For historical reasons the AOT numbers are not consecutive. The first column gives the AOT identifier, the second the AOT title and the third column gives the restriction for the AOT if applied to observations of solar system targets (`not applicable' means that this AOT may not be used for solar system observations, `single pointing' means that no raster maps may be performed, `staring' means that the chopper may not be used and `one entrance aperture' in the case for SWS AOTs means that change of wavelength is not allowed when it involves an automatic change of the entrance aperture.
AOT AOT Title Solar System
CAM01 General Observation single pointing
CAM03 Beam Switching not applicable
CAM04 Spectral Observations single pointing
CAM05* Polarisation single pointing
LWS01 Grating Wavelength Range Spectrum single pointing
LWS02 Grating Line Spectra single pointing
LWS03 Fabry-Pérot Wavelength Range Spectrum single pointing
LWS04 Fabry-Pérot Line Spectra single pointing
PHT03 General Multi-filter Photometry with PHT-P single pointing, staring
PHT04 General Multi-aperture Photometry with PHT-P single pointing, staring
PHT05 Absolute Photometry with PHT-P staring
PHT17 Sparse Map with PHT-P (start AOT) not applicable
PHT18 Sparse Map with PHT-P (intermediate AOT(s)) not applicable
PHT19 Sparse Map with PHT-P (end AOT) not applicable
PHT22 Multi-filter Photometry with PHT-C staring
PHT25 Absolute Photometry with PHT-C single pointing, staring
PHT32 Multi-filter Map / Linear Scan with PHT-C not applicable
PHT37 Sparse Map with PHT-C (start AOT) not applicable
PHT38 Sparse Map with PHT-C (intermediate AOTs) not applicable
PHT39 Sparse Map with PHT-C (end AOT) not applicable
PHT40 Spectrophotometry with PHT-S single pointing, staring
PHT50* Single Filter Polarimetry with PHT-P
single pointing, staring
PHT51* Single Filter Polarimetry with PHT-C
single pointing, staring
SWS01 Low-Resolution Full Grating Scan one entrance aperture
SWS02 Grating Line Profile Scan one entrance aperture
SWS06 Grating Scan one entrance aperture
SWS07 Combined Fabry-Pérot Line Scan and SW Grating Scan one entrance
aperture
* Polarisation observations with ISOCAM and ISOPHOT will be implemented in operations by a different route than that for the standard ``AOT-based'' observing modes; from the point of view of proposers, there will be no difference in the procedure to enter polarisation observations until after the end of the Phase 1 review by OTAC.