Table 4
UV excess, u-band excess luminosity, Ṁacc and Ṁacc variability estimates for NGC 2264 accreting members.
| Mon-ID | (u − g) exc. | (u − r) exc.1 | log  /L⊙1 |
|
1
|
log Ṁmax/Ṁmed 2 | log Ṁmed/Ṁmin 3 |
|
|
|||||||
| Mon-000007 | –0.16 | –0.65 | –1.50 | –7.17 | –7.22 | 0.32 | |
| Mon-000011 | –0.97 | –1.95 | –0.88 | –7.53 | –6.73 | 0.24 | 0.19 |
| Mon-000017 | 0.03 | –0.27 | –2.14 | –8.24* | 0.02 | ||
| Mon-000028 | –1.79 | –1.40 | –3.38 | –8.90 | –9.13 | 0.40 | 0.59 |
| Mon-000040 | –0.46 | –0.34 | –3.89 | –9.24 | –9.37 | 0.20 | 0.55 |
| Mon-000042 | –0.17 | –0.01 | –5.08 | –9.34 | –9.48* | ||
| Mon-000053 | –0.35 | –0.11 | –4.31 | –9.06 | –9.46 | 0.33 | |
| Mon-000056 | 0.04 | 0.01 | –8.24* | ||||
| Mon-000059 | –1.91 | –1.11 | –3.32 | –8.36 | –8.91 | 0.26 | 0.57 |
| Mon-000063 | –0.53 | –1.03 | –2.56 | –8.62 | –8.21 | 0.15 | |
Notes. A full version of the Table is available at the CDS. A portion is shown here for guidance regarding its form and content.
Variability range detected around the median Ṁacc level during the 2 week-long ur monitoring. If no accretion activity is detected above the detection limit for the object at the minimum/median luminosity level, but some significant accretion is detected at the brightest state, only the upper variability bar is reported (i.e., log Ṁmax/Ṁmed(upper)); if the object is a non-detection in accretion, no variability measurement is reported.
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