{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:XFCGHMUYYYNLP4JEMOXS5JJMLV","short_pith_number":"pith:XFCGHMUY","schema_version":"1.0","canonical_sha256":"b94463b298c61ab7f12463af2ea52c5d64ed99ee7309d3d602a736871e58ea93","source":{"kind":"arxiv","id":"1610.09798","version":1},"attestation_state":"computed","paper":{"title":"Tracking galaxy evolution through low frequency radio continuum observations using SKA and Citizen-science Research using Multi-wavelength data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Ananda Hota (UM-DAE CEBS, Chiranjib Konar (Amity Univ., C. S. Stalin (IIA, India), Megha Rajoria (RAD@home), Mumbai, Pradeepta K. Mohanty (RAD@home), Pratik Dabhade (RAD@home), RAD@home, RAD@home), Sagar Sethi (RAD@home), Sai Arun Dharmik Bhoga (RAD@home), Sravani Vaddi (NCRA-TIFR","submitted_at":"2016-10-31T06:12:45Z","abstract_excerpt":"We present a review on galaxy black hole co-evolution through merger, star formation and AGN-jet feedback. We highlight results on transitional galaxies (e.g. NGC1482, NGC6764, NGC3801, Speca, RAD-18 etc.) which has data from Giant Meterwave Radio Telescope (GMRT) and other sub-mm, IR, optical, UV and X-ray telescopes. The `smoking gun' relic-evidences of past AGN-jet feedback which is believed to have quenched star formation in transitional galaxies are still missing. Relic radio lobes, as old as a few hundred Myr, can be best detected at low radio frequencies with the GMRT, LOFAR and in futu"},"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":"1610.09798","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-10-31T06:12:45Z","cross_cats_sorted":[],"title_canon_sha256":"d6ecbbc8060a015f91c37ac8cbdd19dcdad56dd10a5cd1d3e1c3ed59bf12bc7e","abstract_canon_sha256":"c5fc3d30bd4faddce08dc0ffcd761b44cc92a8ba689b526bda75b5473a34ea06"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:54:27.991600Z","signature_b64":"/X8QkQRG+JQ7UnAFlY8AW4SirLY1Juzk2Psr4pJDg1173+MeBdvw1rKfaYEl+WHDKP08BfMtfqeXZYJ1hTS2Aw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b94463b298c61ab7f12463af2ea52c5d64ed99ee7309d3d602a736871e58ea93","last_reissued_at":"2026-05-18T00:54:27.990850Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:54:27.990850Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Tracking galaxy evolution through low frequency radio continuum observations using SKA and Citizen-science Research using Multi-wavelength data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Ananda Hota (UM-DAE CEBS, Chiranjib Konar (Amity Univ., C. S. Stalin (IIA, India), Megha Rajoria (RAD@home), Mumbai, Pradeepta K. Mohanty (RAD@home), Pratik Dabhade (RAD@home), RAD@home, RAD@home), Sagar Sethi (RAD@home), Sai Arun Dharmik Bhoga (RAD@home), Sravani Vaddi (NCRA-TIFR","submitted_at":"2016-10-31T06:12:45Z","abstract_excerpt":"We present a review on galaxy black hole co-evolution through merger, star formation and AGN-jet feedback. We highlight results on transitional galaxies (e.g. NGC1482, NGC6764, NGC3801, Speca, RAD-18 etc.) which has data from Giant Meterwave Radio Telescope (GMRT) and other sub-mm, IR, optical, UV and X-ray telescopes. The `smoking gun' relic-evidences of past AGN-jet feedback which is believed to have quenched star formation in transitional galaxies are still missing. Relic radio lobes, as old as a few hundred Myr, can be best detected at low radio frequencies with the GMRT, LOFAR and in futu"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1610.09798","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"1610.09798","created_at":"2026-05-18T00:54:27.990979+00:00"},{"alias_kind":"arxiv_version","alias_value":"1610.09798v1","created_at":"2026-05-18T00:54:27.990979+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1610.09798","created_at":"2026-05-18T00:54:27.990979+00:00"},{"alias_kind":"pith_short_12","alias_value":"XFCGHMUYYYNL","created_at":"2026-05-18T12:30:51.357362+00:00"},{"alias_kind":"pith_short_16","alias_value":"XFCGHMUYYYNLP4JE","created_at":"2026-05-18T12:30:51.357362+00:00"},{"alias_kind":"pith_short_8","alias_value":"XFCGHMUY","created_at":"2026-05-18T12:30:51.357362+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/XFCGHMUYYYNLP4JEMOXS5JJMLV","json":"https://pith.science/pith/XFCGHMUYYYNLP4JEMOXS5JJMLV.json","graph_json":"https://pith.science/api/pith-number/XFCGHMUYYYNLP4JEMOXS5JJMLV/graph.json","events_json":"https://pith.science/api/pith-number/XFCGHMUYYYNLP4JEMOXS5JJMLV/events.json","paper":"https://pith.science/paper/XFCGHMUY"},"agent_actions":{"view_html":"https://pith.science/pith/XFCGHMUYYYNLP4JEMOXS5JJMLV","download_json":"https://pith.science/pith/XFCGHMUYYYNLP4JEMOXS5JJMLV.json","view_paper":"https://pith.science/paper/XFCGHMUY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1610.09798&json=true","fetch_graph":"https://pith.science/api/pith-number/XFCGHMUYYYNLP4JEMOXS5JJMLV/graph.json","fetch_events":"https://pith.science/api/pith-number/XFCGHMUYYYNLP4JEMOXS5JJMLV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XFCGHMUYYYNLP4JEMOXS5JJMLV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XFCGHMUYYYNLP4JEMOXS5JJMLV/action/storage_attestation","attest_author":"https://pith.science/pith/XFCGHMUYYYNLP4JEMOXS5JJMLV/action/author_attestation","sign_citation":"https://pith.science/pith/XFCGHMUYYYNLP4JEMOXS5JJMLV/action/citation_signature","submit_replication":"https://pith.science/pith/XFCGHMUYYYNLP4JEMOXS5JJMLV/action/replication_record"}},"created_at":"2026-05-18T00:54:27.990979+00:00","updated_at":"2026-05-18T00:54:27.990979+00:00"}