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 CSP-I and 234 spectra of 127 SNe Ia obtained during CSP-II. We also present 216 optical spectra of 46 historical SNe Ia, including 53 spectra of 30 SNe Ia observed by the Calán/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 spectroscopic and photometric properties of SNe Ia. Specifically, we define two samples: one consisting of SNe Ia discovered by targeted searches (most of them CSP-I objects) and the other composed of SNe Ia discovered by untargeted searches, which includes most of the CSP-II objects. The analyzed correlations are similar for both samples. We find a larger incidence of SNe Ia belonging to the cool and broad-line Branch subtypes among the events discovered by targeted searches, shallow-silicon SNe Ia are present with similar frequencies in both samples, while core normal SNe Ia are more frequent in untargeted searches.
Optical Spectroscopy of Type Ia Supernovae by the Carnegie Supernova Projects I and II
- Creators
- Morrell, N.
- Phillips, M. M.
- Folatelli, G.
- Stritzinger, M. D.
- Hamuy, M.
- Suntzeff, N. B.
- Hsiao, E. Y.
- Taddia, F.
- Burns, C. R.
- Hoeflich, P.
- Ashall, C.
- Contreras, C.
- Galbany, L.
- Lu, J.
- Piro, A. L.
- Anais, J.
- Baron, E.
- Burrow, A.
- Busta, L.
- Campillay, A.
- Castellón, S.
- Corco, C.
- Diamond, T.
- Freedman, W. L.
- Gonzalez, C.
- Krisciunas, K.
- Kumar, S.
- Persson, S. E.
- Serón, J.
- Shahbandeh, M.
- Torres, S.
- Uddin, S. A.
- Anderson, J. P.
- Baltay, C.
- Gall, C.
- Goobar, A.
- Hadjiyska, E.
- Holmbo, S.
- Kasliwal, M.1
- Lidman, C.
- Marion, G. H.
- Mazzali, P. A.
- Nugent, P.
- Perlmutter, S.
- Pignata, G.
- Rabinowitz, D.
- Roth, M.
- Ryder, S. D.
- Shappee, B. J.
- Vinkó, J.
- Wheeler, J. C.
- de Jaeger, T.
- Lira, P.
- Ruiz, M. T.
- Rich, J. A.
- Prieto, J. L.
- Di Mille, F.
- Osip, D.
- Blanc, G.
- Palunas, P.
Abstract
Copyright and License
© 2024. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
Acknowledgement
The work of the CSP has been supported by the National Science Foundation under grants AST0306969, AST0607438, AST1008343, AST1613426, AST1613455, and AST1613472. CSP-II was also supported in part by funding from the Danish Villum FONDEN (grant Nos. 13261 and 28021) and the Independent Research Fund Denmark (IRFD) by a Sapere Aude II Fellowship awarded to M.D.S. Additional IRFD funding comes from Project 1 (8021-00170B) and Project 2 (10.46540/2032-00022B) grants. This paper includes data gathered with the 6.5 m Magellan Telescopes located at Las Campanas Observatory, the Gemini South, Cerro Pachón, Chile, and Gemini North, Maunakea, Hawaii (Gemini Program Nos. GS-2011B-Q-15-150-002 and GN-2013A-Q-68-82-002). Also based on observations collected at the European Organization for Astronomical Research in the Southern Hemisphere, Chile (ESO Programs 164.H-0376 and 0102.D-0095). C.G. is supported by a research grant (25501) by the Villum FONDEN. M.H. acknowledges support from FONDECYT-Chile through grants 92/0312 and 1060808; the National Science Foundation through grants GF-1002-96 and GF-1002-97; the Association of Universities for Research in Astronomy, Inc., under NSF Cooperative Agreement AST-8947990 and from Fundación Andes under project C-12984; the Hubble Fellowship grant HST-HF-01139.01-A (awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS 5-26555); and the Carnegie Postdoctoral Fellowship. This work has been funded by ANID, Millennium Science Initiative, ICN12_009. L.G. acknowledges financial support from the Spanish Ministerio de Ciencia e Innovación (MCIN), the Agencia Estatal de Investigación (AEI) 10.13039/501100011033, and the European Social Fund (ESF) "Investing in your future" under the 2019 Ramón y Cajal program RYC2019-027683-I and the PID2020-115253GA-I00 HOSTFLOWS project, from Centro Superior de Investigaciones Científicas (CSIC) under the PIE project 20215AT016, and the program Unidad de Excelencia María de Maeztu CEX2020-001058-M. C.A. acknowledges support by NASA grants JWST-GO-02114, JWST-GO-02122, and JWST-GO-04436.024-A; and JPL grant SS03-17-23. The research of J.C.W. and J.V. is supported by NSF AST-1813825. J.V. is also supported by OTKA grant K-142534 of the National Research, Development and Innovation Office, Hungary. The authors want to thank an anonymous referee for their kind report and useful suggestions.
