ISOPHOT Project
at the Max-Planck-Institut für Astronomie


What is ISOPHOT?

ISOPHOT is one of the four focal plane instruments (ISOPHOT, ISOCAM, LWS, SWS) of the European Space Agency (ESA)'s Infrared Space Observatory (ISO). ISO was the first versatile infrared space observatory, allowing diffraction limited imaging and spectroscopy and it opened a new wavelength region in the far infrared (110…240 µm). ISO was cooled by 2300 litres of superfluid helium to a temperature near absolute zero (-273°C). It achieved a sensitivity 100 times better than the exploring IRAS-mission in the year 1983. ISO's scientific goals were the exploration of the cold and dust hidden universe as well as the spectroscopic analysis of the interstellar and circumstellar matter.

ISOPHOT is an imaging photopolarimeter for the wavelength range 2.5 ... 240 µm and includes a low-resolution spectrometer for the 2.5 ... 12 µm range. ISO was launched on 17 November 1995 into a highly excentric 24h orbit with an apogee at 70 000 km well outside the earth's radiation belts. The mission ended on 08 April 1998; data were gained for 29 months, 11 months longer than originally predicted. More information on the mission is found on the ISO facts page of ESA.
ISOPHOT was designed and built by a consortium of various science institutes and industrial enterprises in Europe under the leadership of the Principal Investigator (PI), Prof. Dietrich Lemke at the Max-Planck-Institut für Astronomie (MPIA). For more information on the ISOPHOT instrument, its observing modes, the calibration, the data reduction and the data products see The ISO Handbook, Volume IV: PHT - The Imaging Photo-Polarimeter.

The observations ranged from comets and dust in the solar system to deep surveys of galaxies in the young universe. In April 2002, i.e. 4 years after the end of the ISO-mission about 30% of the scientific data obtained had been reduced. This resulted in 770 papers in journals with referee system and more than 1000 conference contributions. More scientific impact from the huge data base can be expected within the next few years by "archive observations" during "ISO's Active Archive Phase". ISO's Legacy Archive is open to all astronomers.

MPIA delivered the ISOPHOT-Instrument to Europe's ISO-Satellite.


What is the ISOPHOT Data Centre?

The ISOPHOT Data Centre was set up on the campus of MPIA to optimise the scientific return of ISOPHOT. It is one of a group of specialised data centres for ISO. (Have a look at the aerial photograph of MPIA.) Under the leadership of the Principal Investigator, Dietrich Lemke and the management of Ulrich Klaas the team's main tasks are:

  • Support of the astronomical community in the analysis and interpretation of ISOPHOT data. Guest users of the centre's facilities are always welcome. Please contact phthelp@mpia.de
  • Scientific analysis of ISO observing programmes and follow-up observations in the optical and submm (Publication lists). Main topics are:
    • Composition of the interstellar medium, the early phases of star formation.
    • The energy mechanisms in starburst galaxies and the unified scheme of quasars and radio galaxies.
    • Evaluation of the ISOPHOT Serendipitous Sky Survey at 170 micron (new astrophysical window) and the extraction of more than thousand very cold galaxies and hundreds of cold clouds in our galaxy.
    • Infrared Background Project (zodiacal light, structure and colours of the galactic infrared cirrus, the cosmic far infrared background and the earliest stages of galaxy formation).
  • ISOPHOT Interactive Analysis (PIA) software: contribution in development, testing, documentation and user support.
  • Archiving of all ISOPHOT data: more than 15000 pointed observations and more than 12000 slew observations of the ISOPHOT Serendipity Survey.
  • Improved calibration of the ISOPHOT data products (28 observing modes).
  • Scientific validation and upgrades of the ISOPHOT automatic data reduction pipeline software in collaboration with the UK ISO Data Centre at RAL.

The ISOPHOT data centre continuously offers research opportunities for postdocs, for students to work on their physics diploma or Ph.D. making use of the unique ISO-misssion data base.
 
Slews of 150000 degree total lengths were gained "free of cost" during the
serendipity survey. They contain about 3000 galaxies.

 


ISOPHOT Team at MPIA (phthelp@mpia.de)
Last modified: September 16, 2002