Link dedicated to the photometry of astronomical transients, AGN, Exoplanets, Nova, SN, comets and many more.
Exo-Planet, Class confirmed:
WASP-43b
Imaged/Calibration/Image solve:
PRiSM v11
Photometry and Data Fitting:
HOPS 2.6.8/Platform: Python 3.7.6
Instrument:
CCD: ATIK-383L+ mono
FILTERS: R
TELESCOPE: C11, 1623.0mm
Site:
ORIGIN: Cepheid Observatory, India, Vorion Scientific, India
SITELAT: +24:55:00:00
SITELONG:+75:33:58:99
Observers:
V.K.Agnihotri, B. Kumar, S. Mahawar, K.Vora
Remark:
Sky Clear
End
Exo-Planet, Class confirmed:
HAT-P-21b
Imaged/Calibration/Image solve:
PRiSM v11
Photometry and Data Fitting:
HOPS 2.6.8/Platform: Python 3.7.6
Instrument:
CCD: ATIK-383L+ mono
FILTERS: R
TELESCOPE: C11, 1623.0mm
Site:
ORIGIN: Cepheid Observatory, India, Vorion Scientific, India
SITELAT: +24:55:00:00
SITELONG:+75:33:58:99
Observers:
V.K.Agnihotri, B. Kumar, S. Mahawar, K.Vora
Remark:
Sky Clear
End
Image:
Object: TCP J09370380+1657350
DATE-OBS: 2021-01-13T20:16:18
EXPTIME: 1200.0 (seconds) for V/R/I
SUBFRMS: 10
OBJCTRA: 09 37 03.80
OBJCTDEC: +16 57 35.00
Instrument:
Catalog: UCAC4/USNOB1
Bessell (B): +*.*, Bessell (V): +14.614
Bessell (R): +14.848, Bessell (I): +14.734
CCD: ATIK-383L+
FILTERS: V/R/I
TELESCOPE: C11, 1623.0mm
PRiSMv10, Astrometrica
Site:
ORIGIN: Cepheid Observatory, India, Vorion Scientific, India
SITELAT: +24:55:00:00
SITELONG:+75:33:58:99
Observers:
K.Vora, V.K.Agnihotri, B. Kumar, S. Mahawar,
Remark:
Sky Clear. V and R band magnitudes are estimated using UCAC4 catalog. I band magnitude is estimated using USNOB1 catalog.
End
Sample Marked Image
2459228.32211 14.848 R R 136.93 27.223 UCAC4 TCP
2459228.33774 14.734 I I 73.31 26.073 USNOB1 TCP
2459228.35160 14.614 V V 242.13 27.536 UCAC4 TCP
—– end —–
M67/NGC2682 image using B & R band filters. The exposure time normalized for CCD sensitivity (means more exposure in B band w.r.t band). We see the more stars in R Band compare to B band.
Filter Response Curves for Baader UBVRI filters:
TCP J15360165-1642561, 2019-01-03T00:02:17.28
Astrometry: Catalog UCAC4, J2000
RA(2000)= 15h36m01.725s DEC(2000)= -16°42’58.66”
UT3.002 R MAGNITUDE= 14.27 ±0.22
UT3.004 I MAGNITUDE= 14.57 ±0.13
UT3.006 V MAGNITUDE= 14.13 ±0.10
telescope details: 0.28m Schmidt–Cassegrain+CCD
Filters Bessell BVRI
Imaged: K. Vora (Vorion Scientific Observatory, AHD, India)
Measured V. K. Agnihotri (Cepheid Observatory, RBT,India)
Exo-Planet Observations, Class confirmed K2-29b Imaged/Calibration/Image solve: PRiSM v11Photometry and Data Fitting: HOPS 2.6.4/Platform: Python 3.7.6C11/F5.7+CCDCepheid Observatory IndiaVorion Scientific Observatory India Sky Condition: Average We are happy to add Mai Wada as co-observer for exoplanet observation, working in university of arts of London, UK. Her painting for exoplanet K2-18-2 was appreciated in EPSC2019 together with Exoclock project admins Dr. A. Kokori and Dr. A. Tsiaras. Find her work here: https://www.maiwada.com/exoplanet-project
Exo-Planet Observations, Class confirmed
HAT-P-32b
Imaged/Calibration/Image solve: PRiSM v11
Photometry and Data Fitting: HOPS 2.6.4/Platform: Python 3.7.6
C11/F5.7+CCD
Cepheid Observatory India
Vorion Scientific Observatory India
Sky Condition: Excellent
Exo-Planet Observations, Class confirmed WASP-135b Imaged/Calibration/Image solve: PRiSM v11Photometry and Data Fitting: HOPS 2.6.1/Platform: Python 3.7.6 C8/F6.3+CCD Cepheid Observatory India Vorion Scientific Observatory India Sky Condition: Excellent
Exo-Planet Observations, Class confirmed TrES-1b Imaged/Calibration/Image solve: PRiSM v11 Photometry and Data Fitting: HOPS 2.6.1/Platform: Python 3.7.6 C8/F6.3+CCD Cepheid Observatory India Vorion Scientific Observatory India Sky Condition: Excellent
Exo-Planet Observations, Class confirmed
TrES-3b
Imaged/Calibration/Image solve: PRiSM v11
Photometry and Data Fitting: HOPS 2.6.1/Platform: Python 3.7.6
C8/F6.3+CCD
Cepheid Observatory India
Vorion Scientific Observatory India
Sky Condition: Good/Full Moon
