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Study the connection between the masing disk and obscuring torus in Seyfert 2 galaxies.\n  Methods. We present a uniform X-ray spectral analysis of the high energy properties of 14 nearby megamaser Active Galactic Nuclei observed by NuSTAR. We use a simple analytical model to localize the maser disk and understand its connection with the torus by combining NuSTAR spectral parameters with available physical quantities from VLBI mapping.\n  Results. Most of the sources analyzed are heavily obscured, showing a column density in excess of $\\sim 10^{23}$ cm$^{-2}$. In particular, $79\\%$ are Com"},"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":"1602.03185","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-02-09T21:00:03Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"6367fb2abd04c0a067c75974c5a01a6bc10a22be1a8044190ef90607e41f5ba9","abstract_canon_sha256":"3211ce5c0393c07c09fb22d9d75cfc6a4f292224abf379fd205b4c003797fe3f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:17:17.400523Z","signature_b64":"Su/7E6w79CxsvuTPGFK9B7BwMAfOb/lIc5Cc7/VLJ0ZIpDqs3f+2RueJUdrrbL6sB9g7IN5rq+7d4OEFkXcNCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"94561b24af111bcbeb9232d2383007ecd1b4a3e9a00b312fb69cde54dd7ab40f","last_reissued_at":"2026-05-18T01:17:17.399978Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:17:17.399978Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"NuSTAR observations of water megamaser AGN","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"A. Comastri, A. Masini, C. J. Hailey, C. Ricci, D. R. Ballantyne, D. Stern, E. Rivers, F. A. Harrison, F. E. Bauer, F. E. Christensen, G. Madejski, I. Zaw, M. Balokovi\\'c, M. Brightman, M. J. Koss, P. Gandhi, S. E. Boggs, S. Puccetti, W. N. Brandt, W. W. Craig, W. W. Zhang","submitted_at":"2016-02-09T21:00:03Z","abstract_excerpt":"Aims. Study the connection between the masing disk and obscuring torus in Seyfert 2 galaxies.\n  Methods. We present a uniform X-ray spectral analysis of the high energy properties of 14 nearby megamaser Active Galactic Nuclei observed by NuSTAR. We use a simple analytical model to localize the maser disk and understand its connection with the torus by combining NuSTAR spectral parameters with available physical quantities from VLBI mapping.\n  Results. Most of the sources analyzed are heavily obscured, showing a column density in excess of $\\sim 10^{23}$ cm$^{-2}$. 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