PKS0213-13

Flux data

Available Data Downloads

Images, Maps, Spectra and SEDs

(definitions)Definitions.html
link to NED pagehttp://nedwww.ipac.caltech.edu/cgi-bin/nph-objsearch?objname=3c62&extend=no&hconst=73&omegam=0.27&omegav=0.73&corr_z=1&out_csys=Equatorial&out_equinox=J2000.0&obj_sort=RA+or+Longitude&of=pre_text&zv_breaker=30000.0&list_limit=5&img_stamp=YES

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

Chandra

VLA 5GHzPKS0213-13_files/0213-13.ICL001.7
ESO Optical spectraPKS0213-13_files/s0213.zip

Spitzer IRS spectra

PKS0213-13

5GHz map

Morganti et al. (1993)

PKS0213-13

Optical spectrum taken with ESO telescopes.

Tadhunter et al. (1993)

PKS0213-13

Spitzer IRS spectra

Dicken et al. (in preperation)

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

PKS0213-13

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)

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Wavelength/
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            	-	        -	                 -http://adsabs.harvard.edu/abs/1993MNRAS.263.1023Mhttp://adsabs.harvard.edu/abs/1993MNRAS.263..999Thttp://adsabs.harvard.edu/abs/2008ApJ...678..712Dhttp://adsabs.harvard.edu/abs/2008ApJ...678..712Dhttp://adsabs.harvard.edu/abs/2008ApJ...678..712Dhttp://adsabs.harvard.edu/abs/2008ApJ...678..712Dhttp://adsabs.harvard.edu/abs/2008ApJ...678..712Dshapeimage_19_link_0shapeimage_19_link_1shapeimage_19_link_2shapeimage_19_link_3shapeimage_19_link_4shapeimage_19_link_5shapeimage_19_link_6

Other name:

Redshift:

RA (j2000):

Dec (j2000):

Optical class:

Radio Class:

0.147

02 15 37.5

-12 59 30.5

NLRG

FRII

3C62

Gemini imagePKS0213-13_files/p0213.fits

PKS0213-13

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

Inskip et al. (2010)


N

E

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

Notes

    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

PKS0213-13

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)