Facilities
Magellan:Baade (IMACS imaging spectrograph) - , Magellan:Clay - Magellan II Landon Clay Telescope (LDSS3, MagE, MIKE), Du Pont (WFCCD, B&C spectrograph, MODSPEC), ESO 3.6 m (EFOSC-2), NTT (EMMI), ESO 1.52 m (B&C spectrograph), VLT:Yepun (MUSE), NOT (ALFOSC), Gemini:South (GMOS), Gemini:Gillett (GMOS), CTIO 1.0 m (B&C spectrograph), CTIO 1.5 m (R-C spectrograph), Blanco (R-C spectrograph), UH 2.2 m, KPNO 2.1 m (Gold camera), MMT (red channel), Shane (Cassegrain spectrograph), Nickel (Cassegrain spectrograph), FLWO 1.5 m (Z- Machine), ESO:Schmidt (QUEST camera), SO:Schmidt, Uppsala Schmidt, SO:1.5m, PO:1.2m, OGLE, ASAS-SN, PS1, Kiso:Schmidt, ISSP, MASTER, Skymapper, CTIO:Schmidt, CTIO:0.9m
Files
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Additional details
- ISSN
- 1538-4357
- National Science Foundation
- AST-0306969
- National Science Foundation
- AST-0607438
- National Science Foundation
- AST-1008343
- National Science Foundation
- AST-1613426
- National Science Foundation
- AST-1613455
- National Science Foundation
- AST-1613472
- Villum Fonden
- 13261
- Villum Fonden
- 28021
- Danmarks Frie Forskningsfond
- 8021-00170B
- Danmarks Frie Forskningsfond
- 10.46540/2032-00022B
- Villum Fonden
- 25501
- Fondo Nacional de Desarrollo Científico y Tecnológico
- 92/0312
- Fondo Nacional de Desarrollo Científico y Tecnológico
- 1060808
- National Science Foundation
- GF-1002-96
- National Science Foundation
- GF-1002-97
- National Science Foundation
- AST-8947990
- National Aeronautics and Space Administration
- NASA Hubble Fellowship HST-HF-01139.01-A
- National Aeronautics and Space Administration
- NAS 5-26555
- Carnegie Institution for Science
- Agencia Nacional de Investigación y Desarrollo
- ICN12_009
- Agencia Estatal de Investigación
- 10.13039/501100011033
- Ministerio de Ciencia, Innovación y Universidades
- Ramón y Cajal program RYC2019-027683-I
- Ministerio de Ciencia, Innovación y Universidades
- PID2020-115253GA-I00
- Consejo Superior de Investigaciones Científicas
- 20215AT016
- Ministerio de Ciencia, Innovación y Universidades
- CEX2020-001058-M
- National Aeronautics and Space Administration
- JWST-GO-02114
- National Aeronautics and Space Administration
- JWST-GO-02122
- National Aeronautics and Space Administration
- JWST-GO-04436.024-A
- Jet Propulsion Laboratory
- SS03-17-23
- National Science Foundation
- AST-1813825
- National Research, Development and Innovation Office
- K-142534
- Caltech groups
- Astronomy Department