Link dedicated to the photometry of astronomical transients, AGN, Exoplanets, Nova, SN, comets and many more.
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
Exo-Planet Observations, Class confirmed
XO-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: Good
Exo-Planet Observations, Class confirmed
HAT-P-54b
Imaged/Calibration/Image solve: PRiSM v11
Photometry and Data Fitting: HOPS 2.5.6/Platform: Python 3.7.6
C11/F5.12+CCD
Cepheid Observatory India
Vorion Scientific Observatory India
Exo-Planet Observations, Class confirmed
HAT-P-12b
Imaged/Calibration/Image solve: PRiSM v11
Photometry and Data Fitting: HOPS 2.5.6/Platform: Python 3.7.6
C11/F5.12+CCD
Cepheid Observatory India
Vorion Scientific Observatory India
Exo-Planet Observations, Class confirmed Wasp-65b Imaged/Calibration/Image solve: PRiSM v11Photometry and Data Fitting: HOPS 2.5.6/Platform: Python 3.7.6C11/F5.12+CCDCepheid Observatory IndiaVorion Scientific Observatory India
Exo-Planet Observations, Class confirmed Wasp-104b Imaged/Calibration/Image solve: PRiSM v11Photometry and Data Fitting: HOPS 2.5.6/Platform: Python 3.7.6C11/F5.12+CCDSome of data could not be used for Wasp-104b during transit due to bad sky conditions.Cepheid Observatory IndiaVorion Scientific Observatory India
SN 2020jfo: Astrometry/Photometry (V/R/I)
R/ MAGNITUDE= 15.00, RA(2000) = 12h21m50.475s, DEC(2000)= +04°28’54.26”
V/ MAGNITUDE= 14.84, RA(2000) = 12h21m50.476s, DEC(2000)= +04°28’54.48”
I/ MAGNITUDE= 14.88, RA(2000) = 12h21m50.482s, DEC(2000)= +04°28’54.35”
DATE-OBS= 2020-05-07T14:54:40.87
SWCREATE= PRISMv10/ UCAC4
ORIGIN = Cepheid Observatory
OBSERVER= Agnihotri V K, K Bikash, Mahawar S, Vora K
INSTRUME= ARTEMIS CCD ATIK-383L
TELESCOP= C8/1286.0mm/208.0mm
Cepheid Observatory India
Vorion Scientific Observatory India
Adding Multiband Photometry data TCP J15472959-0532144.
Astrometry: Catalog UCAC4, J2000
RA= 15h47m29.84s DEC= -05°32’17.94”
UT 30.988 R MAGNITUDE= 13.61 ±0.10
UT 30.991 I MAGNITUDE= 13.71 ±0.10
UT 30.993 V MAGNITUDE= 13.51 ±0.09
UT 30.998 B MAGNITUDE= 13.63 ±0.23
Tele: 0.28m Schmidt–Cassegrain+CCD +Bessell BVRI
PRiSMv10
http://www.cbat.eps.harvard.edu/…/J15472959-0532144.html
Imaged: K. Vora, Vorion Scientific Observatory, AHD, India
Measured: V.K. Agnihotri, Cepheid’s Observatory RBT, India
WASP-12b, Class Exoplanet Confirmed.
Mid-time: 2456176.668258 ± 7.8e-05 BJDTDB
Period: 1.0914203 ± 1.4e-07 days
Rband Depth*: 17.35 mmag
Duration*:n3.02 hours
Teff: 6300 K, Log(g): 4.11 cm/s2, Fe/H: 0.3 dex
Rp/Rs: 0.11761006, a/Rs: 2.981
AstroImageJ 3.3.1
Cepheid Observatory India
Vorion Scientific Observatory India
