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Nouveau transit
10/10/2026
HATS-33 b
16
Eduardo Fernández Lajús, Complejo Astronomico El Leoncito, Argentina, 10/10/2026
0.60 m "Helen Sawyer Hogg" (HSH) Telescope + SBIG STL 1001-E CCD Camera
. . .
Nouvelle observation
10/10/2026
HATS-33
15
Eduardo Fernández Lajús, Complejo Astronomico El Leoncito, Argentina, 09/10/2026
0.60 m "Helen Sawyer Hogg" (HSH) Telescope + SBIG STL 1001-E CCD Camera
. . .
Nouveau minimum
10/10/2026
RT And
44
Albert Smith, Chiefland Astronomy Village. Bortle 3., 17/01/2026
Same as above
. . .
Nouvelle observation
09/10/2026
RT And
44
Albert Smith, Chiefland Astronomy Village. Bortle 3., 16/01/2026
Same as above
. . .
Nouvelle observation
09/10/2026
FZ Ori
18
Albert Smith, Chiefland Astronomy Village. Bortle 3., 28/01/2026
Same as above
. . .
Nouvelle observation
09/10/2026
XO-6
79
Manfred Raetz, Privatsternwarte Herges-Hallenberg, 03/10/2026
SCT 280 / 1870 (C11 with Starizona reducer) CCD: MII G2-1600 filter : Astrodon ExoPlanet-BB (V to IR)
. . .
Nouvelle observation
09/10/2026
UU Aqr
5
Boaz Ron Zohar And David Pundak, Kinneret Observatory, Israel 32.7125 N, 35.5000 E, 10/09/2026
0.28-m f/2.2 RASA 11 (Bareket Astro) + QHY one-shot colour, 3.76 um
Observed at Kinneret Observatory with a one-shot colour camera; the red channel of the Bayer matrix, untransformed, hence TR.
Differential magnitudes, instrumental zero point (target minus an ensemble of 9 comparison stars).
A field star falls in the target's sky annulus; the annulus was narrowed to 10.1-16.2 px to exclude it.
Observed at Kinneret Observatory with a one-shot colour camera; the red channel of the Bayer matrix, untransformed, hence TR.
Differential magnitudes, instrumental zero point (target minus an ensemble of 9 comparison stars).
A field star falls in the target's sky annulus; the annulus was narrowed to 10.1-16.2 px to exclude it.
. . .
Nouvelle observation
09/10/2026
UU Aqr
5
Boaz Ron Zohar And David Pundak, Kinneret Observatory, Israel 32.7125 N, 35.5000 E, 10/09/2026
0.28-m f/2.2 RASA 11 (Bareket Astro) + QHY one-shot colour, 3.76 um
Observed at Kinneret Observatory with a one-shot colour camera; the green channel of the Bayer matrix, untransformed, hence TV.
Differential magnitudes, instrumental zero point (target minus an ensemble of 9 comparison stars).
A field star falls in the target's sky annulus; the annulus was narrowed to 10.1-16.2 px to exclude it.
Observed at Kinneret Observatory with a one-shot colour camera; the green channel of the Bayer matrix, untransformed, hence TV.
Differential magnitudes, instrumental zero point (target minus an ensemble of 9 comparison stars).
A field star falls in the target's sky annulus; the annulus was narrowed to 10.1-16.2 px to exclude it.
. . .
Nouvelle observation
09/10/2026
UU Aqr
5
Boaz Ron Zohar And David Pundak, Kinneret Observatory, Israel 32.7125 N, 35.5000 E, 10/09/2026
0.28-m f/2.2 RASA 11 (Bareket Astro) + QHY one-shot colour, 3.76 um
Observed at Kinneret Observatory with a one-shot colour camera; the blue channel of the Bayer matrix, untransformed, hence TB.
Differential magnitudes, instrumental zero point (target minus an ensemble of 9 comparison stars).
A field star falls in the target's sky annulus; the annulus was narrowed to 10.1-16.2 px to exclude it.
Observed at Kinneret Observatory with a one-shot colour camera; the blue channel of the Bayer matrix, untransformed, hence TB.
Differential magnitudes, instrumental zero point (target minus an ensemble of 9 comparison stars).
A field star falls in the target's sky annulus; the annulus was narrowed to 10.1-16.2 px to exclude it.
. . .
0.28-m f/2.2 RASA 11 (Bareket Astro) + QHY one-shot colour, 3.76 um
Observed at Kinneret Observatory with a one-shot colour camera; the red channel of the Bayer matrix, used as an approximation to Johnson R. No colour transformation was applied.
Differential magnitudes, instrumental zero point (target minus an ensemble of 12 comparison stars).
A companion 11.8 px from the target contributes light inside the aperture, so the measured depth is diluted and is a lower limit.
