Comet 62P/Tsuchinshan

Image Info:
Object: 62P/Tsuchinshan
DATE-OBS: 2024 02 17.91579
EXPTIME(mins): 50
SUBFRMS: 25
OBJCTRA: 12 41 09.25
OBJCTDEC: 10 00 49.3
Binning: 1 X 1
Plate Scale: 1.24″ /Pixel
Orientation: North Right/ East Up
Catalogs & Filter Magnitude Results:
Astrometry Catalog: ATLAS
Photometry Catalog: ATLAS
Imaging Filter: CLEAR
Photometry Mag: +12.6 R
Comet Afrho @ 10,000 km: 127 cm
Instruments:
CCD: SX 814 Trius (3.69µm x 3.69µm)
TELESCOPE: 132MM APO, 615mm
PRiSMv11, Tycho 11.1.0
Site:
ORIGIN: Cepheid Observatory, India
SITELAT: +24:55:00:00
SITELONG:+75:33:58:99
Observers:
Cepheid Observatory
Remark:
Sky Clear

Photometry: HAT-P-24b

Exo-Planet, Class confirmed:
HAT-P-24b
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 = 0.0911 ± 0.0056 (expected: 0.097 ± 0.0012)
O-C = -1.05 ± 2.16 minutes
Diagnostics
Transit SNR = 8.14 (good:≥5, acceptable:≥3)
(strong detection of the transit)
Rp/Rs drift = -1.03σ (good:≤2, acceptable:≤3)
(Rp/Rs in good agreement with the literature)
AutoCorrelation = 0.199 (good:≤0.264, acceptable:≤0.321)
(no systematics in the data)
Shapiro = 0.009 (good:≤0.021, acceptable:≤0.033)
(few or no outliers in the data)

Photometry: KPS-1b

Exo-Planet, Class confirmed:
KPS-1b
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 = 0.107 ± 0.01 (expected: 0.114 ± 0.004)
O-C = -0.45 ± 4.03 minutes
Diagnostics
Transit SNR = 5.39 (good:≥5, acceptable:≥3)
(strong detection of the transit)
Rp/Rs drift = -0.65σ (good:≤2, acceptable:≤3)
(Rp/Rs in good agreement with the literature)
AutoCorrelation = 0.217 (good:≤0.296, acceptable:≤0.362)
(no systematics in the data)
Shapiro = 0.011 (good:≤0.027, acceptable:≤0.045)
(few or no outliers in the data)

Photometry: TOI-2842b

Exo-Planet, Class confirmed:
TOI-2842b
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 = 0.0924 ± 0.0034 (expected: 0.0931 ± 0.0012)
O-C = 2.14 ± 2.45 minutes
Diagnostics
Transit SNR = 13.68 (good:≥5, acceptable:≥3)
(strong detection of the transit)
Rp/Rs drift = -0.18σ (good:≤2, acceptable:≤3)
(Rp/Rs in good agreement with the literature)
AutoCorrelation = 0.188 (good:≤0.297, acceptable:≤0.363)
(no systematics in the data)
Shapiro = 0.015 (good:≤0.028, acceptable:≤0.045)
(few or no outliers in the data)

Photometry: HAT-P-9b

Photometry: HAT-P-9b
Exo-Planet, Class confirmed:
HAT-P-9b
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 = 0.1041 ± 0.0041 (expected: 0.107 ± 0.0009)
O-C = -1.35 ± 1.24 minutes
Diagnostics
Transit SNR = 12.73 (good:≥5, acceptable:≥3)
(strong detection of the transit)
Rp/Rs drift = -0.69σ (good:≤2, acceptable:≤3)
(Rp/Rs in good agreement with the literature)
AutoCorrelation = 0.195 (good:≤0.252, acceptable:≤0.306)
(no systematics in the data)
Shapiro = 0.015 (good:≤0.019, acceptable:≤0.03)
(few or no outliers in the data)

Photometry: WASP-140b

Exo-Planet, Class confirmed:
WASP-140b
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 = 0.1496 ± 0.0078 (expected: 0.1432 ± 0.007)
O-C = -2.2 ± 1.12 minutes
Diagnostics
Transit SNR = 10.86 (good:≥5, acceptable:≥3)
(strong detection of the transit)
Rp/Rs drift = 0.61σ (good:≤2, acceptable:≤3)
(Rp/Rs in good agreement with the literature)
AutoCorrelation = 0.201 (good:≤0.303, acceptable:≤0.37)
(no systematics in the data)
Shapiro = 0.009 (good:≤0.029, acceptable:≤0.047)
(few or no outliers in the data)

Photometry: TOI-1811b

Exo-Planet, Class confirmed:
TOI-1811b
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 = 0.133 ± 0.0045 (expected: 0.13272 ± 0.00072)
O-C = -4.36 ± 1.43 minutes
Diagnostics
Transit SNR = 14.95 (good:≥5, acceptable:≥3)
(strong detection of the transit)
Rp/Rs drift = 0.06σ (good:≤2, acceptable:≤3)
(Rp/Rs in good agreement with the literature)
AutoCorrelation = 0.254 (good:≤0.311, acceptable:≤0.38)
(no systematics in the data)
Shapiro = 0.022 (good:≤0.031, acceptable:≤0.051)
(few or no outliers in the data)

Photometry:HAT-P-30b

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)

Photometry:HAT-P-61b

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)

Photometry: WASP-50b

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)