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Table 2

Detected shell candidates in NGC 3923.

Label Major-axis radius [′′] Prominence Data Detection method Figures Note

S1 +1170 2 MC 1 A.1 largest
S2 952 4 MC 1 A.1, A.2 MP, 907–1012′′, highly uncertain, possibly merged star halos
S3 846 1 MC 1 A.1, A.2, A.8 narrow, connected with the “progenitor”
S4 630 3 MC 1 A.1, A.2, A.8 MP, 640–590′′, irregular, diffuse, near the end of the “stream”
S5 +490 3 MC 1 A.1, A.3, A.8 MP, possibly other tidal feature, small azimuthal extent, opposite S8, connected with the “hook”, shells at lower radii have surface brightness increased at the azimuth of this shell
S6 430 4 MC 3 A.2, A.3 MP, very diffuse and faint, highly uncertain
S7 +363 1 MC 1 A.1, A.3, A.8
S8 338 3 MC 3 A.2, A.3, A.8 MP, not on axis, only in the eastern half, opposite S5, shells at lower radii are brighter on the azimuth of S8
S9 +331 3 MC 3 A.3 copies the edge of S7 but lower azimuthal extent
S10 280 1 MC 1 A.3, A.8
S11 +260 3 MC 3 A.3 MP, very diffuse, a smooth step in surface brightness, possibly other tidal feature
S12 237 4 MC 3 A.3 MP, sharp-edged, small azimuthal extent, possibly other tidal feature
S13 +203 1 MC 1 A.3, A.8
S14 150 1 MC 1 A.3
S15 +146 2 MC 1 A.3, A.4
S16 +130 1 MC, HST 1 A.4
S17 120 3 MC, HST 1 A.4 MP
S18 103 1 MC, HST 1 A.4
S19 +99.5 3 MC, HST 3 A.4
S20 92.0 4 HST 3 A.4 MP, very faint and diffuse, smooth step in surface brightness, possibly other tidal feature
S21 +90.6 3 MC, HST 3 A.4 MP
S22 78.4 2 MC, HST 1 A.4, A.5 sharpness varies with azimuth
S23 +72.8 2 MC, HST 1 A.4, A.5, A.6
S24 71.4 3 MC, HST 3 A.4, A.5 MP, not on axis, only in the western half, diffuse, possibly other tidal feature
S25 68.6 1 MC, HST 1 A.4, A.5
S26 +64.8 3 MC, HST 3 A.4, A.5
S27 +60.0 2 MC, HST 1 A.4, A.5
S28 60.0 3 MC, HST 3 A.4, A.5 MP, diffuse, possibly other tidal feature
S29 55.9 1 MC, HST 1 A.5, A.6
S30 +51.0 1 MC, HST 1 A.5 very prominent
S31 49.0 3 MC, HST 3 A.5 MP, diffuse, possibly other tidal feature
S32 +45.4 3 HST 3 A.5 MP, diffuse, probably the shell at 41.5′′ in Sikkema et al. (2007)
S33 44.7 1 MC, HST 1 A.5, A.6, A.7 very prominent
S34 +38.0 3 MC, HST 3 A.5 MP, very faint on axis, well defined on the western half
S35 37.5 3 MC, HST 3 A.5, A.7 diffuse
S36 +34.8 1 MC, HST 1 A.5, A.6, A.7
S37 30.8 3 HST 2 A.6, A.7 bright smooth step in surface brightness, possibly other tidal feature, probably the shell at −28.7′′ in Sikkema et al. (2007)
S38 +29.5 1 MC, HST 1 A.5, A.6, A.7
S39 24.2 4 MC, HST 3 A.6, A.7 MP, highly questionable, faint, small azimuthal extent, possibly edge of a faint dust cloud
S40 +19.8 1 MC, HST 2 A.6, A.7 very prominent after model subraction, abrupt cutoff in azimuth
S41 18.1 1 MC, HST 1 A.6, A.7 abrupt cutoff in azimuth
S42 10.8 3 MC, HST 3 A.7 MP, very faint

Notes. Label – Shell designation. Radius – Shell radius in arcseconds. Shells lying on the north-eastern side of the galaxy have the positive sign; the shells on the south-western side of the galaxy have the negative sign. Prominence – 1 = Prominent and sharp-edged; 2 = Prominent and diffuse-edged; 3 = Faint but probably existent; 4 = Questionable. Data – The image where the shell was detected: our observation with MegaCam (MC) or the archival HST image (Sikkema et al. 2006). Detection method – A method allowing a good detection of the shell: 1 = No processing; 2 = Model subtraction; 3 = Minimum masking (Sect. 2.3, Appendix B). Figures – The figures showing the shell. Notes – MP = Missed by the previous observations.

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