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We find [Fe/H]=-0.79$\\pm$0.02 dex and [Fe/H]=-0.69$\\pm$0.02 dex for NGC 6569 and NGC 6624, respectively and an average $\\alpha$-elements enhancement of $\\approx$+0.43$\\pm$0.02 dex and +0.39$\\pm$0.02 dex, consistent with previous measurements on other metal-rich Bulge clusters. We measure accurate radial velocities of $\\rm <v_r>=-47\\pm 4 km s^{-1}$ and $\\rm <v_r>=+51\\pm 3 km s^{-1}$ and veloc"},"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":"1103.0233","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-03-01T17:38:21Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"0d986ba86645e1e79359d95c8ec878b50d8ecf41a56d5d919bfde4e8f46295c1","abstract_canon_sha256":"e1c242a1edd6cf672c3df0c407b94fc48520234f2875d345cbb9be127ffb77a8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:03:01.570526Z","signature_b64":"DIJta6aCF/IqXAI7957oeo/5ja7iMN02VDCdPPOuuyKz84IEpTFFZHCuv6Oi3WNMnp5pXutWHU4HobO+bziHAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5f535c72d0b31d8f2c0806a16050e3e4c77a4eca8c5bc1deb9076adf4dd5ab6e","last_reissued_at":"2026-05-18T02:03:01.569789Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:03:01.569789Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"High resolution near-IR spectra of NGC 6624 and NGC 6569","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"E. Valenti, L. Origlia, R.M. Rich","submitted_at":"2011-03-01T17:38:21Z","abstract_excerpt":"We present the first abundances analysis based on high-resolution infrared (IR) echelle spectra of NGC 6569 and NGC 6624, two moderately reddened globular clusters located in the outer bulge of the Galaxy. We find [Fe/H]=-0.79$\\pm$0.02 dex and [Fe/H]=-0.69$\\pm$0.02 dex for NGC 6569 and NGC 6624, respectively and an average $\\alpha$-elements enhancement of $\\approx$+0.43$\\pm$0.02 dex and +0.39$\\pm$0.02 dex, consistent with previous measurements on other metal-rich Bulge clusters. 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