The list shows occultations of possible double stars during February. Although the main emphasis remains on stars with separations < 2", now that the more detailed lunar limb profile from LOLA is available, some wider pairs are included. Doubles predicted to be occulted by the Moon during February 2019 and visible from parts of Australia or New Zealand are included. The listing is a very abbreviated version of predictions produced by Occult plus an indication of the region of visibility. Observers need to generate their own precise predictions using Occult.
The list below is generated by OCCULT for a 25cm telescope. Some of the events could be beyond the reach of smaller telescopes. Observations of all pairs in the list are highly desirable. Those showing an OCc number have been reported as non-instantaneous at a lunar occultation. Confirmation or otherwise of any double nature is wanted.
*** Kepler stars: the nights on which they are occulted are indicated. Individual Keplers are only shown if they are also a known or possible double. Light curve of occultations of all Kepler stars are desired.
Please send reports of all observations of these stars to Brian Loader at brian.loader@slingshot.co.nz, including any made in earlier months and not so far reported. And of course if you observe a stepped event for a star, which is not a known double, please report this. More details about reporting follow the predictions.
ARCHIVING OCCULTATION LIGHT CURVES
For ALL lunar occultations: single, double and Kepler K2 stars a csv file should be prepared for archiving. This can be done through the OBSERVATIONS EDITOR of OCCULT.
It will be necessary to generate a light curve using LIMOVIE and save or copy its csv file. You will also need to note the time, hh:mm:ss.sss of one frame and the corresponding frame number.
Then in the Observations Editor select the entry for the star and use the menu bar option to create a Light Curve Report. Follow the instructions on the new screen which appears. There is a help file. It is suggested that light curve reports be emailed in batches rather than singly. They are sent directly to Dave Herald from the program.
******************************************************************************** d P Star Mag % Double details WDS or Area of Feb No v ill magnitudes sepn PA° OCC # Visibility 1 r 187079 9.6 8- : AB 9.7 12.9 4.7" 299.7 B 1888 RBTSCM 1 R 2708 5.9 8- : AB 6.0 8.4 138.0 WSI 90 RBTSCM 1 r X 44422 9.8 8- : ** 9.8 0.7" 262.0 OCc1743 SCM 2 r 188239 9.4 4- : AB 9.5 12.0 0.70" 284.0 RST5548 RB : AC 9.5 10.6 10.6" 333.1 HJ 2875 RB 7 d *** Kepler Stars occulted, light curves are desired RBTC 7 d X184816#10.0 5+ : AB 10.0 10.1 3.6" 111.0 STF2581 RB X184816: B star is SAO146537 *** X184816 is in the Kepler2 program {ID = 246025901} 8 d *** Kepler Stars occulted, light curves are desired RBS,AkWCh 11 d 110398 9.3 34+ : ** 9.1 10.1 0.20" 277.0 OCc1179 ,I 13 D 581 6.8 55+ : AB 6.9 11.1 3.6" 237.3 HEI 31 RBTSC,AkWChI 13 d *** Kepler Stars occulted, light curves are desired RCM 14 d *** Kepler Stars occulted, light curves are desired RBTSCM,Ak 14 d 94178 9.5 66+ : AB 9.6 11.5 3.9" 192.8 A 2426 SCM 15 d 77519 8.9 75+ : AC 12.9 12.9 6.3" 249.1 J 2731 ,AkWCh 15 d 77553 8.1 76+ : AB 9.1 9.2 0.18" 229.6 HU 39° ,AkWChI 15 D 77678# 7.7 76+ : ** 8.8 8.8 0.10" 151.0 OCc 882 RBTSC 16 D 1059 6.9 86+ : ** 7.7 7.7 0.10" 230.0 OCc 820 RBTSCM,I 17 d 1216 7.5 93+ : ** 8.5 8.5 0.08" 280.0 OCc 250 RBT 17 d 79953 7.8 94+ : AB 7.8 11.2 2.39" 241.7 HO 351 RBTS 18 d 98314 8.9 