Obscured star clusters in the inner Milky Way - How many massive young clusters are still awaiting detection

Open Access

Table 2

Performance of the algorithm on various parameters.

Parameters	No. of candidates	Median ang. radius, arcmin	Mean no. of stars	Recovered number (fract.)
(30, 6′)	283	3.8′	50	11 (11.1%)
(30, 3′)	288	3.8′	51	12 (12.1%)
(12, 6′)	2014	2.4′	19	44 (44.4%)
(12, 3′)	1853	2.3′	19	44 (44.4%)
(12, 1′)	722	1.3′	19	33 (33.3%)

Notes. Parameters (min_samples, eps); the number of identified candidates; their median angular radius in arcminutes; the mean number of stars per candidate; and the number and fraction of recovered objects with respect to the 99 bona fide clusters in this region, listed in SIMBAD.

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.