\begin{table}%t2
\caption{\label{smz}H$_2$ jets and outflows in Orion~A, from the catalogue of Sta02.}
%\centering
\small
\begin{tabular}{@{}ccccc ccccc ccccc cc@{}}
   \hline\hline
%&&&&&&&&&&&&&&&& \\[-8pt]
SMZ  & RA$^{{a}}$    & Dec$^{{a}}$           & Outflow$^{{b}}$    & $\alpha^{{b}}$ 
 & 850\mic $^{{c}}$  & $Ap_{850}$$^{{c}}$    & $I_{850}$$^{{c}}$  &  $F_{850}$$^{{c}}$
 & 1200\mic $^{{d}}$ & $Ap_{1200}$$^{{d}}$   & $I_{1200}$$^{{d}}$ &  $F_{1200}$$^{{d}}$
 & $L$$^{{e}}$       & $\theta$$^{{e}}$      & PA$^{{e}}$         & HH$^{{f}}$ 
  \\
& (J2000)  & (J2000) & source  & & peak & (arcsec) & (Jy) & (Jy/bm) & peak & (\arcsec ) & (Jy) & (Jy/bm) & (\arcmin ) & (deg) & (deg) &  \\
   \hline
1     & 5:35:19.3 & --4:55:45 & IRS~1  & --0.27 & no obs          &   --   & --  &  --   &undetected & --         &  --  &  --   & 0.3     & 20 & 68      &    -- \\  
2     & 5:35:31.6 & --5:00:14 & IRS~2  & --1.04 & undetected      &   --   & --  &  --   &undetected & --         &  --  &  --   & 0.4     & -- & 140     &    -- \\  
3     & 5:35:18.3 & --5:00:33 & IRS~3  &  0.31 & AN-535182-50021 & 19 $\times$ 14  & 5.9 &  2.13 & MMS~3     & 22 $\times$ 14(92)  & 0.48 &  0.57 & 5.2     & 30 & 85      &    -- \\  
4     & 5:35:23.5 & --5:01:29 & IRS~4  &  2.35 & AN-535235-50132 & 21 $\times$ 16  & 9.7 &  6.23 & MMS~4     & 137 $\times$ 50(147)& 4.64 &  1.93 & 0.5     & -- & 170     &    -- \\  
5     & 5:35:22.4 & --5:01:14 & IRS~5  &  2.90 & AN-535224-50114 & 13 $\times$ 10  & 3.9 &  2.60 & MMS~5     & 14 $\times$ 13(150) & 2.07 &  0.52 & 0.6     & 50 & 90      & 293   \\  
6     & 5:35:26.6 & --5:03:55 & IRS~6  &  1.53 & AN-535265-50356 & 37 $\times$ 28  & 6.5 &  1.63 & MMS~6     & 27 $\times$ 23(163) & 2.22 &  0.31 & 13      & -- & 85      &294/295\\  
7     & 5:35:28.0 & --5:04:58 & IRS~7  &  1.04 & AN-535274-50511 & 32 $\times$ 23  & 5.3 &  0.44 & MMS~7     & 35 $\times$ 16(136) & 0.44 &  0.12 &$ \sim$6 & 10 & 30      &    -- \\  
8     & (5:35:42.1& --5:04:39)&  ?     &  --   & ?               &   --   & --  &  --   & ?         & --         & --   &  --   &  --     & -- & --      &    -- \\  
9     & 5:35:25.8 & --5:05:44 & IRS~9  &  1.54 & AN-535258-50551 & 38 $\times$ 22  & 6.3 &  1.55 & MMS~9     & 35 $\times$ 20(50)  & 1.31 &  0.24 & 2.8     & 42 & 80      & 330   \\  
10    & 5:35:31.5 & --5:05:47 & IRS~10 & -0.12 & AN-535324-50547 & 50 $\times$ 28  & 5.3 &  0.42 & MMS~10    & 44 $\times$ 31(27)  & 2.22 &  0.12 & 1.5     & 15 & 50      & 287   \\   
11/13 & 5:35:23.3 & --5:07:10 & IRS~11 &  0.17 & AN-535236-50711 & 16 $\times$ 13  & 2.5 &  1.11 & MMS~11    & 31 $\times$ 18(122) & 1.08 &  0.20 & $\sim$1 & -- &$\sim$20 &    -- \\  
12    & 5:35:27.7 & --5:07:04 & IRS~12 &  1.85 & AN-535279-50711 & 18 $\times$ 14  & 0.8 &  0.24 & MMS~12    & 29 $\times$ 23(173) & 0.54 &  0.11 & 0.3     & -- & 8       &    -- \\  
14/16 & 5:35:25.6 & --5:07:57 & IRS~14 &  0.93 & emission        &   --   & --  &  0.43 & MMS~14    & 20 $\times$ 15(47)  & 0.27 &  0.06 & $\sim$4 & 35 & 40      & 383   \\  
15    & 5:35:22.4 & --5:08:05 & IRS~15 & -0.10 & AN-535222-50817 & 18 $\times$ 14  & 1.2 &  0.38 & MMS~15    & 20 $\times$ 15(98)  & 0.29 &  0.09 & 0.4     & -- &$\sim$45 & 385   \\  
