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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.
. . .
0.40-m f/5 + CCD ST7 + R
# NAME V 706 Cyg
# VAR 21:35:56.0 +40:50:48 2452137.4072 0.46625592 13.2-14.6 (BRKA 2005)
# OBS Martin Lehky (Hradec Kralove CZ; 0.40-m f/5 reflector + CCD ST7)
# FLT R
# RED CMunipack 1.1.18 + AVE 2.51
# NOTE 16/17 VII 2007; R_230_60s (103/37); minimum P
# NOTE 2454298.48706 +/- 0.00012; 20070716 23:41:22 (UT) GEO
# COND clear weather
# NAME V 706 Cyg
# VAR 21:35:56.0 +40:50:48 2452137.4072 0.46625592 13.2-14.6 (BRKA 2005)
# OBS Martin Lehky (Hradec Kralove CZ; 0.40-m f/5 reflector + CCD ST7)
# FLT R
# RED CMunipack 1.1.18 + AVE 2.51
# NOTE 16/17 VII 2007; R_230_60s (103/37); minimum P
# NOTE 2454298.48706 +/- 0.00012; 20070716 23:41:22 (UT) GEO
# COND clear weather
. . .
0.40-m f/5 + CCD ST7 + R
# NAME V 706 Cyg
# VAR 21:35:56.0 +40:50:48 2452137.4072 0.46625592 13.2-14.6 (BRKA 2005)
# OBS Martin Lehky (Hradec Kralove CZ; 0.40-m f/5 reflector + CCD ST7)
# FLT R
# RED CMunipack 1.1.18 + AVE 2.51
# NOTE 16/17 VII 2007; R_230_60s (103/37); minimum P
# NOTE 2454298.48706 +/- 0.00012; 20070716 23:41:22 (UT) GEO
# COND clear weather
# NAME V 706 Cyg
# VAR 21:35:56.0 +40:50:48 2452137.4072 0.46625592 13.2-14.6 (BRKA 2005)
# OBS Martin Lehky (Hradec Kralove CZ; 0.40-m f/5 reflector + CCD ST7)
# FLT R
# RED CMunipack 1.1.18 + AVE 2.51
# NOTE 16/17 VII 2007; R_230_60s (103/37); minimum P
# NOTE 2454298.48706 +/- 0.00012; 20070716 23:41:22 (UT) GEO
# COND clear weather
. . .