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Table 3.

Differences between the Di24 multiple-image catalogue and this work.

This work Di24 Systems
BCD K26.3, K62.3, K71.3*, K82, K87, K89,
K90, K91, K95, K98, K99, K100,
K106, K109, K115

/ C1, C2, C3
/ K14.5*, K14.6*, K96.3, C4, C5,
C6, C7, C8, C9, C10, C11, C12,
C13, C14, C15

A K1.3, K17.3, K25.2, K27, K45.3,
(quartz) K48, K51, K56, K57.3, K58, K59
K60, K61, K75, K77.4

/ BCD K3.3, K27.3, K47.3, K56.3, K59.3,
K60.3, K73.3, K78.3, K79.3, K83.3,
K86, K92, K93, K94, K104,
K108, K112, K113, K114, K115.4,
K116, K117, K118, K119

Notes. The first column represents the category of the system in this work (gold, silver, bronze or not included in our catalogues). The second column represents the category in Di24 (A for spectroscopically confirmed images, B and C for good candidates without spectroscopic confirmation and D for least reliable candidates). The first part of the table represents newly discovered systems (or individual images) and systems promoted into our gold category based on spectroscopic redshifts. The second part of the table represents systems we excluded or downgraded to silver or bronze categories upon our inspection. The Di24 IDs are renamed as described at the beginning of Sect. 3. Multiple images marked with * are added/upgraded based on Be23 catalogue. Multiple-image systems belonging to the same background object (e.g. K115a and K115b) are written only once for conciseness.

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