The DOI matches its Crossref record; 88 of the 88 references it cites were found in a registry or an index.
Determining the Type, Redshift, and Age of a Supernova Spectrum
Open accessAbstract
We present an algorithm to identify the type of an SN spectrum and to determine its redshift and age. This algorithm, based on the correlation techniques of Tonry & Davis, is implemented in the Supernova Identification (SNID) code. It is used by members of ongoing high-redshift SN searches to distinguish between Type Ia and Ib/c SNe and to identify "peculiar" SNe Ia. We develop a diagnostic to quantify the quality of a correlation between the input and template spectra, which enables a formal evaluation of the associated redshift error. Furthermore, by comparing the correlation redshifts obtained using SNID with those determined from narrow lines in the SN host galaxy spectrum, we show that accurate redshifts (with a typical error σ z ≲ 0.01) can be determined for SNe Ia without a spectrum of the host galaxy. Last, the age of an input spectrum is determined with a typical accuracy σ t ≲ 3 days, shown here by using high-redshift SNe Ia with well-sampled light curves. The success of the correlation technique confirms the similarity of some SNe Ia at low and high redshifts. The SNID code, which will be made available to the community, can also be used for comparative studies of SN spectra, as well as comparisons between data and models.
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Cites
Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
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Self-citationMeasurements of Ω and Λ from 42 High‐Redshift Supernovae
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Riess, A. G., Strolger, L., Tonry, J., Casertano, S., Ferguson, H. C., Mobasher, B., Challis, P., Filippenko, A. V., Jha, S., Li, W., et al. (2004) · The Astrophysical Journal · doi:10.1086/383612 · Cited by 4,315 · cited 1×
“1 (Tonry et al. 2003; Knop et al. 2003; Barris et al. 2004), but also at higher redshifts where the universal expansion is in a decelerating phase (Riess et al. 2004).”
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The 2dF Galaxy Redshift Survey: spectra and redshifts
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The absolute magnitudes of Type IA supernovae
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Cosmological Results from High‐z Supernovae
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Self-citationA survey of galaxy redshifts. I - Data reduction techniques
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Cited by
The X-ray counterpart to the gravitational-wave event GW170817
Troja, E., Piro, L., van Eerten, H., Wollaeger, R. T., Im, M., Fox, O. D., Butler, N. R., Cenko, S. B., Sakamoto, T., Fryer, C. L., et al. (2017) · Nature · doi:10.1038/nature24290 · Cited by 874
WISeREP—An Interactive Supernova Data Repository
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Self-citationTHE 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
Villar, V. A., Hosseinzadeh, G., Berger, E., Ntampaka, M., Jones, D. O., Challis, P., Chornock, R., Drout, M. R., Foley, R. J., Kirshner, R. P., et al. (2020) · The Astrophysical Journal · doi:10.3847/1538-4357/abc6fd · Cited by 92
Pierel, J. D. R., Newman, A. B., Dhawan, S., Gu, M., Joshi, B. A., Li, T., Schuldt, S., Strolger, L. G., Suyu, S. H., Caminha, G. B., et al. (2024) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/ad4648 · Cited by 56
Metadata
- Authors
- Blondin, S., & Tonry, J. L.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2007-09-10
- Volume
- 666
- Issue
- 2
- Pages
- 1024-1047
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2070951133
- Cited by
- 507
- References
- 88
- FWCI
- 9.06
- Type
- journal article
- Language
- en
- Open access
- bronze
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