17    & 5:35:27.0 & --5:09:54 & IRS~17?&  0.54 & emission        &   --   & --  &  5.80 & MMS~17    & 25 $\times$ 22(41)  & 6.06 &  1.07 & 1.8     & 50 & 25      & 887   \\  
18    &(5:35:29.6 & --5:08:58)&   ?    &  --   & ?               &   --   & --  &  --   & ?         & --         & --   &  --   &  --     & 50 & --      &    -- \\  
19    & 5:35:26.8 & --5:09:25 & IRS~19 & -0.03 & emission        &   --   & --  &  1.90 & MMS~19    & 20 $\times$ 15(92)  & 0.87 &  0.28 & 0.5     & -- & 100     & 384   \\  
20    & 5:35:25.7 & --5:09:49 & IRS~20 &  0.14 & emission        &   --   & --  &  1.45 & emission  & --         & --   &  0.36 & 0.7     & -- & 175     &    -- \\  
21/22 & 5:35:26.9 & --5:11:07 & IRS~21 & -1.01 & emission        &   --   & --  &  0.33 & emission  & --         & --   &  0.10 & 1.6     & -- & 175     &    -- \\  
23    & 5:35:24.7 & --5:10:30 & IRS~23 &  1.18 & emission        &   --   & --  &  0.53 & MMS~23    & 20 $\times$ 16(175) & 0.48 &  0.18 &$\sim$4  & -- & 17      &    -- \\  
24    & 5:35:23.3 & --5:12:03 & IRS~24 &  1.37 & AN-535234-51205 & 21 $\times$ 16  & 3.2 &  1.28 & MMS~24    & 16 $\times$ 12(174) & 0.44 &  0.35 & 1.5     & 27 & 61      & 536   \\  
25    & 5:35:20.1 & --5:13:16 & IRS~25 &  0.04 & emission        &   --   & --  &  0.87 & MMS~25    & 23 $\times$ 12(126) & 0.65 &  0.29 & 3.0     & -- & 160     & 44/535\\   
26    &(5:35:10.9 & --5:23:12)&   ?    & --    & ?               &   --   & --  &  --   & ?         & --         & --   &  --   & 2.6     & -- & 125     &    -- \\  
27    &(5:35:11.6 & --5:23:41)&   ?    & --    & ?               &   --   & --  &  --   & ?         & --         & --   &  --   &  --     & -- & --      & 510?  \\  
28    &(5:35:10.9 & --5:23:46)&   ?    & --    & ?               &   --   & --  &  --   & ?         & --         & --   &  --   &  --     & -- & --      & 510?  \\  
29    & 5:34:40.9 & --5:31:44 & IRS~29 &  1.47 & no obs          &   --   & --  &  --   & MMS~29    & 21 $\times$ 16(160) & 0.42 &  0.16 & 5.0     & 20 & 156     &    -- \\  
30    & 5:35:18.3 & --5:31:42 & IRS~30 & --0.36 & undetected      &   --   & --  &  --   & MMS~30    & 18 $\times$ 17(64)  & 0.06 &  0.03 & 0.9     & -- & 25      & 540   \\   
31    & 5:34:35.5 & --5:39:59 & IRS~31 &  1.01 & no obs          &   --   & --  &  --   & MMS~31    & 33 $\times$ 25(22)  & 0.26 &  0.06 & 0.9     & 60 & 150     &    -- \\  
32    &(5:35:11.4 & --5:39:38)& ?      & --    & ?               &   --   & --  &  --   & ?         & --         & --   &  --   & 0.8     & -- & 170     &    -- \\  
33    & 5:34:51.9 & --5:41:33 & IRS~33?& 1.64  & undetected      &   --   & --  &  --   &undetected & --         & --   &  --   & 0.5     & -- & 134     &    -- \\  
34    & 5:35:09.9 & --5:43:45 & IRS~34 & 1.54  & undetected      &   --   & --  &  --   &undetected & --         & --   &  --   & --      & -- & --      &    -- \\  
35    & 5:34:46.9 & --5:44:51 & IRS~35?& 0.73  & undetected      &   --   & --  &  --   &undetected & --         & --   &  --   & 1.0     & -- & 58      &    -- \\  
