SDSS J124059.53+163949.1
All names: SDSS J124059.53+163949.14, Gaia DR3 3935184448324205184, Gaia EDR3 3935184448324205184, SDSS J124059.53+163949.1, SDSS J124059.52+163949.1, Gaia DR2 3935184448324205184
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | SDSS DR10 | MWDD H | Gaia DR2 | Stilism | Kepler et al. 2015 | Simbad | Vincent et al. 2023 |
|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 12 40 59.53 (0.5) | 12 40 59.53 | 12 40 59.53 (0.6) | 12 40 59.52 (0.5) | ||||||
| Declination | 16 39 48.89 (0.2) | 16 39 49.12 | 16 39 48.90 (0.4) | 16 39 49.22 (0.2) | ||||||
| Spectral type | DA: | DA: | DA | DA | ||||||
| Effective temperature | [K] | 7607.0 | 7410.0 (91) | |||||||
| log(g) | [cgs] | 7.79 | 7.76 (0.1) | |||||||
| Mass | [M☉] | 0.477 | 0.485 (0.06) | |||||||
| log(Luminosity) | [L☉] | |||||||||
| Cooling age | [Gyr] | 0.9234 | ||||||||
| log(H/He) | ||||||||||
| log(C/He) | ||||||||||
| log(Ca/He) | ||||||||||
| log(Ca/H) | ||||||||||
| log(C/H) | ||||||||||
| log(N/H) | ||||||||||
| log(O/H) | ||||||||||
| log(Na/H) | ||||||||||
| log(Mg/H) | ||||||||||
| log(Al/H) | ||||||||||
| log(Si/H) | ||||||||||
| log(P/H) | ||||||||||
| log(S/H) | ||||||||||
| log(Sc/H) | ||||||||||
| log(Ti/H) | ||||||||||
| log(Cr/H) | ||||||||||
| log(Mn/H) | ||||||||||
| log(Fe/H) | ||||||||||
| log(Ni/H) | ||||||||||
| Parallax | [mas] | 4.19 (0.5) | 3.71 (0.8) | 4.19 (0.5) | ||||||
| Distance | [pc] | 238.52 (29) | 269.88 (57) | 238.52 (29) | ||||||
| Composition | H | |||||||||
| Proper motion (right ascension) | [mas/yr] | 6.785976771 (0.7) | 5.39998959 (2) | 6.786 (0.7) | ||||||
| Proper motion (declination) | [mas/yr] | -20.75029223 (0.5) | -20.2228687 (0.7) | -20.75 (0.5) | ||||||
| Variability | ||||||||||
| Magnetic | ||||||||||
| Bd | [MG] | |||||||||
| Infrared excess (disk) | ||||||||||
| Binarity | ||||||||||
| B magnitude | ||||||||||
| V magnitude | ||||||||||
| R magnitude | ||||||||||
| I magnitude | ||||||||||
| J magnitude | ||||||||||
| H magnitude | ||||||||||
| K magnitude | ||||||||||
| u magnitude | 20.65 (0.07) | 20.63 (0.07) | 20.65 (0.07) | |||||||
| g magnitude | 20.16 (0.02) | 20.16 (0.02) | 20.16 (0.02) | |||||||
| r magnitude | 20.05 (0.02) | 20.04 (0.03) | 20.05 (0.02) | |||||||
| i magnitude | 20.06 (0.03) | 20.06 (0.03) | 20.06 (0.03) | |||||||
| z magnitude | 19.95 (0.09) | 19.96 (0.09) | 19.95 (0.09) | |||||||
| G magnitude | 20.01 (0.05) | 20.08 | 20.01 (0.005) | |||||||
| BP magnitude | 20.13 (0.05) | 20.03 | ||||||||
| RP magnitude | 19.89 (0.06) | 19.70 | ||||||||
| Pan g magnitude | 20.13 (0.02) | |||||||||
| Pan r magnitude | 20.03 (0.02) | |||||||||
| Pan i magnitude | 20.08 (0.02) | |||||||||
| Pan z magnitude | 20.08 (0.03) | |||||||||
| Pan y magnitude | 19.98 (0.2) | |||||||||
| E(B-V) | 0.026 | |||||||||
* Constant surface field
Special notes:
Spectra
Controls
Normalize at:
Normalize by mean flux
Range:
x:
to
y:
to
Spectra available:
Spectra without link are available upon request
Absorption lines
Photometric filters
BVRI
ugriz
Photometric fit
