Table A.1
First few sources of the current LBCS catalogue.
L326144 | 00:00:00.990 | 68:10:03.000 | 2015-03-19 | 11:39:55 | XXX-XXXXX | 43 |
L269677 | 00:00:41.620 | 39:18:03.499 | 2015-03-05 | 12:38:02 | XXXXXXXXX | 53 |
L325856 | 00:00:41.620 | 39:18:03.499 | 2015-03-19 | 11:09:45 | SXX-XXXXP | 56 |
L269693 | 00:00:42.390 | 35:57:41.602 | 2015-03-05 | 12:38:02 | PPPPPXXPP | 53 |
L325860 | 00:00:42.390 | 35:57:41.602 | 2015-03-19 | 11:09:45 | PXP-PPSPP | 56 |
L410226 | 00:00:46.920 | 11:14:29.000 | 2015-11-09 | 19:30:06 | XXXXXXXXX | 30 |
L397819 | 00:00:49.470 | 32:55:47.701 | 2015-07-30 | 02:51:00 | XSPSXPSSX | 41 |
L269863 | 00:00:51.240 | 51:57:20.200 | 2015-03-05 | 12:44:02 | PPPPPXPPP | 53 |
L323730 | 00:00:51.240 | 51:57:20.200 | 2015-03-18 | 12:02:04 | PPP-PXXPP | 40 |
L269321 | 00:00:53.120 | 40:54:01.501 | 2015-03-05 | 12:26:02 | PPPPPPPPP | 63 |
L325788 | 00:00:53.120 | 40:54:01.501 | 2015-03-19 | 11:03:43 | PPP-PPPPP | 66 |
L410198 | 00:00:53.120 | 40:54:01.501 | 2015-11-09 | 19:36:08 | PPPPPPPPP | 70 |
L269649 | 00:00:54.520 | 38:02:44.999 | 2015-03-05 | 12:38:02 | PXXXPXXXP | 53 |
L325870 | 00:00:54.520 | 38:02:44.999 | 2015-03-19 | 11:09:45 | PXP-PXXXP | 56 |
L269313 | 00:01:01.520 | 41:49:29.201 | 2015-03-05 | 12:26:02 | PPPPPXPPP | 63 |
L325796 | 00:01:01.520 | 41:49:29.201 | 2015-03-19 | 11:03:43 | PPP-PXPSP | 66 |
L410206 | 00:01:01.520 | 41:49:29.201 | 2015-11-09 | 19:36:08 | PPPPPSSSP | 70 |
L410220 | 00:01:02.320 | 10:35:49.600 | 2015-11-09 | 19:30:06 | XXXXXXXXX | 30 |
Notes. Columns are the LBCS observation number (equivalent to that maintained in the LOFAR Long-Term Archive); the right ascension of pointing position of the observation of the source; the declination of the pointing position; the observing date and time; the description of the source fringe detections to each of the LOFAR international stations (see text); and a quality flag for the observation in terms of the proportion of sources in a single observation that are detected. In general, below 20% indicates a possibly bad observation and below 10% indicates an observation that is likely to be bad.
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