<=== observer ===> "PSARA",\ "Saraceno, P.S.",\ "Istituto Fisica Spazio Interplanetario",\ "Consiglio Nazionale Ricerche",\ "G.Galilei",\ "",\ "00044",\ "Frascati - Roma",\ "Italy",\ "39 6 94186240",\ "39 6 9426814",\ "saraceno@hp.ifsi.fra.cnr.it" <=== proposal ===> "EARLY",1,2,\ {"Star formation","circumstellar disks","circumstellar envelopes",\ "bipolar outflows"},\ {"LWS consortium","P.Ade","M.Barlow","E.Caux","C.Ceccarelli","P.Clegg",\ "M.Cohen","J.Fischer","I.Furniss","B.Glencross","M.Griffin","K. King",\ "R.Liseau","D.Lorenzetti","F.Palla","D.Naylor","B.Nisini","N.Rieu",\ "P.Saraceno","H.Smith","L.Spinoglio","G.White"} <=== title ===> Pre M.S. evolution: The early phase of star formation <=== abstract ===> SCIENTIFIC ABSTRACT The main objective of the LWS proposals on Pre-Main Sequence evolution is the understanding of the evolution of matter from the dilute, cold interstellar state of the dark molecular clouds to the compact, hot stellar state of the main-sequence stars. The present proposal deals with the earlier evolutionary phase. The discovery of a real protostar, i.e. an object that derives the majority of its luminosity from the accretion of infalling material, is one of the most important observations for our understanding of the overall stellar evolution. While a number of plausible candidates do exist among the IRAS Class I sources, fully convincing kinematic evidence for infall is still missing. Far-infrared spectroscopy may be one of the means to provide this evidence. An essential condition for the formation of stars in molecular clouds is the presence of dense clumps of matter, as revealed both from molecular lines (e.g. NH_3 and CS) and millimetre continuum emitted by circumstellar dust. These clumps are often coincident with Class I sources. We therefore consider dense molecular cores and the IR sources associated with millimetric emission as the prime candidates for studying the earliest evolutionary stages of star formation. Both spectrometers will be used in low resolution mode, in order to detect the various spectral features expected to trace the different physical conditions around the accreting protostellar objects. From the outside (at scales of hundreds of astronomical units) we expect to detect: - molecular emission from various species (such as water and CO), tracing the parental material; - fine structure lines such as the [OI]63.157 micron, tracing the transition region between fully ionised and molecular gas; - the high quantum number hydrogen recombination lines tracing, together with the IR coronal lines, the hotter and denser gas of the regions close to the accretion shock. - the velocity field can be comparing the observed line intensities with the models of the emitting regions. Using the grating spectrometers the properties of the solid state matter will also be studied directly