Table 3: Tuning of the adaptive binning. Counts inside a time bin for a given source total counts.
Source total counts Counts inside a time bin

0-500 15

500-1000 25

1000-2000 35

2000-4000 50

4000-6000 80

6000< 100

**Table 3:** Tuning of the adaptive binning. Counts inside a time bin for a given source total counts.
Source total counts	Counts inside a time bin
0-500	15
500-1000	25
1000-2000	35
2000-4000	50
4000-6000	80
6000<	100

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observation and data analysis
	3 Comparison with Chandra source detections
	4 IR properties of the XMM-Newton sources
	5 X-ray detection of young bona fide brown dwarfs
	6 X-ray properties of Young Stellar Objects in the $\rho$ Ophiuchi cloud
	7 Summary and conclusions
	References
	Online Material
	Appendix A: Method to compute the X-ray count rate upper limit
	Appendix B: Comparison between Chandra and XMM-Newton determination of $N_{\rm H}$