Unveiling the near-infrared structure of the massive-young stellar object NGC 3603 IRS 9A* with sparse aperture masking and spectroastrometry

Free Access

Table 4

Comparison of the root mean square error (RMSError) between the different models of IRS 9A.

Data set	Best SED-only fit^a	Vehoff+2010	Best V² model
	(No. 3006825)	(No. 3012790)	(this work)

NACO/SAM K_s-filter	6.3	6.3	3.1
NACO/SAM L′-filter	25.2	25.4	4.9
T-ReCS data	20.4	20.0	9.4
MIDI data	8.4	4.4	3.5
SED	2.29	2.98	3.4

Notes.

^(a)

This is the best-fit model to the SED, obtained with Robitaille’s online fitting tool.

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.