Notes. Column description: (Col. 1) 3CR name; (Col. 2) redshift from Spinrad et al. (1985); (Col. 3) morphological FR type from Buttiglione et al. (2009) and spectroscopic classification into High Excitation Galaxy (HEG) or Broad Line Object (BLO) from Buttiglione et al. (2009). Except for 3C 433 and 3C 458, all the unclassified objects could be considered FR II according to their morphology and 178 MHz luminosities. (Col. 4) Angular size of the radio emission in arcsec; (Col. 5) position angle of the radio source, generally measured from hot spot to hot spot. (Col. 6) References for the radio properties: 1.) Privon et al. (2008), 2.) Martel et al. (1999), 3.) de Koff et al. (1996), 4.) Saripalli & Subrahmanyan (2009); (Col. 7) Chandra observation identification number; (Col. 8) approved exposure time for the observation in ks. (Col. 9) off-axis angle coordinate in arcmin. (Col. 10) morphology of the soft (0.5–2 keV) X-ray emission: extended (ext), possibly extended (poss. ext), unresolved (unres), non detected (non det). X-ray jets have been seen in 3C 15: Kataoka et al. (2003), 3C 31: Hardcastle et al. (2002), 3C 66B: Hardcastle et al. (2001), 3C 78: Massaro et al. (2008) 3C 264: Perlman et al. (2010), 3C 270: Worrall et al. (2010), 3C 273: Sambruna et al. (2001b), 3C 296: Hardcastle et al. (2005b), 3C 346: Dulwich et al. (2009), 3C 371: Pesce et al. (2001), 3C 465: Hardcastle et al. (2005a). (Col. 11) Angular size of the soft X-ray emission in arcsec; (Col. 12) Position angle of the more extended direction in the X-ray image; (Col. 13) Morphology of the optical emission line region as Col. 9; (Col. 14) Angular size of the emission line region in arcsec; (Col. 15) Position angle of the more extended direction in the optical line images; (Col. 16) references for the optical line region properties: 1.) Privon et al. (2008), 2.) Tremblay et al. (2009), 3.) McCarthy et al. (1995), 4.) Baum et al. (1988), 5.) Martel et al. (2004), 6.) Edwards et al. (2009), 7.) Sarzi et al. (2006), 8.) Hes et al. (1996), 9.) Prieto & Zhao (1997), 10.) Hippelein et al. (1996), 11.) Morganti et al. (1992), 12.) Husemann et al. (2008); (Col. 17) host galaxy major axis position angle from de Koff et al. (1996),