Issue |
A&A
Volume 518, July-August 2010
Herschel: the first science highlights
|
|
---|---|---|
Article Number | L94 | |
Number of page(s) | 5 | |
Section | Letters | |
DOI | https://doi.org/10.1051/0004-6361/201014612 | |
Published online | 16 July 2010 |
Online Material
Appendix A: SABOCA and LABOCA submillimeter maps
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Figure A.1:
Full submillimeter maps. Left: SABOCA, displayed at the original
resolution of 7
|
Open with DEXTER |
Appendix B: PANIC H and K
photometry
Table B.1: PANIC NGC 1999 near-IR colors of background stars.
Five faint stars are visible in the PANIC H and
images.
Their positions and photometry are listed in Table B.1.
Photometric calibration was performed with 2MASS
photometry of comparison fields containing 20 2MASS sources and verified with
a 2MASS star in the science field. Photometry was conducted with the IRAF task
apphot.
The measured
color was used to estimate the extinction
AV toward the stars. We assumed an intrinsic
color of 0.17,
derived as the median
colors of stars in an unreddened
control field near Orion (Megeath et al., in prep). We adopted the reddening law
of Indebetouw et al. (2005) to convert
excess into K-band
extinction AK, from which we obtained the optical extinction as
,
corresponding to a total to selective extinction
RV between the diffuse ISM value of 3.1 and the higher values (up to 5)
found for dense clouds (e.g. Campeggio et al. 2007).
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