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Spectroscopy made easy: A new tool for fitting observations with synthetic spectra
Open accessAbstract
We describe a new software package that may be used to determine stellar and atomic parameters by matching observed spectra with synthetic spectra generated from parameterized atmospheres. A nonlinear least squares algorithm is used to solve for any subset of allowed parameters, which include atomic data ( and van der Waals damping constants), model atmosphere specifications (, ), elemental abundances, and radial, turbulent, and rotational velocities. LTE synthesis software handles discontiguous spectral intervals and complex atomic blends. As a demonstration, we fit 26 FeI lines in the NSO Solar Atlas (Kurucz et al. 1984), determining various solar and atomic parameters.
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KEPLER'S FIRST ROCKY PLANET: KEPLER-10b
Batalha, N. M., Borucki, W. J., Bryson, S. T., Buchhave, L. A., Caldwell, D. A., Christensen-Dalsgaard, J., Ciardi, D., Dunham, E. W., Fressin, F., Gautier, T. N., et al. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/729/1/27 · Cited by 531
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Blanco-Cuaresma, S., Soubiran, C., Heiter, U., & Jofré, P. (2014) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201423945 · Cited by 513
THE MASS OF KOI-94d AND A RELATION FOR PLANET RADIUS, MASS, AND INCIDENT FLUX
Weiss, L. M., Marcy, G. W., Rowe, J. F., Howard, A. W., Isaacson, H., Fortney, J. J., Miller, N., Demory, B.-O., Fischer, D. A., Adams, E. R., et al. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/768/1/14 · Cited by 302
PLANETARY CANDIDATES OBSERVED BY KEPLER . VI. PLANET SAMPLE FROM Q1–Q16 (47 MONTHS)
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Metadata
- Authors
- Valenti, J. A., & Piskunov, N.
- Venue
- Astronomy and Astrophysics Supplement Series
- Publisher
- EDP Sciences
- Published
- 1996-09
- Volume
- 118
- Issue
- 3
- Pages
- 595-603
- ISSN
- 0365-0138 (ISSN-L)
- 1286-4846
- OpenAlex
- W2117914263
- Cited by
- 913
- References
- 0
- FWCI
- 3.63
- Type
- journal article
- Language
- en
- Open access
- green
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- Valenti, J. A., & Piskunov, N. (1996). Spectroscopy made easy: A new tool for fitting observations with synthetic spectra. Astronomy and Astrophysics Supplement Series. https://doi.org/10.1051/aas%3A1996222
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Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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