The DOI matches its Crossref record; 64 of the 64 references it cites were found in a registry or an index.
NEARBY SUPERNOVA FACTORY OBSERVATIONS OF SN 2007if: FIRST TOTAL MASS MEASUREMENT OF A SUPER-CHANDRASEKHAR-MASS PROGENITOR
Open accessAbstract
We present photometric and spectroscopic observations of SN 2007if, an overluminous ( M V = −20.4), red ( B − V = 0.16 at B -band maximum), slow-rising ( t rise = 24 days) type Ia supernova (SN Ia) in a very faint ( M g = −14.10) host galaxy. A spectrum at 5 days past B -band maximum light is a direct match to the super-Chandrasekhar-mass candidate SN Ia 2003fg, showing Si ii and C ii at ∼9000 km s −1 . A high signal-to-noise co-addition of the SN spectral time series reveals no Na i D absorption, suggesting negligible reddening in the host galaxy, and the late-time color evolution has the same slope as the Lira relation for normal SNe Ia. The ejecta appear to be well mixed, with no strong maximum in I band and a diversity of iron-peak lines appearing in near-maximum-light spectra. SN 2007if also displays a plateau in the Si ii velocity extending as late as +10 days, which we interpret as evidence for an overdense shell in the SN ejecta. We calculate the bolometric light curve of the SN and use it and the Si ii velocity evolution to constrain the mass of the shell and the underlying SN ejecta, and demonstrate that SN 2007if is strongly inconsistent with a Chandrasekhar-mass scenario. Within the context of a "tamped detonation" model appropriate for double-degenerate mergers, and assuming no host extinction, we estimate the total mass of the system to be 2.4 ± 0.2 M ☉ , with 1.6 ± 0.1 M ☉ of 56 Ni and with 0.3–0.5 M ☉ in the form of an envelope of unburned carbon/oxygen. Our modeling demonstrates that the kinematics of shell entrainment provide a more efficient mechanism than incomplete nuclear burning for producing the low velocities typical of super-Chandrasekhar-mass SNe Ia.
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Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
Riess, A. G., Filippenko, A. V., Challis, P., Clocchiatti, A., Diercks, A., Garnavich, P. M., Gilliland, R. L., Hogan, C. J., Jha, S., Kirshner, R. P., et al. (1998) · The Astronomical Journal · doi:10.1086/300499 · Cited by 19,704
Measurements of Ω and Λ from 42 High‐Redshift Supernovae
Perlmutter, S., Aldering, G., Goldhaber, G., Knop, R. A., Nugent, P., Castro, P. G., Deustua, S., Fabbro, S., Goobar, A., Groom, D. E., et al. (1999) · The Astrophysical Journal · doi:10.1086/307221 · Cited by 18,062
Self-citationSchlegel, D. J., Finkbeiner, D. P., & Davis, M. (1998) · The Astrophysical Journal · doi:10.1086/305772 · Cited by 15,126
SExtractor: Software for source extraction
Bertin, E., & Arnouts, S. (1996) · Astronomy and Astrophysics Supplement Series · doi:10.1051/aas:1996164 · Cited by 10,866
Astronomical Data Analysis Software and Systems
Argyle, R. W., Bunclark, P., & Lewis, J. R. (2008) · Cited by 4,399
UBVRI photometric standard stars in the magnitude range 11.5-16.0 around the celestial equator
Landolt, A. U. (1992) · The Astronomical Journal · doi:10.1086/116242 · Cited by 4,168
Monet, D. G., Levine, S. E., Canzian, B., Ables, H. D., Bird, A. R., Dahn, C. C., Guetter, H. H., Harris, H. C., Henden, A. A., Leggett, S. K., et al. (2003) · The Astronomical Journal · doi:10.1086/345888 · Cited by 2,117
The Keck Low-Resolution Imaging Spectrometer
Oke, J. B., Cohen, J. G., Carr, M., Cromer, J., Dingizian, A., Harris, F. H., Labrecque, S., Lucinio, R., Schaal, W., Epps, H., et al. (1995) · Publications of the Astronomical Society of the Pacific · doi:10.1086/133562 · Cited by 2,099
Cosmic‐Ray Rejection by Laplacian Edge Detection
van Dokkum, P. G. (2001) · Publications of the Astronomical Society of the Pacific · doi:10.1086/323894 · Cited by 1,626
Binaries and Supernovae of Type I
Whelan, J., & Icko, J. I. (1973) · The Astrophysical Journal · doi:10.1086/152565 · Cited by 1,268
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The Evolution of Compact Binary Star Systems
Postnov, K. A., & Yungelson, L. R. (2014) · Living Reviews in Relativity · doi:10.12942/lrr-2014-3 · Cited by 486
THE CARNEGIE SUPERNOVA PROJECT: SECOND PHOTOMETRY DATA RELEASE OF LOW-REDSHIFT TYPE Ia SUPERNOVAE
Stritzinger, M. D., Phillips, M. M., Boldt, L. N., Burns, C., Campillay, A., Contreras, C., Gonzalez, S., Folatelli, G., Morrell, N., Krzeminski, W., et al. (2011) · The Astronomical Journal · doi:10.1088/0004-6256/142/5/156 · Cited by 286
Stellar structure models in modified theories of gravity: Lessons and challenges
Olmo, G. J., Rubiera-Garcia, D., & Wojnar, A. (2020) · Physics Reports · doi:10.1016/j.physrep.2020.07.001 · Cited by 253
Metadata
- Authors
- Scalzo, R. A., Aldering, G., Antilogus, P., Aragon, C., Bailey, S., Baltay, C., Bongard, S., Buton, C., Childress, M., Chotard, N., Copin, Y., Fakhouri, H. K., Gal-Yam, A., Gangler, E., Hoyer, S., Kasliwal, M., Loken, S., Nugent, P., Pain, R., Pécontal, E., Pereira, R., Perlmutter, S., Rabinowitz, D., Rau, A., Rigaudier, G., Runge, K., Smadja, G., Tao, C., Thomas, R. C., Weaver, B., & Wu, C.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2010-03-30
- Volume
- 713
- Issue
- 2
- Pages
- 1073-1094
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2172169673
- Cited by
- 371
- References
- 64
- FWCI
- 15.86
- Type
- journal article
- Language
- en
- Open access
- bronze
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- CoChat. (2026). Citation check: NEARBY SUPERNOVA FACTORY OBSERVATIONS OF SN 2007if: FIRST TOTAL MASS MEASUREMENT OF A SUPER-CHANDRASEKHAR-MASS PROGENITOR. https://app.cochat.ai/papers/10.1088/0004-637x/713/2/1073
- The paper
- Scalzo, R. A., Aldering, G., Antilogus, P., Aragon, C., Bailey, S., Baltay, C., Bongard, S., Buton, C., Childress, M., Chotard, N., Copin, Y., Fakhouri, H. K., Gal-Yam, A., Gangler, E., Hoyer, S., Kasliwal, M., Loken, S., Nugent, P., Pain, R., . . . Wu, C. (2010). NEARBY SUPERNOVA FACTORY OBSERVATIONS OF SN 2007if: FIRST TOTAL MASS MEASUREMENT OF A SUPER-CHANDRASEKHAR-MASS PROGENITOR. The Astrophysical Journal. https://doi.org/10.1088/0004-637x/713/2/1073
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