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COBE

DIRBE Small Source Spectral Energy Distributions


This interactive service permits browsing of the DIRBE data for preliminary investigations of potential point sources. Definitive studies of DIRBE point sources should be conducted using the DIRBE Point Source Photometry Research Tool, which extracts photometry from the time-ordered data (see section 5.6.6 of the DIRBE Explanatory Supplement). Given an on-source position and offsets for reference positions, this service displays the on-source, average off-source, and difference intensities for the DIRBE wavelength range, 1.25-240 microns. A brief explanation of this form is available.

Enter the coordinates and select the system and epoch of the position of interest. For the reference positions, specify the angular offsets, the directions, and the system. The integral flux will be estimated for the wavelength integration range specified.

On-source position
(e.g., 10h16m24s or 10.273)
(e.g., -25d19m34s or -25.33)
 
-or-
(e.g., NGC 7538)


Reference positions
Offset directions: (select at least two directions)
(decimal degrees)

Integration range
(microns, >= 1.25)
(microns, <= 240)
A service of the HEASARC and of the Astrophysics Science Division at NASA/GSFC
Goddard Space Flight Center, National Aeronautics and Space Administration
HEASARC Director: Dr. Alan P. Smale
LAMBDA Director: Dr. Eric R. Switzer
NASA Official: Dr. Eric R. Switzer
Web Curator: Mr. Michael R. Greason