Measurement of the stellar irradiance f - inaoe

More documents

Recommendations

Info

Comparison of the STIS model (black) with the Kurucz (2003) model (red) that has effective temperature 9550 K and log g = 3.95 from H to H . The observations and theory agree to 1%.
Comparison as in Fig. 6 for the Balmer continuum region. Systematic differences of up to 3% are prevalent. The top panel has an expanded vertical scale in comparison with the bottom panel.
Page 1: Measurement of the stellar irradian
Page 5 and 6: Some basic notations : (R = radius
Page 7 and 8: Energy received at Earth : (stellar
Page 9 and 10: monochromatic magnitude of Vega (Ok
Page 11 and 12: Cohen et al.1992, AJ, 104, 1650
Page 13: Ratio of the final STIS fluxes for
Page 17 and 18: Catalogues of SED Jacoby et al, 198
Page 19 and 20: Some results uvby photometry : Comp
Page 21 and 22: Zero-point of synthetic photometric
Page 23: What is measured ? Heterochromatic
Page 28 and 29: Heterochromatic extinction : effect
Page 30 and 31: A(λ=V) R = -------------------- E(
Page 32 and 33: ( from: B. Chen at al A&A 336, 137,

Measurement of the stellar irradiance f - inaoe

You also want an ePaper? Increase the reach of your titles

Delete template?

Save as template?