TOI-3908 (トランジット惑星)
RA: 13h 47m 07.91s, DE: +42° 44' 09.65" (206.7829567000, 42.7360142034)
2026/04/23, 23:17 - 2026/04/24, 01:39 (UTC)
- 観測者: Federico Palaia, Mauro Santarossa, Mirko Gusmaroli
- 作成者: Federico Palaia
- 作成: 2026/04/28, 16:17
- 更新: 2026/04/28, 16:19
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観測所:
Civico Osservatorio Astronomico di Rozzano
Lat: +45°, Long: +09° - 観測装置: Meade ACF 16", Moravian G4-9000, clear and RGB filters
- 測光バンド: Luminance
- 基準時: Gjd
- 光度: Flux
注釈:
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.
トランジットの決定
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2461154.51387 (2026/04/24, 00:19)
惑星名: TOI-3908 .01
HJDmid: 2461154.51714 +/- 0.00077
太陽中心補正: 0.00327
トランジットの深さ (Mag): 0.02914 +/- 0.00144
トランジットの継続時間 (Min): 110.82 +/- 3.09
標準偏差 (mmag): 3.08
データクオリティーの指標: 2
データの密度 (data/min): 0.41
フィッティングアルゴリズム: オリジナルのETD
注釈: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.
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2461154.51378 (2026/04/24, 00:19)
惑星名: TOI-3908 .01
HJDmid: 2461154.51705 +/- 0.00111
太陽中心補正: 0.00327
トランジットの深さ (Mag): 0.03340 +/- 0.00182
トランジットの継続時間 (Min): 129.12 +/- 4.47
標準偏差 (mmag): 2.26
データクオリティーの指標: 1
データの密度 (data/min): 0.41
フィッティングアルゴリズム: オリジナルのETD
注釈: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.
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