Exo-Planet, Class confirmed:
TOI-3714b
Imaged/Calibration/Image solve:
PRiSMv11
Photometry and Data Fitting:
HOPS 3.1.2/Platform: Python 3.9
Instrument:
CCD: Atik383L+ (KAF8300M)
FILTERS: Luminance
TELESCOPE: C11, 1670.0 mm
Site:
ORIGIN: Cepheid Observatory India
SITELAT: +24:55:00:00
SITELONG:+75:33:58:99
Observers:
Cepheid Observatory India, VS Observatory India
Remark:
Sky Clear

Results
Rp/Rs = 0.205 ± 0.01 (expected: 0.204 ± 0.003)
O-C = -3.62 ± 1.28 minutes
Quality check
Residuals STD (Standard Deviation) = 13.867 ‰
Diagnostics
Step 1: Transit SNR = 10.3
Transit SNR is good (strong detection of the transit)
Step 2: Rp/Rs drift = 0.1σ
The Rp/Rs drift is good (Rp/Rs in good agreement with the literature)
Step 3: Auto Correlation = 0.304
The Auto Correlation is good (no systematics in the data)
Step 4: Shapiro test = 0.028
The Shapiro test is good (few or no outliers in the data)

Exo-Planet, Class confirmed:
WASP-177b
Imaged/Calibration/Image solve:
PRiSMv11
Photometry and Data Fitting:
HOPS 3.1.2/Platform: Python 3.9
Instrument:
CCD: Atik383L+ (KAF8300M)
FILTERS: Luminance
TELESCOPE: C11, 1670.0 mm
Site:
ORIGIN: Cepheid Observatory India
SITELAT: +24:55:00:00
SITELONG:+75:33:58:99
Observers:
Cepheid Observatory India, VS Observatory India
Remark:
Sky Clear

Results
Rp/Rs = 0.139 ± 0.012 (expected: 0.136 ± 0.0129)
O-C = -0.09 ± 3.46 minutes
Quality check
Residuals STD (Standard Deviation) = 3.816 ‰
Based on your past observations, this is better than expected (3.82 ‰).
Diagnostics
Step 1: Transit SNR = 6.45
Transit SNR is good (strong detection of the transit)
Step 2: Rp/Rs drift = 0.17σ
The Rp/Rs drift is good (Rp/Rs in good agreement with the literature)
Step 3: Auto Correlation = 0.46
Step 4: Shapiro test = 0.012
The Shapiro test is good (few or no outliers in the data)