Peter K. G. Williams (CfA) • @pkgw@mastodon.world
on behalf of the DASCH team
AAS243 (New Orleans, LA) — 2024 Jan 10
Annie Jump Cannon. Bettmann / Getty Images
Learn more: dasch.cfa.harvard.edu
Photometry from the Harvard plates: ~15B V-band magnitudes, all-sky, ~110-year time baseline, depths of V ~ 14–16, rms ~ 0.15 mag.
The DASCH scanner circa 2006
The primary DASCH scanning effort (~450k plates) is about 97% complete.
After a hiatus, scanning resumed in November, and we estimate completion in April …
… if the DASCH scanner cooperates and there are no major mishaps.
Currently scanning about 180 “A” plates per day.
RY Cnc (same data plotted twice)
We have refreshed the “Cannon” data portal (accessed via dasch.cfa.harvard.edu)
Current data restrictions: FITS mosaics and sources at b < 0 are upon-request
These restrictions will be relaxed soon (months or even weeks)
Also soon: a new “Starglass” plate information portal and API! Foregrounding historical as well as astrophysical connections, especially the “women computers”.
Atop that, plan to build an astroquery package, sample notebooks, tutorials, etc.
Thanks for your attention!
Peter K. G. Williams • pwilliams@cfa.harvard.edu • @pkgw@mastodon.world • newton.cx/~peter/
The DASCH project at Harvard is grateful for partial support from NSF grants AST-0407380, AST-0909073, and AST-1313370; which should be acknowledged in all papers making use of DASCH data. We acknowledge the one-time gift of the Cornel and Cynthia K. Sarosdy Fund for DASCH, and thank Grzegorz Pojmanski of the ASAS project for providing some of the source code on which the DASCH scientific data access portal was based. The ongoing AAVSO Photometric All-Sky Survey (APASS) has improved DASCH photometric calibration and is funded by the Robert Martin Ayers Sciences Fund.
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