The DOI matches its Crossref record; 4 of the 4 references it cites were found in a registry or an index.
The Dartmouth Stellar Evolution Database
Open accessAbstract
The ever-expanding depth and quality of photometric and spectroscopic observations of stellar populations increase the need for theoretical models in regions of age-composition parameter space that are largely unexplored at present. Stellar evolution models that employ the most advanced physics and cover a wide range of compositions are needed to extract the most information from current observations of both resolved and unresolved stellar populations. The Dartmouth Stellar Evolution Database is a collection of stellar evolution tracks and isochrones that spans a range of [Fe/H] from –2.5 to +0.5, [α/Fe] from –0.2 to +0.8 (for [Fe/H] ⩽ 0) or +0.2 (for [Fe/H] > 0), and initial He mass fractions from Y = 0.245 to 0.40. Stellar evolution tracks were computed for masses between 0.1 and 4 M ☉ , allowing isochrones to be generated for ages as young as 250 Myr. For the range in masses where the core He flash occurs, separate He-burning tracks were computed starting from the zero age horizontal branch. The tracks and isochrones have been transformed to the observational plane in a variety of photometric systems including standard UBV ( RI ) C , Stromgren uvby , SDSS ugriz , 2MASS JHK s , and HST ACS/WFC and WFPC2. The Dartmouth Stellar Evolution Database is accessible through a Web site at http://stellar.dartmouth.edu/~models/ where all tracks, isochrones, and additional files can be downloaded.
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Schlegel, D. J., Finkbeiner, D. P., & Davis, M. (1998) · The Astrophysical Journal · doi:10.1086/305772 · Cited by 15,126
Spergel, D. N., Verde, L., Peiris, H. V., Komatsu, E., Nolta, M. R., Bennett, C. L., Halpern, M., Hinshaw, G., Jarosik, N., Kogut, A., et al. (2003) · The Astrophysical Journal Supplement Series · doi:10.1086/377226 · Cited by 10,976
A Catalog of Parameters for Globular Clusters in the Milky Way
Harris, W. E. (1996) · The Astronomical Journal · doi:10.1086/118116 · Cited by 4,500 · cited 1×
“Plotted on top of the M 13 data in Figure 11 are isochrones with [Fe/H]=-1.5, [α/Fe]=+0.2 at 11 and 13 Gyr assuming a distance modulus of 14.4 in agreement with Harris (1996).”
MethodInfluentialFerguson, J. W., Alexander, D. R., Allard, F., Barman, T., Bodnarik, J. G., Hauschildt, P. H., Heffner‐Wong, A., & Tamanai, A. (2005) · The Astrophysical Journal · doi:10.1086/428642 · Cited by 1,327
Self-citation
Cited by
MESA ISOCHRONES AND STELLAR TRACKS (MIST). I. SOLAR-SCALED MODELS
Choi, J., Dotter, A., Conroy, C., Cantiello, M., Paxton, B., & Johnson, B. D. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/823/2/102 · Cited by 2,922
Self-citationTHE OCCURRENCE RATE OF SMALL PLANETS AROUND SMALL STARS
Dressing, C. D., & Charbonneau, D. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/767/1/95 · Cited by 749
Extreme Water Loss and Abiotic O 2 Buildup on Planets Throughout the Habitable Zones of M Dwarfs
Luger, R., & Barnes, R. (2015) · Astrobiology · doi:10.1089/ast.2014.1231 · Cited by 585
Pecaut, M. J., Mamajek, E. E., & Bubar, E. J. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/746/2/154 · Cited by 564
“Using the Dotter et al. (2008) models, we then estimate the intrinsic dispersion in ages using the dispersions from our real and simulated populations.”
BackgroundMethodResultInfluentialWeisz, D. R., Dolphin, A. E., Skillman, E. D., Holtzman, J., Gilbert, K. M., Dalcanton, J. J., & Williams, B. F. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/789/2/147 · Cited by 499
Metadata
- Authors
- Dotter, A., Chaboyer, B., Jevremović, D., Kostov, V., Baron, E., & Ferguson, J. W.
- Venue
- The Astrophysical Journal Supplement Series
- Publisher
- American Astronomical Society
- Published
- 2008-09
- Volume
- 178
- Issue
- 1
- Pages
- 89-101
- ISSN
- 0067-0049 (ISSN-L)
- 1538-4365
- OpenAlex
- W2041942393
- Cited by
- 1,717
- References
- 4
- FWCI
- 25.35
- Type
- journal article
- Language
- en
- Open access
- bronze
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