in the observed shape of the "continuum" and, perhaps, also indirectly from the determination of the relative elemental abundances. In particular, we may obtain unexpected results regarding the phases of the dust in extremely dense interstellar environments, where grain evolution can be quite different from that of the diffuse medium. OBSERVATION SUMMARY Full spectral scans using the LWS in grating mode are planned for all our targets. The "on source" integration time for LWS Grating spectra are computed in order to observe with S/N=10 lines of 2 10^-20 W/cm^2. For the brightest sources this limit is reduced in order to observe with S/N=10 lines that are 1/200 of their 60 um continuum. In presence of an "outflow" the "off source" observation is done carrying out a map (in "raster scan") of the flow with a full grating spectrum in each point of the map. The total integration time spent on all the points of the map will be similar to the one spent on the single "on source" point; the reference "off source" point will be therefore built by binning together all the points of the map. A full SWS grating scan is foreseen for all the objects (with the exception of the objects that will be observed in the SWS guaranteed time) with a 25 um IRAS flux sufficient to give S/N=10 on a line that is 1/30 of the continuum in the SWS01 mode. We also scan with SWS01 mode those points in the flow where evidence of near-infrared shock excited emission exists. We have chosen a few template objects representative of the evolutionary stages addressed in this proposal for FP observations of lines expected to be excited in the different physical regimes. <=== scientific_justification ===> Allocated time per priorities and AOTs (autumn launch) LWS01 SWS01 LWS03-LWS04 top 40% 83154 5620 - second 30% 36805 26600 1818 third 30% 40330 5580 20396 ---------------------------------------------- TOT 160289 37800 22214 Allocated time per priorities and AOTs (spring launch) LWS01 SWS01 LWS03-LWS04 top 40% 64983 14680 6908 second 30% 56802 7420 682 third 30% 35811 7440 22234 ---------------------------------------------- TOT 157596 29540 29824 ***************** AOT LWS01: Full grating scans from 43 to 196.7 microns with spectral sample of 4 and fast-on flag are required for all sources. The following table contains the information needed to evaluate the integration times according to the code specified in the table for each individual source. The meaning of the code number is given at the bottom of the table. Name hole Code F(25um) F(60um) F(100um) F(OI)(10^-15 W/m2) 6300A 63um HH46 IRS o 1 6.4 25.8 57.3 IRAS12496-7650 o 1 85.6 104.9 87.4 HH52 o 1 HH53A o 1 HH54 o 1 HH54B o 1 IRAS13547-3944 o 1 8.9 67.0 202.0 L134A o 9 4.0 5.0 9.0 VLA1623 o 2 30.0 470.0 525.0 WL16 o 2 40.0 202.0 202.0 EL29 o 2 82.0 230.0 590.0 RhoOphB1 o 1 15.0 43.0 108.0 IRS37 o 1 12.0 85.0 