Zi-Yang
Zhao, Yi-Han
Liu, Jifeng
High Energy Astrophysical Phenomena
Cosmology and Nongalactic Astrophysics
Astrophysics of Galaxies
Solar and Stellar Astrophysics
Early-time flux excesses in Type Ia supernovae (SNe~Ia) offer a unique insight into their progenitor systems and explosion mechanisms. Although individual early-excess events and larger searches have been reported, demographic studies remain limited by sample size. We present a systematic search for early-time excess emission in a volume-limited sample ($z<0.06$) of SNe~Ia based on the Zwicky Transient Facility Data Release 2 (ZTF DR2). Using ZTF $g$- and $r$-band light curves, we identify candidates showing early-excesses shortly after the explosion time, and we apply conservative coverage and quality requirements to build reliable ``excess'' and ``no-excess'' bump and no-bump catalogs. From an initial sample of 1547 SNe~Ia, our final catalogs contain 42 early-excess and 110 no-excess events. We compare the two populations using SN and host environment parameters from ZTF DR2 and quantify the differences using two-sample statistical tests. We find the strongest differences are in SN light-curve properties: early-excess events have larger SALT2 stretch $x_1$ ($7.91σ$) and larger $r$-band secondary-maximum flux $\mathcal{F}_{r_2}$ ($6.25σ$), while differences in SALT2 color $c$ are weak ($0.57σ$). Early-excess events also favor bluer $(g-z)_{\rm local}$ ($3.41σ$) and lower $\log_{10} (M_*/M_\odot)_{\rm local}$ ($2.73σ$). Our results connect early excesses with SNe~Ia diversity, and motivate further analyses of upcoming larger samples.
title Not All Who Wander Are Lost: Early Excess Demographics in the Volume-limited ZTF DR2 SN Ia Sample
topic High Energy Astrophysical Phenomena
Cosmology and Nongalactic Astrophysics
Astrophysics of Galaxies
Solar and Stellar Astrophysics
url https://arxiv.org/abs/2605.14437