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HASH: the Hong Kong/AAO/Strasbourg H-alpha planetary nebula database

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arxiv 1603.07042 v2 pith:TUP6WZNB submitted 2016-03-23 astro-ph.SR astro-ph.GAastro-ph.IM

classification astro-ph.SRastro-ph.GAastro-ph.IM
keywords hashdatadatabasegalacticknownreliableaccessibleaccurate
verification ladder T0 review T1 audit T2 compute T3 formal
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By incorporating our major recent discoveries with re-measured and verified contents of existing catalogues we provide, for the first time, an accessible, reliable, on-line SQL database for essential, up-to date information for all known Galactic PNe. We have attempted to: i) reliably remove PN mimics/false ID's that have biased previous studies and ii) provide accurate positions, sizes, morphologies, multi-wavelength imagery and spectroscopy. We also provide a link to CDS/Vizier for the archival history of each object and other valuable links to external data. With the HASH interface, users can sift, select, browse, collate, investigate, download and visualise the entire currently known Galactic PNe diversity. HASH provides the community with the most complete and reliable data with which to undertake new science.

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Forward citations

Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Central-star extinctions towards planetary nebulae

    astro-ph.SR 2025-09 conditional novelty 7.0 of 10

    By fitting model spectra to central-star photometry, the paper produces a homogeneous E(B-V) extinction catalog for 162 extended planetary nebulae that agrees with interstellar dust maps, identifies new binaries, and ...

  2. Unveiling compact planetary nebulae: Broad-band survey analysis and LAMOST confirmation

    astro-ph.SR 2025-05 conditional novelty 6.0 of 10

    A new Gaia plus Pan-STARRS color-color selection method identifies compact planetary nebulae and yields the discovery of the high-ionization PN J020808.63+491401.0, confirmed by LAMOST spectroscopy and Cloudy modeling.

  3. Studying hot evolved stars with ultraviolet spectroscopy

    astro-ph.IM 2026-06 unverdicted novelty 2.0 of 10

    Review of UV spectroscopy applications to hot evolved stars, emphasizing HST contributions and the need for continued observations ahead of HWO.

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