190.0 IRS43 o 1 27.0 136.0 136.0 IRS44 o 1 47.0 110.0 360.0 IRAS16293-2422 o 2 1.8 254.0 1000.0 IRAS18148-0440 o 1 7.0 89.0 164.0 IRAS18273+0113 o 1 3.2 153.0 746.0 HH80 o 9 HH80N o 9 HH81 o 9 GGD27IRS o 2 347.0 2770.0 3710.0 L 723 o 1 0.4 6.8 22.0 B335 o 1 <0.3 8.3 42.0 HH119 A o 1 HH119 B o 1 HH119 C o 1 B361 o/s 1 0.9 17.0 38.0 NGC7129-FIRS2 o/s 1 2.0 67.0 153.0 IRAS22343+7501 o/s 1 26.0 66.0 79.0 IRAS22376+7455 o/s 1 5.6 32.0 66.0 IRAS22541+6154 o/s 1 8.2 133.0 477.0 L1448 o/s 1 2.0 4.0 10.0 RNO15FIR s 1 5.4 53.0 100.0 NGC1333 IRAS1 o/s 1 19.0 55.0 73.0 HH12 E o/s 1 SSV13 o/s 2 45.0 203.0 355.0 HH7A o/s 1 NGC1333 IRAS4 o/s 1 2.0 30.0 143.0 IRAS03282+3035 s 1 <0.3 2.3 13.0 B5-IRS1 s 1 5.5 18.0 22.0 L1489-VLA1 s 1 18.0 52.8 65.7 L1551-IRS5 o/s 2 106.0 373.0 456.0 HH 34 s 1 HH 34 IRS s 1 7.0 27.0 117.0 HH 42 s 7 6.6 IRAS05338-0647 s 1 5.2 123.0 321.0 VLA1 s 1 2.0 4.0 10.0 HH1C s 6 1.25 HH2C s 6 1.1 HH43 s 7 6.5 HH43 IRS s 1 1.0 4.0 9.0 SSV59 s 1 7.0 25.0 78.0 HH24A s 1 MLY25 s 1 8.5 73.0 150.0 NGC2264G s 1 2.0 4.0 10.0 Code: time assigned according to the following criteria: 1. to detect lines of 2 10^(-16) W/m2 at S/N = 10. 2. to detect lines which are 1/200 of their 60um emission at S/N = 10. 6. HH objects: to observe a line which is 1/10 of the [OI]63.157um line as extimated from the observed [OI]63.15700 A line. 7. HH objects: to observe a line which is 1/10 of the observed [OI]63.157um line. 9. to detect lines of 1 10^(-15) W/m2 at S/N=10. AOT LWS03: Fabry-Perot scans covering a range of 1000km s-1, with 2 samples per resolution element. The following table gives the lines and corrected spectral ranges to be observed in the source HH80. For the hole in Orion: object line# w-start* w-end* HH80: [OI]63.157 63.10 63.32 [OI]145.50 145.37 145.87 [CII]157.74 157.61 158.13 OH 119.23+119.44 119.24 119.54 H2O 99.49 99.40 99.74 H2O 116.78 116.68 117.08 H2O 187.8 187.65 188.25 # rest wavelength * corrected for proper motion AOT LWS04: Fabry-Perot scans with 9 resolution elements and 4 samples per resolution element. The following table give the sources and lines to be observed. For the hole in Sagittarius: HH7A: [OI]63.157,145.53, [CII]157.74, [OIII]51.69,88.16, OH 119.23,119.44, H2O 116.78,121.721,146.922,187.80 NGC1333 IRAS1: [OI]63.157, [CII]157.74, HI 88.730,111.815, CO 153.267,162.812,173.631, H2O 82.032,99.493,116.78,187.80 L1551 IRS5: [OI]63.157, [CII]157.74, HI 88.730,111.815, CO 153.267,162.812,173.631, H2O 82.032,99.493,116.78,187.80 SSV13: [OI]63.157, [CII]157.74, HI 88.730,111.815, CO 153.267,162.812,173.631, H2O 82.032,99.493,116.78,187.80 For the hole in Orion: IRAS16293-2422: [OI]63.157, [CII]157.74, HI 88.730,111.815, CO 153.267,162.812,173.631, H2O 82.032,99.493,116.78,187.80 Elias 29: [OI]63.157, [CII]157.74, HI 88.730,111.815, CO 153.267,162.812,173.631, H2O 82.032,99.493,116.78,187.80 The integration times