36    &(5:35:10.0 & --5:45:06)& ?      & --    & ?               &   --   & --  &  --   & ?         & --         & --   &  --   & --      & -- & --      &    -- \\    
37    & 5:35:05.5 & --5:51:54 & IRS~37 & 0.77  & no obs          &   --   & --  &  --   &undetected & --         & --   &  --   & --      & -- & --      &    -- \\  
38    & 5:35:08.6 & --5:55:54 & IRS~38 & 1.80  & no obs          &   --   & --  &  --   & MMS~38    & 19 $\times$ 15(121) & 0.88 &  0.31 &$\sim$7  & 10 &$\sim$150&    -- \\  
39    & 5:35:09.0 & --5:58:28 & IRS~39 & 1.06  & emission        &   --   & --  &  0.41 & MMS~39    & 19 $\times$ 15(155) & 0.54 &  0.17 &$>$3     & 20 & $\sim$30&    -- \\  
40    & 5:35:33.2 & --6:06:10 & IRS~40?& 0.46  & emission        &   --   & --  &  --   &undetected & --         & --   &  --   & 3.8     & -- & 16      &    -- \\  
41    & 5:35:13.4 & --5:57:58 & IRS~41 & 2.30  & no obs          &   --   & --  &  --   & MMS~41    & 19 $\times$ 14(153) & 0.79 &  0.21 & 6.0     & -- & 9       &    -- \\  
42    & 5:35:22.2 & --6:13:06 & IRS~42 & 1.21  & AS-535213-61313 & 26 $\times$ 17  & 0.7 &  0.14 & MMS~42    & 57 $\times$ 37(35)  & 0.88 &  0.06 & 5.0     & 12 & 69      &    -- \\  
43    & 5:35:52.0 & --6:10:02 & IRS~43 & 0.37  & AS-535524-61007 & 33 $\times$ 19  & 1.3 &  0.49 & MMS~43    & 22 $\times$ 16(150) & 0.58 &  0.19 &$\sim$2  & -- &$\sim$45 &    -- \\  
44    & 5:35:45.2 & --6:11:44 & IRS~44?& --1.19 & undetected      &   --   & --  &  --   &undetected & --         & --   &  --   & 1.3     & -- & 132     &    -- \\  
45    & 5:36:17.3 & --6:11:11 & IRS~45 & 0.93  & undetected      &   --   & --  &  --   & MMS~45    & 32 $\times$ 22(166) & 0.22 &  0.04 & 2.3     & 60 & 3       &    -- \\  
46    & 5:36:37.0 & --6:14:58 & IRS~46 & 0.51  & AS-536366-61459 & 19 $\times$ 13  & 0.8 &  0.30 & MMS~46    & 29 $\times$ 20(128) & 0.52 &  0.11 &$\sim$0.5& -- &$\sim$0  & 304   \\ 
47    &(5:35:38.1 & --6:15:08)& ?      & --    & ?               &   --   & --  &  --   & ?         & --         & --   &  --   & 0.9     & -- & 155     &    -- \\
      \hline
48    & 5:36:10.5 & --6:19:55 & ?      & --    & ?               &   --   & --  &  --   & ?         & --         & --   &  --   & 1.4     & -- & 40      & 299   \\  
49    & 5:36:19.5 & --6:22:12 & IRS~49 & 0.79  & AS-536196-62209 & 77 $\times$ 44  & 15.8&  1.92 & MMS~49    & 20 $\times$ 9(88)   & 0.16 &  0.53 &$\sim$34 & -- & 175     & 303   \\ 
50    & 5:36:11.5 & --6:22:22 & IRS~50?& --0.90 & undetected      &   --   & --  &  --   &undetected & --         & --   &  --   & 2.0     & -- &$\sim$170&    -- \\ 
51    & 5:36:24.6 & --6:22:41 & IRS~51 & 1.23  & AS-536250-62241 & 49 $\times$ 27  & 3.1 &  0.59 & MMS~51    & 52 $\times$ 24(155) & 1.39 &  0.12 &$>$4.0   & 40 & 69      & 301   \\ 
52    &(5:36:39.1 & --6:22:38)& ?      & --    & ?               &   --   & --  &  --   & ?         & --         & --   &  --   &  --     & -- & --      &    -- \\ 
53    & 5:36:18.8 & --6:22:10 & IRS~53 & 2.47  & AS-536196-62209 & 77 $\times$ 44  & 15.8&  3.72 & MMS~53    & 17 $\times$ 16(38)  & 3.09 &  1.01 & 0.6     & -- & 45      &    -- \\ 
