Table 2
Magnitude table.
Region | SAGE_Designationa | GC09_Designation | Uc | B | V | I | Jd | H | Ks | [3.6]e | [4.5] | [5.8] | [8.0] | 24 μm | αf | βf | Setg | |||
(mag) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | |||||||||
|
||||||||||||||||||||
N11 | J045850.69-660745.4 | NONE | 19.54 | 19.701 | 19.448 | 18.915 | 18.34 | 17.69 | 99.999 | 15.442 | 15.403 | 12.538 | 10.782 | 8.3 | 1 | 4 | 1 | |||
N44 | J052212.56-675832.1 | Y052212.57-675832.3 | 99.999 | 99.999 | 99.999 | 99.999 | 17.13 | 15.69 | 13.48 | 9.597 | 8.004 | 6.618 | 5.264 | 99.999 | 3 | 0 | 3 | |||
N51 | J052749.97-672540.1 | NONE | 17.527 | 18.314 | 18.198 | 18.051 | 17.86 | 17.44 | 16.89 | 14.675 | 14.36 | 12.384 | 10.692 | 6.395 | 3 | 2 | 1 | |||
N113 | POOR MATCH | Y051315.73-692135.9 | 99.999 | 99.999 | 99.999 | 99.999 | 16.18 | 15.4 | 14.66 | 11.51 | 11.27 | 8.69 | 6.97 | 2.09 | 5 | 0 | 1 | |||
N144 | J052613.39-684715.0 | Y052613.41-684714.9 | 20.294 | 19.289 | 17.913 | 17.189 | 15.77 | 15.18 | 14.33 | 12.379 | 11.589 | 10.202 | 8.167 | 3.659 | 5 | 0 | 1 | |||
N160 | J053922.76-693011.6 | Y053922.74-693011.7 | 99.999 | 19.407 | 18.718 | 18.628 | 18.13 | 17.26 | 16.23 | 14.029 | 13.612 | 11.851 1 | 99.999 | 99.999 | 1 | 1 | 4 | |||
N160 | J054050.87-695001.9 | NONE | 99.999 | 99.999 | 99.999 | 99.999 | 18.21 | 17.05 | 15.86 | 13.888 | 13.229 | 12.35 | 11.298 | 7.717 | 0 | 5 | 6 | |||
N206 | J052959.68-710436.8 | NONE | 17.577 | 18.082 | 17.974 | 17.789 | 99.999 | 18.23 | 17.21 | 99.999 | 14.391 | 12.384 | 10.923 | 7.3 | 1 | 3 | 2 |
Notes. Magnitude information for all well-fit YSO candidates as well as that for 358 candidates from W08, GC09, Chen et al. (2009), Romita et al. (2010), and Chen et al. (2010), which we do not consider well-fit. Null magnitudes are listed as “99.999”. The full online table also has columns for RA and Dec in J2000 degrees, W08_Designation, Other_Designation as described in Table 3, whether the source is well-fit, error bars on all magnitudes. For 109 sources with little or no SAGE photometry, we include the original photometry from GC09, Chen et al. (2009), or Chen et al. (2010); for these we list SAGE Designation as “None” or “Poor Match”. Sources classified as Transition or Multiple objects by Romita et al. (2010) are not included.
Optical photometry from MCPS (Zaritsky et al. 1997).
Near-IR photometry from IRSF (Kato et al. 2007).
Infrared photometry from SAGE (Meixner et al. 2006).
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