Table 2
Source fluxes as obtained in the Spitzer (3.6 μm, 4.5 μm, 5.8 μm, and 8.0 μm) and Herschel (70 μm, 160 μm, 250 μm, 350 μm, and 500 μm) bands, complemented with LABOCA 870 μm photometry and JHKs photometry as obtained with HAWK-I or from the 2MASS point-source catalogue.
Jet source | 3.6 μm | 4.5 μm | 5.8 μm | 8.0 μm | 70 μm | 160 μm | 250 μm | 350 μm | 500 μm | 870 μm | J | H | Ks | |
[mJy] | [mJy] | [mJy] | [mJy] | [Jy] | [Jy] | [Jy] | [Jy] | [Jy] | [Jy] | [mJy] | [mJy] | [mJy] | ||
|
||||||||||||||
HH666 IR | J104351.5–595521 | 137 | 238 | 338 | 405 | 64.6 | 70.5 | 43.9 | 25.6 | 11.4 | – | 0.33a | 1.9a | 12a |
HH902 IR | J104401.8–593030 | – | 4.17 | 29.6 | 70.0 | – | – | – | – | – | – | – | – | – |
HH903 IR | J104556.4–600608 | 2.68 | 6.24 | 35.4 | 115 | 19.1 | 55.7 | 37.9 | 16.7 | 8.07 | 2.03 | – | – | – |
HH1004 IR | J104644.8–601021 | 4.75 | 6.58 | 15.2 | – | 10.6 | 23.9 | – | – | – | – | 0.0540 | 0.206 | 0.624 |
HH1005 IR | J104644.2–601035 | – | 2.50 | – | – | 14.8 | 44.4 | 55.0 | 26.6 | 12.0 | 1.89 | – | – | – |
HH1006 IR | J104632.9–600354 | 2.57 | 3.06 | 10.6 | 23.1 | – | – | – | – | – | – | – | – | – |
HH1008/c-2 IR | J104445.4–595555 | 44.8 | 117 | 326 | 461 | 103 | 120 | 59.9 | 23.2 | 9.32 | 1.90 | 4.71 | 10.8 | 22.8 |
HH1010 IR | J104148.7–594338 | 2.11 | 3.96 | 10.8 | – | 5.67 | 12.5 | – | – | – | – | – | – | – |
HH1012 IR | J104438.7–593008 | 5.29 | 5.27 | 5.92 | – | – | – | – | – | – | – | – | – | – |
HH1013 IR | J104419.2–592612 | 8.46 | 11.7 | 16.7 | 25.1 | – | – | – | – | – | – | – | – | – |
HH1017 IR | J104441.5–593357 | 4.98 | 5.12 | – | – | – | – | – | – | – | – | – | – | – |
HH1018 IR | J104452.9–594526 | 4.54 | 5.39 | – | 10.5 | – | – | – | – | – | – | – | – | – |
HHc-1 IR | J104405.4–592941 | 6.00 | – | – | – | – | – | – | – | – | – | – | – | – |
HHc-3 IR | J104504.6–600303 | 0.611 | 0.712 | 2.34 | 5.02 | – | – | – | – | – | – | – | – | – |
HHc-5 IR | J104509.4–600203 | 20.0 | 21.1 | 27.9 | 41.2 | 8.12 | 18.1 | – | – | – | – | 1.02 | 3.17 | 6.52 |
HHc-6 IR | J104509.2–600220 | – | 1.29 | – | – | – | – | – | – | – | – | – | – | – |
HHc-7 IR | J104513.0–600259 | 2.25 | 2.00 | – | – | – | – | – | – | – | – | – | – | – |
HHc-8 IR | J104512.0–600310 | 5.48 | 8.33 | 13.2 | 16.0 | – | – | – | – | – | – | – | – | – |
HHc-13 IR | J104400.6–595427 | 13.2 | 12.5 | 13.8 | 17.1 | – | – | – | – | – | – | – | – | – |
HHc-15 IR | J104353.9–593245 | 274 | 285 | 283 | 239 | – | – | – | – | – | – | – | – | – |
EGO | J104040.5–585319 | – | 13.4 | 16.3 | 12.6 | 53.2 | 79.4 | 52.7 | 26.8 | 12.7 | – | – | – | – |
EGO | J104248.1–592529 | 265 | 318 | 440 | – | 57.3 | 85.9 | 65.4 | 39.4 | 21.8 | 5.73 | 14.0 | – | 58.1 |
EGO | J104813.4–595848 | 5.34 | 9.52 | 15.2 | 14.6 | 33.4 | 49.8 | 36.2 | 19.6 | 10.5 | 2.09 | – | – | – |
G287.10-0.73 | J104114.3–593239 | 0.645 | 1.42 | – | – | 7.36 | 31.0 | 32.2 | 28.3 | – | – | – | – | – |
G287.95-1.13 | J104542.0–601732 | – | 5.80 | – | – | 18.4 | 38.2 | 51.0 | 23.8 | – | – | – | – | – |
G288.26-1.14a | J104750.3–602618 | 2.83 | 6.70 | – | – | 20.0 | 65.0 | – | – | – | – | – | – | – |
G288.26-1.14b | J104752.1–602627 | 4.02 | 14.5 | 28.8 | 31.3 | – | – | – | – | – | – | – | – | – |
G288.26-1.14c | J104750.9–602625 | 1.13 | 1.93 | – | – | – | – | – | – | - | – | – | – | – |
G288.26-1.14d | J104751.7–602624 | 2.25 | – | – | – | – | – | – | – | – | – | – | – | – |
CGO | J104325.5–591645 | 8.99 | 20.8 | 44.5 | 63.0 | 1.95 | 6.93 | – | – | – | – | – | – | – |
CGO | J104325.7–591660 | 1.60 | 3.26 | 6.69 | 8.22 | – | – | 10.5 | 7.10 | 4.78 | – | – | – | – |
CGO | J104450.4–593303 | 3.18 | 21.3 | 9.17 | 12.0 | – | – | – | – | – | – | – | – | – |
CGO | J104455.7–592554 | 10.6 | 15.4 | – | 39.6 | 32.7 | 57.4 | 48.8 | – | – | 3.11 | 0.821 | 1.64 | 2.75 |
CGO | J104528.6–591319 | 37.1 | 52.7 | – | – | 9.96 | 24.1 | 17.2 | 9.46 | – | 0.923 | 5.63 | 14.6 | 26.1 |
MHO1605 IR | J104351.5–593911 | 1.27 | 1.79 | 8.19 | 17.9 | – | – | – | – | – | – | – | – | – |
MHO1610 IR | J104608.3–594525 | – | 1.26 | – | – | 8.68 | 13.6 | 10.3 | 4.80 | – | – | – | – | – |
Notes. The first column indicates the type of the associated jet object: EGO for extended green objects, CGO for green point sources. The EGOs from Smith et al. (2010b) bear the identifiers given there. For sources of Herbig-Haro objects and Herbig-Haro candidates the identifier of the corresponding jet object following Smith et al. (2010a) is given, for the MHOs their catalogue number as assigned by Preibisch et al. (2011b). For all sources their coordinates are given in the second column.
For HH 666 IR we adopted the JHKs fluxes measured by Smith et al. (2004) with SOFI.
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