Table 1
Photometry of W1835+4355 from near-IR to sub-mm.
| Instrument | Band | Flux density (error) | Ref. |
|
|
|||
| Spitzer IRAC1 | 3.6 μm | 51.5 (2.2) μJy | Wu12 |
| Spitzer IRAC2 | 4.5 μm | 142.8 (3.0) μJy | Wu12 |
| WISE W3 | 12 μm | 6790 (190) μJy | IRSA |
| WISE W4 | 22 μm | 24.6 (1.0) mJy | IRSA |
| Herschel PACS | 70 μm | 40.9 (4.1) mJy | this work |
| Herschel PACS | 160 μm | 79.3 (7.9) mJy | this work |
| Herschel SPIRE | 250 μm | 81.0 (8.1) mJy | this work |
| Herschel SPIRE | 350 μm | 72.0 (7.2) mJy | this work |
| Herschel SPIRE | 500 μm | 33.0 (3.3) mJy | this work |
| SCUBA-2 | 850 μm | 8.0 (1.5) mJy | J14 |
Notes. Spitzer IRAC data are derived from warm-mission observations; WISE data are taken from the AllWISE source catalog at IRSA. Nominal W4 flux density has been corrected by a factor of 0.90 which applies for steeply rising mid-IR SEDs (see http://wise2.ipac.caltech.edu/docs/release/allsky/expsup/sec4_4h.html). Errors of 10% are reported for Herschel flux densities.
Reference. Wu12: Wu et al. (2012); J14: Jones et al. (2014).
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