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Table A.1

Tidal streams found in this work, including previously known features and new discoveries (28 host galaxies), with detection confidence levels (DCL) 3 and 4.

ID Galaxy morphology Distance (Mpc) log (stellar mass) (M) DCL Tags Comments
NGC 681 SAB 33.600 10.752 4 S C This work
NGC 718 SAB 21.400 10.283 3 C E Very faint arc-like feature to the north plus possible overdensity to the south
NGC 936 SB0 20.683 10.926 3 C E Double arc-like feature; hints of warped disk
NGC 1055 SBb 16.630 10.739 4 O Martínez-Delgado et al. (2010)
NGC 1084 SAc 21.225 10.619 4 C Martínez-Delgado et al. (2010)
NGC 2775 SAab 17.000 10.870 4 S This work; MD+
NGC 2859 (R)SB0 27.333 10.882 3 C Sph Two possible partially disrupted satellites within a ring, with leading and trailing tails
NGC 3034 I0 3.777 10.449 2 E O Possible spike features
NGC 3041 SAB 26.350 10.437 4 C This work
NGC 3049 SBab 30.775 10.132 4 S C E This work; MD+
NGC 3185 (R)SBa 24.725 10.215 3 C E O Very faint loop connected to the disk, with a compact object embedded on it
NGC 3277 SA 25.000 10.375 1 S Possible shells very close to the halo
NGC 3521 SABbc 12.078 11.030 4 S C E O Martínez-Delgado et al. (2010)
NGC 3611 SAa 33.300 10.462 4 C Schweizer & Seitzer (1990); This work
NGC 3628 Sb 11.300 10.805 4 Sph Martínez-Delgado et al. (2010)
NGC 3631 SAc 13.102 10.163 4 E O This work; MD+
NGC 3675 SA 17.200 10.919 1 E Candidate tidal overdensities, not clearly distinguishable from disk warping
NGC 3682 SA0 ND 10.230 4 S This work
NGC 3729 SB 20.183 10.233 3 Sph E Possible satellite being disrupted
NGC 3877 SA 15.612 10.445 1 E O Asymmetrical and coplanar spike extending from the disk
NGC 3949 SA 18.341 10.246 3 S E Possible shell very close to the outer disk
NGC 4013 Sb 18.600 10.630 4 E O Martínez-Delgado et al. (2010)
NGC 4051 SAB 14.575 10.359 3 Sph E O Possible compact object with halo and tail, plus an overdensity south of the galaxy
NGC 4111 SA0 15.550 10.452 4 Sph O Brodie et al. (2014)
NGC 4203 SAB0 14.940 10.528 4 Sph Paudel & Ree (2014); This work
NGC 4262 SB0 20.510 10.377 2 E Two overdensities not clearly related to tidal features, perhaps part of the disk
NGC 4293 (R)SB0 14.320 10.418 3 E O Clear substructure in the inner halo, very close to the disk
NGC 4394 (R)SB 16.800 10.440 3 E Possible extended disk features, or tidal arcs surrounding the galaxy
NGC 4414 SAc 18.312 10.883 4 S de Blok et al. (2014)
NGC 4494 E 13.841 10.542 2 O Possible diffuse substructure, resembling symmetric spikes in an elliptical galaxy
NGC 4519 SB 28.411 10.191 3 C E Filamentary feature with two components, likely related to either the halo or the disk
NGC 4569 SABab 12.352 10.638 4 E O Martínez-Delgado et al. (2010)
NGC 4594 SAa 10.390 11.253 4 C Malin & Hadley (1997)
NGC 4631 SBd 6.050 10.127 4 E O Martínez-Delgado et al. (2015)
NGC 4643 SB0 25.700 11.028 4 C Sph This work
NGC 4651 SAc 26.708 10.844 4 S C E O Martínez-Delgado et al. (2010)
NGC 4691 (R)SB0 22.500 10.479 2 E O Possible outer halo overdensity with the appearance of a dense stellar cloud
NGC 4753 I0 16.869 10.930 4 E Steiman-Cameron et al. (1992)
NGC 4762 SB0 22.460 10.848 2 E O An interesting case of disk warping with mixed tidal features
NGC 4772 SAa 30.475 10.747 4 E Haynes et al. (2000)
NGC 4866 SA0 23.800 10.689 1 E O Unclassifiable disk feature to the right of the galaxy, possibly with tidal origin
NGC 5055 SAbc 8.333 10.778 4 C O Martínez-Delgado et al. (2010)
NGC 5364 SA 19.513 10.614 3 E O Giant tidal structure west of the galaxy
NGC 5506 S pec 23.833 10.122 3 C O Distorted, asymmetric tidal features connected to each side of the disk
NGC 5576 E 23.930 10.770 1 S Possible diffuse shells
NGC 5750 SB0 33.633 10.741 4 E O This work
NGC 5806 SAB 25.541 10.585 3 C S E Diffuse extended overdensity, with a shell or arc-like feature very close to the disk
NGC 5907 SAc 16.636 10.871 4 C Martínez-Delgado et al. (2010)
NGC 7241 SB ND 10.263 4 E O Leaman et al. (2015)
NGC 7742 SAb 22.200 10.343 4 S C This work
NGC 7743 (R)SB0 21.433 10.447 4 C E This work; MD+

Notes. Diffuse-light overdensities, with their physical nature yet to be confirmed (23 host galaxies) are also included, with DCL 1 and 2. This implies a total of 51 galaxies with any type of tidal features related to them. Distances and stellar masses were taken from S4 G, while their morphology was extracted from NED database. Additionally, substructures we found have been tagged: S for shells; C for curved, arcuated features, including anything coherent and stream like; Sph for spheroidal satellites and partially disrupted cores; E for extensions of the central galaxy (e.g., warps and spiral arms); and O for any other type of less common features (wedges, radial spikes, fuzzy clouds of debris, etc.). For known substructures, references of previous studies have been supplied. MD+ refers to Martínez-Delgado et al. (in prep.), a forthcoming paper.

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