\begin{table}%t1
\caption{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.~\ref{sec-survey:id_and_quant})
  within each core   using the c2d standard morphology keywords (\citealt{enoch2006:perseus}, see Sect.~\ref{sec-survey:prop_overview} for a description).}\label{tab-survey:c2d-MAMBO_sampel}
%\centerline
 {\small \begin{tabular}{lllllll}
\hline \hline \noalign{\smallskip}
 c2d Name & Other names & Distance$^a$ & Type$^b$ &  Region$^c$ & Spitzer data$^d$ & Morphology keywords$^e$\\
  & & pc \\ \hline 
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\\
\hline
\end{tabular}}
\medskip
 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]~\citet{obayashi1998:l1333}, via association; [2]
\citet{kenyon1994:tau_auriga}; [3] \citet{murdin1977:l_orionis}; [4]
\citet{genzel1989:orion}, via association to L1630; [5]
\citet{franco1989:high-latitude_distances}; [6]
\citet{straizys2003:distances}; [7]
\citet{herbig1983:hh_proper-motions}, via association to L673; [8]
\citet{dobashi1994:cygnus}, and association to L1041; [9]
\citet{straizys1992:distances}, and association with L1172; [10] via
reddening, following \citet{bourke1995:bhr}; [11]
\citet{kun1998:cep_flare}; [12] \citet{pagani1996:b164}, via
association to B164; [13] \citet{kun1993:l1251}; and [14]
\citet{yonekura1997:cepheus_cassiopeia}, 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.~\ref{sec-survey:id_and_quant}), 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.~\ref{sec-survey:ass_protostars} for a discussion of the
association between YSOs and dense cores; $^c$ the designation of regions roughly follows
\citet{dame1987:co_survey}, \citet{maddalena1986:ori_mon}, \citet{yonekura1997:cepheus_cassiopeia}, and \citet{dobashi1994:cygnus}; $^d$ cores with data from the c2d project \citep{evans2003:c2d} 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 \citet{enoch2006:perseus}. See Sect.~\ref{sec-survey:prop_overview} for a description.
\end{table}