Table 1
Faint secondary standards observed by Herschel-PACS.
| Model flux prediction (mJy) | Spectral type | Reference | ||||
|---|---|---|---|---|---|---|
| HD | Other name | f70 | f100 | f160 | ||
| 62509 | β Gem | 2457 (±5.73%) | 1190 (±5.73%) | 455.9 (±5.73%) | K0IIIb | Cohen et al. (1996)a |
| 12929 | α Ari | 1707 (±5.9%) | 831.4 (±5.9%) | 321.0 (±5.9%) | K2III | Cohen et al. (1996)a |
| 32887 | ε Lep | 1182 (±5.9%) | 576.2 (±5.9%) | 222.7 (±5.9%) | K4III | Cohen et al. (1996)a |
| 198542 | ω Cap | 857.7 (±6.03%) | 418.0 (±6.03%) | 161.5 (±6.03%) | M0III | Cohen et al. (1996)a |
| 148387 | η Dra | 479.5 (±3.38%) | 232.6 (±3.45%) | 89.4 (±3.51%) | G8III | Hammersley et al. (1998)b |
| 180711 | δ Dra | 428.9 (±5.7%) | 207.7 (±5.7%) | 79.6 (±5.7%) | G9III | Cohen et al. (1996)a |
| 139669 | θ Umi | 286.2 (±5.67%) | 139.5 (±5.67%) | 53.9 (±5.67%) | K5III | Cohen et al. (1996)a |
| 41047 | HR 2131 | 195.6 (±5.96%) | 95.4 (±5.96%) | 36.9 (±5.96%) | K5III | Cohen et al. (1996)a |
| 170693 | 42 Dra | 153.7 ± 4.6 | 75.3 (±3.0%) | 29.4 (±3.0%) | K1.5III | Gordon et al. (2007) |
| 138265 | HR 5755 | 115.9 ± 4.0 | 56.8 (±3.5%) | 22.2 (±3.5%) | K5III | Gordon et al. (2007) |
| 159330 | HR 6540 | 64.2 ± 2.1 | 31.5 (±3.3%) | 12.3 (±3.3%) | K2III | Gordon et al. (2007) |
| 152222 | SAO 17226 | 39.4 ± 1.9 | 19.3 (±5.0%) | 7.5 (±5.0%) | K2III | Gordon et al. (2007) |
| 39608 | SAO 249364 | 30.9 ± 1.2 | 15.1 (±4.0%) | 5.9 (±4.0%) | K5III | Gordon et al. (2007) |
| 181597 | HR 7341 | 28.0 (±3.29%) | 13.6 (±3.34%) | 5.2 (±3.42%) | K1III | Hammersley et al. (1998)b |
| 15008 | δ Hyi | 22.9 ± 0.8 | 11.2 (±3.5%) | 4.4 (±3.5%) | A1/2V | Gordon et al. (2007) |
| 156729 | e Her | 12.0 (±3.21%) | 5.8 (±3.25%) | 2.2 (±3.28%) | A2V | Hammersley et al. (1998)b |
| 168009 | HR 6847 | 10.0 (±3.40%) | 4.9 (±3.45%) | 1.9 (±3.50%) | G2V | Hammersley et al. (1998)b |
Notes. Source fluxes from Gordon et al. (2007) are for an effective wavelength of 71.42 μm and have been colour-corrected to the PACScentral wavelength of 70 μm by dividing by the factor 0.961 (cf. Müller et al. 2011) for a Rayleigh-Jeans-tail-type SED. 100 and 160 μm fluxes for these sources are then extrapolated values for this adopted SED. Source flux models are from (a) http://general-tools.cosmos.esa.int/iso/users/expl_lib/ISO/wwwcal/isoprep/cohen/extraps/, (b) http://general-tools.cosmos.esa.int/iso/users/expl_lib/ISO/wwwcal/isoprep/gbpp/.
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.