Model SED of Uranus
The following Table contains the model SED of Uranus used for the calibration
of ISOPHOT at long wavelengths as provided by Abbas in December 1996 in
different units.
Uranus, Abbas, (see plots)
Note that the flux densities are given per unit solid angle.
Uranus' angular diameter at different dates can be found in the
Astronomical Almanac. Typical value is 3".55 (==> 2.33E-10 sr).
Model SEDs of Uranus calculated at
several dates during the ISO mission are shown in units of Janskys versus
wavelength below:
Uranus on March 30, 1996,
(plot)
Uranus on April 26, 1996,
(plot)
Uranus on October 9, 1996,
(plot)
Uranus on October 16, 1996,
(plot)
Uranus on May 21, 1997,
(plot)
Model SED of Neptune
The following Tables contain model SED for Neptune used for the calibration
of ISOPHOT at long wavelengths as provided by Abbas in December 1996 for
several dates during the ISO mission:
Neptune on March 30, 1996,
(plot)
Neptune on April 19, 1996,
(plot)
Neptune on October 9, 1996,
(plot)
Neptune on October 16, 1996,
(plot)
Neptune on November 6, 1996,
(plot)
Neptune on March 26, 1997,
(plot)
Neptune on May 13, 1997,
(plot)
Last update: 11-07-2000 by
Pedro Garcia-Lario