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Table 1

Archival data used to perform a multiwavelength study in the cores detected at 870 μm.

Telescope/ Filter1 (λ1) Filter2 (λ2) Filter3 (λ3) Filter4 (λ4) Filter5 (λ5)
instrument or survey

ESO 2.2 m/WFIa Rc (651.7 nm) Hα (658.8 nm) NB665 (665.6 nm) SII (676.3 nm) Ic (783.8 nm)
ESO 2.2m/WFIa I (826.9 nm) MB856 (856.2 nm) MB914 (914.8 nm) Z (964.8 nm)
VLT/VIMOSa I (817.1 nm)
ESO 1 m/DENIS I (0.8 μm) J (1.2 μm) Ks (2.1 μm)
Mt. Hopkins-CTIO/2MASS J (1.2 μm) H (1.7 μm) K (2.2 μm))
WISE W1 (3.4 μm) W2 (4.6 μm) W3 (12 μm) W4 (22 μm)
Spitzer/IRACb I1 (3.6 μm) I2 (4.5 μm) I3 (5.8 μm) I4 (8.0 μm)
Spitzer/MIPSb M1 (24 μm) M2 (70 μm)
Herschel/PACSc Blue (70 μm) Red (160 μm)
Herschel/SPIREc Blue (250 μm) Green (350 μm) Red (500 μm)
AKARI/IRC S9W (9 μm) L18W (18 μm)
AKARI/FIS N60 (65 μm) WIDE-S (90 μm) WIDE-L (140 μm) N160 (160 μm)

Notes.

(a)

Archival ESO Projects 2064.I-0559, 67.C-0225(A), 077.C-0339(A), 075.C-0294(C), and 68.C-0311(A), for WFI data, and 072.C-0046(B) for VIMOS.

(b)

These data are part of the legacy project “cores to disks” (c2d; see Evans et al. 2003).

(c)

Data part of the Herschel guaranteed time key programme “Gould Belt survey” (KPGT_andre_1; PI: Philippe André).

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