Table 3.
Known lenses in the KIDS DR4 footprint.
ID | pSTAR | pQSO | pGALAXY |
---|---|---|---|
J004941.90−275225.87 | 2.0E−5 | 1.0E−5 | 0.9999 |
J033238.22−275653.32 | 2.0E−5 | 1.0E−5 | 0.9999 |
J115252.26+004733.11 | 2.0E−5 | 1.0E−5 | 0.9999 |
J220132.76−320144.73 | 0.0004 | 4.0E−5 | 0.9999 |
J234416.95−305625.98 | 0.0004 | 0.0012 | 0.9983 |
J105644.89−005933.34 | 7.0E−4 | 0.9978 | 0.0015 |
J112320.73+013747.53 | 0.0086 | 0.9829 | 0.0085 |
J142758.89−012130.31 | 0.0035 | 0.9831 | 0.0134 |
J025257.87−324908.65 | 0.0011 | 0.9950 | 0.0039 |
J145847.59−020205.87 | 0.0004 | 0.0011 | 0.9985 |
J145847.66−020204.86 | 2.0E−5 | 3.0E−5 | 0.9999 |
J032606.87−312254.21 | 0.0019 | 0.9944 | 0.0037 |
J032606.78−312253.52 | 0.0023 | 0.9793 | 0.0184 |
J143228.96−010613.51 | 0.0006 | 0.9980 | 0.0014 |
J143229.25−010615.98 | 0.0008 | 0.9966 | 0.0025 |
J104237.27+002301.42 | 0.0477 | 0.8637 | 0.0886 |
J104237.24+002302.76 | 0.0652 | 0.7721 | 0.1627 |
J092455.82+021923.69 | 0.0078 | 0.8909 | 0.1012 |
J092455.82+021925.30 | 0.0059 | 0.4543 | 0.5397 |
J122608.10−000602.31 | 0.0046 | 0.9610 | 0.0343 |
J122608.03−000602.25 | 0.0199 | 0.5048 | 0.4752 |
J122608.13−000559.09 | 0.0009 | 0.0016 | 0.9997 |
J133534.80+011805.61 | 0.0128 | 0.9806 | 0.0066 |
J133534.87+011804.45 | 0.0056 | 0.9797 | 0.0066 |
J133534.97+011809.32 | 0.0013 | 0.0050 | 0.9937 |
J152720.14+014139.66 | 0.0058 | 0.9617 | 0.0325 |
J152720.27+014140.96 | 0.0005 | 0.0006 | 0.9999 |
Notes. All of them are recovered in our extragalactic catalogue, 8 out of 17 have multiple matches. For the single ones (upper “block”), 5 out of 17 are classified as GALAXY and 4 out of 17 as QSO. For the multiple matches, half of the time all the components belong to the same family (middle “block”) and the other half of the time they belong to different families (bottom “block”). We report for each component of each system the J2000 coordinates in the ID column (in the usual “hhmmss.ss ± ddmmss.ss” format), and the probability of belonging to each of the three classification families, highlighting the highest probability in bold.
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