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We aim to obtain the Galactic trajectory of LS 5039 and PSR J1825-1446 to find their origin in the Galaxy, and in particular to check their association with SNR G016.8-01.1 to restrict their age. Methods. By means of radio and optical observations we obtained the proper motion and the space velocity of the sources. Results. The proper motion of PSR J1825-1446 corresponds to a transverse space velocity of 690 km/s at a distance of 5 kpc"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1205.2080","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2012-05-09T19:53:30Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"6add5171c3cfd05025268b9fbc212bbfb4fb660d73ff84642c5c07b7b0926478","abstract_canon_sha256":"955329bb2557bf68b6362ba5565b69332f739c608a86a812ba8557878ded93c9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:57:34.282683Z","signature_b64":"hGVJoFL8/dSEz0eQSKQd7dS1c2t1O/am3Fpi15Qbq+SfzzVRBQkYomOGJ7zsvDBwcSxGZCQxV7kKRGCpQfPAAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"73bb87f0d541b06aa9bf8cac6ffd3ed2ab30a12c0decc9dfb257211ce5ddc21e","last_reissued_at":"2026-05-18T01:57:34.282025Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:57:34.282025Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On the origin of LS 5039 and PSR J1825-1446","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"A. G. Lyne, B. W. Stappers, J. Mold\\'on, J. M. Paredes, M. Kramer, M. Rib\\'o, V. Dhawan, W. Brisken","submitted_at":"2012-05-09T19:53:30Z","abstract_excerpt":"Context. The gamma-ray binary LS 5039 and the isolated pulsar PSR J1825-1446 were proposed to have been formed in the supernova remnant (SNR) G016.8-01.1. Aims. We aim to obtain the Galactic trajectory of LS 5039 and PSR J1825-1446 to find their origin in the Galaxy, and in particular to check their association with SNR G016.8-01.1 to restrict their age. Methods. By means of radio and optical observations we obtained the proper motion and the space velocity of the sources. Results. 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