54    &(5:36:31.0 & --6:24:49)& ?      & --    & ?               &   --   & --  &  --   & ?         & --         & --   &  --   &  --     & -- & --      &    -- \\ 
55    & 5:35:29.8 & --6:26:59 & IRS~55 & 1.77  & AS-535297-62701 & 27 $\times$ 19  & 1.7 &  0.83 & MMS~55    & 14 $\times$ 13(4)   & 1.92 &  0.26 & 17      & -- & 165     & 34    \\ 
56    & 5:35:30.9 & --6:26:32 & IRS~56 & 1.16  & AS-535305-62622 & 32 $\times$ 21  & 1.6 &  0.26 & MMS~56    & 54 $\times$ 38(168) & 1.34 &  0.09 & 1.8     &  4 & 8       &    -- \\ 
57    &(5:36:56.9 & --6:34:17)& ?      & --    & ?               &   --   & --  &  --   & ?         & --         & --   &  --   &  --     & -- & --      & 292   \\ 
58    & 5:37:00.5 & --6:37:11 & IRS~58 & -0.16 & AS-537004-63715 & 36 $\times$ 19  & 1.5 &  0.44 & MMS~58    & 63 $\times$ 38(179) & 2.22 &  0.15 & 4.0     & 12 & 60      &    -- \\ 
59    & 5:36:36.1 & --6:38:52 & V380~Ori-NE&-- & AS-536361-63857 & 38 $\times$ 18  & 1.8 &  0.93 & MMS~59    & 38 $\times$ 18(167) & 1.62 &  0.35 & 2.0     & 18 &$\sim$0  &    -- \\ 
60    &(5:36:22.0 & --6:41:42)& ?      & --    & ?               &   --   & --  &  --   & ?         & --         & --   &  --   &  --     & -- & --      & 35    \\ 
61    & 5:36:18.9 & --6:45:23 & IRS~61?& 2.07  & emission        &  --    & --  &  0.88 & emission  & --         & --   &  0.25 &$\sim$3.6& -- &$\sim$165&    -- \\ 
62    &(5:36:11.6 & --6:43:04)& ?      & --    & ?               &  --    & --  &  --   & ?         & --         & --   &  --   &  --     & -- & --      & 3     \\ 
63    & 5:36:25.1 & --6:44:42 & IRS~63 & 0.04  & AS-536259-64440 & 38 $\times$ 27  & 2.2 &  0.47 & MMS~63    & 58 $\times$ 48(20)  & 2.91 &  0.17 & 0.5     & 36 &$\sim$45 & 147   \\ 
64    & 5:36:22.8 & --6:46:06 &HH~1/2-VLA& --  & AS-536229-64618 & 52 $\times$ 30  & 6.2 &  1.36 & MMS~64    & 42 $\times$ 27(25)  & 5.61 &  0.42 &$>$3     & 32 &$\sim$145& 1/2   \\ 
65    &(5:36:21.2 & --6:46:08)& ?      & --    & ?               &  --    & --  &  --   & --        & --         & --   &  --   & 1.9     & -- & 110     & 144   \\ 
66    & 5:38:40.5 & --6:58:22 & IRS~66 & -0.04 & no obs          &  --    & --  &  --   & MMS~66    & 13 $\times$ 13(168) & 0.93 &  0.19 & 2.6     &  4 & 130     &    -- \\ 
67    & 5:37:57.0 & --7:06:56 & IRS~67 & 2.07  & no obs          &  --    & --  &  --   & MMS~67    & 22 $\times$ 20(98)  & 0.79 &  0.14 & 16      & 18 & 126     &38/43/64\\ 
68    & 5:38:07.5 & --7:08:29 & IRS~68 & 0.25  & no obs          &  --    & --  &  --   & MMS~68    & 24 $\times$ 17(2)   & 0.12 &  0.02 & 1.2     & 10 & 130     &    -- \\ 
69    & 5:39:05.8 & --7:10:39 & IRS~69 & 2.63  & no obs          &  --    & --  &  --   &undetected & --         & --   &  --   &$\sim$0.4& -- & 90      &    -- \\ 
70    & 5:38:42.8 & --7:12:44 & IRS~70 & --0.23 & no obs          &  --    & --  &  --   & MMS~70    & 15 $\times$ 11(145) & 0.07 &  0.04 &$\sim$1.7& 30 &$\sim$135& 449   \\ 
71    & 5:39:00.9 & --7:20:23 & IRS~71 & 1.55  & no obs          &  --    & --  &  --   & MMS~71    & 65 $\times$ 31(173) & 0.40 &  0.01 & 0.9     & -- & 128     &    -- \\ 
72    & 5:39:19.6 & --7:26:19 & IRS~72b& 0.33  & no obs          &  --    & --  &  --   & MMS~72    & 22 $\times$ 20(176) & 3.17 &  0.30 & 5.4     & 70 & 65      & 469   \\ 
