PKS0427-53

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=0427-53&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

1.4GHzPKS0427-53_files/0428HIcont.fits
ESO Optical spectraPKS0427-53_files/s0427.zip

PKS0427-53

5GHz

Morganti et al. (1993)

PKS0427-53

Optical spectrum taken with ESO telescopes.

Tadhunter et al. (1993)

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PreviousPKS0409-75.html
Wavelength/ Frequency Flux Units Reference 5GHz 3.41 Jy Morganti et al. (1993) [OIII] λ5007 < -15.39 Log erg/cm2/s Tadhunter et al. (1993) http://adsabs.harvard.edu/abs/1993MNRAS.263.1023Mhttp://adsabs.harvard.edu/abs/1993MNRAS.263..999Tshapeimage_15_link_0shapeimage_15_link_1

Other name:

Redshift:

RA (j2000):

Dec (j2000):

Optical class:

Radio Class:

0.038

04 29 7.6

-53 49 38

WLRG

FRI

-

N

E

UK Schmidt image, λ 4680A, width 2 arcmins.

SOFI K-band dataPKS0427-53_files/out_0428.fits

PKS0427-53

K-band SOFI (2.2 microns) image. 2x2 arcmins.

Inskip et al. (2010)


N

E

Notes

    The FRI radio source PKS 0427−53 is hosted by the eastern component of a dumbbell galaxy system (Carter et al. 1989). It presents an interesting radio structure, with a long tongue of emission seen extending westward from the western lobe in the 843-Mhz Molongo images (Jones & McAdam 1992). Our ATCA image shows only the inner lobes and a distinct core (Morganti et al. 1993). The extended emission in this image is not reliably represented.

    The optical spectrum reveals no emission lines and the continuum appears typical of early-type galaxies (Tadhunter et al. 1993, Wills et al. 2004).


    5 GHz ATCA radio map

ATCA 5GHz