\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}