| Show | Sort | Column | Constraint | Explain (UCD) |
| | | RAICRS | deg | (i) Right Ascension of Gaia source (ICRS at epoch 2015.5), as given by the Gaia DR2 catalogue (GAIA_RA) (pos.eq.ra;meta.main) (POS_EQ_RA_MAIN) |
| | | DEICRS | deg | (i) Declination of Gaia source (ICRS at epoch 2015.5), as given by the Gaia DR2 catalogue (GAIA_DEC) (pos.eq.dec;meta.main) (POS_EQ_DEC_MAIN) |
| | | GAIA-WISE | | Display the Gaia DR2 (Cat. I/345) and AllWISE (Cat. II/328) data (meta.ref.url) (DATA_LINK) |
| | | GAIA | | (i) ID of Gaia source, as given by the Gaia DR2 catalogue (GAIA_ID) (meta.id;meta.main) (ID_MAIN) |
| | | WISE | (char) | (i) ID of WISE object, as given by the AllWISE catalogue (WISE_ID) (meta.id.cross) (ID_CROSSID) |
| | | RAWdeg | deg | Right Ascension of WISE source (J2000), as given by the AllWISE catalogue (WISE_RA) (pos.eq.ra) (POS_EQ_RA_OTHER) |
| | | DEWdeg | deg | Declination of WISE source (J2000), as given by the AllWISE catalogue (WISE_DEC) (pos.eq.dec) (POS_EQ_DEC_OTHER) |
| | | gmag | mag | Gaia G magnitude, as given by the Gaia DR2 catalogue (G_MAG) (phot.mag;em.opt) (PHOT_MAG_OPTICAL) |
| | | W1mag | mag | WISE w1mpro magnitude, as given by the AllWISE catalogue (W1_MAG) (phot.mag;em.IR.3-4um) (PHOT_IR_3.4) |
| | | W2mag | mag | WISE w2mpro magnitude, as given by the AllWISE catalogue (W2_MAG) (phot.mag;em.IR.4-8um) (PHOT_IR_4.2) |
| | | W3mag | mag | WISE w3mpro magnitude, as given by the AllWISE catalogue (W3_MAG) (phot.flux.density;em.IR.8-15um) (PHOT_FLUX_IR_12) |
| | | W4mag | mag | WISE w4mpro magnitude, as given by the AllWISE catalogue (W4_MAG) (phot.flux.density;em.IR.15-30um) (PHOT_FLUX_IR_25) |
| | | MatchP | | Overall probability that the Gaia and WISE sources are detections of the same object, as given by equation 26 of Wilson & Naylor (2018MNRAS.473.5570W) (MATCH_P) (stat.fit.goodness) (STAT_PROBABILITY) |
| | | eta | | Photometric logarithmic likelihood ratio of Gaia-WISE match, as described by equation 37 of Wilson & Naylor (2018MNRAS.473.5570W) (ETA) (stat.likelihood;phot;arith.ratio) (STAT_LIKELIHOOD-RATIO) |
| | | xi | | Astrometric logarithmic likelihood ratio of Gaia-WISE match, as described by equation 38 of Wilson & Naylor (2018MNRAS.473.5570W) (XI) (stat.likelihood) (STAT_LIKELIHOOD-RATIO) |
| | | ContP1 | | Probability of WISE source having contaminant of at least 1% relative flux given its separation from its corresponding Gaia detection, as given by equation 12 of Wilson & Naylor (2018b, this paper) (CONT_P1) (stat.fit.goodness) (STAT_PROBABILITY) |
| | | ContP10 | | Probability of WISE source having contaminant of at least 10% relative flux given its separation from its corresponding Gaia detection (CONT_P10) (stat.fit.goodness) (STAT_PROBABILITY) |
| | | avgCont | | Mean contaminating relative flux within PSFs when constructing h_offsets for WISE sources at the local density, magnitude and intrinsic positional uncertainty of the primary source (AVG_CONT) (stat.fit.goodness) (STAT_PROBABILITY) |
ALL cols | | | |