Sasmirala Individual Information for 3C 135
Description
3C 135 is a FR II radio source identified with the elliptical galaxy LEDA 16952 at a redshift of z = 0.1274 (D ~ 620 Mpc). It contains a radio-loud Sy 2 nucleus [veron-cetty_catalogue_1996] with polarized broad emission lines [cohen_polarimetry_1999]. 3C 135 features the classical FR II supergalactic-scale biconical radio lobes in the east-west directions (PA~ 75∘; e.g., [leahy_study_1997]). No Spitzer data are available for 3C 135, and it appears as a point source in the WISE images. 3C 135 was imaged with VISIR in the broad SIC filter in 2006 but remained undetected [van_der_wolk_dust_2010]. Our derived upper limit on the nuclear MIR flux is two times higher than the value given by [van_der_wolk_dust_2010].
- [cohen_polarimetry_1999] Marshall H. Cohen, Patrick M. Ogle, Hien D. Tran, Robert W. Goodrich, and Joseph S. Miller. Polarimetry and unification of low-redshift radio galaxies . AJ , 118 pp. 1963–1987, November 1999.
- [leahy_study_1997] J. P. Leahy, A. R. S. Black, J. Dennett-Thorpe, M. J. Hardcastle, S. Komissarov, R. A. Perley, J. M. Riley, and P. A. G. Scheuer. A study of FRII radio galaxies with z<0.15 - II. high-resolution maps of 11 sources at 3.6 CM . MNRAS , 291 pp. 20–53, October 1997.
- [van_der_wolk_dust_2010] G. van der Wolk, P. D. Barthel, R. F. Peletier, and J. W. Pel. Dust tori in radio galaxies . A&A , 511 pp. 64, February 2010.
- [veron-cetty_catalogue_1996] M.-P. Veron-Cetty and P. Veron. A Catalogue of quasars and active nuclei . ESO Scientific Report. ESO, 7th edition, 1996.
Images
Optical image (DSS, red filter). Displayed are the central 4 arcmin with North being up and East to the left. The colour scaling is linear with white corresponding to the median background (BG) and black to the 0.01% pixels with the highest intensity.
SEDs
MIR SED. The description of the symbols in all the SED plots (where present) is the following: Grey crosses and solid lines mark the Spitzer/IRAC, MIPS and IRS data. The colour coding of the other symbols is as follows: green for COMICS, magenta for Michelle, blue for T-ReCS and red for VISIR data. Darker-coloured solid lines mark spectra of the corresponding instrument. The black filled circles mark the nuclear 12 and 18 micron continuum emission estimate from the data (where present). The ticks on the top axis mark positions of common MIR emission lines, while the light grey horizontal bars mark wavelength ranges affected by the silicate 10 and 18 micron features.