were computed in order to detect with S/N = 10 lines of integrated flux 1-3 10(-19)W/cm2, and 100 Km/sec wide. AOT SWS01: Full grating scans from 2.43 to 45 microns with a detector reset time of 2 sec, requiring 25 minutes of integration time per object (+overheads). ********************** Time distribution for autumn launch targets Team top 40% second 30% last 30% LWS 88774 65223 66306 total 88774 65223 66306 Time distribution for spring launch targets Team top 40% second 30% last 30% LWS 86571 64904 65485 total 86571 64904 65485 ********************** Raster scans information autumn launch targets No Name coord. center M dM N dN P.A. 2 L1448 flow 3.37692 30.53722 1 0 3 173 157.5 3 L1448 flow 3.37578 30.58528 1 0 3 27 156 5 IRAS1 Off Sr. 3.42597 31.05361 1 0 2 200 0 8 SSV13 flow 3.43247 31.10306 4 100 6 100 0 17 L1551 Off. S 4.47783 18.02833 1 0 2 100 48 18 HH 46 OFF. S. 8.40389 -50.84778 1 0 3 98 57 22 12496-7650flow 12.82928 -76.84250 3 100 3 100 90 23 12522-7640flow 12.85767 -76.69778 3 100 3 100 90 30 13547-3944CG12 13.91122 -39.73528 1 0 2 50 90 31 13547-3944flow 13.91167 -39.78083 1 0 2 154 159 32 L134A 15.84947 -4.44361 3 100 3 100 0 34 VLA 1623 flow 16.39025 -24.29611 1 0 7 50 124 36 WL 16 Off 16.40008 -24.51028 1 0 2 200 176 37 El29-WL16 16.40211 -24.51028 1 0 3 100 86 40 rhoOphB1-IRS37 16.40228 -24.37167 1 0 3 100 164 41 IRS37 Off 16.40228 -24.37167 1 0 2 200 74 42 IRS43-44 16.40728 -24.54806 1 0 3 78 11 43 IRS44 Off 16.40728 -24.54806 1 0 2 156 101 45 16293-2422flow 16.49017 -24.36750 1 0 4 100 90 48 18148-0440flow 18.24739 -4.68306 1 0 2 200 90 62 GGD 27 IRS 18.27028 -20.81361 1 0 3 100 0 65 18273+0113flow 18.28833 1.22056 1 0 2 200 0 68 L 723 flow 19.26150 19.11250 3 100 5 100 106 74 B335 flow 19.57642 7.45667 3 100 7 100 90 78 B361 flow 21.17528 47.20056 1 0 2 200 90 80 NGC7129 flow 21.69908 65.85833 3 100 6 100 0 81 22343+7501flow 22.56353 75.97112 5 200 4 200 127 87 22541+6154 Off 22.75228 61.90583 1 0 2 360 135 spring_launch_targets No Name coord. center M dM N dN P.A. 2 L1448 flow 3.37692 30.53722 1 0 3 173 157.5 3 L1448 flow 3.37578 30.58528 1 0 3 27 156 5 RNO15 FIRflow 3.41006 30.04444 3 100 7 100 135 9 IRAS1 Off Sr. 3.42597 31.05361 1 0 2 200 0 12 SSV13 flow 3.43247 31.10306 4 100 6 100 0 25 03282+3035flow 3.47089 30.58722 1 0 4 100 124 26 03282+3035 3.47367 30.56750 1 0 2 26 82 28 B5 IRS1flo 3.74219 32.70834 2 100 6 100 90 29 L1489-VLA1flow 4.02633 26.17972 4 100 3 100 0 31 L1551blue str 4.45778 17.76556 1 0 5 200 48 32 L1551blue lobe 4.47097 17.93583 5 100 9 100 48 36 L1551red lobe 4.48308 18.08861 5 100 7 100 48 37 L1551red str. 4.49433 18.23445 1 0 5 200 48 58 HH34 IRS 5.55100 -6.48056 1 0 3 110 166 40 HH42 5.55942 -5.10861 1 0 2 100 90 43 05338-0647Off. 5.56486 -6.79306 4 100 3 100 90 49 HH43 IRS 5.59503 -7.16917 1 0 3 73 125 52 SSV59 flow 5.72586 -0.22806 4 100 5 100 0 56 MLY 25 Off Sr. 6.63806 