In this channel the target's smooth variation is only 1.3 times that of the comparison stars, so the dip is not established here; the curve is published as data, not as a detection.
A field star falls in the target's sky annulus; the annulus was widened to 26.3-29.7 px to exclude it.
The meridian flip falls inside the series; 5 frames were taken after it.
Observed at Kinneret Observatory with a one-shot colour camera; the red channel of the Bayer matrix, used as an approximation to Johnson R. No colour transformation was applied.
Differential magnitudes, instrumental zero point (target minus an ensemble of 12 comparison stars).
A companion 11.8 px from the target contributes light inside the aperture, so the measured depth is diluted and is a lower limit.
In this channel the target's smooth variation is only 1.3 times that of the comparison stars, so the dip is not established here; the curve is published as data, not as a detection.
A field star falls in the target's sky annulus; the annulus was widened to 26.3-29.7 px to exclude it.
The meridian flip falls inside the series; 5 frames were taken after it.
. . .
0.28-m f/2.2 RASA 11 (Bareket Astro) + QHY one-shot colour, 3.76 um
Observed at Kinneret Observatory with a one-shot colour camera; the blue channel of the Bayer matrix, used as an approximation to Johnson B. No colour transformation was applied.
Differential magnitudes, instrumental zero point (target minus an ensemble of 4 comparison stars).
A companion 11.8 px from the target contributes light inside the aperture, so the measured depth is diluted and is a lower limit.
No baseline after the dip - the series ends before the star returns to its out-of-eclipse level, so the mid-time is not determined.
A field star falls in the target's sky annulus; the annulus was widened to 26.3-29.7 px to exclude it.
The meridian flip falls inside the series; 5 frames were taken after it.
Observed at Kinneret Observatory with a one-shot colour camera; the blue channel of the Bayer matrix, used as an approximation to Johnson B. No colour transformation was applied.
Differential magnitudes, instrumental zero point (target minus an ensemble of 4 comparison stars).
A companion 11.8 px from the target contributes light inside the aperture, so the measured depth is diluted and is a lower limit.
No baseline after the dip - the series ends before the star returns to its out-of-eclipse level, so the mid-time is not determined.
A field star falls in the target's sky annulus; the annulus was widened to 26.3-29.7 px to exclude it.
The meridian flip falls inside the series; 5 frames were taken after it.
. . .
0.28-m f/2.2 RASA 11 (Bareket Astro) + QHY one-shot colour, 3.76 um
Observed at Kinneret Observatory with a one-shot colour camera; the green channel of the Bayer matrix, used as an approximation to Johnson V. No colour transformation was applied.
Differential magnitudes, instrumental zero point (target minus an ensemble of 8 comparison stars).
A companion 11.8 px from the target contributes light inside the aperture, so the measured depth is diluted and is a lower limit.
A field star falls in the target's sky annulus; the annulus was widened to 26.3-29.7 px to exclude it.
The meridian flip falls inside the series; 5 frames were taken after it.
Observed at Kinneret Observatory with a one-shot colour camera; the green channel of the Bayer matrix, used as an approximation to Johnson V. No colour transformation was applied.
Differential magnitudes, instrumental zero point (target minus an ensemble of 8 comparison stars).
A companion 11.8 px from the target contributes light inside the aperture, so the measured depth is diluted and is a lower limit.
A field star falls in the target's sky annulus; the annulus was widened to 26.3-29.7 px to exclude it.
The meridian flip falls inside the series; 5 frames were taken after it.
. . .
0.28-m f/2.2 RASA 11 (Bareket Astro) + QHY one-shot colour, 3.76 um
Observed at Kinneret Observatory with a one-shot colour camera; the red channel of the Bayer matrix, used as an approximation to Johnson R. No colour transformation was applied.
Differential magnitudes, instrumental zero point (target minus an ensemble of 4 comparison stars).
A field star falls in the target's sky annulus; the annulus was widened to 26.9-30.7 px to exclude it.
Observed at Kinneret Observatory with a one-shot colour camera; the red channel of the Bayer matrix, used as an approximation to Johnson R. No colour transformation was applied.
Differential magnitudes, instrumental zero point (target minus an ensemble of 4 comparison stars).
A field star falls in the target's sky annulus; the annulus was widened to 26.9-30.7 px to exclude it.
. . .
0.28-m f/2.2 RASA 11 (Bareket Astro) + QHY one-shot colour, 3.76 um
Observed at Kinneret Observatory with a one-shot colour camera; the green channel of the Bayer matrix, used as an approximation to Johnson V. No colour transformation was applied.
Differential magnitudes, instrumental zero point (target minus an ensemble of 12 comparison stars).
A field star falls in the target's sky annulus; the annulus was widened to 26.9-30.7 px to exclude it.
The star field chart shows the channel R selection; the comparison stars are chosen per channel and differ slightly in G.
