TOI-3908 (Tranzitující exoplaneta)

RA: 13h 47m 07.91s, DE: +42° 44' 09.65" (206.7829567000, 42.7360142034)

23.04.2026, 23:17 - 24.04.2026, 01:39 (UTC)

Údaje:

  • Pozorovatel: Federico Palaia, Mauro Santarossa, Mirko Gusmaroli
  • Vytvořil: Federico Palaia
  • Vytvořeno: 28.04.2026, 16:17
  • Změněno: 28.04.2026, 16:19
  • Stanice: Civico Osservatorio Astronomico di Rozzano
    Lat: +45°, Long: +09°
  • Přístroj: Meade ACF 16", Moravian G4-9000, clear and RGB filters
  • Fotometrický obor: Luminance
  • Časový standard: Gjd
  • Jasnost v: Flux
Poznámka:
Data reduction and analysis were performed using the HOPS software.

Further observations and analysis are required to confirm the nature of the system and to verify the planetary candidate.
Stanovené tranzity
  • 2461154.51387 (24.04.2026, 00:19)
    Označení planety: TOI-3908 .01
    HJDmid: 2461154.51714 +/- 0.00077
    Heliocentrická korekce: 0.00327
    Hloubka tranzitu (Mag): 0.02914 +/- 0.00144
    Délka tranzitu (Min): 110.82 +/- 3.09
    Standardní odchylka (mmag): 3.08
    Index kvality dat: 2
    Hustota dat (data/min): 0.41
    Fitovací algoritmus: Původní ETD  
    Poznámka:
    Data reduction and analysis were performed using the HOPS software.
    
    The resulting light curve differs significantly from what is expected for a typical exoplanet transit. In particular, the shape of the signal appears more consistent with that of an eclipsing binary star rather than a planetary transit.
    
    Further observations and analysis are therefore required to confirm the nature of the system and to verify the planetary candidate.
  • 2461154.51378 (24.04.2026, 00:19)
    Označení planety: TOI-3908 .01
    HJDmid: 2461154.51705 +/- 0.00111
    Heliocentrická korekce: 0.00327
    Hloubka tranzitu (Mag): 0.03340 +/- 0.00182
    Délka tranzitu (Min): 129.12 +/- 4.47
    Standardní odchylka (mmag): 2.26
    Index kvality dat: 1
    Hustota dat (data/min): 0.41
    Fitovací algoritmus: Původní ETD  
    Poznámka:
    Data reduction and analysis were performed using the HOPS software.
    
    Further observations and analysis are required to confirm the nature of the system and to verify the planetary candidate.
Akce:

Světelná křivka
Okolí objektu, srovnávací a kontrolní hvězdy
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