<?xml version='1.0'?><?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?><ri:Resource created="2015-07-16T09:19:00Z" status="active" updated="2024-06-07T12:01:03Z" version="1.2" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/RegistryInterface/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/RegistryInterface.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:DataService"><title>Download guard for hsoy dump</title><identifier>ivo://org.gavo.dc/hsoy/q/download</identifier><altIdentifier>doi:10.21938/HP1ASPBYWElyXb6qdqyolg</altIdentifier><curation><publisher>The GAVO DC team</publisher><creator><name>Demleitner, M.</name></creator><creator><name>Röser, S.</name></creator><creator><name>Altmann, M.</name></creator><creator><name>Bastian, U.</name></creator><creator><name>Schilbach, E.</name></creator><date role="Updated">2017-02-01T00:00:00Z</date><date role="updated">2017-01-31</date><contact><name>GAVO Data Centre Team</name><address>Mönchhofstrasse 12-14, D-69120 Heidelberg</address><email>gavo@ari.uni-heidelberg.de</email><telephone>+49 6221 54 1837</telephone></contact></curation><content><subject>stars</subject><subject>surveys</subject><subject>astrometry</subject><subject>proper-motions</subject><description>
HSOY is a catalog of 583'001'653 objects with precise astrometry based on
PPMXL and Gaia DR1.  Typical formal errors at mean epoch in proper motion are
below 1 mas/yr for objects brighter than 10 mag, and about 5 mas/yr at the
faint end (about 20 mag). South of -30 degrees, astrometry is significantly
worse.  HSOY also contains, where available, USNO-B, Gaia, and 2MASS
photometry.  HSOY's positions and proper motions are given for epoch J2000.
The catalog becomes severely incomplete faintwards of 16 mag in the G-band.
The mean epochs are typically very close to Gaia's J2015.

HSOY still contains about 0.7% spurious close
"binaries" (non-matched stars) from the original USNO-B (marked with non-NULL
clone).  Also, failed matches within Gaia DR1 contribute another 1.5% spurious
pairs (marked with non-NULL comp).  In both cases, astrometry presumably is
sub-standard.

More information is available at http://dc.g-vo.org/hsoy.</description><source format="bibcode">2017A&amp;A...600L...4A</source><referenceURL>http://dc.g-vo.org/hsoy/q/download/info</referenceURL><contentLevel>Research</contentLevel></content><rights rightsURI="https://spdx.org/licenses/CC0-1.0.html">To the extent possible under law, the publisher has waived all copyright and related or neighboring rights to HSOY.  For details, see the `Creative Commons CC0 1.0 Public Domain dedication &lt;http://creativecommons.org/publicdomain/zero/1.0/&gt;`_.  Of course, you should still give proper credit when using this data as required by good scientific practice.

.. image:: /static/img/cc0.png
   :alt: [CC0]

</rights><instrument>Gaia</instrument><coverage><spatial>0/0-11</spatial><temporal>51544 51544</temporal><spectral>8.277e-20 5.369e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">http://dc.g-vo.org/hsoy/q/download/coverage</footprint><waveband>Optical</waveband></coverage></ri:Resource>