Exo-Planet, Class confirmed:
WASP-32b
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 = 0.1062 ± 0.0027 (expected: 0.1114 ± 0.0018)
O-C = -0.89 ± 1.58 minutes
Diagnostics
Transit SNR = 19.74 (good:≥5, acceptable:≥3)
(strong detection of the transit)
Rp/Rs drift = -1.6σ (good:≤2, acceptable:≤3)
(Rp/Rs in good agreement with the literature)
AutoCorrelation = 0.268 (good:≤0.355, acceptable:≤0.436)
(no systematics in the data)
Shapiro = 0.016 (good:≤0.042, acceptable:≤0.071)
(few or no outliers in the data)

Exo-Planet, Class confirmed:
K2-295b
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 = 0.1443 ± 0.0059 (expected: 0.1304 ± 0.0014)
O-C = -0.84 ± 2.16 minutes
Diagnostics
Transit SNR = 12.28 (good:≥5, acceptable:≥3)
(strong detection of the transit)
Rp/Rs drift = 2.29σ (good:≤2, acceptable:≤3)
(Rp/Rs in marginal agreement with the literature)
AutoCorrelation = 0.274 (good:≤0.33, acceptable:≤0.404)
(no systematics in the data)
Shapiro = 0.009 (good:≤0.035, acceptable:≤0.059)
(few or no outliers in the data)

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)

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)

Exo-Planet, Class confirmed:
HAT-P-25b
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 = 0.1231 ± 0.0042 (expected: 0.1269 ± 0.0011)
O-C = -2.81 ± 1.87 minutes
Quality check
Residuals STD (Standard Deviation) = 4.698 ‰
Based on your past observations, this is better than expected (6.164 ‰).
Diagnostics
Step 1: Transit SNR = 14.7
Transit SNR is good (strong detection of the transit)!
Step 2: Rp/Rs drift = -0.88σ
The Rp/Rs drift is good (Rp/Rs in good agreement with the literature)!
Step 3: Auto Correlation = 0.204
The Auto Correlation is good (no systematics in the data)
Step 4: Shapiro test = 0.006
The Shapiro test is good (few or no outliers in the data)

Exo-Planet, Class confirmed:
TrES-5b
Imaged/Calibration/Image solve:
PRiSM v11
Photometry and Data Fitting:
HOPS 3.1.2/Platform: Python 3.9
Instrument:
CCD: Atik383L+ (KAF8300M)
FILTERS: Clear
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
R_p/R_s = 0.1361 ± 0.0049 (expected: 0.142 ± 0.0009)
O-C = 0.8 ± 1.87 minutes

Quality check
Residuals STD (Standard Deviation) = 5.915 ‰
Based on your past observations, this is better than expected (7.704 ‰). Great!

Diagnostics
Step 1: Transit SNR = 13.97
Transit SNR is good (strong detection of the transit)!
Step 2: R_p/R_s drift = -1.18σ
The R_p/R_s drift is good (R_p/R_s in good agreement with the literature)!
Step 3: Auto Correlation = 0.151
The Auto Correlation is good (no systematics in the data)!
Step 4: Shapiro test = 0.005
The Shapiro test is good (few or no outliers in the data)!

Exo-Planet, Class confirmed:
CoRoT-1b
Imaged/Calibration/Image solve:
PRiSM v11
Photometry and Data Fitting:
HOPS 3.1.0/Platform: Python 3.9
Instrument:
CCD: SX-35 (KAF11002M)
FILTERS: Luminance
TELESCOPE: RC14, 1945.0 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

Exo-Planet, Class confirmed:
HAT-P-36b
Imaged/Calibration/Image solve:
PRiSM v11
Photometry and Data Fitting:
HOPS 3.1.0/Platform: Python 3.9
Instrument:
CCD: SX-35 (KAF11002M)
FILTERS: Luminance
TELESCOPE: RC14, 1945.0 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

Exo-Planet, Class confirmed:
XO-2NB
Imaged/Calibration/Image solve:
PRiSM v11
Photometry and Data Fitting:
HOPS 3.1.0/Platform: Python 3.9
Instrument:
CCD: SX-35 (KAF11002M)
FILTERS: Luminance
TELESCOPE: RC14, 1945.0 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