Testing for redshift evolution of Type Ia supernovae using the strongly lensed PS1-10afx at z = 1.4

Free Access

Table 3

Properties of the nearby SNe Ia used for the median spectrum at phase + 1.2d.

SN name	SN 2009ig	SN 2013dy	SN 1981B	SN 2001ba	SN 2011fe	SN 2011by	SN 2005df	SN 1992A
z_helio	0.007589	0.00383	0.005101^c	0.029557^c	0.002000	0.002843	0.004350	0.001447^c
A _V	0.01	0.15	0.35^d	0.016^d	0.08	0.03	0.001	0.016^d
MW A_V	0.088	0.92	0.0682^d	0.176^d	0.024	0.038	0.090	0.046^d
Δm₁₅(B)	0.89(0.02)	0.92(0.03)	1.01(0.10) ^d	1.01(0.11) ^d	1.10(0.04)	1.14(0.03)	1.21(0.04)	1.47(0.11) ^d
instr.	Swift ^a	STIS/HST^b	IUE^d	STIS/HST^d	Swift ^a	Swift ^a	Swift ^a	IUE^d
sp. phase	+1.6^a	+ 1.2 d^b	+1.8 d^d	+3.8 d^d	+ 0.1+ 3.0 d^a	+ 1.1 d^a	+ 1.6 d^a	− 0.2+ 2.4 d^d

Notes. Uncertainties of the light-curve shape parameter Δm₁₅(B) are given in parentheses.

Reference. ;

^(a)

Smitka et al. (2016);

^(b)

Pan et al. (2015)

^(c)

From NED;

^(d)

Foley et al. (2008b).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.