3D Parameter Maps of Red Clump Stars in the Milky Way -- Absolute Magnitudes and Intrinsic Colors
<p>Catalog, application and supplementary figures for the RC paper.</p> <p>1100mRC_WC2021new.fits.zip -- RC catalog</p> <p>Gaia photometric RC sample with 11 million RCs selected based on {\it Gaia}'s EDR3 parallax, our 3D parameter maps, and extinction--distance profile.</p> <p>ra, dec -- position; dm -- distance modulus; av -- V-band extinction</p> <p>dm1 -- corrected distance modulus; av1 -- corrected extinction. used for low-extinction RCs</p> <p>edm -- uncertainty of distance modulus; flag -- 1: high probability RCs, 0: low probability RCs.</p> <p> </p> <p>RC_calculator_linux.zip -- application RC2021 and installer for linux</p> <p>RC_calculator_mac.zip -- application RC2021 and installer for mac </p> <p>The application to estimate the absolute magnitudes and intrinsic colors for RCs with the APOGEE or LAMOST parameters</p> <p> </p> <p>eps -- the best applicable ranges for using application.</p> <p>pd_APOGEE.eps and pd_LAMOST.eps -- Probability densities of each parameter for absolute magnitude training set (orange) and the whole sample (blue). </p> <p>pd_APOGEE_color.eps and pd_LAMOST_color.eps -- Probability densities of each parameter for intrinsic color training set (orange) and the whole sample (blue). </p>
ShareScore
40/100
Overall dataset sharing score
Score breakdown
These five areas show where the dataset supports — or may limit — practical reuse.
- Stewardship
- 8
- Harmonization
- 4
- Access
- 16
- Reuse readiness
- 8
- Engagement
- 4