73    & 5:39:22.3 & --7:26:45 & IRS~73 & --0.37 & no obs          &  --    & --  &  --   & MMS~73    & 15 $\times$ 10(24)  & 0.34 &  0.09 & 2.3     & 14 & 133     & 470   \\ 
74    &(5:40:23.7 & --7:20:32)& ?      & --    & no obs          &  --    & --  &  --   & ?         & --         & --   &  --   &$>$1.0   & -- & 53      &    -- \\ 
75    &(5:40:25.8 & --7:22:14)& ?      & --    & no obs          &  --    & --  &  --   & ?         & --         & --   &  --   &$>$1.5   & -- & 45      &    -- \\ 
76    & 5:39:55.9 & --7:30:28 & IRS~76 & 2.70  & no obs          &  --    & --  &  --   & MMS~76    & 16 $\times$ 15(117) & 2.62 &  0.55 & 14      & -- &$\sim$60 &  65   \\  
      \hline
\end{tabular}
\medskip
$^{{a}}$ Position of the H$_2$ outflow source if one is listed in Col.~4.  Otherwise, the position of the brightest knot in the flow is given (enclosed in brackets). Note that the well-known
sources of the HH~1/2, HH~83 and V380-Ori-NE flows were not identified in our tables of Spitzer protostars or disc-excess sources. \\
$^{{b}}$ Most likely H$_2$ outflow source from the Spitzer photometry together with the spectral index, $\alpha$.  Just a question mark means there is no obvious H$_2$~flow source candidate. \\
$^{{c}}$ 850\mic\ dust core coincident with the H$_2$~outflow source (from Nutter \& \mbox{Ward-Thompson} \cite{nut07}).  The source must lie within a 14\arcsec~radius (the JCMT~beam at~850\mic) of the core position given by Nutter \& Ward-Thompson in their Table~A.1.  ''Emission'' or ``undetected'' means that no core appears in their table.  However, ``emission'' means that the source identified in Col.~4 is associated with diffuse 850\mic~emission (surface brightness
$>$100~mJy~beam$^{-1}$, which is roughly equivalent to~5$\sigma$); a question mark means there are cores (or emission) in the vicinity which could be associated with the outflow or its source; ``no~obs'' means that the outflow is outside the bounds of the SCUBA~map.  The core size (major/minor axis dimensions), $Ap_{850}$, and integrated flux, $I_{850}$, are given for each core; $F_{850}$ is the flux, in Jy~beam$^{-1}$, measured towards each IRS source (not necessarily the
peak flux of the associated core). \\
$^{{d}}$ Same as for the 850\mic\ cores, but for cores identified from our analysis of the 1200\mic\ observations of Stanke et~al. (in~prep.). In this case the source must lie within 11\arcsec\
of the core centroid; ``emission'' corresponds to a surface brightness $>$75~mJy~beam$^{-1}$ ($\sim$$5\sigma$). The values given in brackets in the $Ap_{1200}$~column are the orientation of the core major axis (this information was not available for the 850\mic~cores). \\
$^{{e}}$ Entire length ($L$) of all H$_2$ knots (in both lobes), or the distance from the source to the most distant H$_2$~knot if only one flow lobe is identified; opening angle~($\theta$) measured
from a cone centred on the outflow source that includes all H$_2$~features in the flow; position angle~(PA) measured east of north. \\
$^{{f}}$ Associated HH objects, if any are known.
\end{table}