Open Access

Table A.1.

Properties used for the selection of the non-confirmed candidates.

Target R.A. Dec. drop S888MHz magz drop magz–magW2 dro Telescope
(deg) (deg) (Survey) (mJy beam−1) (mag AB) (AB – Vega) (arcsec)
RACS J0010−53 2.526012 −53.589526 r-drop (D) 1.2±0.4 20.84±0.04 1.64 3.35 1.47 VLT
RACS J0249−28 42.311270 −28.855045 i-drop (D) 5.1±0.5 20.83±0.03 1.23 3.09 2.01 VLT
RACS J0420−47 65.043381 −47.723408 r-drop (D) 10.3±0.7 21.22±0.04 1.62 3.63 2.13 VLT
RACS J0427−53 66.930894 −53.393840 i-drop (D) 3.6±0.6 20.04±0.01 1.08 3.20 1.47 VLT
RACS J0616−48 94.199469 −48.347094 i-drop (D) 2.1±0.8 21.24±0.03 1.39 3.37 2.76 VLT
RACS J0622−51 95.743477 −51.020087 r-drop (D) 1.9±0.7 20.74±0.03 1.82 3.72 2.71 ATCA*
RACS J0905−10 136.262847 −10.426427 r-drop (P) 6.2±1.4 20.15±0.07 1.58 2.41 1.14 LBT
RACS J1521−00 230.377454 −0.300307 r-drop (P) 12.6±0.5 20.98±0.16 1.27 3.51 0.37 LBT
RACS J1552−29 238.041957 −29.255812 r-drop (P) 6.4±0.3 19.92±0.05 1.28 3.72 1.20 AAT
RACS J1557−18 239.321655 −18.041279 r-drop (P) 1.2±0.4 20.36±0.03 1.91 4.24 1.12 LBT
RACS J1614+14 243.735217 +14.315941 r-drop (P) 1.6±0.4 20.27±0.03 1.53 3.80 0.91 LBT
RACS J1722+29 260.728554 +29.108219 i-drop (P) 1.5±0.4 21.29±0.13 1.64 < 2.3 1.30 LBT
RACS J1802+10 270.599597 +10.922134 r-drop (P) 6.1±0.7 20.27±0.06 1.58 3.89 1.02 LBT
RACS J2015−17 303.930440 −17.577126 r-drop (P) 1.6±0.3 20.96±0.09 1.82 3.90 0.27 TNG
RACS J2021−20 305.411544 −20.655044 r-drop (P) 2.5±0.5 20.67±0.04 1.52 3.61 1.23 AAT
RACS J2044−16 311.087282 −16.383996 r-drop (P) 1.5±0.4 20.70±0.06 1.74 < 1.7 1.11 AAT
RACS J2103−40 315.773997 −40.697616 r-drop (D) 3.0±0.5 20.97±0.04 1.96 3.97 2.91 VLT

Not observed yet
RACS J0632−59 98.245905 −59.567634 r-drop (D) 1.2±0.4 21.01±0.04 1.81 2.93 1.14
RACS J0721+34 110.480455 +34.5776441 i-drop (P) 2.1±0.5 21.29±0.15 3.74 < 2.3 1.42
RACS J0937−21 144.310777 −21.019468 i-drop (P) 1.0±0.3 20.82±0.03 1.22 < 1.8 2.85
RACS J1536−28 234.204898 −28.4014139 i-drop (P) 1.8±0.3 21.04±0.09 1.53 4.62 2.05

Notes. Col. (1, 2, 3): Name and coordinates of the source. Col. (4): Type of dropout and survey the source was selected from, in brackets. Col. (5): Peak flux density at 888 MHz from the RACS-low source lists. Col. (6):z-band magnitude from DES or Pan-STARRS. Col. (7): Dropout r − i or i − z depending on the type of dropout in Col. 4. Col. (8):z − W2 colour, where z is in the AB system and W2 in the Vega one. In case of a non-detection in the W2 filter, we assumed an upper limit of magW2 = 19; Col. (9): Radio-to-optical distance. Col. (10): Telescope used for the identification. The ‘*’ indicates radio telescopes used to get more accurate position of the radio counterpart and discard the radio-optical association.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.