<=== 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