10.30278 1 0 2 200 90 58 NGC2264G flow 6.64167 9.98167 1 0 4 100 90 60 B361 flow 21.17528 47.20056 1 0 2 200 90 62 NGC7129 flow 21.69908 65.85833 3 100 6 100 0 63 22343+7501flow 22.56353 75.97112 5 200 4 200 127 68 22541+6154 Off 22.75228 61.90583 1 0 2 360 135 <=== autumn_launch_targets ===> 1, "LWS01",1.0,"N","L1448 ", 3.37619, 30.55972,1950,0.,0., 2426, 2 2, "LWS01",1.0,"N","L1448 flow ", 3.37692, 30.53722,1950,0.,0., 2287, 0 3, "SWS01",3.0,"N","L1448 flow ", 3.37578, 30.58528,1950,0.,0., 5580, 0 4, "LWS01",1.0,"N","NGC1333 IRAS1 ", 3.42597, 31.05361,1950,0.,0., 2426, 5 5, "LWS01",1.0,"N","IRAS1 Off Sr. ", 3.42597, 31.05361,1950,0.,0., 2190, 6 6, "LWS01",1.0,"N","HH12 E ", 3.43158, 31.16333,1950,0.,0., 2266, 0 7, "SWS01",2.0,"N","HH12 E ", 3.43158, 31.16333,1950,0.,0., 1980,10 8, "LWS01",1.0,"N","SSV13 flow ", 3.43247, 31.10306,1950,0.,0., 8110, 0 9, "LWS01",1.0,"N","HH7red lobe ", 3.43261, 31.10028,1950,0.,0., 2426,11 10, "SWS01",2.0,"N","HH7red lobe ", 3.43261, 31.10028,1950,0.,0., 1820,14 11, "LWS01",1.0,"N","SSV13 ", 3.43283, 31.09556,1950,0.,0., 2266,13 12, "SWS01",1.0,"N","SSV13 ", 3.43283, 31.09556,1950,0.,0., 1980,15 13, "LWS01",1.0,"N","HH7A ", 3.43411, 31.08611,1950,0.,0., 2426, 0 14, "SWS01",2.0,"N","HH7A ", 3.43411, 31.08611,1950,0.,0., 1820, 0 15, "LWS01",1.0,"N","NGC1333 IRAS4 ", 3.43489, 31.05055,1950,0.,0., 2266, 0 16, "LWS01",1.0,"N","L1551 IRS5 ", 4.47783, 18.02833,1950,0.,0., 1048,17 17, "LWS01",1.0,"N","L1551IRS5 Off.", 4.47783, 18.02833,1950,0.,0., 744, 0 18, "LWS01",1.0,"N","HH 46 Off. ", 8.40389, -50.84778,1950,0.,0., 2350,20 19, "SWS01",2.0,"N","HH 46 IRS ", 8.40458, -50.84528,1950,0.,0., 1980, 0 20, "LWS01",1.0,"N","HH 46 IRS ", 8.40458, -50.84528,1950,0.,0., 2426, 0 21, "LWS01",3.0,"N","12496-7650 ", 12.82722, -76.84583,1950,0.,0., 2266,22 22, "LWS01",3.0,"N","12496-7650flow", 12.82928, -76.84250,1950,0.,0., 2629, 0 23, "LWS01",3.0,"N","12522-7640flow", 12.85767, -76.69778,1950,0.,0., 2789, 0 24, "LWS01",2.0,"N","HH 52 ", 12.85778, -76.69305,1950,0.,0., 2426,25 25, "SWS01",2.0,"N","HH 52 ", 12.85778, -76.69305,1950,0.,0., 1820,26 26, "LWS01",2.0,"N","HH 53A ", 12.86006, -76.68667,1950,0.,0., 2266,27 27, "SWS01",2.0,"N","HH 53A ", 12.86006, -76.68667,1950,0.,0., 1820, 0 28, "SWS01",2.0,"N","HH 54 ", 12.86906, -76.67111,1950,0.,0., 1980,29 29, "LWS01",2.0,"N","HH 54B ", 12.86961, -76.66778,1950,0.,0., 2426, 0 30, "LWS01",3.0,"N","13547-3944CG12", 13.91122, -39.73528,1950,0.,0., 4287,31 31, "LWS01",3.0,"N","13547-3944flow", 13.91167, -39.78083,1950,0.,0., 2190, 0 32, "LWS01",3.0,"N","L134A ", 15.84947, -4.44361,1950,0.,0., 5309, 0 33, "LWS01",1.0,"N","VLA 1623 ", 16.39025, -24.29611,1950,0.,0., 2266,34 34, "LWS01",1.0,"N","VLA 1623 flow ", 16.39025, -24.29611,1950,0.,0., 1136, 0 35, "SWS01",2.0,"N","WL 16 ", 16.40008, -24.51222,1950,0.,0., 1980, 0 36, "LWS01",1.0,"N","WL 16 Off ", 16.40008, -24.51028,1950,0.,0., 