V0607 Dra (Eclipsing binary)

RA: 19h 50m 21.40s, DE: +70° 17' 14.00" (297.5891666617, 70.2872222219)

Gsc: GSC 04449-00995, Other: G4449.00995, Gcvs: V0607 Dra

11/18/2020, 16:08 - 11/18/2020, 22:46 (UTC)

Data:

  • Observer: Marian Urbaník
  • Created: 11/23/2020, 12:34 UTC
  • Station: Kysucká hvezdáreň
  • Instrument: SKY-WATCHER ED 80/520 + MII G2-8300
  • Photometric band: V
  • Time standard: GJD
  • Brightness in: Mag
  • Magnitude type: Relative (V−C)
Note:
CCD+V,exp.28 s,comp.UCAC4-802-027753,2x2.
Determined minima
  • P: 2459172.188620 (11/18/2020, 16:31 UTC)
    HJDmin: 2459172.189580 +/- 0.000780  
    Heliocentric correction: 0.000960
    Note:
    CCD+V,exp.28 s,comp.UCAC4-802-027753,2x2.
    
    ----- EBFit result: -----
    Tmin = 2459172.18862
    Error (1 sigma): +0.00080/-0.00076 (Bootstrapping), +0.00024/-0.00027 (Prayer bead), +0.00054/-0.00054 (LSM)
    Error (95% CI):  +0.00162/-0.00199 (Bootstrapping), +0.00045/-0.00048 (Prayer bead)
    LSM: chi^2 = 38.3, n_freedom = 18
    
  • S: 2459172.331310 (11/18/2020, 19:57 UTC)
    HJDmin: 2459172.332270 +/- 0.001530  
    Heliocentric correction: 0.000960
    Note:
    CCD+V,exp.28 s,comp.UCAC4-802-027753,2x2.
    
    ----- EBFit result: -----
    Tmin = 2459172.33131
    Error (1 sigma): +0.00160/-0.00146 (Bootstrapping), +0.00098/-0.00085 (Prayer bead), +0.00118/-0.00118 (LSM)
    Error (95% CI):  +0.00341/-0.00268 (Bootstrapping), +0.00285/-0.00208 (Prayer bead)
    LSM: chi^2 = 57.1, n_freedom = 42
    
  • S: 2459172.330660 (11/18/2020, 19:56 UTC)
    HJDmin: 2459172.331628 +/- 0.000994  
    Heliocentric correction: 0.000968
    Note:
    CCD+V,exp.28 s,comp.UCAC4-802-027753,2x2.
  • P: 2459172.188493 (11/18/2020, 16:31 UTC)
    HJDmin: 2459172.189462 +/- 0.000872  
    Heliocentric correction: 0.000969
    Note:
    CCD+V,exp.28 s,comp.UCAC4-802-027753,2x2.
Actions:

Light curve
Field identification - Star field chart
Field identification - Explicitly named stars

No comparison or check stars are explicitly listed for this observation. They should be marked in the star field chart.

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