Mapping accretion and its variability in the young open cluster NGC 2264: a study based on u-band photometry

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Volume 570 (October 2014)

A&A, 570 (2014) A82

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Table A.2

List of NGC 2264 members, with no apparent accretion activity from previous surveys, reclassified as CTTS from this accretion-based census of the population of NGC 2264.

Mon-ID	RA	Dec	Selection criteria	Additional information¹

Mon-000293	100.25166	9.68758	UV
Mon-000316	100.23172	9.64025	UV	IR excess; likely CTTS based on IRAC light curve
Mon-000340	100.48304	9.67968	UV	flat IRAC light curve
Mon-000507	100.26089	9.85702	UV	flat IRAC light curve; possible 8 μm excess
Mon-000685	100.18949	9.81950	UV	flat IRAC light curve
Mon-000718	100.26733	9.34567	UV	flat IRAC light curve
Mon-000750	100.32659	9.52487	UV	flat IRAC light curve; possible 8 μm excess
Mon-000823	100.20891	9.95111	UV
Mon-000914	100.21629	9.63220	UV	very strong IR excess
Mon-000957	100.19014	9.20354	UV	IR excess
Mon-000959	100.18845	9.26850	var	IR excess
Mon-001060	100.12844	10.00076	UV	IR excess; likely CTTS based on IRAC light curve
Mon-001211	99.95979	9.52143	UV	IR excess
Mon-001224	100.06953	9.67295	UV
Mon-001241	100.14078	9.81216	UV	IR excess; likely CTTS based on IRAC light curve
Mon-001267	100.14299	9.42142	var	strong IR excess; IRAC light curve of YSO
Mon-001280	99.91768	9.30604	UV	strong IR excess
Mon-001576	100.13291	10.11898	UV	strong MIPS 24 μm excess
Mon-001582	100.49939	10.06379	UV	strong IR excess

Notes. Selection criteria: UV = UV excess; var = multi-year variability.

⁽¹⁾

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

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