Exo-Planet, Class confirmed:
HAT-P-30b
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: RC14, 1938.0 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 = 0.1121 ± 0.0024 (expected: 0.1109 ± 0.0016)
O-C = 2.64 ± 1.38 minutes
Diagnostics
Step 1: Transit SNR = 23.87
Transit SNR is good (strong detection of the transit)!
Step 2: Rp/Rs drift = 0.42σ
The Rp/Rs drift is good (Rp/Rs in good agreement with the literature)
Step 3: AutoCorrelation = 0.266
The AutoCorrelation is good (no systematics in the data)
Step 4: Shapiro test = 0.007
The Shapiro test is good (few or no outliers in the data)

Exo-Planet, Class confirmed:
HAT-P-61b
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: RC14, 1938.0 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 = 0.0955 ± 0.0088 (expected: 0.0984 ± 0.0025)
O-C = -3.11 ± 4.9 minutes
Diagnostics
Transit SNR = 5.46 (good:≥5, acceptable:≥3)
(strong detection of the transit)
Rp/Rs drift = -0.32σ (good:≤2, acceptable:≤3)
(Rp/Rs in good agreement with the literature)
AutoCorrelation = 0.204 (good:≤0.335, acceptable:≤0.41)
(no systematics in the data)
Shapiro = 0.008 (good:≤0.037, acceptable:≤0.061)
(few or no outliers in the data)

Exo-Planet, Class confirmed:
WASP-50b
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: RC14, 1938.0 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 = 0.1476 ± 0.0025 (expected: 0.1404 ± 0.0012)
O-C = -2.56 ± 0.85 minutes
Diagnostics
Transit SNR = 29.83 (good:≥5, acceptable:≥3)
(strong detection of the transit)
Rp/Rs drift = 2.6σ (good:≤2, acceptable:≤3)
(Rp/Rs in marginal agreement with the literature)
AutoCorrelation = 0.228 (good:≤0.326, acceptable:≤0.399)
(no systematics in the data)
Shapiro = 0.017 (good:≤0.034, acceptable:≤0.057)
(few or no outliers in the data)

Exo-Planet, Class confirmed:
HAT-P-56b
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: RC14, 1938.0 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 = 0.1061 ± 0.0027 (expected: 0.1054 ± 0.0009)
O-C = 3.2 ± 1.34 minutes
Diagnostics
Transit SNR = 20.1 (good:≥5, acceptable:≥3)
(strong detection of the transit)
Rp/Rs drift = 0.25σ (good:≤2, acceptable:≤3)
(Rp/Rs in good agreement with the literature)
AutoCorrelation = 0.227 (good:≤0.279, acceptable:≤0.34)
(no systematics in the data)
Shapiro = 0.007 (good:≤0.024, acceptable:≤0.038)
(few or no outliers in the data)

Exo-Planet, Class confirmed:
TOI-1518b
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: RC14, 1947.0 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 = 0.1074 ± 0.0087 (expected: 0.0988 ± 0.0015)
O-C = -9.05 ± 2.3 minutes
Diagnostics
Transit SNR = 7.03 (good:≥5, acceptable:≥3)
(strong detection of the transit)
Rp/Rs drift = 0.97σ (good:≤2, acceptable:≤3)
(Rp/Rs in good agreement with the literature)
AutoCorrelation = 0.212 (good:≤0.321, acceptable:≤0.393)
(no systematics in the data)
Shapiro = 0.004 (good:≤0.033, acceptable:≤0.055)
(few or no outliers in the data)

Photometry: WASP-77Ab
Exo-Planet, Class confirmed:
WASP-77Ab
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: RC14, 1947.0 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 = 0.1242 ± 0.0022 (expected: 0.1301 ± 0.0007)
O-C = 2.27 ± 0.65 minutes
Diagnostics
Transit SNR = 28.3 (good:≥5, acceptable:≥3)
(strong detection of the transit)
Rp/Rs drift = -2.56σ (good:≤2, acceptable:≤3)
(Rp/Rs in marginal agreement with the literature)
AutoCorrelation = 0.249 (good:≤0.317, acceptable:≤0.388)
(no systematics in the data)
Shapiro = 0.012 (good:≤0.032, acceptable:≤0.053)
(few or no outliers in the data)

Exo-Planet, Class confirmed:
TOI-1516b
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: RC14, 1947.0 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 = 0.1204 ± 0.0024 (expected: 0.1224 ± 0.0005)
O-C = -2.3 ± 1.15 minutes
Diagnostics
Transit SNR = 25.13 (good:≥5, acceptable:≥3)
(strong detection of the transit)
Rp/Rs drift = -0.82σ (good:≤2, acceptable:≤3)
(Rp/Rs in good agreement with the literature)
AutoCorrelation = 0.363 (good:≤0.302, acceptable:≤0.369)
(weak systematics in the data)
Shapiro = 0.008 (good:≤0.029, acceptable:≤0.047)
(few or no outliers in the data)

Exo-Planet, Class confirmed:
TOI-3693b
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: RC14, 1947.0 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 = 0.1468 ± 0.0023 (expected: 0.14608 ± 0.001403)
O-C = -2.71 ± 1.22 minutes
Diagnostics
Transit SNR = 32.03 (good:≥5, acceptable:≥3)
(strong detection of the transit)
Rp/Rs drift = 0.27σ (good:≤2, acceptable:≤3)
(Rp/Rs in good agreement with the literature)
AutoCorrelation = 0.266 (good:≤0.301, acceptable:≤0.367)
(no systematics in the data)
Shapiro = 0.016 (good:≤0.028, acceptable:≤0.046)
(few or no outliers in the data)

Exo-Planet, Class confirmed:
TOI-4145Ab
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: RC14, 1947.0 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 = 0.1453 ± 0.0035 (expected: 0.14195 ± 0.001338)
O-C = -1.76 ± 1.31 minutes
Diagnostics
Transit SNR = 21.2 (good:≥5, acceptable:≥3)
(strong detection of the transit)
Rp/Rs drift = 0.89σ (good:≤2, acceptable:≤3)
(Rp/Rs in good agreement with the literature)
AutoCorrelation = 0.182 (good:≤0.321, acceptable:≤0.393)
(no systematics in the data)
Shapiro = 0.017 (good:≤0.033, acceptable:≤0.055)
(few or no outliers in the data)

Photometry: HAT-P-62b
Exo-Planet, Class confirmed:
HAT-P-62b
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: RC14, 1947.0 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 = 0.0968 ± 0.0041 (expected: 0.0942 ± 0.0019)
O-C = -5.87 ± 2.88 minutes
Diagnostics
Transit SNR = 11.82 (good:≥5, acceptable:≥3)
(strong detection of the transit)
Rp/Rs drift = 0.58σ (good:≤2, acceptable:≤3)
(Rp/Rs in good agreement with the literature)
AutoCorrelation = 0.215 (good:≤0.306, acceptable:≤0.374)
(no systematics in the data)
Shapiro = 0.022 (good:≤0.03, acceptable:≤0.049)
(few or no outliers in the data)