From the Bochum Galactic Disk Survey, time series have been obtained in the
r and i bands on an (up to) nightly basis. Depending on the field, the time
series contain up to more than 300 nights over 9 years. Each measurement in
r and i represents the averaged flux over 10 minutes of observation
(from 9 averaged 10s images). Additionally, intermittent measurements
in Johnson UVB, Sloan z and the narrowbands OIII, NB, Halpha and SII
have been recorded as well.
The Bochum Galactic Disk Survey is a project to monitor the stellar content
of the Galactic disk in a 6 degree wide stripe centered on the Galactic
plane. The data has been recorded from September 2010 to September 2019 in
Sloan r and i simultaneously with the Robotic Bochum Twin Telescope (RoBoTT)
at the Universitaetssternwarte Bochum near Cerro Armazones in the Chilean
Atacama desert. It contains measurements of about 2x10^7 stars over nine
years.
The source images are available from ivo://org.gavo.dc/bgds/q/sia.
Bochum Galactic Disk Survey (BGDS) DR2 light curves browser service
From the Bochum Galactic Disk Survey, time series have been obtained in the
r and i bands on an (up to) nightly basis. Depending on the field, the time
series contain up to more than 300 nights over 9 years. Each measurement in
r and i represents the averaged flux over 10 minutes of observation
(from 9 averaged 10s images). Additionally, intermittent measurements
in Johnson UVB, Sloan z and the narrowbands OIII, NB, Halpha and SII
have been recorded as well.
The Bochum Galactic Disk Survey is a project to monitor the stellar content
of the Galactic disk in a 6 degree wide stripe centered on the Galactic
plane. The data has been recorded from September 2010 to September 2019 in
Sloan r and i simultaneously with the Robotic Bochum Twin Telescope (RoBoTT)
at the Universitaetssternwarte Bochum near Cerro Armazones in the Chilean
Atacama desert. It contains measurements of about 2x10^7 stars over nine
years.
The source images are available from ivo://org.gavo.dc/bgds/q/sia.
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