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Table 2

B, V, and infrared photometry of sources in SMCB2.

No. No.m α (2000) δ (2000) B err V err J err H err K err [3.6] err [4.5] err [5.8] err [8.0] err [24] err [70] err [160] err Type Remarks
18ph 0 47 52.08 –73 16 41.24 14.04 0.11 13.66 0.12 11.42 0.09 9.90 0.08 6.05 0.01 I
19 0 47 52.39 –73 17 11.83 17.38 0.05 16.05 0.04 14.10 0.03 10.70 0.01 9.40 0.01 8.25 0.01 7.09 0.01 3.43d 0.03 –0.63 0.02 I
29 0 47 53.54 –73 17 10.19 16.54 0.04 15.72 0.03 14.48 0.04 11.97 0.02 11.18 0.02 9.96 0.02 8.77 0.06 3.43d 0.03 –0.63 0.02 I
33 0 47 54.96 –73 17 24.72 16.00 0.02 14.97 0.02 14.55 0.03 13.78 0.13 13.38 0.08 12.22 0.11 11.15 0.12 6.05 0.10 I
75 0 48 01.27 –73 16 59.22 17.74 0.07 17.58 0.26 16.73 0.22 14.43 0.07 14.25 0.04 11.95 0.04 10.53 0.08 6.79 0.01 II
108 0 48 04.39 –73 15 21.60 19.00 0.10 16.90 0.03 16.17 0.05 14.84 0.03 12.50 0.03 11.57 0.02 10.44 0.02 8.86 0.02 3.60 0.01 I
118 0 48 04.98 –73 17 55.58 17.87 0.08 16.51 0.06 15.14 0.06 12.76 0.03 11.41 0.02 10.27 0.02 9.00 0.02 3.06 0.01 –1.06 0.01 I
127 0 48 05.77 –73 17 43.58 16.06 0.02 14.76 0.02 13.44 0.02 11.33 0.02 10.50 0.01 9.75 0.01 8.69 0.01 5.28 0.01 II
154p 0 48 07.76 –73 14 28.99 18.57 0.08 18.45 0.08 17.97 0.07 17.20 0.10 16.78 0.13 13.90 0.14 13.50 0.19 11.57 0.10 10.12 0.15 4.69 0.02 II
169m2 10069 0 48 08.60 –73 14 54.69 14.82 0.02 14.28 0.02 13.68 0.05 13.15 0.06 12.37 0.05 11.22 0.06 10.27 0.04 8.73 0.03 7.02 0.09 0.05 0.004 –3.51 0.01 –5.24 0.02 I N26A-Bt
170n 0 48 08.52 –73 14 54.31 15.76 0.04 15.45 0.03 14.67 0.04 14.54 0.04 13.86 0.03 11.78 0.06 III N26-Ac
172n 0 48 08.74 –73 14 54.53 14.53 0.04 13.85 0.04 13.06 0.03 11.43 0.06 I N26-Cc
173n 0 48 08.96 –73 14 53.70 16.87 0.06 16.45 0.03 15.24 0.04 14.95 0.04 14.34 0.04 12.78 0.08 III N26-Bc

Notes. This table is available in its entirety at the CDS. The portion shown here includes the data for the YSO candidates only.

(†)

For JHKs uncertainties see Sect. 2.1.1; for BV see Sect. 2.1.2; for IRAC and MIPS see Gordon et al. (2011); for IRSF see Kato et al. (2007).

(c)

Component of N26.

(d)

Stars 19 and 29 are not resolved in the 24 μm and 70 μm bands. We assume their intensity emission to be half of the integrated intensity.

(m)

Massey catalog number.

(m2)

The integrated magnitudes of 169 or N26 are adopted from Massey (2002) for BV and 2MASS for JHKs.

(n)

JHKL’ magnitudes obtained using NACO data.

(p)

As the photometry in the SAGE catalog is not complete, the magnitudes of IRAC and the 24 μm bands were derived from the images using Daophot.

(ph)

In this catalog the photometry of this star is not complete either. As its FWHM is larger than the PSF (~4″), the magnitudes were derived from a sum of profiles crossing the whole star and a neighboring isolated star used as standard.

(t)

Labeled in Testor (2001).

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