Table 1
Photometric data points for the Butterfly Star used in the modeling.
λ [μm] | Flux density [mJy] | Instrument | Reference | |
|
||||
22 | 213 ± 9 | WISE | (1) | |
24 | 241 ± 2 | SST/MIPS | (2) | |
71 | 4800 ± 480 | SST/MIPS | (2) | |
350 | 2869 ± 21 | CSO/SHARC-II | (3) | |
800 | 342 ± 57 | JCMT/UKT14 | (4) | |
894 | 287 ± 40 | SMA | (5) | |
1100 | 149 ± 19 | JCMT/UKT14 | (4) | |
1364 | 101 ± 10 | PdBI | (6) | |
2730 | 22 ± 2 | OVRO | (7) |
Notes.WISE: Wide-Field Infrared Survey Explorer; MIPS: Multiband Imaging Photometer for Spitzer; CSO: Caltech Submillimeter Observatory; SHARC-II: Submillimetre High Angular Resolution Camera; JCMT: James Clerk Maxwell Telescope; OVRO: Owens Valley Radio Observatory.Apertures: 22 μm: 16.5″; 24 μm: 10″; 71 μm: 20″; 350 μm: 30″; 800 μm: 16″; 1100 μm: 18.7″.
Reference. (1) WISE ALL-Sky Data Release; (2) Robitaille et al. (2007); (3) Andrews & Williams (2005); (4) Moriarty-Schieven et al. (1994); (5) Wolf et al. (2008); (6) This work; (7) Wolf et al. (2003).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.