Table 1: Dense cores covered by the c2d MAMBO survey. The table lists, from left to right, the core name adopted within the c2d collaboration, names for the cores adopted by other authors, the core distance, the type of the core (i.e., starless, YSO, or VeLLO), the approximate galactic environment of the dense core, and whether Spitzer data is available for the core. The last column gives a rough description of the morphology of the subcores (i.e., extended substructures; see Sect. 3.2) within each core using the c2d standard morphology keywords (Enoch et al. 2006, see Sect. 3.3 for a description).

c2d Name		 Other names Distancea Typeb Regionc Spitzer datad Morphology keywordse
    pc        
L1355   $200 \pm 50^1$ s.l. Cepheus Flare c2d elongated, extended
L1521B-2 B217B $140 \pm 10^2$ s.l. Taurus c2d multiple, elongated, extended
L1521F   $140 \pm 10^2$ Ve. Taurus c2d elongated, extended
L1521-2   $140 \pm 10^2$ s.l. Taurus c2d round, extended
L1524-4   $140 \pm 10^2$ s.l. Taurus c2d multiple, round to elongated, extended
B18-1 TMC-2A $140 \pm 10^2$ s.l. Taurus c2d multiple, round to elongated, extended
TMC-2 L1529 $140 \pm 10^2$ s.l. Taurus c2d multiple, elongated, extended
B18-2   $140 \pm 10^2$ s.l. Taurus c2d multiple, elongated, extended
B18-4 TMC-3 $140 \pm 10^2$ YSO Taurus IRAC, MIPS multiple, elongated, extended
B18-5   $140 \pm 10^2$ s.l. Taurus c2d multiple, elongated, extended
TMC-1C B220 $140 \pm 10^2$ s.l. Taurus c2d multiple, elongated, extended
TMC-1 L1534 $140 \pm 10^2$ s.l. Taurus c2d multiple, elongated, extended
L1507A   $140 \pm 10^2$ s.l. Taurus c2d multiple, round to elongated, extended
L1582A B32 $ 400 \pm 40^3$ YSO $\lambda$ Orionis IRAC, MIPS multiple, elongated, extended
IRAS05413 HH212-mm $450 \pm 50^4$ YSO Orion B IRAC, MIPS multiple, round to elongated, extended
L1622A   $450 \pm 50^4$ s.l. Orion East IRAC, MIPS multiple, elongated, extended
L183 L134N $110 \pm 10^5$ s.l. north of Ophiuchus IRAC, MIPS multiple, round to elongated, extended
L438 CB119 $270 \pm 50^6$ s.l. Aquila Rift c2d round, extended
L492 CB128 $270 \pm 50^6$ s.l. Aquila Rift c2d elongated, extended
CB188 L673-1 $300 \pm 100^7$ YSO Aquila Rift, Cloud B c2d elongated, extended
L673-7   $300 \pm 100^7$ Ve. Aquila Rift, Cloud B c2d multiple, round to elongated, extended
L675 CB193 $300 \pm 100^7$ s.l. Aquila Rift, Cloud B c2d elongated, weak
L1100 CB224 $400 \pm 50^8$ YSO northern Cyg OB7   elongated, extended
L1041-2   $400 \pm 50^8$ YSO northern Cyg OB7   multiple, round to elongated, extended
L1148 L1147 $325 \pm 25^9$ Ve. Cepheus Flare c2d multiple, elongated, extended
L1155E L1158 $325 \pm 25^9$ s.l. Cepheus Flare c2d multiple, elongated, extended
L1082C-2   $400 \pm 50^{10}$ s.l. Cyg OB7   elongated, extended
L1082C   $400 \pm 50^{10}$ YSO Cyg OB7   elongated, extended
L1082A B150 $400 \pm 50^{10}$ YSO Cyg OB7   multiple, round to elongated, extended
L1228   $200 \pm 50^{11}$ YSO Cepheus Flare c2d round, extended
Bern48 RNO129 $200 \pm 50^{11}$ YSO Cepheus Flare c2d round, extended
L1172A   $288 \pm 25^9$ YSO Cepheus Flare IRAC, MIPS multiple, round, extended
L1177 CB230 $288 \pm 25^9$ YSO Cepheus Flare IRAC round, extended
L1021   $250 \pm 50^{12}$ s.l. Cyg OB7 c2d elongated, extended
L1014   $250 \pm 50^{12}$ Ve. Cyg OB7 c2d elongated, extended
L1103-2 L1106 $250 \pm 50^{12}$ s.l. Cyg OB7   elongated, extended
L1251A   $300 \pm 50^{13}$ YSO Cepheus Flare c2d multiple, round to elongated, extended
L1197   $300 \pm 50^{14}$ s.l. Cepheus Flare c2d elongated, extended
Notes: a standard c2d distances (Bourke, priv. comm.), derived by reddening methods or association (in position-velocity space) to objects of known distance. The individual references are: [1] Obayashi et al. (1998), via association; [2] Kenyon et al. (1994); [3] Murdin & Penston (1977); [4] Genzel & Stutzki (1989), via association to L1630; [5] Franco (1989); [6] Straizys et al. (2003); [7] Herbig & Jones (1983), via association to L673; [8] Dobashi et al. (1994), and association to L1041; [9] Straizys et al. (1992), and association with L1172; [10] via reddening, following Bourke et al. (1995); [11] Kun (1998); [12] Pagani & Breart de Boisanger (1996), via association to B164; [13] Kun & Prusti (1993); and [14] Yonekura et al. (1997), via association to L1192/L1200; b the abbreviations mark starless cores (``s.l.''; these have no known star within the core boundaries defined in Sect. 3.2), YSO cores (``YSO''; YSOs within the core boundaries), and VeLLO cores (``Ve.''; VeLLOs within the core boundaries). The cores L1521-2, B18-1, TMC-1, and L1622A are excluded from the YSO category since the YSOs are off the main core body. See Sect. 4.1 for a discussion of the association between YSOs and dense cores; c the designation of regions roughly follows Dame et al. (1987), Maddalena et al. (1986), Yonekura et al. (1997), and Dobashi et al. (1994); d cores with data from the c2d project (Evans et al. 2003) are labeled ``c2d''. For other cores existing Spitzer imaging data is indicated in the table, and the Spitzer program numbers and PIs are: GO 3584 (Padgett) and GO 20302 (Andre) for B18-4; GO 20339 (Stauffer) for L1582A; GO 3315 (Noriega-Crespo) and GTO 47 (Fazio) for IRAS05413; GTO 47 (Fazio) for L1622A; GTO 94 (Lawrence) and GTO 53 (Rieke) for L183; L 30574 (Allen) and IOC 717 (Rieke) for L1172A; and GTO 124 (Gehrz) for L1177; e the c2d standard keywords are adopted from the c2d Bolocam survey by Enoch et al. (2006). See Sect. 3.3 for a description.

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