<?xml version='1.0'?><?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?><ri:Resource created="2009-07-21T08:32:00Z" status="active" updated="2024-02-06T08:59:19Z" version="1.2" xmlns:g-colstat="http://dc.g-vo.org/ColStats-1" 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://dc.g-vo.org/ColStats-1 http://vo.ari.uni-heidelberg.de/docs/schemata/Colstats.xsd 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:CatalogResource"><title>A Database of Circumstellar OH Masers</title><shortName>ohmaser.masers</shortName><identifier>ivo://org.gavo.dc/ohmaser/q/masers</identifier><curation><publisher>The GAVO DC team</publisher><creator><name>Engels, D.</name><logo>http://dc.g-vo.org/ohmaser/q/scs/static/uhlogo.png</logo></creator><creator><name>Bunzel, F.</name></creator><date role="Updated">2015-09-02T00:00:00Z</date><date role="Updated">2015-07-09</date><version>2.4</version><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>astrophysical-masers</subject><subject>surveys</subject><subject>asymptotic-giant-branch-stars</subject><description>Maser data proper.</description><source format="bibcode">2015A&amp;A...582A..68E</source><referenceURL>http://dc.g-vo.org/tableinfo/ohmaser.masers</referenceURL></content><coverage><spatial>1/0,2,13,21,23,28,30-31,41
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maser emission in the transitions at 1612, 1665, and 1667 MHz. The
database contains OH maser observations selected from the literature .
These observations belong to more than 6000 different objects. The
database consists of three tables: The main table ("masers"),
interferometric followup observations ("maps") and monitoring programs
("monitor").</description><table><name>ohmaser.masers</name><description>Maser data proper.</description><nrows>13655</nrows><column><name>measure_no</name><description>Unique measurement identifier</description><ucd>meta.id;meta.main</ucd><stats><min>1</min><percentile03>410.62</percentile03><median>6837.0</median><percentile97>25691.379999999997</percentile97><max>34179</max><fillFactor>1.0</fillFactor></stats><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>source_no</name><description>Unique, artificial source identifier</description><ucd>meta.code</ucd><stats><min>1</min><percentile03>222.62</percentile03><median>6038.0</median><percentile97>25500.0</percentile97><max>34174</max><fillFactor>1.0</fillFactor></stats><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>flag</name><description>Non-null if this measurement is considered the best available at a particular frequency. Lower means higher confidence.</description><ucd>meta.code</ucd><stats><min>1</min><percentile03>1.0</percentile03><median>1.0</median><percentile97>3.0</percentile97><max>3</max><fillFactor>0.7250824</fillFactor></stats><dataType xsi:type="vs:VOTableType">short</dataType><flag>nullable</flag></column><column><name>source_name</name><description>Name of the observed source. The name given in the reference is usually kept.</description><ucd>meta.id</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType></column><column><name>frequency</name><description>Observed frequency</description><unit>MHz</unit><ucd>em.freq</ucd><stats><min>1612</min><percentile03>1612.0</percentile03><median>1612.0</median><percentile97>1667.0</percentile97><max>1667</max><fillFactor>1.0</fillFactor><option>1612</option><option>1665</option><option>1667</option></stats><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>spec_type</name><description>S -- Single peak of maser emission; D -- Double peak of maser emission; I -- Irregular spectral profile, multiple emission peaks.</description><ucd>meta.code;src.spType</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>ra_raw</name><description>J2000 RA</description><ucd>pos.eq.ra</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>de_raw</name><description>J2000 Dec</description><ucd>pos.eq.dec</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>veloc_blue</name><description>Velocity of the blue-shifted maser peak. For single-peak masers it contains the line velocity.</description><unit>km/s</unit><ucd>phys.veloc.expansion;pos.bodyrc</ucd><stats><min>-374</min><percentile03>-148.48</percentile03><median>0.3</median><percentile97>127.645</percentile97><max>365.2</max><fillFactor>0.362944</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>veloc_red</name><description>Velocity of the red-shifted maser peak in km/s. It contains the line velocity for a single peak maser if it corresponds to the red-shifted peak in other observations.</description><unit>km/s</unit><ucd>phys.veloc.expansion;pos.bodyrc</ucd><stats><min>-336.2</min><percentile03>-123.908</percentile03><median>22.1</median><percentile97>151.963</percentile97><max>319.6</max><fillFactor>0.298792</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>veloc_central</name><description>Radial velocity of the central star. If veloc_central is not given in the reference, it is calculated.