Table B.1
Combined VCNS Spitzer photometric infrared excess source catalog.
| VCNS – J | J | H | K s | [3.6] | [4.5] | [5.8] | [8.0] | S/N | S/N | S/N | S/N | S/N | S/N | S/N |
| [ J2000 ] | [mag] | [mag] | [mag] | [mag] | [mag] | [mag] | [mag] | (FJ) | (FH) | (FKs) | (F[3.6]) | (F[4.5]) | (F[5.8]) | (F[8.0]) |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) | (13) | (14) | (15) |
|
|
||||||||||||||
| 103346.62−595137.5 | 17.28 | 15.48 | 15.02 | −9.99 | 13.68 | −9.99 | −9.99 | 56.4 | 104.2 | 79.7 | −9.9 | 19.8 | −9.9 | −9.9 |
| 103347.48−595319.2 | 15.83 | 14.18 | 13.09 | 11.37 | 10.58 | 9.64 | 8.61 | 145.7 | 222.1 | 241.3 | 278.1 | 341.1 | 143.5 | 157.4 |
| 103347.96−594953.7 | 18.10 | 16.39 | 15.27 | 13.48 | 12.63 | −9.99 | 11.22 | 29.9 | 56.0 | 67.9 | 40.9 | 49.2 | −9.9 | 18.5 |
| 103349.07−594349.4 | 18.21 | 16.02 | 14.85 | 13.58 | 12.91 | −9.99 | −9.99 | 28.1 | 72.5 | 89.3 | 41.4 | 40.2 | −9.9 | −9.9 |
| 103349.36−594345.4 | 18.19 | 15.95 | 14.53 | 12.49 | 11.69 | 11.53 | −9.99 | 28.6 | 76.1 | 109.9 | 130.2 | 142.0 | 28.0 | −9.9 |
| 103349.77−594242.2 | 15.13 | 14.09 | 13.54 | 12.92 | 12.67 | 11.88 | −9.99 | 212.0 | 233.5 | 194.6 | 69.1 | 54.3 | 14.9 | −9.9 |
| 103349.94−595347.3 | 16.29 | 15.07 | 14.34 | 13.55 | 13.29 | −9.99 | −9.99 | 108.4 | 134.9 | 119.2 | 37.6 | 26.4 | −9.9 | −9.9 |
| 103350.28−595147.2 | 18.84 | 16.87 | 15.83 | 14.11 | 13.30 | 12.42 | −9.99 | 16.3 | 39.0 | 45.1 | 21.4 | 26.4 | 10.1 | −9.9 |
| ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... |
| 105202.57−600421.5 | 16.54 | 15.36 | 14.82 | 14.26 | 14.12 | −9.99 | −9.99 | 85.0 | 111.7 | 91.9 | 20.3 | 12.9 | −9.9 | −9.9 |
Notes. Table B.1 is available at the CDS. A portion is shown here for guidance regarding its form and content. The meaning of the columns is as follows: Cols. (1): source name, based on the J2000 celestial coordinates. Columns (2) to (4): near-infrared VCNS photometry in the J-, H-, and Ks-bands. Columns (5) to (8): mid-infrared Spitzer photometry in the [3.6], [4.5], [5.8], and [8.0] IRAC bands. Objects without photometry in a band are marked by the number − 9.99. Columns (9) to (15): signal-to-noise ratio of the individual photometric flux measurements in Cols. (2) to (8).
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