Observed at Kinneret Observatory with a one-shot colour camera; the green channel of the Bayer matrix, used as an approximation to Johnson V. No colour transformation was applied.
Differential magnitudes, instrumental zero point (target minus an ensemble of 12 comparison stars).
A field star falls in the target's sky annulus; the annulus was widened to 26.9-30.7 px to exclude it.
The star field chart shows the channel R selection; the comparison stars are chosen per channel and differ slightly in G.
. . .
0.28-m f/2.2 RASA 11 (Bareket Astro) + QHY one-shot colour, 3.76 um
Observed at Kinneret Observatory with a one-shot colour camera; the blue channel of the Bayer matrix, untransformed, hence TB.
Differential magnitudes, instrumental zero point (target minus an ensemble of 11 comparison stars).
A field star falls in the target's sky annulus; the annulus was widened to 26.9-30.7 px to exclude it.
The star field chart shows the channel R selection; the comparison stars are chosen per channel and differ slightly in B.
Observed at Kinneret Observatory with a one-shot colour camera; the blue channel of the Bayer matrix, untransformed, hence TB.
Differential magnitudes, instrumental zero point (target minus an ensemble of 11 comparison stars).
A field star falls in the target's sky annulus; the annulus was widened to 26.9-30.7 px to exclude it.
The star field chart shows the channel R selection; the comparison stars are chosen per channel and differ slightly in B.
. . .
Nouvelle observation
09/10/2026
WASP-52
248
Boaz Ron Zohar, LCO Sutherland (CPT), SAAO, South Africa 32.3806 S, 20.8099 E, 1760 m, 24/08/2026
0.35-m f/3 PlaneWave Delta Rho + QHY600 (0m4-16, sq45)
Observed with the LCO 0.4-m network (Global Sky Partners).
Differential magnitudes, instrumental zero point (target minus an ensemble of 11 comparison stars).
Full transit covered, with 40 min of baseline before ingress and 16 min after egress.
Observed with the LCO 0.4-m network (Global Sky Partners).
Differential magnitudes, instrumental zero point (target minus an ensemble of 11 comparison stars).
Full transit covered, with 40 min of baseline before ingress and 16 min after egress.
. . .
Nouvelle observation
09/10/2026
RW Tri
10
Boaz Ron Zohar, LCO Teide (TFN), Tenerife 28.3003 N, 16.5117 W, 2390 m, 02/10/2026
0.35-m f/3 PlaneWave Delta Rho + QHY600
Observed with the LCO 0.4-m network (Global Sky Partners). Ingress not covered - the series begins inside the eclipse.
Differential magnitudes, instrumental zero point
(target minus an ensemble of 12 comparison stars)
Egress complete, so the depth is a lower limit.
Observed with the LCO 0.4-m network (Global Sky Partners). Ingress not covered - the series begins inside the eclipse.
Differential magnitudes, instrumental zero point
(target minus an ensemble of 12 comparison stars)
Egress complete, so the depth is a lower limit.
. . .
Nouveau minimum
09/10/2026
ER Ori
20
Albert Smith, Chiefland Astronomy Village. Bortle 3., 03/02/2026
Seestar S50.
. . .
Nouvelle observation
09/10/2026
ER Ori
20
Albert Smith, Chiefland Astronomy Village. Bortle 3., 03/02/2026
Seestar S50.
. . .
Nouvelle observation
08/10/2026
WASP-148
9
Manfred Raetz, Privatsternwarte Herges-Hallenberg, 09/05/2022
SCT 280 / 1870 (C11 with Starizona reducer) CCD: MII G2-1600 filter : Astrodon ExoPlanet-BB (V to IR)
. . .
Nouvelle observation
08/10/2026
V1179 Cas
94
Ladislav Šmelcer, Hvězdárna Valašské Meziříčí, 07/10/2026
Newton 500 + C4 16000
. . .
Nouvelle observation
08/10/2026
V1178 Cas
49
Ladislav Šmelcer, Hvězdárna Valašské Meziříčí, 07/10/2026
Newton 500 + C4 16000
. . .
Nouvelle observation
08/10/2026
CzeV1456
117
Ladislav Šmelcer, Hvězdárna Valašské Meziříčí, 07/10/2026
Newton 500 + C4 16000
. . .
Nouvelle observation
08/10/2026
CzeV837
160
Ladislav Šmelcer, Hvězdárna Valašské Meziříčí, 07/10/2026
Newton 500 + C4 16000
. . .
Nouvelle observation
08/10/2026
CzeV772
228
Ladislav Šmelcer, Hvězdárna Valašské Meziříčí, 07/10/2026
Newton 500 + C4 16000
. . .
Nouvelle observation
08/10/2026
CzeV590
309
Ladislav Šmelcer, Hvězdárna Valašské Meziříčí, 07/10/2026
Newton 500 + C4 16000
. . .