Table 6: (The complete table (215 rows) is only available in electronic form at the CDS). Magnitudes for all sources (including foreground sources and sources below the 90% completeness limit) in 30 Doradus. Stars with measurements in all four bands are listed first. Then stars with measurements in K and L only, and finally stars just detected in L-band. Column 1 gives the source id. Columns 2 and 3 the RA and Dec respectively in J2000. The coordinates for sources found in all four bands are from the point source catalogue, positions for the remaining stars are determined from reference 2MASS images. Columns 4, 6, 8 and 10 give the $\it JHK$ - and L-band magnitudes respectively. Columns 5, 7, 9 and 11 give the photometric errors. For sources detected in all bands, the JHK magnitudes and errors are taken from the 2MASS PSC. A "null'' as error indicates that no photometric error was given in the PSC. The L-band errors are combined from the errors in daophot and the errors due to the zero point correction. Sources only detected in the K- and L-bands have magnitudes from this work. For sources not detected at J, H or K the upper limits on these magnitudes are 15.8, 15.1 and 14.3 respectively. Stars with an IR-excess are marked with an "e'' in Col. 12 (comments). Likely foreground stars are marked with "fg''. Stars that matched sources in Rubio et al. (1998), Brandner et al. (2001) and Parker et al. (1993) are marked with "Rubio'', "Brandner'' and "Parker'' respectively together with the id assigned in the respective papers.
id RA (J2000) Dec (J2000) m_J $\sigma_{J}$ m_H $\sigma_{H}$ m_K $\sigma_{K}$ m_L $\sigma_{L}$ comments

(h m s) (d m s)

1 5 37 50.2 -69 04 24.2 10.0 0.02 09.5 0.02 09.4 0.02 09.7 0.05

2 5 37 50.5 -69 04 02.3 14.7 0.04 12.8 0.03 11.4 0.02 09.4 0.05 e

3 5 37 54.7 -69 09 03.2 10.3 0.02 09.4 0.02 09.1 0.02 09.1 0.08

4 5 37 57.0 -69 03 38.9 12.9 0.02 11.9 0.03 11.6 0.03 10.8 0.05 e

5 5 37 58.1 -69 05 03.8 12.6 0.02 11.6 0.03 11.2 0.02 10.9 0.05

$\vdots$

**Table 6:** (The complete table (215 rows) is only available in electronic form at the CDS). Magnitudes for all sources (including foreground sources and sources below the 90% completeness limit) in 30 Doradus. Stars with measurements in all four bands are listed first. Then stars with measurements in K and L only, and finally stars just detected in L-band. Column 1 gives the source id. Columns 2 and 3 the RA and Dec respectively in J2000. The coordinates for sources found in all four bands are from the point source catalogue, positions for the remaining stars are determined from reference 2MASS images. Columns 4, 6, 8 and 10 give the $\it JHK$ - and L-band magnitudes respectively. Columns 5, 7, 9 and 11 give the photometric errors. For sources detected in all bands, the *JHK* magnitudes and errors are taken from the 2MASS PSC. A "null'' as error indicates that no photometric error was given in the PSC. The L-band errors are combined from the errors in daophot and the errors due to the zero point correction. Sources only detected in the K- and L-bands have magnitudes from this work. For sources not detected at J, H or K the upper limits on these magnitudes are 15.8, 15.1 and 14.3 respectively. Stars with an IR-excess are marked with an "e'' in Col. 12 (comments). Likely foreground stars are marked with "fg''. Stars that matched sources in Rubio et al. (1998), Brandner et al. (2001) and Parker et al. (1993) are marked with "Rubio'', "Brandner'' and "Parker'' respectively together with the id assigned in the respective papers.
id	RA (J2000)	Dec (J2000)	m_J	$\sigma_{J}$	m_H	$\sigma_{H}$	m_K	$\sigma_{K}$	m_L	$\sigma_{L}$	comments
	(h m s)	(d m s)
1	5 37 50.2	-69 04 24.2	10.0	0.02	09.5	0.02	09.4	0.02	09.7	0.05
2	5 37 50.5	-69 04 02.3	14.7	0.04	12.8	0.03	11.4	0.02	09.4	0.05	e
3	5 37 54.7	-69 09 03.2	10.3	0.02	09.4	0.02	09.1	0.02	09.1	0.08
4	5 37 57.0	-69 03 38.9	12.9	0.02	11.9	0.03	11.6	0.03	10.8	0.05	e
5	5 37 58.1	-69 05 03.8	12.6	0.02	11.6	0.03	11.2	0.02	10.9	0.05
$\vdots$

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations
	3 Results
	4 Analysis
	5 Discussion
	6 Conclusions
	References