98+ : ** 9.7 9.7 0.25" 98.0 OCc1077 RBTSCM,AkWChI 18 d *** Kepler Stars occulted, light curves are desired CM,Ak 20 r 99474 8.4 98- : AB 8.59 9.87 0.59" 301.5 A 2775 RBTSC,AkWChI 21 R 1739 6.4 95- : ** 7.3 7.3 0.05" 350.0 OCc1432 RBTSCM,AkWChI 23 r *** Kepler Stars occulted, light curves are desired RBTSCM,AkWChI 23 r 139678 8.6 78- : ** 8.8 8.8 0.10" 90.0 OCc 35 R 24 r 158854# 8.9 68- : AB 9.30 9.84 0.40" 228.8 RST3898 RBTSCM,AkWChI 25 r 159415# 8.2 59- : AB 8.78 9.09 0.02" 85.0 HDS2210 ,ChI *** 159415 is in the Kepler2 program {ID = 250128530} 159415 is double: AB 8.78 9.09 0.024" 85.0 25 r X 39817# 9.6 59- : AB 10.4 10.6 1.4" 308.9 HLD 25 ,AkWCh 25 r X 39946 9.8 58- : AB 9.8 12.1 4.0" 341.8 HU 478 BTSCM,AkI *** X 39946 is in the Kepler2 program {ID = 250065113} 25 r *** Kepler Stars occulted, light curves are desired RBTSC,AkWChI 26 r *** Kepler Stars occulted, light curves are desired RBTS 26 r X 41272 10.3 47- : ** 9.7 10.5 0.02" 257.0 OCc 512 RBT 27 r 2497* 6.5 39- : ** 7.8 7.8 1.3" 105.0 OCc 529 ,WChI *** 2497 is in the Kepler2 program {ID = 234426962} 27 r 160511 8.1 39- : AB 8.2 10.9 0.50" 325.0 HDS2455 ,AkWChI 27 r X 42385 10.0 38- : AB 10.1 10.9 2.3" 131.3 I 599 ,AkW *** X 42385 is in the Kepler2 program {ID = 226690780} 27 r *** Kepler Stars occulted, light curves are desired RBTSCM,AkW 28 R 2638 5.3 29- : Aab 5.3 8.4 203.0 SNA 82 ,AkWChI : AB 5.4 10.6 1.3" 78.2 TOK 59 ,AkWChI : AC 5.2 12.9 2.3" 356.0 SNA 82 ,AkWChI : AD 5.2 12.2 7.1" 108.0 SNA 82 ,AkWChI 28 r 2642# 7.0 29- : AB 7.24 8.89 0.03" 138.4 MCA 51 ,ChI 28 r X 43966 9.1 28- : AB 9.2 9.1 2.7" 42.8 HLD 144 RBTSCM X 43966: B star is X156588 28 r X 44023 10.4 27- : AB 10.4 10.6 3.1" 184.0 HU 239 R Visibility codes: Australia: R Rockhampton, B Brisbane, T Tamworth, S Sydney, C Canberra, M Melbourne NZ (following a ,) Ak Auckland, W Wellington, Ch Christchurch, I Invercargill. ---------------------------------------------------------------------- Stars with previous occultation observations: #: Observations indicating double - these need further checking *: Observations not showing double - need confirmation !: Recent video discoveries - confirmation needed. ?: Uncertain double observation, confirmation or otherwise needed A WDS number followed by a ° sign indicates the double has a known orbit. ==================================================================
The most convenient way of reporting is to use Dave Herald's OCCULT which has a Double Star report option in the Observations editor. Before using it, generate a light curve with Limovie and copy to the clip board. Your graph will be attached to the email which you can then send to brian.loader@slingshot.co.nz.
Otherwise in reporting please include your name and positional data as for other occultations reports, also your telescope type and method of observing and timekeeping.
For each event give the star name and the times of each step of the event with the corresponding accuracy. The limb PA, Rv and Cct of the event would also be useful.
In addition to measures of the PA and separation of binary stars, there is also a need for an estimate of the magnitude difference. An estimate of this can be made from the step sizes shown by Limovie data. So if possible a determination should be made of the size of each step together with an estimate of accuracy.
Please also report cases where a double event is predicted but none detected. These are especially likely with stars shown with an OCc designation
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