Flux data

Available Data Downloads

Images, Maps, Spectra and SEDs

link to NED page

Infrared data

Radio data

Optical data

X-Ray data

Spitzer 70um DataPKS0213-13_files/0213_70um.fits
Spitzer 160um DataPKS0213-13_files/0213_160um.fits


VLA 5GHzPKS0213-13_files/0213-13.ICL001.7
ESO Optical spectraPKS0213-13_files/

Spitzer IRS spectra


5GHz map

Morganti et al. (1993)


Optical spectrum taken with ESO telescopes.

Tadhunter et al. (1993)


Spitzer IRS spectra

Dicken et al. (in preperation)

Spitzer 24um DataPKS0213-13_files/0213_24um.fits


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.

Dicken et al. (2008)

Next objectPKS0235-19.html
Frequency       Flux      Units	                Reference                
5GHz	         1.8	       Jy                       Morganti et al. (1993)
[OIII]                 -13.68       Log erg/cm2/s    Tadhunter et al. (1993)
15GHz core	 -             mJy                	Dicken et al. (2008)
22 GHz core	 -             mJy	                 Dicken et al. (2008)
24 microns	40.2	       mJy	                 Dicken et al. (2008)
70 microns	37.1         mJy	                 Dicken et al. (2008)
160 microns	<51.1       mJy	                 Dicken et al. (2008)
X-ray            	-	        -	                 -

Other name:


RA (j2000):

Dec (j2000):

Optical class:

Radio Class:


02 15 37.5

-12 59 30.5




Gemini imagePKS0213-13_files/p0213.fits


K-band SOFI (2.2 microns) image. 30x30 arcsecs.

Inskip et al. (2010)



SOFI K-band dataPKS0213-13_files/out_0213.fits


    The Gemini optical image of this NLRG/FRII galaxy reveals a clear system of shells with a surface brightness of μ_V = 24.7 mag arcsec−2 for the brighter shell (∼20 kpc to the north) and 25.1 mag arcsec−2 for the eastern and outer shell (∼27 kpc from the nucleus: Ramos Almeida et al. 2011a). Our long-slit spectrum of this galaxy shows that emission- line contamination is not a serious issue for the shell structure to the NE.

    The optical spectrum reveals high ionization emission lines, and the continuum appears typical of early type galaxies.

Gemini/GMOS-S: median filtered image

    5 GHz VLA radio map


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.

Dicken et al. (2008)