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Table A.1

List of new candidate members from the accretion-based census of the population of NGC 2264.

Mon-ID RA Dec Selection criteria Additional information1
Mon-001428 100.19257 9.71302 UV, var I likely CTTS based on IRAC light curve
Mon-005009 100.54131 9.79834 var II, lc irregular IRAC/CoRoT light curves
Mon-005278 100.64755 9.43207 UV, var II IR excess
Mon-005326 100.62129 9.44550 UV
Mon-005385 100.35425 9.75632 UV, var I flat IRAC light curve
Mon-005455 100.21510 9.37313 UV flat IRAC light curve
Mon-005596 100.51573 9.45916 var I flat IRAC light curve
Mon-005664 100.22703 9.15885 UV spotted-like CoRoT light curve
Mon-005745 100.51810 9.16134 UV
Mon-005807 100.28199 9.23241 UV, var I
Mon-005836 100.37121 9.30430 UV flat IRAC light curve
Mon-006037* 99.87232 9.72772 var II, lc spotted-like CoRoT light curve
Mon-006079 99.87132 9.71070 UV, var I, var II eclipsing binary/very short period binary
Mon-006144 99.92838 9.55441 UV flat IRAC light curve
Mon-006183 99.97203 9.82939 UV, var II flat IRAC light curve
Mon-006286 100.12552 9.19233 UV
Mon-006324 99.95310 9.29308 UV
Mon-006325 100.06032 9.22705 UV, var II
Mon-006369 99.87573 9.29094 varI, var II
Mon-006398 99.81027 9.61444 UV, var II flat IRAC light curve
Mon-006409 99.81342 9.64136 UV flat IRAC light curve
Mon-006429 99.79541 9.53839 UV, var I, var II strong IR excess; IRAC light curve of YSO
Mon-006465 99.85484 9.54391 UV, var I, var II eclipsing binary
Mon-006491 99.85625 9.52760 UV, var II, lc IR excess; CoRoT light curve of CTTS
Mon-006498 99.82751 9.39888 UV flat IRAC light curve
Mon-006515 99.77643 9.66813 UV
Mon-006873 99.79239 9.15089 var I, var II
Mon-006902 99.75107 9.23571 var I, var II
Mon-006930 99.76703 9.27055 var II, lc likely CTTS based on CoRoT light curve
Mon-006950 99.77920 9.85195 UV, var II
Mon-006985 99.77939 10.11909 UV, var II
Mon-006986 99.79149 10.08689 UV, var I, var II, lc likely CTTS based on CoRoT light curve
Mon-006991 99.84169 10.10648 var II, lc likely CTTS based on CoRoT light curve; IR excess
Mon-006999 99.86647 10.06352 var I
Mon-007004 99.85813 10.08544 UV
Mon-007018 99.97253 10.10931 var I, var II
Mon-007402 100.62534 9.94183 var I
Mon-007418 100.57599 10.05188 UV
Mon-007461 100.24085 10.11788 UV, var II probable MIPS 24 μm excess
Mon-007496 100.51515 10.08836 var I, var II
Mon-007845 99.89187 9.40008 UV
Mon-008139 99.75653 10.07972 UV
Mon-008140 99.80434 9.61337 UV, var II
Mon-008141 100.66490 9.67704 UV
Mon-008142 99.76824 9.69662 UV, var I, var II
Mon-014132 99.76480 9.27109 var II, lc AA Tau-type CoRoT light curve; IR excess
Mon-020662 100.21076 10.03841 UV
Mon-021771 100.51792 9.57561 var I, var II flat IRAC light curve
Mon-025015 99.96704 9.40013 UV
Mon-025101 99.85223 9.92528 UV, var II
Mon-124054 100.39085 9.92262 UV, var I

Notes. Selection criteria: UV = UV excess; var I = multi-year variability; var II = mid-term variability (i.e., on week timescales); lc = light curve morphology.

(1)

From Spitzer IRAC and/or CoRoT monitoring obtained during the CSI 2264 campaign (and/or additional IR photometry), when available.

(*)

WTTS candidate member.

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