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Galactic OH Masers (Engels 2008)
A compilation of galactic stellar sources observed for OH maser
emission in the transition at 1612, 1665, and 1667 MHz. The database
contains 12725 OH maser observations at frequencies 1612, 1665, and
1667 MHz selected from the literature . These observations belong to
6245 different objects.
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GAVO Data Center TAP service
The GAVO data center's TAP end point. The Table Access Protocol (TAP)
lets you execute queries against our database tables, inspect various
metadata, and upload your own data. It is thus the VO's premier way to
access public data holdings.
Tables exposed through this endpoint include: \tablesForTAP.
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GAVO DC Custom Uploading Crossmatcher
A plain positional crossmatch service that allows file and URL uploads
to be crossmatched to DC-internal tables. In general, you want to use
TAP for this kind of thing when it is available, but in a pinch it
might come in handy. Larger catalogues that can be matched against
include 2MASS, USNO-B, PPMX, CARS, and more.
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Global TAP Schema Simple Search
The global TAP schema collects information on tables and columns from
known TAP servers. This facilitates locating queriable data by physics
(via UCD) or keywords (via description).
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Lens Image Archive
A collection of images of lensed quasars from various sources.
Included are images from Maidanak Observatory
(ivo://org.gavo.dc/maidanak/res/rawframes/siap), Apache Point
Observatory, from the MiNDSTEp project
(ivo://org.gavo.dc/danish/red/q), and from the Liverpool Robotic
Telescope (ivo://org.gavo.dc/liverpool/res/rawframes/q).
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Light Pollution Weather
We give continuous night and day light measurements at all natural
outdoor light levels by a network of low-cost lightmeters. Developed
to start simple, global continuous high cadence monitoring of night
sky brightness and artificial night sky brightening (light pollution)
in 2009. The lightmeter network is a project of the Thüringer
Landessternwarte, Tautenburg, Germany and the Kuffner-Sternwarte
society at the Kuffner-Observatory, Vienna, Austria.
It started as part of the Dark Skies Awareness cornerstone of the
International Year of Astronomy.
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Liverpool Quasar Lens Monitoring
This collection includes optical monitorings of gravitationally lensed
quasars. The frames can be used to make light curves of quasar images
and field objects. From quasar light curves, one may measure time
delays and flux ratios, analyse variability and chromaticity, etc.
These direct analyses/measurements are basic tools for different
astrophysical studies, e.g., expansion rate of the Universe, mechanism
of intrinsic variability in quasars, accretion disk structure,
supermassive black holes, dark halos of galaxies (dust, collapsed dark
matter, smoothly distributed dark matter,...)