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UW-WSU Nebular Emission-Line Filters

UW-WSU Nebular Emission-Line Filters

Not on-site at APO, but can be obtained on loan--contact Jeff Morgan at UWash, morgan/astro.washington.edu


CENTER(Å) PASSBAND(Å) NEBULAR LINE (OR CONTINUUM)

4861 60 Hbeta 5007 60 [O III] 6301 10 [O I] -- [S III]6312A line is supressed 6563 10 Halpha -- [N II]6584 and 6583 lines are suppressed 6583 10 [N II] -- Halpha line is suppressed 6728 80 [S II]6717+6731 4686 60 He II 4760 100 blue cont or Fe II 8290 195 red cont. See also the Hodge filter set below. 9532 50 [S III]
The following filters are privately owned but generally available

6717*        3        [S II]  - bought for Io torus study
6731*        3        [S II]             "
5895*        5        [Na I]             "
6565**      20        part of Hodge galaxy redshifted Halpha + [N II] set
6585**      20                           "                          
6603**      20                           "                          
*Jeff Morgan
**Paul Hodge


Almost all are 3-cavity interference filters, so the passbands are very rectangular (sharp cutoffs). The peak transmissions vary, being generally highest at longer wavelengths and wider filter passbands. The narrower filters are designed to mask nearby bright nebular lines. All filters are 2x2 inches, 1/2-inch thick and cost a lot of money.

The following filters are availble when not in use locally. (Local use is generally limited to May - Sept.). Its best to request the filters two months prior to needing them.

The filters are available to loan to APO observers who request them provided that they agree to cover all costs of shipping and, if damaged, replacement. The promise to cover these costs must be signed by someone who can allocate the funds for replacement which, for the narrower filters, can exceed $1000. We ask that the filters be handled ONLY by experienced APO site personnel.


Documentation provided by Bruce Balick, balick/astro.washington.edu

APO Filters Homepage