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Table 1

Young nearby regions (top) and associations (bottom) included in this study.

Name Age Distance Membership and SpT Spitzer photometry Number of sources
(Myr) (pc)

25 Orionis 7–10 330 (1) (1) 46
Cha I 2 160–165 (2) (3) (4) (3) (4) 212
Cha II 2 ± 2 178 ± 18 (5) (38) 47
CrA 1–3 138 ± 16 (6) (7) (8) (9) (39) 35
IC 348 2 285–315 (10) (11) (38) (40) 298
λ Orionis 4 400 ± 40 (12) (41) 114
Lupus 1–1.5 140 – 200 (13) (14) (15) (16) (38) 217
NGC 1333 1 235 ± 18 (17) (42) 74
Ophiuchus 2–5 120–145 (18) (19) (20) (21) (38) 258
σ Orionis 2–3 440 ± 30 (22) (23) (24) (25) (26) (27) (28) (43) 104
Serpens 2 230 ± 20 (17) (29) (38) 142
Taurus 1–2 140 (30) (31) (32) (33) (32) (33) 265
Upper Sco 11 ± 2 140 (34) (35) (36) (35) 405

AB Dor 50–100 34 (37) ... 92
Argus 40 106 (37) ... 51
β Pic 10 31 (37) ... 54
Carina 30 85 (37) ... 37
Columba 30 82 (37) ... 58
η Cha 4–9 108 (37) ... 27
Octantis 20 141 (37) ... 17
Tuc-Hor 30 48 (37) ... 49
TW Hya 8 48 (37) ... 25

Notes. Ages and distances are from Reipurth (2008a, b) unless specified. We also tabulate references to the different studies used to compile the sample of objects and to the Spitzer photometry, as well as the number of sources for each region.

Reference. (1) Hernández et al. (2007a); (2) Luhman (2007); (3) Luhman et al. (2008a); (4) Luhman & Muench (2008); (5) Spezzi et al. (2008); (6) Neuhäuser et al. (2000); (7) Nisini et al. (2005); (8) Sicilia-Aguilar et al. (2008); (9) Sicilia-Aguilar et al. (2011); (10) Luhman et al. (2003); (11) Alves de Oliveira et al. (2013); (12) Bayo et al. (2011); (13) Krautter et al. (1997); (14) Allen et al. (2007); (15) Comerón (2008); (16) Mortier et al. (2011); (17) Winston et al. (2009); (18) Natta et al. (2002); (19) Wilking et al. (2005); (20) Alves de Oliveira et al. (2010); (21) Erickson et al. (2011); (22) Zapatero Osorio et al. (2002); (23) Muzerolle et al. (2003); (24) Barrado y Navascués et al. (2003); (25) Franciosini et al. (2006); (26) Caballero (2007); (27) Sacco et al. (2008); (28) Rigliaco et al. (2012); (29) Oliveira et al. (2009); (30) Luhman (2004); (31) Monin et al. (2010); (32) Rebull et al. (2010); (33) Rebull et al. (2011); (34) Preibisch et al. (2002); (35) Carpenter et al. (2006); (36) Lodieu et al. (2011); (37) Torres et al. (2008); (38) Evans et al. (2009); (39) Peterson et al. (2011); (40) Lada et al. (2006); (41) Barrado y Navascués et al. (2007); (42) Gutermuth et al. (2008); (43) Luhman et al. (2008b).

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