GMOS South Filters

The GMOS filters u', g', r', i' and z' are similar to the filters used by the Sloan Digital Sky Survey (SDSS). A description of the SDSS photometric system is presented in Fukugita et al. (1996, AJ, 111, 1748). See the description of optical photometric standard stars for details on the photometric standard calibration.

The filter CaT is a 150nm broad-band filter approximately centered on the Ca Triplet.

The filters Ha, HaC, OIII, OIIIC and SII are narrow-band filters for H-alpha, H-alpha continuum, ionized oxygen, ionized oxygen continuum and ionized sulphur, respectively.

The filters GG455, OG515, RG610 and RG780 are 5mm thick Schott glass filters. These are long-pass filters which can be used to block 2nd-order contamination of the spectra or limit the wavelength range to allow multiple slit-banks in the multi-aperture mode.

Transmission curves based on lab measurements are available for the filters.

The table list the properties of the filters based on laboratory measurements. The wavelength interval given in the tables is the interval within which the transmission is larger than 50 per cent. For the long-pass filters and the filter z_G0328 the wavelength at the 50 per cent transmission at short wavelength edge is given.

Some of the filters can be combined; the allowed combinations are listed last in the table.

Imaging with GMOS requires use of a color filter (ugriz, CaT) or a narrow band filter. The long-pass filters GG455, OG515, RG610 and RG780 are not suitable for imaging. Also imaging without a filter is not available.

Users may supply their own filters for queue observations; see filter policy and specifications for details.

Last update October 04, 2005; Rodrigo Carrasco