</description><unit>km/s</unit><ucd>phys.veloc.expansion;pos.bodyrc</ucd><stats><min>-355.1</min><percentile03>-138</percentile03><median>9.4</median><percentile97>137.508</percentile97><max>365.2</max><fillFactor>0.370926</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>veloc_shell</name><description>Outflow Velocity of the shell. If vexp is not given in the reference it is calculated.</description><unit>km/s</unit><ucd>phys.veloc.expansion;pos.bodyrc</ucd><stats><min>-48.8</min><percentile03>1.4</percentile03><median>13.8</median><percentile97>24</percentile97><max>87.5</max><fillFactor>0.300037</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>veloc_err</name><description>Uncertainty of velocity values. Taken from the velocity resolution of the observation. It is actually a lower limit of the uncertainty, because the lines are usually much broader than velocity resolution of the observing equipment.</description><unit>km/s</unit><ucd>stat.error;phys.veloc.expansion;pos.bodyrc</ucd><stats><min>0</min><percentile03>0.1</percentile03><median>0.9</median><percentile97>1.5</percentile97><max>2.27</max><fillFactor>0.945441</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>flux_dens_flag</name><description>NULL -- flux density columns contain detections; &lt; -- non-detection at level flux density blue (3 sigma); &gt; -- flux density blue contains a lower limit for the flux; = -- source only gives fluxes; . -- flux density blue contains probable detection; : -- flux density red contains probable detection; &amp; -- both flux densities contain probable detections</description><ucd>meta.code</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>flux_dens_blue</name><description>Flux Density of the blue-shifted maser peak. For single-peak masers it contains its flux density.</description><unit>Jy</unit><ucd>phot.flux.density;em.radio.1500-3000MHz</ucd><stats><min>-3.22</min><percentile03>0.02</percentile03><median>0.2</median><percentile97>7.60424</percentile97><max>1921</max><fillFactor>0.977664</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>flux_dens_red</name><description>Flux Density of the red-shifted maser peak. It contains the flux density for a single peak maser, if it corresponds to the red-shifted peak in other observations.</description><unit>Jy</unit><ucd>phot.flux.density;em.radio.1500-3000MHz</ucd><stats><min>-1.33</min><percentile03>0.038</percentile03><median>0.69</median><percentile97>27.2852</percentile97><max>597.28</max><fillFactor>0.295643</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>int_flux_red</name><description>Integrated flux of red peak</description><unit>1e-22W.m**-2</unit><ucd>phot.flux.density;em.radio.1500-3000MHz</ucd><stats><min>0.002</min><percentile03>0.022</percentile03><median>0.639</median><percentile97>26.0034</percentile97><max>238.1</max><fillFactor>0.0407177</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>int_flux_blue</name><description>Integrated flux of blue peak</description><unit>1e-22W.m**-2</unit><ucd>phot.flux.density;em.radio.1500-3000MHz</ucd><stats><min>-0.312</min><percentile03>0.02565</percentile03><median>0.548</median><percentile97>25.1922</percentile97><max>1152.4</max><fillFactor>0.048041</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ref_key</name><description>Internal key for the originating paper, see ohmasers.bibrefs.</description><ucd>meta.bib</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>rapub</name><description>RA of object, from source</description><unit>deg</unit><ucd>pos.eq.ra</ucd><stats><min>0.0273417</min><percentile03>39.2598</percentile03><median>268.065</median><percentile97>334.999</percentile97><max>359.767</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>depub</name><description>Dec of object, from source</description><unit>deg</unit><ucd>pos.eq.dec</ucd><stats><min>-87.3389</min><percentile03>-62.369</percentile03><median>-2.57944</median><percentile97>60.9416</percentile97><max>86.6369</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>raj2000</name><description>Selected best RA, J2000</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><stats><min>0.0273417</min><percentile03>39.2583</percentile03><median>268.065</median><percentile97>334.999</percentile97><max>359.767</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">double</dataType><flag>indexed</flag><flag>nullable</flag></column><column><name>dej2000</name><description>Selected best Dec, J2000</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><stats><min>-87.3389</min><percentile03>-62.369</percentile03><median>-2.58053</median><percentile97>60.9411</percentile97><max>86.6369</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">double</dataType><flag>indexed</flag><flag>nullable</flag></column><column><name>mapurl</name><description>URL to information on an interferometric followup observation for this object.</description><ucd>meta.ref.url</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>monitorurl</name><description>URL to information on a monitor programme for this object.</description><ucd>meta.ref.url</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><foreignKey><targetTable>ohmaser.bibrefs</targetTable><fkColumn><fromColumn>ref_key</fromColumn><targetColumn>ref_key</targetColumn></fkColumn></foreignKey></table></schema></tableset></ri:Resource>