ASTEROIDAL OCCULTATION - REPORT FORM

    +------------------------------+  +-------------------------------+
    |            EAON              |  |            IOTA/ES            |
    |                              |  |   INTERNATIONAL OCCULTATION   |
    |     EUROPEAN  ASTEROIDAL     |  |      TIMING  ASSOCIATION      |
    |     OCCULTATION NETWORK      |  |       EUROPEAN SECTION        |
    +------------------------------+  +-------------------------------+

1 DATE:                  2020 September 13 19:24:35  (UTC)

  STAR:                  UCAC4: 333-118357       mv: 13.3  mag
  ASTEROID:              (2882) Tedesco 	 mv: 16.6  mag  (diam. 22.0 km)
                         combined magnitude:     mv: 13.2  mag
                         delta-magnitude:        mv:  3.35 mag

2 OBSERVER: 
  Name:                  Josef KAESER / Abbr: Kaeser J Observatory
  E-mail:                j.kaeser@datacomm.ch
  Address:               Muehlefeld 1, CH - 5015 Erlinsbach, Switzerland

3 OBSERVING STATION: 
  Nearest city:          5000 Aarau, Switzerland
  Station:               Sternwarte Schafmatt (IAU Observatory Code: B77)
  Latitude:              N 47° 25' 12.88" (WGS84)
  Longitude:             E 07° 57' 02.95" (WGS84)
  Altitude:              820 m (MSL)      (WGS84)

  Predicted occultation: yes (located 6 km South-Est of the predicted center line)
  With of path:          56   km
  Probability:           16.2 %
  
  Single station:        Joseph KAESER

                         +----------------------------------+
4 TIMING OF EVENT:       |                                  |
                         |  OCCULTATION RECORDED: POSITIVE  |
                         |                                  |
                         +----------------------------------+
  Type of event:
   S = Start observation I = Interrupt-start   D = Disappearance
   B = Blink             F = Flash             E = End observation
   I = Interrupt-end     R = Reappearance      
   M = Mid-event         P = Predicted time

  Event  Time (UTC)      Accuracy     Comments
  Code   HH MM SS.sss    S.sss
  
   S     19 22 17        +/-0.040 s : Start observation (UTC)
   D     19 24 34.690    +/-0.080 s : Disappearance     (UTC)
   R     19 24 35.730    +/-0.080 s : Reappearance      (UTC)
   E     19 26 56        +/-0.040 s : End observation   (UTC)

   Duration:    1.040 s  +/-0.110 s : (predicted: max. 1.4 s)

   M     19 24 35.210	 +/-0.080 s : Mid-event         (UTC)
   P     19 24 35	 +/-3.000 s : Predicted time    (UTC)
        
5 TELESCOPE: 
  Type:                  Cassegrain Astrograph (LOMO / P. Keller)
  Aperture:              450 mm      
  Focal length:          1500 mm f/3.3 (primary focus) 
  Magnification:         focal (resulting field of view: 14.8' x 11.8')
  Mount:                 equatorial
  Motor drive:           yes

6 TIMING & RECORDING:
  Time source:           GPS unit: US Global Sat EM-406A (internal)
  Sensor:                1/2" Watec 910HX-RC (CCIR) (6.47 x 4.83 mm)
                         752 x 582 px (8.6 x 8.3 my) 
  Frame grabber:         LogiLink VG0005B USB2.0
  Time  insertion:       Video Time Inserter IOTA-VTI v3 with GPS
			 Video frame time (Vt)

7 OBSERVING CONDITIONS:
  Atmospheric transp.:   fair
  Wind:                  1    m/s 
  Temperature:           +20  °C
  Relative humidity:     71   %
  Atmospheric pressure:  1024 hPa
  Moonlight:             no   (below horizon)
  Star image stability:  good  (occulted star 15° above horizon)
  Minor planet visible:  no    (brightness 16.6 mag)
  
8 ADDITIONAL COMMENTS:    
  Shutter mode:                x4 
  Integration time (It)  =     0.080 s
  Correction time  (Ct)  =    -0.060 s (evaluation in frames)
  Tolerance value        =  +/-0.040 s (evaluation in frames)
  Video frame time       =     Vt
  Reported event time    =     Vt + Ct (correction time applied) 
  Video editing software:      VirtualDub v1.10.4
  Light measurement tool:      Tangra v3.6.17
  The reported times and tolerances concerning (D)isappearance, (R)eappearance,
  (M)id-event and Duration was analysed by E. Frappa (using AOTA software).

  No evidence of any satellite was found in the range of -138/+141 seconds.

9 CREDITS:
  Jonas Schenker for helpful assistance.