Table 2
Details of the sources with absolute DR2 radial velocities (RV in km s−1) greater than 500 km s−1 and not on the B19 list.
| DR2 source ID | RV | #(a) | BJ (b) | RF (b) |  |
 |
α (c) | β (c) | Contaminated by |  |
|---|---|---|---|---|---|---|---|---|---|---|
| 4658865791827681536 | −987.5 | 4 | 2MASS(d) | PPMXL | 10.7 | 16.3 | 0.00 | 0.00 | 4658865791827521408 | 11.8 |
| 5966712023814100736 | −967.7 | 2 | PPXML | GSC23 | 11.1 | 14.9 | 0.00 | 0.00 | ? | 11.9 |
| 5305975869928712320 | −830.6 | 2 | 2MASS(e) | 2MASS(e) | 10.0 | 12.8 | 0.05 | 0.66 | 5305975869928710912 | 5.8 |
| 5413575658354375040 | 500.1 | 2 | 2MASS(f) | 2MASS(f) | 12.0 | 12.0 | 0.00 | 0.98 | Glob. clust. NGC 3210 | N/A |
| 5827538590793373696 | 902.6 | 2 | PPXML | PPXML | 11.1 | 15.9 | 0.00 | 0.00 | 5827538590793371776 | 10.9 |
| 4092328917916154368 | 937.5 | 2 | 2MASS(g) | 2MASS(g) | 11.4 | 14.4 | 0.70 | 0.00 | 4092328917911305984 | 8.6 |
Notes. (a) # is the number of DR2 transits. (b)Photometry used to derive BJ and RF. (Smart & Nicastro 2014, Table A.3 gives the photometric transformation numbers to convert 2MASS J and K to BJ and RF, respectively,as 41 and 42, whereas Smart & Nicastro 2013 mistakenly gives them as 42 and 41, respectively.). (c) α and β give the fraction of RP transits that are contaminated and deblended, respectively (see Sect. 3.5 for more details). (d) 2MASS J and K photometry is biased by a nearby star that has contaminated the background estimation: Cfg = c (see Cutri et al. 2003 for details of 2MASS flags). (e) Source is not detected in 2MASS J magnitude band, so this magnitude is an upper limit: Qflg = U, Rflg = 0. Source is detected in 2MASS K magnitude band, but it is biased by a nearby star that has contaminated the background estimation: Cfg = c. (f) 2MASS K magnitude may be contaminated by a diffraction spike from a nearby star: Cfg = d. (g) Source is not detected in 2MASS J and K magnitude bands, so these magnitudes are upper limits: Qflg = U, Rflg = 0.
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