Table 3
Comparison of 891 GHz HCN laser and NIR photon luminosities.
| Object | λ | Sλ | Catalogue | Lλ | Lλ/L891 |
|---|---|---|---|---|---|
| (μm) | (Jy) | (photons s−1) | |||
| IRC+10216(*) | 3.35 | 1330 | unWISE | 2.4 × 1044 | 0.39 |
| CIT 6 | 3.35 | 580 | unWISE | 7.4 × 1044 | 0.46 |
| Y CVn | 3.35 | 934 | unWISE | 3.6 × 1044 | 2.57 |
| 3.52 | 931 | DIRBE | 3.6 × 1044 | 2.57 | |
| S Cep | 3.35 | 837 | unWISE | 8.7 × 1044 | 1.07 |
| 3.52 | 775 | DIRBE | 8.1 × 1044 | 1 | |
| IRC+50096 | 3.35 | 288 | unWISE | 8.7 × 1044 | 1.05 |
| 3.52 | 313 | DIRBE | 9.5 × 1044 | 1.14 | |
| V Cyg | 3.35 | 683 | unWISE | 7.2 × 1044 | 0.83 |
| II Lup | 3.35 | 203 | unWISE | 4.7 × 1044 | 0.49 |
| 3.52 | 295 | DIRBE | 6.8 × 1044 | 0.72 |
Notes. Flux densities obtained from the VizieR database (Ochsenbein et al. 2000) via http://vizier.cds.unistra.fr/vizier/sed/. The unblurred, coadds of the Wide-field Infrared Survey Explorer (WISE) imaging (unWISE; Lang 2014); Diffuse Infrared Background Experiment (DIRBE; Smith et al. 2004; Price et al. 2010).(*) The 891 GHz HCN laser data observed in 2010 May 13 were used here.
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