Optical Spectroscopy of Type Ia Supernovae by the Carnegie Supernova Projects I and II
N. Morrell (1), M. M. Phillips (1), G. Folatelli (2, 3), M. D., Stritzinger (4), M. Hamuy (5), N. B. Suntzeff (6), E. Y. Hsiao (7), F. Taddia, (4), C. R. Burns (8), P. Hoeflich (7), C. Ashall (9), C. Contreras (1), L., Galbany (10, 11), J. Lu (7), A. L. Piro (8), J. Anais (1)

TL;DR
This paper presents a comprehensive collection and analysis of optical spectra of Type Ia Supernovae from the Carnegie Supernova Project and other sources, examining spectroscopic and photometric correlations.
Contribution
It provides the final release of a large spectroscopic dataset of SNe Ia, combining new and historical data, and analyzes correlations between spectroscopic features and photometric properties.
Findings
Identified correlations between spectroscopic parameters and light-curve properties.
Found differences in subtype distributions between targeted and untargeted discovery methods.
Compiled the largest dataset of SNe Ia spectra at maximum light to date.
Abstract
We present the second and final release of optical spectroscopy of Type Ia Supernovae (SNe Ia) obtained during the first and second phases of the Carnegie Supernova Project (CSP-I and CSP-II). The newly released data consist of 148 spectra of 30 SNe Ia observed in the course of the CSP-I, and 234 spectra of 127 SNe Ia obtained during the CSP-II. We also present 216 optical spectra of 46 historical SNe Ia, including 53 spectra of 30 SNe Ia observed by the Cal\'an/Tololo Supernova Survey. We combine these observations with previously published CSP data and publicly-available spectra to compile a large sample of measurements of spectroscopic parameters at maximum light, consisting of pseudo-equivalent widths and expansion velocities of selected features, for 232 CSP and historical SNe Ia (including more than 1000 spectra). Finally, we review some of the strongest correlations between…
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