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Table 5
Solar colors and predictions from models atmospheres. Our synthetic colors (this work) were computed using the Bessell (2005) filters, with zero points based on both the STIS observed and ATLAS9 synthetic spectrum of Vega.
(b–y) | m 1 | c 1 | β | Reference | ||
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Solar colors (this work) | ||||||
0.4105 (±0.0015) | 0.2122 (±0.0018) | 0.3319 (±0.0054) | 2.5915 (±0.0024) | |||
|
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Solar spectra | ||||||
0.406,0.390(±0.004), (b–y) from β | 2.5955(±0.0024) | Olsen (1976), using asteroids | ||||
0.425 | 0.172 | 0.323 | 2.625 | This work, C96 [STIS] | ||
0.421 | 0.178 | 0.350 | 2.595 | This work, C96 [ATLAS9] | ||
0.424 | 0.188 | 0.306 | 2.632 | This work, N99 [STIS] | ||
0.420 | 0.194 | 0.333 | 2.602 | This work, N99 [ATLAS9] | ||
0.400 | 0.195 | 0.305 | 2.631 | This work, N99+N03 [STIS] | ||
0.396 | 0.201 | 0.332 | 2.601 | This work, N99+N03 [ATLAS9] | ||
0.402 | 0.225 | 0.287 | 2.625 | This work, Thuillier (2004) [STIS] | ||
0.398 | 0.231 | 0.314 | 2.595 | This work, Thuillier (2004) [ATLAS9] | ||
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Kurucz models | ||||||
0.371 | 0.214 | 0.243 | Relyea & Kurucz (1978) | |||
0.414 | Kurucz (1991) | |||||
0.355, 0.388 | 0.235 | 0.359 | 2.618, 2.660 | Lester et al. (1986) | ||
2.581 | Smalley & Dworetsky (1995) | |||||
0.393(CM), 0.400(noOV), 0.414(OV) | 0.278 (CM) | 0.339 (CM) | Smalley & Kupka (1997) | |||
0.397(noOVER), 0.410 (OVER) | Castelli et al. (1997) | |||||
2.590 | Castelli & Kurucz (2006) | |||||
0.410 | 0.208 | 0.276 | 2.617 | This work, ATLAS9 [STIS] | ||
0.406 | 0.214 | 0.303 | 2.587 | This work, ATLAS9 [ATLAS9] | ||
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MARCS models | ||||||
0.381 | 0.159 | 0.262 | Vandenberg & Bell (1985) | |||
0.383 | 0.258 | 0.325 | 2.589 | O09 | ||
0.383 | 0.220 | 0.367 | 2.621 | This work, MARCS 2008 [STIS] | ||
0.379 | 0.226 | 0.394 | 2.591 | This work, MARCS 2008 [ATLAS9] | ||
|
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From empirical calibrations or average of solar analogs | ||||||
0.425(±0.015) | Gehren (1981) | |||||
0.407(±0.010) | 2.591(±0.005) | Saxner & Hammarback (1985) | ||||
0.414(±0.003) | Gray (1992) | |||||
0.406(±0.004) | Edvardsson et al. (1993) | |||||
0.404(±0.005) | Cayrel de Strobel (1996) | |||||
0.3999 | 0.2090 | 0.323 | Clem et al. (2004) | |||
0.394 | RM05b | |||||
0.403(±0.013) | 0.200(±0.026) | 0.370(±0.068) | Holmberg et al. (2006) | |||
0.4089(±0.0100) | Casagrande et al. (2010) |
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