Table B.2.
Photometry data table for the six SNe Ia studied.
| Target | z | μ (mag) | MW Av | First light (MJD) | Peak (MJD) | Flux calibration bands |
|---|---|---|---|---|---|---|
| 2021fxy | 0.0094a | 32.87(0.09)b | 0.25327(0.0028) | 59289.71(0.16) | 59305.12(0.34)b | g r (SWOPE)b |
| 2018cnw | 0.024167d | 35.07* | 0.07161(0.0031) | 58283.04(0.28) | 58302.02(0.05)d | g r (ZTF)d |
| 2012fr | 0.005457e | 31.27(0.05)f | 0.05487(0.0012) | 56225.73(0.46)g | 56242.6(0.3)g | g r (SWOPE)g |
| 2021aefx | 0.005284h | 31.27(0.49)i | 0.02449(0.00062) | 59529.85(0.55)h | 59546.67(0.67)h | g r (SWOPE)j |
| 2009ig | 0.008770k | 32.60(0.4)l | 0.08339(0.0025) | 55063.41(0.08)m | 55080.54(0.04)m | B R (KAIT4)m |
| 1994D | 0.002058n | 31.02(0.19)o | 0.05921(0.00031) | - | 49431.5(0.5)p | B Rp |
Notes. Uncertainties are noted in parentheses for values calculated in this work and when given for values taken from the literature. Milky Way extinction corrections were performed using Rv = 3.1, with E(B-V) values through querying the IRSA dust maps (Schlegel et al. 1998).*Calculated from the redshift measurement with H0 = 70.3 km s−1 Mpc (Hotokezaka et al. 2019).
References.a: Rothberg & Joseph (2006), b: DerKacy et al. (2023b), c: Falco et al. (1999), d: Rigault et al. (2025), e: Bureau et al. (1996), f: Freedman et al. (2001), g: Contreras et al. (2018), h: Ni et al. (2023), i: Sabbi et al. (2018), j: Ashall et al. (2022), k: Wong et al. (2006), l: Tully & Fisher (1988), m: Foley et al. (2012), n: Cappellari et al. (2011), o: Wang et al. (2006), p: Richmond et al. (1995).
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