Instrument Sheet Baja Observatory

GROUND BASED NETWORK BAJA OBSERVATORY The Baja Observatory was firstly established in 1955, during the reconstruction after the Second World War, by an amateur astronomer, Mihály Borbás. The observatory is now operated by the University of Szeged. It is primarily used for astronomical research and education. Since 2010, they measure the night sky brightness with an SQM instrument. TYPE OF INSTRUMENT Sky-Quality Meter N° OF STATIONS 1 LOCATION Baja, Hungary COORDINATES 46.18028 °N, 19.01093 °E, 110 m MEASUREMENT POINT Rural area,
Astronomical observatory STATUS Operational DATA AVAILABILITY Yes, freely available TIME RANGE Since 2010 FREQUENCY OF MEASUREMENT Every minute DATA PUBLISHING FREQUENCY Daily DATA PUBLISHING DELAY None OWNER Bajai Obszervatórium and  Szegedi Tudományegyetem MORE INFORMATION CALIBRATED DATA Yes MEASUREMENT UNIT mag/arcsec² WAVELENGTH RANGE 350 – 700 nm FIELD-OF-VIEW ± 20 deg POINTING DIRECTION Zenith DATA VISUALISATION Yes DATA DOWNLOAD Yes DATA FORMAT CSV DATA POLICY Not specified CONTACTS Bajai Obszervatórium FURTHER REFERENCESData of the meteorological station at the Baja Observatory
– Baja Observatory Foundation This repository is managed by INAF as part of the Interreg Central Europe project DARKERSKY4CE, co-funded by the European Union. The views and opinions expressed herein are those of the authors and do not necessarily reflect those of the European Commission. Whilst INAF takes every precaution to ensure that the content is accurate, INAF cannot guarantee that all information or data on the website is correct. Therefore, INAF accepts no responsibility or liability whatsoever with regard to the information or data on the website or for any use which may be made of it.