RC 203 mm + TS 0.67x reducer (f/5.6), IMX571 mono, Baader Sloan filters
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this secondary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461312.37257 +- 0.00195 d.
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this secondary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461312.37257 +- 0.00195 d.
. . .
RC 203 mm + TS 0.67x reducer (f/5.6), IMX571 mono, Baader Sloan filters
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this secondary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461312.37565 +- 0.00174 d.
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this secondary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461312.37565 +- 0.00174 d.
. . .
RC 203 mm + TS 0.67x reducer (f/5.6), IMX571 mono, Baader Sloan filters
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this secondary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461312.37565 +- 0.00174 d.
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this secondary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461312.37565 +- 0.00174 d.
. . .
RC 203 mm + TS 0.67x reducer (f/5.6), IMX571 mono, Baader Sloan filters
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this secondary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461312.37257 +- 0.00195 d.
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this secondary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461312.37257 +- 0.00195 d.
. . .
RC 203 mm + TS 0.67x reducer (f/5.6), IMX571 mono, Baader Sloan filters
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this secondary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461312.37257 +- 0.00195 d.
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this secondary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461312.37257 +- 0.00195 d.
. . .
RC 203 mm + TS 0.67x reducer (f/5.6), IMX571 mono, Baader Sloan filters
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this primary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461311.37586 +- 0.00153 d.
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this primary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461311.37586 +- 0.00153 d.
. . .
RC 203 mm + TS 0.67x reducer (f/5.6), IMX571 mono, Baader Sloan filters
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this primary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461311.37586 +- 0.00153 d.
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this primary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461311.37586 +- 0.00153 d.
. . .
RC 203 mm + TS 0.67x reducer (f/5.6), IMX571 mono, Baader Sloan filters
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this secondary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461310.38175 +- 0.00222 d.
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this secondary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461310.38175 +- 0.00222 d.
. . .
RC 203 mm + TS 0.67x reducer (f/5.6), IMX571 mono, Baader Sloan filters
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this secondary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461310.38175 +- 0.00222 d.
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this secondary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461310.38175 +- 0.00222 d.
. . .
RC 203 mm + TS 0.67x reducer (f/5.6), IMX571 mono, Baader Sloan filters
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this secondary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461310.37802 +- 0.00168 d.
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this secondary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461310.37802 +- 0.00168 d.
. . .
RC 203 mm + TS 0.67x reducer (f/5.6), IMX571 mono, Baader Sloan filters
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this secondary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461310.37802 +- 0.00168 d.
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this secondary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461310.37802 +- 0.00168 d.
. . .
RC 203 mm + TS 0.67x reducer (f/5.6), IMX571 mono, Baader Sloan filters
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this secondary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461288.47481 +- 0.00180 d.
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this secondary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461288.47481 +- 0.00180 d.
. . .
RC 203 mm + TS 0.67x reducer (f/5.6), IMX571 mono, Baader Sloan filters
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this secondary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461288.47481 +- 0.00180 d.
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this secondary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461288.47481 +- 0.00180 d.
. . .
RC 203 mm + TS 0.67x reducer (f/5.6), IMX571 mono, Baader Sloan filters
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this secondary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461288.47423 +- 0.00159 d.
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this secondary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461288.47423 +- 0.00159 d.
. . .
RC 203 mm + TS 0.67x reducer (f/5.6), IMX571 mono, Baader Sloan filters
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this secondary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461288.47423 +- 0.00159 d.
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this secondary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461288.47423 +- 0.00159 d.
. . .
RC 203 mm + TS 0.67x reducer (f/5.6), IMX571 mono, Baader Sloan filters
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this primary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461311.37745 +- 0.00164 d.
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this primary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461311.37745 +- 0.00164 d.
. . .
RC 203 mm + TS 0.67x reducer (f/5.6), IMX571 mono, Baader Sloan filters
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this primary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461311.37745 +- 0.00164 d.
Forced aperture photometry (position from WCS) on co-added runs of 2-3 x 10 s frames; ensemble of ~150 Gaia DR3 GSPC comparison stars (synthetic SDSS). Untransformed. Absolute level uncertain by ~0.05-0.1 mag (position-dependent illumination correction outdated); timing unaffected. Our own fit of this primary minimum (symmetric polynomial, bootstrap errors): BJD_TDB 2461311.37745 +- 0.00164 d.
. . .
New transit
10/1/2026
HAT-P-37 b
166
Marc Bretton, UAI B10 Baronnies Provencales Observatory, 10/4/2014
RC 82 cm - CCD FLI PL230
GENERATED FROM TRANSIT id=3379
GENERATED FROM TRANSIT id=3379
. . .
New transit
10/1/2026
HAT-P-37 b
166
AAAV Astrofili Valdera, Oss Astr G.Galilei-Libbiano Mpc code B33 , 8/11/2014
RC 500 f/6 + CCD FLI Kodak KAF 1001E
GENERATED FROM TRANSIT id=3272
GENERATED FROM TRANSIT id=3272
. . .
New transit
10/1/2026
HAT-P-37 b
166
AAAV Astrofili Valdera, Oss Astr G.Galilei-Libbiano Mpc code B33 , 8/25/2014
RC 500 f/6 + CCD FLI Kodak KAF 1001E
GENERATED FROM TRANSIT id=3298
GENERATED FROM TRANSIT id=3298
. . .
New transit
10/1/2026
HAT-P-37 b
166
AAAV Astrofili Valdera, Oss Astr G.Galilei-Libbiano Mpc code B33 , 9/5/2021
RC 500 f/6 + CCD FLI PROLINE 4710
GENERATED FROM TRANSIT id=9001
GENERATED FROM TRANSIT id=9001
. . .
New minimum
10/1/2026
CzeV1247
5
Filip Walter, Štefánik Observatory, Prague, Czech Republic, 11/4/2017
MARK SCT 406/4060, SBIG ST10XME
V1_ST10_90C2_-10C
V1_ST10_90C2_-10C
. . .
Celestron C14 (SCT 356/3910) + red. 0,7x + SBIG ST9XE
Adopted limb darkening: 0.5 | EXP. 90s | binning 1+1 | FWHM 2.1 px (3.5 arc-sec/pixel) | slight defocus | weather: clear, moisture | bortle 5, encircling light pollution | Photometric aperture radii: 6-12-15 | Moon illumination: 86.4%, distance: 27°
Adopted limb darkening: 0.5 | EXP. 90s | binning 1+1 | FWHM 2.1 px (3.5 arc-sec/pixel) | slight defocus | weather: clear, moisture | bortle 5, encircling light pollution | Photometric aperture radii: 6-12-15 | Moon illumination: 86.4%, distance: 27°
. . .