PKS0430+05

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=3C120&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

ESO Optical spectra

PKS0430+05

Optical spectrum taken with ESO telescopes.

Tadhunter et al. (1993)

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Wavelength/ Frequency Flux Units Reference 5GHz 8.6 Jy Morganti et al. (1993) [OIII] λ5007 -12.54 Log erg/cm2/s Tadhunter et al. (1993) http://adsabs.harvard.edu/abs/1993MNRAS.263.1023Mhttp://adsabs.harvard.edu/abs/1993MNRAS.263..999Tshapeimage_13_link_0shapeimage_13_link_1

Other name:

Redshift:

RA (j2000):

Dec (j2000):

Optical class:

Radio Class:

0.033

04 33 11.1

+05 21 16

G

-

3C120

N

E

UK Schmidt image, λ4680A, width 2 arcmins.

PKS0430+05

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

Inskip et al. (2010)


N

E

SOFI K-band dataPKS0430+05_files/out_0430.fits

Notes

    This nearby BLRG has been extensively studied (Baldwin et al. 1980). Its optical spectrum is quasar like: broad Balmer and FeII lines/ blends and strong [O III] λλ5007, 4959 lines with a blue continuum. Its radio structure has prominent one-sided jet. The K-band near-IR residual flux image of this galaxy displays a narrow excess of flux along the major axis, which then extends into an s-shape to the NW and SE. Previous observations of this source (Sargent 1967; Baldwin et al. 1980; Garcia-Lorenzo et al. 2005) highlight the complexities of its light distribution, which seem to match our own observed model residuals, and suggest that it has been involved in merger activity in the relatively recent past.