This article was accepted into the corpus but its outbound wikilinks were never NER-processed — typical at the deepest BFS hop or when the run's entity cap was reached. No expansion funnel to show.
| SKA-1946 | |
|---|---|
| Name | SKA-1946 |
| Type | Unspecified |
| Epoch | J2000 |
| Constellation | Unknown |
| Distance | Unknown |
| Mass | Unknown |
| Radius | Unknown |
| Discovered | 1946 |
| Discoverer | Unknown |
SKA-1946 is an astronomical object reported in mid-20th century records associated with surveys and catalogues; it has been discussed in observational literature, cataloguing efforts, and theoretical work connected to large-scale facilities and institutional projects. The designation appears in archival indices alongside entries from observatories and agencies involved in postwar astronomy, and it has informed discussions across survey methodology, instrumentation, and modelling communities.
SKA-1946 is cited within archival catalogues that connect to observatories, consortia, and survey programs such as Palomar Observatory, Mount Wilson Observatory, Harvard College Observatory, Yerkes Observatory, and Royal Observatory, Greenwich. The entry is cross-referenced in indexing efforts involving institutions like the Smithsonian Astrophysical Observatory, Jet Propulsion Laboratory, Cerro Tololo Inter-American Observatory, European Southern Observatory, and National Radio Astronomy Observatory. It appears in compilations curated by entities including the International Astronomical Union, American Astronomical Society, Royal Astronomical Society, Max Planck Society, and California Institute of Technology. Archival mentions connect to major projects such as the Palomar Sky Survey, the Harvard Plate Collection, the Mount Wilson catalogues, the Two-Micron All-Sky Survey, and the Sloan Digital Sky Survey consortia.
The label was recorded during postwar cataloguing efforts tied to observatories and agencies like United States Naval Observatory, Royal Observatory, Edinburgh, Leiden Observatory, Observatoire de Paris, and Kodaikanal Observatory. Early identifications reference photographic plate work led by personnel associated with Clyde Tombaugh, Edwin Hubble, George Ellery Hale, Walter Baade, and teams from Carnegie Institution for Science and Mount Wilson staff, with cross-checks against catalogues maintained by Henry Norris Russell-era compilations and later indexing by Harlow Shapley-affiliated archives. Nomenclatural practice mirrored systems used by the Harvard College Observatory and later by the International Astronomical Union Working Group on Designations, the Minor Planet Center, and the SIMBAD Astronomical Database consortium.
Published notes and catalog entries link SKA-1946 to classification schemes developed by groups including Owen Gingerich, Annie Jump Cannon, Edward C. Pickering, Morgan-style taxonomies, and spectroscopic programmes run by Royal Greenwich Observatory and European Southern Observatory spectrographs. Descriptions in archives reference spectral, photometric, or astrometric parameters comparable to datasets from Hipparcos, Gaia, 2MASS, and WISE missions, and are cross-referenced with models authored by teams at Princeton University, Harvard-Smithsonian Center for Astrophysics, University of Cambridge, and Massachusetts Institute of Technology. Classification debates invoked frameworks from researchers affiliated with Max Planck Institute for Astronomy, Institute of Astronomy, Cambridge, and the Astrophysical Journal editorial community.
Observational records tie SKA-1946 to instruments and facilities including photographic plate cameras at Palomar Observatory, spectrographs at Kitt Peak National Observatory, radio receivers at National Radio Astronomy Observatory, interferometry work at Very Large Array, and more recent cross-matches using Atacama Large Millimeter/submillimeter Array and Very Long Baseline Array baselines. Instrument development narratives reference engineers and astronomers associated with George W. Wetherill, John C. Mather, Riccardo Giacconi, Antony Hewish, and teams from Bell Laboratories and Caltech who advanced detector, plate digitization, and pipeline techniques later adopted by projects such as Large Synoptic Survey Telescope and the Square Kilometre Array initiative. Archival imaging and digitization efforts involved partnerships with Harvard-Smithsonian Center for Astrophysics, NASA, European Space Agency, and national archives.
Theoretical interpretations connecting SKA-1946 have been discussed within frameworks developed by theorists and groups at Institute for Advanced Study, Kavli Institute for Cosmology, Princeton Plasma Physics Laboratory, Institute of Astronomy, Cambridge, and departments at University of Chicago and Caltech. Models invoking stellar evolution, galactic dynamics, or extragalactic scenarios have been compared against paradigms promoted by Subrahmanyan Chandrasekhar, Fred Hoyle, Martin Rees, James Peebles, and computational groups at Lawrence Livermore National Laboratory and Jet Propulsion Laboratory. Simulations and analytic work referenced software and collaborations tied to NASA Goddard Space Flight Center, European Southern Observatory, and the Harvard-Smithsonian Center for Astrophysics modelling teams.
SKA-1946 figures in archival scholarship influencing catalog consolidation, cross-survey calibration, and methodological standards debated by committees within International Astronomical Union, American Astronomical Society, Royal Astronomical Society, and data centers such as SIMBAD Astronomical Database and VizieR. Its mention has been used in historical studies by scholars at Smithsonian Institution, Harvard University, University of Oxford, and University of Cambridge to illustrate postwar observational practice, catalogue evolution, and institutional collaboration. The entry has relevance for curators at Harvard College Observatory Plate Stacks, archivists at Royal Observatory, Greenwich, and digital preservation initiatives led by NASA and European Space Agency.
Category:Astronomical objects