1
2
3
4
5
6
7
8
9
10
11
12
13
14
15
16
17
18
19
20
21
22
23
24
25
26
27
28
29
30
31
32
33
34
35
36
37
38
39
40
41
42
43
44
45
46
47
48
49
50
51
52
53
54
55
56
57
58
59
60
61
62
63
64
65
66
67
// This code is generated by generate_code.py, do not modify it manually.
//! This module contains all the known columns in the dr2_neighbourhood table.
use crate;
/// Users wishing to look up the E/DR3 record for an astrophysical source
/// identified in DR2 must NOT simply extract the record from E/DR3 having
/// the same source identifier.
///
/// As described in the detailed description of attribute designation in
/// GaiaSource it is not guaranteed that the same astronomical source will
/// always have the same source identifier in different Data Releases. Hence
/// the only safe way to compare source records between different Data
/// Releases in general is to check the records of proximal source(s) in the
/// same small part of the sky. This table provides the means to do this via
/// a precomputed crossmatch of such sources, taking into account the proper
/// motions available at E/DR3.
///
/// Within the neighbourhood of a given E/DR3 source there may be none, one
/// or (rarely) several possible counterparts in DR2 indicated by rows in
/// this table. This occasional source confusion is an inevitable
/// consequence of the merging, splitting and deletion of identifiers
/// introduced in previous releases during the DR3 processing and results in
/// no guaranteed one–to–one correspondence in source identifiers between
/// the releases.
///
/// For more details of the procedure used to create this crossmatch, see
/// Chapter [chap:archive] in the online documentation.
;
/// The columns in the dr2_neighbourhood table.
/// Collects all the known columns in the dr2_neighbourhood table.