2350,37 37, "LWS01",1.0,"N","El29-WL16 ", 16.40211, -24.51028,1950,0.,0., 6421, 0 38, "LWS04",3.0,"N","El29 ", 16.40211, -24.51028,1950,0.,0., 3544,39 39, "LWS04",3.0,"N","El29 ", 16.40211, -24.51028,1950,0.,0., 462, 0 40, "LWS01",2.0,"N","rhoOphB1-IRS37", 16.40228, -24.37167,1950,0.,0., 6581,41 41, "LWS01",2.0,"N","IRS37 Off ", 16.40228, -24.37167,1950,0.,0., 2190, 0 42, "LWS01",3.0,"N","IRS43-44 ", 16.40728, -24.54806,1950,0.,0., 6581,43 43, "LWS01",3.0,"N","IRS44 Off ", 16.40728, -24.54806,1950,0.,0., 2190, 0 44, "LWS01",1.0,"N","16293-2422 ", 16.48914, -24.37028,1950,0.,0., 1740,45 45, "LWS01",1.0,"N","16293-2422flow", 16.49017, -24.36750,1950,0.,0., 1238, 0 46, "LWS04",3.0,"N","16293-2422 ", 16.48914, -24.37028,1950,0.,0., 3544,47 47, "LWS04",3.0,"N","16293-2422 ", 16.48914, -24.37028,1950,0.,0., 462, 0 48, "LWS01",2.0,"N","18148-0440flow", 18.24739, -4.68306,1950,0.,0., 2350,49 49, "LWS01",2.0,"N","18148-0440 ", 18.24739, -4.68028,1950,0.,0., 2266, 0 50, "LWS01",1.0,"N","HH 80 ", 18.26858, -20.88500,1950,0.,0., 1113,51 51, "SWS01",1.0,"N","HH 80 ", 18.26858, -20.88500,1950,0.,0., 1820,60 52, "LWS03",3.0,"N","HH 80 ", 18.26858, -20.88500,1950,0.,0., 1408,53 53, "LWS03",3.0,"N","HH 80 ", 18.26858, -20.88500,1950,0.,0., 1034,54 54, "LWS03",3.0,"N","HH 80 ", 18.26858, -20.88500,1950,0.,0., 1640,55 55, "LWS03",3.0,"N","HH 80 ", 18.26858, -20.88500,1950,0.,0., 1626,57 56, "LWS03",2.0,"N","HH 80 ", 18.26858, -20.88500,1950,0.,0., 1818, 0 57, "LWS03",3.0,"N","HH 80 ", 18.26858, -20.88500,1950,0.,0., 1696, 0 58, "LWS03",3.0,"N","HH 80 ", 18.26858, -20.88500,1950,0.,0., 1408,59 59, "LWS03",3.0,"N","HH 80 ", 18.26858, -20.88500,1950,0.,0., 3572, 0 60, "LWS01",1.0,"N","HH 81 ", 18.26875, -20.87306,1950,0.,0., 953,61 61, "SWS01",1.0,"N","HH 81 ", 18.26875, -20.87306,1950,0.,0., 1820,62 62, "LWS01",1.0,"N","GGD 27 IRS ", 18.27028, -20.81361,1950,0.,0., 858,63 63, "LWS01",1.0,"N","HH 80 N ", 18.27244, -20.71472,1950,0.,0., 953, 0 64, "SWS01",2.0,"N","HH 80 N ", 18.27244, -20.71472,1950,0.,0., 1980, 0 65, "LWS01",3.0,"N","18273+0113flow", 18.28833, 1.22056,1950,0.,0., 2350,66 66, "LWS01",3.0,"N","18273+0113 ", 18.45500, 1.22056,1950,0.,0., 2266, 0 67, "LWS01",3.0,"N","L 723 ", 19.26150, 19.11250,1950,0.,0., 2426,68 68, "LWS01",3.0,"N","L 723 flow ", 19.26150, 19.11250,1950,0.,0., 5047, 0 69, "LWS01",1.0,"N","HH119 A ", 19.57383, 7.45667,1950,0.,0., 2426,71 70, "SWS01",2.0,"N","HH119 A ", 19.57383, 7.45667,1950,0.,0., 1980,72 71, "LWS01",1.0,"N","HH119 B ", 19.57542, 7.45556,1950,0.,0., 2266,75 72, "SWS01",2.0,"N","HH119 B ", 19.57542, 7.45556,1950,0.,0., 1820,76 73, "LWS01",1.0,"N","B335 ", 19.57642, 7.45667,1950,0.,0., 2226,74 74, "LWS01",1.0,"N","B335 flow ", 19.57642, 7.45667,1950,0.,0., 6997, 0 75, "LWS01",1.0,"N","HH119 C ", 19.57753, 7.45556,1950,0.,0., 2426, 0 76, "SWS01",2.0,"N","HH119 C ", 19.57753, 