  Since 2016, the HI-MaNGA survey has been obtaining neutral hydrogen (which
emits a radio 21cm line) measurements for nearby galaxies which are part of a
survey known as "MaNGA". This has been done using observations at the Green
Bank Radio Telescope (GBT). We use calibration data obtained routinely at the
start of observing runs during this entire period, as well as an extra set of
calibration data obtained in 2019 to check the standard GBT data reduction
calibrations at L-band (1.4 GHz, or 20cm). We find an constant offset of 20% in
the calibration relative to the standard values given in the GBT data reduction
pipeline for data of this type. This correction will be used to improve
measurements for HI-MaNGA.
