Difference between revisions of "SHIPsOtherPhot"
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| − | == | + | To convert between magnitudes and flux density in Jy, use Equation 2 from: http://coolwiki.ipac.caltech.edu/index.php/Units |
| + | F(Vega) is the zero-point flux listed in the table above. | ||
| + | |||
| + | ==Spitzer Apertures and Aperture corrections== | ||
| + | |||
| + | :For MIPS: http://irsa.ipac.caltech.edu/data/SPITZER/docs/mips/mipsinstrumenthandbook/50/ | ||
| + | |||
| + | :For IRAC: http://irsa.ipac.caltech.edu/data/SPITZER/docs/irac/iracinstrumenthandbook/28/#_Toc296497400 | ||
Latest revision as of 22:46, 28 August 2013
Spitzer photometry
| Wavelength | Zeropoint (Jy) | |
|---|---|---|
| IRAC 3.6 | 280.9 | |
| IRAC 4.5 | 179.7 | |
| IRAC 5.8 | 115.0 | |
| IRAC 8.0 | 64.9 | |
| MIPS 24 | 7.17 |
To convert between magnitudes and flux density in Jy, use Equation 2 from: http://coolwiki.ipac.caltech.edu/index.php/Units F(Vega) is the zero-point flux listed in the table above.
