Notes. Columns 1 to 3: names and coordinates from CSA11 (who use the Chandra positions of Forbrich & Preibisch 2007) and SA13. Columns 4 and 5: classification in CSA11 and SA13. Primordial disk (PD), pre-transitional disk (pre-TD), transitional disk (TD), debris disk (DD). A blank field means that the source is either not detected or not mentioned, or that the photometry was affected by extended nebulosity, mostly an issue in the Herschel observations (SA13). Column 6: flux density at 3.5 cm or 3σ upper limits. For the detections, the VLA coordinates from Gaussian fits are given as a comment, together with the estimation of the 3.5 cm flux due to free-free emission from the coadded nondetection epochs. Column 7: primary-beam-corrected noise, measured individually around the position of each source. Column 8: X-ray luminosity in the 0.2–8 keV band from Forbrich & Preibisch (2007). A blank field means that only ~ 10¹ counts were detected, and the X-ray spectral shape and luminosity could not be derived. However, under typical assumptions, their measured count number would imply L_X ~ 1 × 10²⁹ erg s^-1. Column 9: spectral types reported by CSA11. Compiled from Forbrich & Preibisch (2007), Meyer & Wilking (2009), López Martí et al. (2005), and CSA11. Column 10: comments. a) RA = 19:01:34.86, Dec = –37:00.55.8. S_V709,ff ≲ 507 ± 88 μJy. b) RA = 19:01:53.68, Dec = –36:57:08.0. S_RCrA,ff ≲ 183 ± 20 μJy. Intermediate-mass YSO (Acke & van den Ancker 2004). c) RA = 19:01:58.79, Dec = –36:57:49.9. S_TCrA,ff ≲ 170 ± 26 μJy. Intermediate-mass YSO (Acke & van den Ancker 2004).