7.45556,1950,0.,0., 1820, 0 77, "LWS01",2.0,"N","B361 ", 21.17528, 47.20056,1950,0.,0., 2426,78 78, "LWS01",2.0,"N","B361 flow ", 21.17528, 47.20056,1950,0.,0., 2190, 0 79, "LWS01",1.0,"N","NGC7129-FIRS2 ", 21.69767, 65.83055,1950,0.,0., 2426,80 80, "LWS01",1.0,"N","NGC7129 flow ", 21.69908, 65.85833,1950,0.,0., 5086, 0 81, "LWS01",2.0,"N","22343+7501flow", 22.56353, 75.97112,1950,0.,0., 6832, 0 82, "LWS01",2.0,"N","22343+7501 ", 22.57278, 75.02556,1950,0.,0., 2426,83 83, "SWS01",2.0,"N","22343+7501 ", 22.57278, 75.02556,1950,0.,0., 1820, 0 84, "LWS01",2.0,"N","22376+7455 ", 22.62800, 74.93055,1950,0.,0., 2426, 0 85, "LWS01",1.0,"N","22541+6154 ", 22.75228, 61.90583,1950,0.,0., 2426,87 86, "SWS01",2.0,"N","22541+6154 ", 22.75228, 61.90583,1950,0.,0., 1980, 0 87, "LWS01",1.0,"N","22541+6154 Off", 22.75228, 61.90583,1950,0.,0., 2190, 0 <=== spring_launch_targets ===> 1, "LWS01",1.0,"N","L1448 ", 3.37619, 30.55972,1950,0.,0., 2426, 2 2, "LWS01",1.0,"N","L1448 flow ", 3.37692, 30.53722,1950,0.,0., 2287, 0 3, "SWS01",1.0,"N","L1448 flow ", 3.37578, 30.58528,1950,0.,0., 5580, 0 4, "LWS01",3.0,"N","RNO15 FIR ", 3.41006, 30.04444,1950,0.,0., 2426, 5 5, "LWS01",3.0,"N","RNO15 FIRflow ", 3.41006, 30.04444,1950,0.,0., 3448, 0 6, "LWS01",1.0,"N","NGC1333 IRAS1 ", 3.42597, 31.05361,1950,0.,0., 2426, 9 7, "LWS04",3.0,"N","NGC1333 IRAS1 ", 3.42597, 31.05361,1950,0.,0., 6908, 8 8, "LWS04",3.0,"N","NGC1333 IRAS1 ", 3.42597, 31.05361,1950,0.,0., 682, 0 9, "LWS01",1.0,"N","IRAS1 Off Sr. ", 3.42597, 31.05361,1950,0.,0., 2190, 0 10, "LWS01",1.0,"N","HH12 E ", 3.43158, 31.16333,1950,0.,0., 2266,11 11, "SWS01",1.0,"N","HH12 E ", 3.43158, 31.16333,1950,0.,0., 1820, 0 12, "LWS01",1.0,"N","SSV13 flow ", 3.43247, 31.10306,1950,0.,0., 8110, 0 13, "LWS01",1.0,"N","HH7red lobe ", 3.43261, 31.10028,1950,0.,0., 2426,14 14, "SWS01",1.0,"N","HH7red lobe ", 3.43261, 31.10028,1950,0.,0., 1820, 0 15, "LWS01",1.0,"N","SSV13 ", 3.43283, 31.09556,1950,0.,0., 2266,16 16, "SWS01",1.0,"N","SSV13 ", 3.43283, 31.09556,1950,0.,0., 1820, 0 17, "LWS04",1.0,"N","SSV13 ", 3.43283, 31.09556,1950,0.,0., 6908,18 18, "LWS04",2.0,"N","SSV13 ", 3.43283, 31.09556,1950,0.,0., 682, 0 19, "LWS01",1.0,"N","HH7A ", 3.43411, 31.08611,1950,0.,0., 2426,20 20, "SWS01",1.0,"N","HH7A ", 3.43411, 31.08611,1950,0.,0., 1820,23 21, "LWS04",3.0,"N","HH7A ", 3.43411, 31.08611,1950,0.,0., 6510,22 22, "LWS04",3.0,"N","HH7A ", 3.43411, 31.08611,1950,0.,0., 544, 0 23, "LWS01",1.0,"N","NGC1333 IRAS4 ", 3.43489, 31.05055,1950,0.,0., 2266, 0 24, "LWS01",2.0,"N","03282+3035 ", 3.47089, 30.58722,1950,0.,0., 2426,25 25, "LWS01",2.0,"N","03282+3035flow", 3.47089, 30.58722,1950,0.,0., 2384, 0 26, "SWS01",2.0,"N","03282+3035 ", 3.47367, 30.56750,1950,0.,0., 3780, 0 27, "LWS01",3.0,"N","B5 IRS1 ", 3.74219, 32.70834,1950,0.,0., 2426,28 28, "LWS01",3.0,"N","B5 IRS1 flow ", 3.74219, 32.70834,1950,0.,0., 2190, 0 