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PKS2135-14
Spitzer MIPS infrared photometric observations. Left to right: 24 microns, 70 microns and 160 microns (when available). FOV are 5x5 arcmins for 24 microns, 5x2.5 arcmins for 70 microns and 0.5x5 arcmins for 160 microns.
![Wavelength/
Frequency Flux Units Reference
5GHz 1.38 Jy Morganti et al. (1993)
[OIII] λ5007 -12.99 Log erg/cm2/s Tadhunter et al. (1993)
15GHz core 106.3 mJy Dicken et al. (2008)
22 GHz core 44.3 mJy Dicken et al. (2008)
24 microns 104.9 mJy Dicken et al. (2008)
70 microns 113.7 mJy Dicken et al. (2008)
160 microns 118.6 mJy Dicken et al. (2008)
X-ray - - -](PKS2135-14_files/shapeimage_18.png)
Other name:
Redshift:
RA (j2000):
Dec (j2000):
Optical class:
Radio Class:
0.200
21 37 45.18
-14 32 55.5
Q
FRII
OX-158
Gemini/GMOS-S: median filtered image
Notes
PKS2135-14
Spectral energy distribution. The blue solid line is fitted to the data from 109 to 1010 Hz. Extrapolating this line from the radio to the infrared SED tests whether non-thermal synchrotron emission from the lobes can contaminate the Spitzer mid-infrared flux. In this case the lobes emission lies out of the Spitzer beam so cannot contaminate the Spitzer data. The weak, flat spectrum, non-thermal radio core emission is also not likely to contaminate the Spitzer infrared flux data for this object.