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29 April 2022

27 April 2022

  • 02:06 02:06, 27 April 2022 diff hist +15 Kepler-6213.75 is only the star's Kepler Magnitude and that is from a much wider wavelength range compared to the Johnson V magnitude. Actually, Borucki et al 2013 assumes the G band magnitude value as being roughly the same as the V band for the star, and gives that as 14.4. Quoting from Borucki et al 2013, where they're showing no stellar companion exists, "These show a root-mean-square (rms) uncertainty of about 3 m/s, consistent with the RV errors for a g-band magnitude (similar to V) of 14.4 mag."

24 April 2022

22 April 2022

20 April 2022

For 217.44.211.178 talk block log logs filter log
Search for contributionsshowhide
⧼contribs-top⧽
⧼contribs-date⧽

29 April 2022

27 April 2022

  • 02:06 02:06, 27 April 2022 diff hist +15 Kepler-6213.75 is only the star's Kepler Magnitude and that is from a much wider wavelength range compared to the Johnson V magnitude. Actually, Borucki et al 2013 assumes the G band magnitude value as being roughly the same as the V band for the star, and gives that as 14.4. Quoting from Borucki et al 2013, where they're showing no stellar companion exists, "These show a root-mean-square (rms) uncertainty of about 3 m/s, consistent with the RV errors for a g-band magnitude (similar to V) of 14.4 mag."

24 April 2022

22 April 2022

20 April 2022


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