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We endeavor to analyze the stellar density of bulge stars in the same regions using a different stellar population that is characteristic of the young bulge ($\\lesssim 5$ Gyr). Particularly, we use F0-F5 main-sequence stars with distances derived through photometric parallax.\n  METHODS. We extract these stars from extinction-corrected color-magnitude diagrams in the near-infrared of VISTA-VVV data in some bulge regions and calculate the d"},"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":"1606.09627","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-06-30T19:35:16Z","cross_cats_sorted":[],"title_canon_sha256":"945efefa8d90a64b3b78a5e15e069d0b764bad3e8bd96d30e3f46ab96e6a5a7d","abstract_canon_sha256":"968fd791ecce46ee0bab844eb42d33426f4af0aa1d3e0a5e20382ce3fe445033"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:03:49.239242Z","signature_b64":"abyTnfnfEVs1x9UIf4KHi35L5D6wy9tdBgEh8toRQbJe3Q6FtuqMlIn++rvaTTdzcJ/X7GRBH9tjxOFQhsF8DA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0e476a15825de5c1cf8f09fd8ca4540c4a83ae47b77cba6d4d8c2a88b20243b8","last_reissued_at":"2026-05-18T01:03:49.238566Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:03:49.238566Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A case against an X-shaped structure in the Milky Way young bulge","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Martin Lopez-Corredoira","submitted_at":"2016-06-30T19:35:16Z","abstract_excerpt":"CONTEXT. A number of recent papers have claimed the discovery of an X-shape structure in the bulge of our Galaxy in the population of the red clumps.\n  AIMS. We endeavor to analyze the stellar density of bulge stars in the same regions using a different stellar population that is characteristic of the young bulge ($\\lesssim 5$ Gyr). Particularly, we use F0-F5 main-sequence stars with distances derived through photometric parallax.\n  METHODS. 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