Contains the cross match pairs between GAIA EDR3 (gaua_source) and WISE (allwise_sc) in a test region |
Required constraints:
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Name | Type | Length | Unit | Description | Default Value | Unified Content Descriptor |
---|---|---|---|---|---|---|
gaia_designation | varchar | 32 | dimensionless | Unique source designation | meta.id;meta.main | |
gaia_ra | float | 8 | degrees | Celestial Right Ascension | pos.eq.ra;meta.main | |
gaia_dec | float | 8 | degrees | Celestial Declination | pos.eq.dec;meta.main | |
gaia_bp | float | 8 | mag | BP mean magnitude | phot.mag;em.op | |
gaia_g | float | 8 | mag | G-band mean magnitude | phot.mag;em.op | |
gaia_rp | float | 8 | mag | RP mean magnitude | phot.mag;em.op | |
wise_designation | varchar | 32 | dimensionless | Sexagesimal, equatorial position-based source name in the form: hhmmss.ss+ddmmss.s. | meta.id;meta.main | |
wise_ra | float | 8 | degrees | Celestial Right Ascension | pos.eq.ra;meta.main | |
wise_dec | float | 8 | degrees | Celestial Declination | pos.eq.dec;meta.main | |
wise_w1mpro | float | 8 | mag | W1 magnitude measured with profile-fitting photometry, or the magnitude of the 95% confidence brightness upper limit if the W1 flux measurement has SNR<2. | ||
wise_w2mpro | float | 8 | mag | W2 magnitude measured with profile-fitting photometry, or the magnitude of the 95% confidence brightness upper limit if the W2 flux measurement has SNR<2. | ||
wise_w3mpro | float | 8 | mag | W3 magnitude measured with profile-fitting photometry, or the magnitude of the 95% confidence brightness upper limit if the W3 flux measurement has SNR<2. | ||
wise_w4mpro | float | 8 | mag | W4 magnitude measured with profile-fitting photometry, or the magnitude of the 95% confidence brightness upper limit if the W4 flux measurement has SNR<2. | ||
match_p | float | 8 | dimensionless | Overall probability that the Gaia and WISE sources are detections of the same object, as given by equation 26 of Wilson & Naylor (2018a, MNRAS, 473, 5570). | ||
eta | float | 8 | dimensionless | Photometric logarithmic likelihood ratio of Gaia-WISE match, as described by equation 37 of Wilson & Naylor (2018a, MNRAS, 473, 5570). | ||
xi | float | 8 | dimensionless | Astrometric logarithmic likelihood ratio of Gaia-WISE match, as described by equation 38 of Wilson & Naylor (2018a, MNRAS, 473, 5570). | ||
gaia_avg_cont | float | 8 | dimensionless | Mean contaminating relative flux within PSFs when constructing h_offsets for Gaia sources at the local density, magnitude and intrinsic positional uncertainty of the primary source. | ||
wise_avg_cont | float | 8 | dimensionless | 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. | ||
gaia_cont_p1 | float | 8 | dimensionless | Probability of Gaia source having contaminant of at least 1% relative flux given its separation from its corresponding WISE detection, as given by equation 12 of Wilson & Naylor (2018b, MNRAS, 481, 2148). | ||
gaia_cont_p10 | float | 8 | dimensionless | Probability of Gaia source having contaminant of at least 10% relative flux given its separation from its corresponding WISE detection. | ||
wise_cont_p1 | float | 8 | dimensionless | Probability of WISE source having contaminant of at least 1% relative flux given its separation from its corresponding Gaia detection. | ||
wise_cont_p10 | float | 8 | dimensionless | Probability of WISE source having contaminant of at least 10% relative flux given its separation from its corresponding Gaia detection. | ||
sep | float | 8 | arcsec | Angular separation between sources | ||
gaia_source_ID | bigint | 8 | dimensionless | Gaia integer unique source designation | ||
wise_cntr | bigint | 8 | dimensionless | WISE integer unique source designation | ||
Total length | 248 |