29, "LWS01",1.0,"N","L1489-VLA1flow", 4.02633, 26.17972,1950,0.,0., 3530,30 30, "LWS01",1.0,"N","L1489-VLA1 ", 4.02789, 26.17972,1950,0.,0., 2266, 0 31, "LWS01",2.0,"N","L1551blue str.", 4.45778, 17.76556,1950,0.,0., 1957,37 32, "LWS01",1.0,"N","L1551blue lobe", 4.47097, 17.93583,1950,0.,0.,14957, 0 33, "LWS01",1.0,"N","L1551 IRS5 ", 4.47783, 18.02833,1950,0.,0., 1048, 0 34, "LWS04",3.0,"N","L1551 IRS5 ", 4.47783, 18.02833,1950,0.,0., 6908,35 35, "LWS04",3.0,"N","L1551 IRS5 ", 4.47783, 18.02833,1950,0.,0., 682, 0 36, "LWS01",2.0,"N","L1551red lobe ", 4.48308, 18.08861,1950,0.,0.,11010, 0 37, "LWS01",2.0,"N","L1551red str. ", 4.49433, 18.23445,1950,0.,0., 1957, 0 38, "LWS01",3.0,"N","HH34 IRS ", 5.55100, -6.48056,1950,0.,0., 6581,39 39, "SWS01",3.0,"N","HH34 ", 5.55144, -6.50944,1950,0.,0., 1820, 0 40, "LWS01",3.0,"N","HH42 ", 5.55942, -5.10861,1950,0.,0., 3770, 0 41, "LWS01",2.0,"N","05338-0647 ", 5.56469, -6.78750,1950,0.,0., 2266,42 42, "SWS01",2.0,"N","05338-0647 ", 5.56469, -6.78750,1950,0.,0., 1820,43 43, "LWS01",2.0,"N","05338-0647Off.", 5.56486, -6.79306,1950,0.,0., 3370, 0 44, "LWS01",2.0,"N","HH1C ", 5.56522, -6.78306,1950,0.,0., 2062,46 45, "SWS01",3.0,"N","HH1C ", 5.56522, -6.78306,1950,0.,0., 1980,48 46, "LWS01",2.0,"N","VLA1 ", 5.56583, -6.79917,1950,0.,0., 1902,47 47, "LWS01",2.0,"N","HH2C ", 5.56658, -6.81556,1950,0.,0., 1902, 0 48, "SWS01",3.0,"N","HH2C ", 5.56658, -6.81556,1950,0.,0., 1820, 0 49, "LWS01",1.0,"N","HH43 IRS ", 5.59503, -7.16917,1950,0.,0., 6581,50 50, "SWS01",1.0,"N","HH43 ", 5.59581, -7.18528,1950,0.,0., 1820, 0 51, "LWS01",3.0,"N","SSV59 ", 5.72533, -0.25611,1950,0.,0., 2426,52 52, "LWS01",3.0,"N","SSV59 flow ", 5.72586, -0.22806,1950,0.,0., 5502, 0 53, "LWS01",3.0,"N","HH24A ", 5.72656, -0.19222,1950,0.,0., 2426,54 54, "SWS01",3.0,"N","HH24A ", 5.72656, -0.19222,1950,0.,0., 1820, 0 55, "LWS01",3.0,"N","MLY 25 ", 6.63806, 10.30278,1950,0.,0., 2426,56 56, "LWS01",3.0,"N","MLY 25 Off Sr.", 6.63806, 10.30278,1950,0.,0., 2190, 0 57, "LWS01",2.0,"N","NGC2264G ", 6.63992, 9.98167,1950,0.,0., 2426,58 58, "LWS01",2.0,"N","NGC2264G flow ", 6.64167, 9.98167,1950,0.,0., 2384, 0 59, "LWS01",2.0,"N","B361 ", 21.17528, 47.20056,1950,0.,0., 2426,60 60, "LWS01",2.0,"N","B361 flow ", 21.17528, 47.20056,1950,0.,0., 2190, 0 61, "LWS01",1.0,"N","NGC7129-FIRS2 ", 21.69767, 65.83055,1950,0.,0., 2426,62 62, "LWS01",1.0,"N","NGC7129 flow ", 21.69908, 65.85833,1950,0.,0., 5086, 0 63, "LWS01",2.0,"N","22343+7501flow", 22.56353, 75.97112,1950,0.,0., 6832, 0 64, "LWS01",2.0,"N","22343+7501 ", 22.57278, 75.02556,1950,0.,0., 2426,65 65, "SWS01",2.0,"N","22343+7501 ", 22.57278, 75.02556,1950,0.,0., 1820,66 66, "LWS01",2.0,"N","22376+7455 ", 22.62800, 74.93055,1950,0.,0., 2266, 0 67, "LWS01",2.0,"N","22541+6154 ", 22.75228, 61.90583,1950,0.,0., 2426,68 68, "LWS01",2.0,"N","22541+6154 Off", 22.75228, 61.90583,1950,0.,0., 2190, 0