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IR Compendium: M87 |
| Wavelength (microns) | Flux (Janskys) | Reference |
|---|---|---|
| 1.235 | 3.27 | Jarrett et al, 2003, AJ, 125, 525. |
| 1.662 | 3.81 | Jarrett et al, 2003, AJ, 125, 525. |
| 2.159 | 3.17 | Jarrett et al, 2003, AJ, 125, 525. |
| 10 | 3.00e-2 | Rieke et al, 1978, ApJ, 220, 37. |
| 10.5 | 6.00e-2 | Rieke et al, 1972, ApJ, 176, 95. |
| 12 | 2.19e-1 | Golombek et al, 1988, AJ, 95, 26. |
| 25 | 1.87e-1 | Golombek et al, 1988, AJ, 95, 26. |
| 60 | 5.46e-1 | Golombek et al, 1988, AJ, 95, 26. |
| 100 | 5.59e-1 | Golombek et al, 1988, AJ, 95, 26. |
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This SED was created using the sensitivity and saturation values available in November 2004. The black dots are the object surface brightness calculated by assuming the fluxes listed above are uniformly distributed throughout the beam sizes quoted in the reference papers. The green and red lines are the respective sensitivity and saturation limits for each instrument. The sensitivity values used are for a 5 sigma detection of an extended source with a 500 second exposure. |
2MASS K band (Search the 2MASS LArge Galaxy Atlas)
ISO-CAM 6.7 microns (Search the ISO archive)
5 degree IRAS 12 micron image centered on M87 ( Retrieve IRAS images using OASIS)
ISO-CAM 12 microns (Search the ISO archive)
5 degree IRAS 100 micron image centered on M87 ( Retrieve IRAS images using OASIS)
click image for full 2 to 12 micron spectra with ISO-PHT (Search the ISO archive)
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help@spitzer.caltech.edu http://ssc.spitzer.caltech.edu/documents/compendium/m87/ This file was last modified on Tue Oct 3 15:56:22 2006. |