2007PASP..119..855W

Query : 2007PASP..119..855W

2007PASP..119..855W - Publ. Astron. Soc. Pac., 119, 855-870 (2007/August-0)

The James Clerk Maxwell Telescope legacy survey of nearby star-forming regions in the Gould belt.

WARD-THOMPSON D., DI FRANCESCO J., HATCHELL J., HOGERHEIJDE M.R., NUTTER D., BASTIEN P., BASU S., BONNELL I., BOWEY J., BRUNT C., BUCKLE J., BUTNER H., CAVANAGH B., CHRYSOSTOMOU A., CURTIS E., DAVIS C.J., DENT W.R.F., VAN DISHOECK E., EDMUNDS M.G., FICH M., FIEGE J., FISSEL L., FRIBERG P., FRIESEN R., FRIESWIJK W., FULLER G.A., GOSLING A., GRAVES S., GREAVES J.S., HELMICH F., HILLS R.E., HOLLAND W.S., HOUDE M., JAYAWARDHANA R., JOHNSTONE D., JONCAS G., KIRK H., KIRK J.M., KNEE L.B.G., MATTHEWS B., MATTHEWS H., MATZNER C., MORIARTY-SCHIEVEN G.H., NAYLOR D., PADMAN R., PLUME R., RAWLINGS J.M.C., REDMAN R.O., REID M., RICHER J.S., SHIPMAN R., SIMPSON R.J., SPAANS M., STAMATELLOS D., TSAMIS Y.G., VITI S., WEFERLING B., WHITE G.J., WHITWORTH A.P., WOUTERLOOT J., YATES J. and ZHU M.

Abstract (from CDS):

This paper describes a James Clerk Maxwell Telescope (JCMT) legacy survey that has been awarded roughly 500 hr of observing time to be carried out from 2007 to 2009. In this survey, we will map with SCUBA-2 (Submillimetre Common-User Bolometer Array 2) almost all of the well-known low-mass and intermediate-mass star-forming regions within 0.5 kpc that are accessible from the JCMT. Most of these locations are associated with the Gould Belt. From these observations, we will produce a flux-limited snapshot of star formation near the Sun, providing a legacy of images, as well as point-source and extended-source catalogs, over almost 700 deg2 of sky. The resulting images will yield the first catalog of prestellar and protostellar sources selected by submillimeter continuum emission, and should increase the number of known sources by more than an order of magnitude. We will also obtain with the array receiver HARP (Heterodyne Array Receiver Program) CO maps, in three CO isotopologues, of a large typical sample of prestellar and protostellar sources. We will then map the brightest hundred sources with the SCUBA-2 polarimeter (POL-2), producing the first statistically significant set of polarization maps in the submillimeter. The images and source catalogs will be a powerful reference set for astronomers, providing a detailed legacy archive for future telescopes, including ALMA, Herschel, and JWST.

Abstract Copyright: ∼

Journal keyword(s): ISM

Simbad objects: 48

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Number of rows : 48
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 LDN 1448 DNe 03 22.5 +30 35           ~ 546 0
2 NGC 1333 OpC 03 29 09.2 +31 20 59           ~ 1575 1
3 Barnard 1 MoC 03 33 16.3 +31 07 51           ~ 350 0
4 NAME Per Region reg 03 37 00.0 +31 15 00           ~ 296 0
5 IC 348 OpC 03 44 31.1 +32 10 02           ~ 1476 1
6 NAME [BM89] B5 DNe 03 47 38.3 +32 52 43           ~ 224 0
7 LDN 1471 DNe 03 48.0 +32 54           ~ 349 0
8 LDN 1447 DNe 04 03 23 +40 48.0           ~ 10 0
9 LDN 1473 DNe 04 11.7 +38 10           ~ 26 0
10 NAME [BM89] L1506 PoC 04 18 31.1 +25 19 25           ~ 43 0
11 LDN 1506 DNe 04 20.0 +25 17           ~ 81 0
12 NAME Auriga reg 04 20 00.0 +38 05 00           ~ 238 0
13 LDN 1478 DNe 04 23.3 +37 07           ~ 26 0
14 LDN 1481 DNe 04 39.3 +38 19           ~ 10 0
15 NAME Taurus Complex SFR 04 41.0 +25 52           ~ 4971 0
16 LDN 1496 DNe 04 43.2 +32 06           ~ 8 0
17 M 42 HII 05 35 16.8 -05 23 15           ~ 4411 0
18 NGC 2024 Cl* 05 41 43 -01 50.5           ~ 1198 1
19 Lupus 1 Cld 15 43 02.1 -34 09 06           ~ 320 0
20 Lupus 2 MoC 15 57 08 -37 47.1           ~ 119 1
21 Lupus 5 MoC 16 21 -37.5           ~ 63 0
22 NAME Ophiuchus Molecular Cloud SFR 16 28 06 -24 32.5           ~ 3969 1
23 LDN 1752 DNe 16 29.9 -19 36           ~ 9 0
24 LDN 1709 DNe 16 31 34.8 -24 02 55           ~ 84 0
25 LDN 1689 DNe 16 32 22.5 -24 28 29           ~ 153 0
26 LDN 1729 DNe 16 43.0 -24 06           ~ 31 0
27 LDN 204 DNe 16 47 47.3 -12 05 16           ~ 55 0
28 LDN 137 DNe 16 50.9 -15 25           ~ 9 0
29 NAME Scorpius Complex reg 16 51 00.0 -25 20 00           ~ 44 0
30 LDN 1746 DNe 17 11.3 -27 22           ~ 157 0
31 LDN 1768 DNe 17 20.1 -26 52           ~ 5 0
32 LDN 69 DNe 17 27 58.3 -23 59 58           ~ 7 0
33 NAME the Pipe Nebula DNe 17 30 -25.0           ~ 442 1
34 LDN 52 DNe 17 32 11 -25 25.6           ~ 9 0
35 LDN 432 DNe 17 58 27 -05 40.9           ~ 10 0
36 LDN 503 DNe 18 29 27 -04 39.0           ~ 6 0
37 NAME Serpens Cloud SFR 18 29 49 +01 14.8           ~ 1195 1
38 LDN 571 DNe 18 30.6 +00 02           ~ 4 0
39 LDN 536 DNe 18 34.6 -02 33           ~ 3 0
40 NAME CrA Complex reg 19 15 00.0 -37 30 00           ~ 118 1
41 LDN 1148 DNe 20 40 31.6 +67 21 45           ~ 68 0
42 IRAS 20582+7724 Y*O 20 57 12.9250225656 +77 35 43.656301932           ~ 119 0
43 LDN 1228 DNe 20 57 13 +77 35.8           ~ 131 0
44 LDN 1172 DNe 21 02 27.7 +67 54 08           ~ 57 0
45 NAME Cepheus Region reg 21 20 00.0 +72 30 00           ~ 126 0
46 LDN 1241 DNe 21 50.0 +76 44           ~ 19 0
47 IC 5146 OpC 21 53 29.3 +47 14 46           ~ 507 2
48 LDN 1251 DNe 22 36.1 +75 16           ~ 119 0

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