Free Access

Table A.3.

Estimated uncertainties of mass measurements using astrometric microlensing with Gaia for multiple background sources.

# Name-lens DR2_ID-source DR2_ID-Source DR2_ID-Source Min σMall σMall/Min σM5 − par σM5 − par./Min σMsig. σMsig./Min
DR2_ID-lens (2-parameter) (5-parameter) (sigma) M M % M % M %
1 Proxima Cen 5853498713161902848 5853498713162466688 5853498713181091840 0.12 10% 10% 10%
5853498713160606720 5853498713161549312 5853498713161890304 5853498640098981888
5853498713160604800 5853498713180846720
5853498644442433280 5853498713160651648
5853498644461348864 5853498713180846592
5853498713160648448 5853498713181092224
5853498713160633088 5853498713180840704
5853498713161549440 5853498708818460032

2 5312099874809857024 5312099870497937152 0.07 12%
5312099874795679488

3 Ross 733 4516199313384903936 4516199313402714368 0.43 15% 15%
4516199240734836608

4 LAWD 37 5332606346480229376 5332606522595645824 0.65 16% 36%
5332606522595645952 5332606350774082944 5332606350771972352
5332606350774081280
5332606522574285952
5332606350796954240
5332606350796955904
5332606316412235008
5332606522573342592
5332606518268141952
5332606522572755072

5 61 Cyg B 1872046609337556608 1872046605038072448 0.55 24% 24%
1872046574983497216 1872046609336784256

6 61 Cyg A 1872046609343242368 1872047330897752832 0.63 32% 53%
1872046574983507456 1872046609335739648
1872046605041836928
1872046609335748736

7 L 143-23 5254061535052907008 5254061535097574016 0.12 37% 44%
5254061535097566848 5254061535052928128

8 Innes’ star 5339892367648234240 5339892367683265408 0.33 47% 48%
5339892367683264384

Notes. The table lists the name (Name-Lens) and Gaia DR2 source ID (DR2_ID) of the lens and DR2 source IDs of the background sources. The background sources are grouped into sources where Gaia DR2 only provides the position (2-parameter), sources with a full five-parameter solution (5-parameter), and sources with a five-parameter solution in combination with an expected precision in the along-scan direction better than 0.5 mas (sigma). The assumed mass of the lens is listed in Min, and the expected precisions of the mass determination for the three cases are given in σMx, including the uncertainty due to the errors in the input parameters, as well as the percentage in σMx/Min, where x indicates the use of all background stars (all), background stars with a five-parameters solution (5-par.), and background stars with expected precision in the along-scan direction better than 0.5 mas (sig.).

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.