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Table 1.

Galactic coordinates and heliocentric distance used in this work for Hecules-Aquila Cloud North and South (HAC-N and HAC-S, Belokurov et al. 2007a; Watkins et al. 2009; Sesar et al. 2010; Simion et al. 2014), Virgo OverDensity (VOD, Jurić et al. 2008; Bonaca et al. 2012), and Pisces (Nie et al. 2015; Belokurov et al. 2019).

Name (l, b) [deg] d [kpc] rbr [kpc] (αin, αout)
HAC-S 30 ° < l < 60 ° , − 45 ° < b < −20° 10–20 24 . 8 1.0 + 0.8 $ 24.8^{+0.8}_{-1.0} $ ( 3 . 0 0.1 + 0.1 , 5 . 3 0.2 + 0.2 ) $ (-3.0^{+0.1}_{-0.1}, -5.3^{+0.2}_{-0.2}) $
HAC-N 30 ° < l < 60 ° ,20 ° < b < 45° 10–20 22 . 3 1.2 + 1.3 $ 22.3^{+1.3}_{-1.2} $ ( 2 . 8 0.2 + 0.2 , 5 . 7 0.3 + 0.3 ) $ (-2.8^{+0.2}_{-0.2}, -5.7^{+0.3}_{-0.3}) $
VOD 270 ° < l < 330 ° , − 45 ° < b < −20° 10–20 22 . 4 3.4 + 3.6 $ 22.4^{+3.6}_{-3.4} $ ( 2 . 8 0.3 + 0.4 , 4 . 2 0.2 + 0.2 ) $ (-2.8^{+0.4}_{-0.3}, -4.2^{+0.2}_{-0.2}) $
Pisces (74 ° , − 47 ° ) 60–100 ( 3 . 8 2.5 + 0.7 , 3 . 8 0.3 + 0.2 ) $ (-3.8^{+0.7}_{-2.5}, -3.8^{+0.2}_{-0.3}) $

Notes. For the latter, we indicate the centre of a 20° region satisfying the regions associated with Pisces as in Belokurov et al. (2019) and Conroy et al. (2021). We also show the slopes and break radius, rbr, of a two-power law fit of these regions obtained in this work. For comparison, the average profile within the whole LSDR9 footprint has r br = 19 . 1 1.8 + 1.7 $ r_{\mathrm{br}} = 19.1^{+1.7}_{-1.8} $ kpc and ( α in , α out ) = ( 2 . 9 0.1 + 0.2 , 4 . 5 0.1 + 0.1 ) $ (\alpha_{\mathrm{in}}, \alpha_{\mathrm{out}}) = (-2.9^{+0.2}_{-0.1}, -4.5^{+0.1}_{-0.1}) $.

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