ISOPHOT covers the largest wavelength range on ISO from 2.5 to 240 mu
m. Its scientific capabilities include multi filter and multi-aperture
photometry, polarimetry, imaging and spectrophotometry. All modes can
optionally include a focal plane chopper. The backbone of the photome
tric calibration are internal standard sources checked against celesti
al primary standards. The instrument is in excellent condition with al
l components functioning properly. There is increased detector noise d
ue to the ionizing cosmic radiation affecting the detectability of the
faintest sources. All lessons learnt from operating the instrument in
space are continuously being implemented in the standard data reducti
on software packages available to every observer. Particular strengths
of the instrument include tile detectability of very cold sources, hi
gh resolution mapping and fast spectrophotometry. The far infrared ser
endipity sky survey performed during slews of the satellite has succes
sfully started.