Coming Soon
PI's will be able to utilize the LMT SLR (Spectral Line Reduction) tool through an online interface. This will allow users to reduce the data using the tool to their own specifications.
A video explaining the format of the TAPS pages of data collected using the RSR instrument.
An interactive Jupyter notebook showing how to load in and work with RSR data downloaded from the Archive or TAPS pages.
A memo produced by Dr. Min Yun (2020) describing the process of calculating a frequency-dependent gain from RSR data.
A video explaining the format of the TAPS pages of data collected using the SEQ instrument.
Within this report, Fig. 8 (shown below) gives the standard values for Aperture Efficiency, Main Beam efficiency, and Gain for the LMT at various frequencies. Though this report covers the entire telescope, we highlight data in this table as they are the standard values used when calibrating SEQ data.
If used, please cite the above report (Hughes et. al. (2020)).