EDP Sciences logo
Subscriber Authentication Point
Search
Menu
Home All issues Volume 554 (June 2013) A&A, 554 (2013) A110 Full HTML
Free Access

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.

(a)

Observations from the IRAC instrument (Evans et al. 2003).

(b)

Observation made with P200/MIRLIN on 27 June 1997 (Barsony et al. 2005). This photometry is excluded from the SED fit optimization.

(c)

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.

(d)

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.

(e)

Observation from the MIPS instrument (Padgett et al. 2008).

(f)

Observation details from Johnstone et al. (2004). Error given as ~20% (Jorgensen et al. 2008).

(g)

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.

(h)

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.

(i)

Observation date given as June 1986; the 15th of June assumed (Wilking et al. 1989). This photometry is excluded from the SED fit optimization.

(j)

7 January 1986. No error value given (Simon et al. 1987). This photometry is excluded from the SED fit optimization.

(k)

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.

(l)

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.

(m)

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).

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.