Table 1
YLW 16A photometry.
J | H | K s | 3.6 μma | 4.5 μma | 5.8 μma | 8 μma | 10.8 μm | 70 μme | 850 μmf | 1200 μmg | MJD | Phaseh |
mag | mag | mag | mJy | mJy | mJy | mJy | mJy | mJy | mJy | mJy | days | |
|
||||||||||||
897 ± 66 | 1960 ± 154 | 3730 ± 182 | 5800 ± 350 | 53 071.326 | 0.17 | |||||||
696 ± 70 | 1850 ± 168 | 2430 ± 208 | 3760 ± 345 | 53 092.242 | 0.39 | |||||||
576 | 52 464.5 | 0.62 | ||||||||||
740 ± 148 | ||||||||||||
34700 ± 3250 | ||||||||||||
2650 ± 65b | 50 626 | 0.77 | ||||||||||
8080 ± 91c | ||||||||||||
(5030 ± 460)d | 46 200 or | 0.98 or | ||||||||||
46 596 | 0.26 | |||||||||||
9.84 ± 0.05i | 46 596 | 0.26 | ||||||||||
~8.8j | 46 437 | 0.54 | ||||||||||
17.13 ± 0.1 | 13.25 ± 0.1 | 9.87 ± 0.1 | bright state | |||||||||
17.13 ± 0.1 | 13.60 ± 0.1 | 10.28 ± 0.1 | faint state | |||||||||
42.2, 9.3 mJyk | 53 490 | 0.69 | ||||||||||
351, 344l | 53 469 | 0.46 | ||||||||||
1209, 641m | 54 586.39 | 0.53 |
Notes.
Observations from the IRAC instrument (Evans et al. 2003).
Observation made with P200/MIRLIN on 27 June 1997 (Barsony et al. 2005). This photometry is excluded from the SED fit optimization.
Flux interpolated from 6.7 and 14.3 μm ISOCAM channels (data from Bontemps et al. 2001). Observation date not given (Barsony et al. 2005). This photometry is excluded from the SED fit optimization.
From Table 2 of Wilking et al. (1989); measured flux at 10.2 μm. Date uncertain; both May 1985 and June 1986 observing runs were cited in the text. This photometry is excluded from the SED fit optimization.
Observation from the MIPS instrument (Padgett et al. 2008).
Observation details from Johnstone et al. (2004). Error given as ~20% (Jorgensen et al. 2008).
Obtained between 7−12 July 2002 at the SIMBA bolometer array at the SEST telescope on La Silla, Chile (Stanke et al. 2006). No error value given.
See Sect. 3. YLW 16A was observed to exhibit periodic variability. The light curve was folded such that the bright state corresponds to a phase of ~0.17 to ~0.3.
Observation date given as June 1986; the 15th of June assumed (Wilking et al. 1989). This photometry is excluded from the SED fit optimization.
7 January 1986. No error value given (Simon et al. 1987). This photometry is excluded from the SED fit optimization.
NACO image fluxes of the left and right components in Fig. 1a, scaled to the total flux from the 2MASS measurement in the faint state for Ks.
NACO image fluxes of the left and right components in Fig. 1b, scaled to the total flux from the Spitzer IRAC 3.6 μm measurement in the faint state for L.
CRIRES M-band fluxes of the left and right components in Fig. 1b, scaled to the total flux from the Spitzer IRAC 4.5 μm measurement in the faint state for M, from Herczeg et al. (2011).
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