The URL explaning the format of PPAS observations : http://www.satobs.org/tumble/flashpm.html#PPASformat yy-nnncc yy-mm-dd hh:mm:ss.s ooo sss.s s.s nnn ss.sss comments 77- 2 A 05-06-19 23:41:17.8 BD 163.1 3 3 54.4 +4.3->8.0 82- 16 A 05-06-14 22:13:33.0 BD 252.7 0.2 20 12.64 F; +3.5->inv; note 2 82- 16 A 05-06-19 22:00:20.9 BD 114.1 0.2 9 12.7 F; +2.0->inv; note 6 85- 79 B 05-06-11 23:28:17.0 BD 140.1 2 7 20.0 A; +5.0->inv 85- 79 B 05-06-12 01:10:07.0 BD 78.0 0.2 4 19.5 A; +4.0->inv 87- 11 A 05-06-14 00:47:41.0 BD 210.6 0.5 18 11.7 A'a'; +3.3->8.3 87- 60 A 05-06-19 23:11:59.0 BD 156.9 0.5 14 11.2 A; +3.5->inv 87- 20 B 05-06-14 00:11:13.2 BD 78.2 0.5 2 39.1 A; +6.3->inv 88- 89 A 05-06-19 22:07:24.7 BD 80.0 0.2 11 7.28 F'fFfF'; +5.0->inv; note 7 89- 16 A 05-06-13 21:16:41.6 BD 59.7 0.2 29 2.10 F; +2.3->inv 91- 29 B 05-06-14 01:01:24.1 BD 102.4 1 4 34.1 A; +4.8->inv 91- 82 E 05-06-12 00:10:01.6 BD 20.0 0.2 20 1.00 f'ff_; +6.0->inv; note 1 91- 82 E 05-06-19 23:28:39.5 BD 39.7 0.2 40 0.99 f'ff_; +5.0->inv 93- 20 B 05-06-13 22:39:59.4 BD 95.0 1 2 47.5 A; +6.0->7.5 93- 20 B 05-06-18 21:14:17.8 BD 44.6 1 2 44.6 A; +4.8->8.0 93- 50 A 05-06-13 21:45:34.1 BD 108.2 0.2 8 13.5 Irr; -2->inv; note 3 93- 50 A 05-06-14 21:32:49.8 BD 162.1 0.3 12 13.50 F; -2.0->inv; note 4 95- 2 D 05-06-19 00:44:00.5 BD 187.9 0.5 3 62.6 A; +4.5->8.0 97- 34 C 05-06-14 21:27:01.2 BD 41.0 0.2 30 1.37 F'fF'; +6.0->inv 97- 82 B 05-06-14 01:49:10.7 BD 113.5 0.2 16 7.09 F; +4.0->inv 98- 76 B 05-06-12 01:27:29.3 BD 149.3 5 1 149 A; +4.3->inv 98- 76 B 05-06-19 01:16:51.9 BD 101.3 3 1 101 A; +4.5->8.0 99- 45 B 05-06-14 20:59:59.0 BD 118.3 0.3 20 5.92 A; +4.3->inv 99- 57AD 05-06-18 23:52 BD 57 a; A; +5.0->7.8 02- 36 C 05-06-19 00:28:56.0 BD 118.0 2 2 59 +5.0->7.8 02- 46 B 05-06-13 23:12:46.5 BD 60.0 1 2 30 A; +4.5->inv 02- 46 B 05-06-19 22:31:05.0 BD 245.7 0.3 8 30.7 A; +5.3->inv 03- 37 C 05-06-14 00:04:18.5 BD 141.8 0.2 53 2.68 F; +5.0->inv 03- 37 C 05-06-18 23:36:36.9 BD 230.2 0.2 50 4.61 A; +5.0->inv 03- 37 C 05-06-19 22:46:02.3 BD 89.8 0.3 33 2.72 A; +5.3->inv 03- 46 B 05-06-13 21:02:56.2 BD 43.8 0.5 2 21.9 A'f; +3.0->7.5 04- 12 C 05-06-18 21:39:33 BD 74.1 5 1 74 A; +1.5->inv 04- 21 B 05-06-20 01:02:34.8 BD 220.6 0.5 31 7.12 A; +3.0->inv 04- 37 C 05-06-19 23:53:35.5 BD 179.4 0.5 9 19.9 A; +5.0->inv 05- 2 B 05-06-11 23:47:44.7 BD 274.3 0.2 95 2.887 A, ssf; +6.8->inv 05- 2 B 05-06-13 22:17:29.9 BD 170.3 0.2 50 3.41 A; +4.5->inv 05- 2 B 05-06-18 21:34:17.8 BD 140.8 0.2 40 3.52 A; +5.0->inv 05- 2 B 05-06-19 21:46:37.1 BD 285.6 0.2 40 7.139 A; +5.0->inv; note 5 05- 17 C 05-06-13 21:06:38.2 BD 67.8 0.2 11 6.16 F'f; 4.0->inv notes: 1) 91- 82 E: is it a coincidence that the flashing period equals to 1 second? 2) 82- 16 A: observed after an identification for a person who estimated the limiting magnitude and unintentionally saw three flashes near the star Kochab (beta UMi). 3) 93- 50 A: brightest flash was mag -2.0; flash period derived from intervals between the bright flashes; timings: (4.14 2.48 2.71 1.11 3.19) (2.05 1.86 2.42 2.54 3.43) (6.57 7.46) (4.47 2.92 6.12) 13.43 (8.53 5.03) (7.86 5.73) 13.67 4) 93- 50 A: brightest flash was mag -2.0; flash period derived from intervals between the bright flashes. 5) 05- 2 B: no other maxima seen like in previous observations. 6) 82- 16 A: After five days the max. brightness area was still near Kochab. 7) 88- 89 A: Triggered by EC's observation I added this object to the PPAS program. Flash period derived form the intervals between the orange flashes. There were bright white flashes in between and less bright flashes. 8) 77- 2 A: timings: (16.60 19.45 24.52) (16.95 36.08) 49.54 Bram Dorreman COSPAR 4160 51° 16' 45.5" N 5° 28' 36.6" E (WGS84) 35 m ------------------------------------------------------------------------- Subscribe/Unsubscribe info, Frequently Asked Questions, SeeSat-L archive: http://www.satobs.org/seesat/seesatindex.html
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