Archives of Photographic PLates for Astronomical USE (APPLAUSE) Digitisation of astronomical plates and their integration into the International Virtual Observatory
arXiv:2404.17355 · doi:10.1051/0004-6361/202348793
Abstract
The Archives of Photographic PLates for Astronomical USE (APPLAUSE) project is aimed at digitising astronomical photographic plates from three major German plate collections, making them accessible through integration into the International Virtual Observatory (IVO). Photographic plates and related materials (logbooks, envelopes, etc.) were scanned with commercial flatbed scanners. Astrometric and photometric calibrations were carried out with the developed PyPlate software, using Gaia EDR3 data as a reference. The APPLAUSE data publication complies with IVO standards. The latest data release contains images and metadata from 27 plate collections from the partner institutes in Hamburg, Bamberg, and Potsdam, along with digitised archives provided by Tautenburg, Tartu, and Vatican observatories. Altogether, over two billion calibrated measurements extracted from about 70,000 direct photographic plates can readily be used to create long-term light curves. For instance, we constructed the historic light curve of the enigmatic dipping star KIC 8462852. We found no evidence of previously assumed variations on timescales of decades in our light curve. Potential uses of APPLAUSE images for transient sources can be appreciated by following the development of the nova shell of GK Per (1901) over time and the change in brightness of two extragalactic supernovae. The database holds about 10,000 spectral plates. We made use of objective prism plates to follow the temporal changes of Nova DN Gem through 1912 and 1913, highlighting an outburst in early 1913.
19 pages,2 Tables, 19 figures, A&A accepted
References in corpus (15)
- The Gaia mission
- The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package
- The B & V Light Curves for Recurrent Nova T CrB From 1842--2022, the Unique Pre- and Post-Eruption High-States, the Complex Period Changes, and the Upcoming Eruption in 2025.51.3
- A three-dimensional view of the remnant of Nova Persei 1901 (GK Per)
- Modelling the structure and kinematics of the Firework nebula: The nature of the GK Persei nova shell and its jet-like feature
- The oldest X-ray supernovae: X-ray emission from 1941C, 1959D, 1968D
- A systematic search for novae in M31 on a large set of digitized archival Schmidt plates
- Sonneberg plate photometry for Boyajian's Star in two passbands
- The StarScan plate measuring machine: overview and calibrations
- From Supernova to Remnant: Tracking the Evolution of the Oldest Known X-ray Supernovae
- Astrometry with "Carte du Ciel" plates, San Fernando zone. I. Digitization and measurement using a flatbed scanner
- A search for period changes of eight short-period Type II Cepheids
- Solar observatory Einstein Tower -- Data release of the digitized solar full-disk photographic plate archive
- High-resolution spectroscopy of Boyajian's star during optical dimming events
- Wide-Field Plate Archive of the University Observatory Jena