The documentation for GRIM II includes two different curves for filters that could be the 2.17 micron Br-gamma filter. One is dated 1987, has a peak transmission of 0.69, and a FWHM of 0.029 microns. The other is dated 1992, has a peak transmission of 0.79, and a FWHM of 0.022 microns. To determine which one is actually in the instrument, I took ratios of f/10 spectra of the dome incandescents through the 2.12, 2.17, 2.25, 2.30, and K filters. I used the lab K transmission to estimate the peak transmissions and also measured rough FWHM. Filter 2.12 2.17 2.25 2.30 K transmission (lab) 0.75 0.75 0.72 0.72 Peak transmission (this work) 0.56 0.65 0.78 0.75 Peak transmission (lab) 0.62 0.78 0.75 FWHM (this work) 0.030 0.028 0.025 0.026 FWHM (lab) 0.029 0.024 0.027 I think these measurements are most consistent with the 1987 curve, especially since my measurement of the peak transmission of the 2.12 filter is a bit lower than the lab measurement. Regards, Alan Watson APO APO APO APO APO Apache Point Observatory 3.5m APO APO APO APO APO This is message 33 in the apo35-grim archive. You can find APO the archive on http://www.astro.princeton.edu/APO/apo35-grim/INDEX.html APO To join/leave the list, send mail to apo35-request@astro.princeton.edu APO To post a message, mail it to apo35-grim@astro.princeton.edu APO APO APO APO APO APO APO APO APO APO APO APO APO APO APO APO APO