Flux data
Available Data Downloads
Infrared data
Radio data
Optical data
X-Ray data
Chandra
Spitzer IRS spectra
PKS????
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PKS0625-35
Spitzer IRS spectra
Dicken et al. (in preperation)
PKS0625-35
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 2.12 Jy Morganti et al. (1993)
[OIII] λ5007 <-15.18 Log erg/cm2/s Tadhunter et al. (1993)
15GHz core 571.6 mJy Dicken et al. (2008)
22 GHz core 478.8 mJy Dicken et al. (2008)
24 microns 24.7 mJy Dicken et al. (2008)
70 microns 44.8 mJy Dicken et al. (2008)
160 microns 131.0 mJy Dicken et al. (2008)
X-ray - - -](PKS0625-35_files/shapeimage_17.png)
Other name:
Redshift:
RA (j2000):
Dec (j2000):
Optical class:
Radio Class:
BL Lac/WLRG
FRI
OH-342
N
E
-35 29 16.3
06 27 6.65
0.055
Gemini/GMOS-S: median filtered image
Notes
Based on its relatively featureless optical continuum and strong core emission at optical and radio wavelengths, Wills et al. (2004) argue that PKS 0625−35 is a BL Lac. Our deep Gemin image of this low-redshift WLRG does not reveal any morphological peculiarity associated with a merger or interaction (Ramos Almeida et al. 2011a), but a one-sided jet pointing to the SE can be seen, which was also found by Inskip et al. (2010) in their residual NIR image. The detection of this jet supports the classification of this object as a BL-Lac by Wills et al. (2004).
Based on the extrapolation of the high frequency radio core component towards the infrared region of the spectral energy distribution, it is possible that the non-thermal core synchrotron emission makes a substantial contribution to the MFIR flux in this radio galaxy (Dicken et al. 2008).
Images, Maps, Spectra and SEDs
PKS0625-35
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. However, extrapolating the, flat spectrum, radio core SED into the infrared, shows that the core synchrotron emission could be a possible source of non-thermal contamination to the thermal infrared flux.
