Table C.1.
Additional candidates catalogue
oid | ra | dec | Redshift | Fitted Period | Error Period | Log(M) | Error Log(M) | ![]() |
CRTS obs |
---|---|---|---|---|---|---|---|---|---|
722214100002451 | 246.183 | 43.994 | 1.93 | 1517 | 55 | 9.24 | 0.02 | 1.08 | No |
762207400010289 | 253.448 | 46.594 | 2.29 | 1547 | 650 | 8.1 | 0.14 | 1.23 | Yes |
796215300002648 | 254.941 | 57.525 | 2.05 | 1354 | 45 | 0.92 | No | ||
721210400000714 | 237.562 | 41.418 | 1.89 | 1527 | 720 | 8.81 | 0.05 | 1.21 | Yes |
760213300014840 | 237.592 | 49.784 | 2.09 | 1545 | 722 | 8.69 | 0.07 | 1.02 | Yes |
792206200005745 | 214.018 | 54.177 | 1.48 | 1773 | 27 | 9.17 | 0.02 | 1.16 | No |
792210400012079 | 216.131 | 55.414 | 2.36 | 1477 | 696 | 9.31 | 0.05 | 1.17 | Yes |
793210300003169 | 225.462 | 55.544 | 1.15 | 1512 | 613 | 9.28 | 0.03 | 0.96 | Yes |
793213100021821 | 228.540 | 57.820 | 2.33 | 817 | 25 | 9.67 | 0.17 | 1.01 | No |
793216100016751 | 235.480 | 54.179 | 0.85 | 788 | 18 | 8.66 | 0.06 | 1.22 | No |
795211400020541 | 231.904 | 59.202 | 0.93 | 1283 | 509 | 9.83 | 0.23 | 0.95 | Yes |
823203400004287 | 238.373 | 61.827 | 2.44 | 1538 | 620 | 9.64 | 0.04 | 1.26 | Yes |
823205300004979 | 234.299 | 61.807 | 2.65 | 1534 | 398 | 9.34 | 0.07 | 0.88 | Yes |
678211200026561 | 239.653 | 35.532 | 2.09 | 1530 | 475 | 8.87 | 0.02 | 1.08 | Yes |
678213400006806 | 244.586 | 31.964 | 0.19 | 1520 | 289 | 1.26 | Yes | ||
720206400001109 | 229.529 | 42.999 | 2.04 | 1495 | 632 | 9.21 | 0.11 | 1.08 | Yes |
760216400003842 | 243.705 | 44.680 | 0.46 | 1470 | 26 | 1.06 | No | ||
792209300011535 | 215.639 | 55.088 | 1.02 | 1227 | 33 | 8.72 | 0.06 | 1.28 | No |
793206400000506 | 226.619 | 58.033 | 0.92 | 1527 | 592 | 8.06 | 0.08 | 1.22 | Yes |
Notes. First 20 lines of the catalogue of weak MBBH candidates. Columns in the catalogue show from left to right, the ZTF object ID (oid), the right ascension (R.A.) and declination (Dec.) of the sources in degrees, their redshift z, their identified period and 1 σ error in days, their Log(M) and 1 σ error in M⊙, the reduced chi square and finally if the object has CRTS observations. The full catalogue is available at the CDS.
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