Photometry: WASP-44b

Exo-Planet, Class confirmed:
WASP-44b
Imaged/Calibration/Image solve:
PRiSM v11
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 = 0.1238 ± 0.0042 (expected: 0.126 ± 0.003)
O-C = 0.6 ± 1.32 minutes
Quality check
Residuals STD (Standard Deviation) = 3.695 ‰
Based on your past observations, this is better than expected (5.734 ‰).
Diagnostics
Step 1: Transit SNR = 14.8
Transit SNR is good (strong detection of the transit)
Step 2: Rp/Rs drift = -0.43σ
The Rp/Rs drift is good (Rp/Rs in good agreement with the literature)
Step 3: AutoCorrelation = 0.185
The AutoCorrelation is good (no systematics in the data)
Step 4: Shapiro test = 0.019
The Shapiro test is good (few or no outliers in the data)