<?xml version='1.0'?><?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?><ri:Resource created="2012-04-25T19:19:00Z" status="active" updated="2024-12-27T08:31:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:g-colstat="http://dc.g-vo.org/ColStats-1" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vg="http://www.ivoa.net/xml/VORegistry/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/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd 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/VORegistry/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VORegistry.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:CatalogService"><title>Reference HII Regions for Abundance Determination (SCS)</title><shortName>HII props scs</shortName><identifier>ivo://org.gavo.dc/hiicounter/q/scs</identifier><curation><publisher>The GAVO DC team</publisher><creator><name>Pilyugin, L.S.</name></creator><creator><name>Grebel, E.K.</name></creator><creator><name>Mattsson, L.</name></creator><date role="Updated">2012-05-02T00:00:00Z</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>interstellar-abundances</subject><subject>h-ii-regions</subject><description> A table containing reference data for HII regions. We also give a
source code to compute abundances and electron temperatures in HII
regions from strong emission lines.</description><source format="bibcode">2012MNRAS.424.2316P</source><referenceURL>https://dc.g-vo.org/hiicounter/q/scs/info</referenceURL><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://org.gavo.dc/tap">GAVO Data Center TAP service</relatedResource></relationship></content><rights>If you use the data or software distributed here, please reference
2012MNRAS.424.2316P. This research was funded in part by SFB 881 "The
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source code to compute abundances and electron temperatures in HII
regions from strong emission lines.</description><table><name>hiicounter.data</name><description> A table containing reference data for HII regions. We also give a
source code to compute abundances and electron temperatures in HII
regions from strong emission lines.</description><nrows>414</nrows><column><name>ident</name><description>Identifier of the HII region in this catalog</description><ucd>meta.id;meta.main</ucd><stats><min>1</min><percentile03>13.389999999999999</percentile03><median>207.5</median><percentile97>401.61</percentile97><max>414</max><fillFactor>1.0</fillFactor></stats><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>logr3</name><description>Log of [OIII] R_3 line intensity relative to Hβ</description><ucd>spect.line.intensity;arith.ratio</ucd><stats><min>-1.057</min><percentile03>-0.27447</percentile03><median>0.744</median><percentile97>0.99583</percentile97><max>1.091</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logr2</name><description>Log of [OII] R_2 line intensity relative to Hβ</description><ucd>spect.line.intensity;arith.ratio</ucd><stats><min>-0.662</min><percentile03>-0.45387</percentile03><median>0.207</median><percentile97>0.54566</percentile97><max>0.653</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logn2</name><description>Log of [NII] N_2 line intensity relative to Hβ</description><ucd>spect.line.intensity;arith.ratio</ucd><stats><min>-1.973</min><percentile03>-1.762</percentile03><median>-0.898</median><percentile97>0.12049</percentile97><max>0.333</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logs2</name><description>Log of [SII] S_2 line intensity relative to Hβ</description><ucd>spect.line.intensity;arith.ratio</ucd><stats><min>-1.509</min><percentile03>-1.2647</percentile03><median>-0.6135</median><percentile97>-0.16639</percentile97><max>-0.058</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>o_h</name><description>T_e-based oxygen abundance given as 12+log(O/H)</description><ucd>phys.abund;arith.ratio</ucd><stats><min>7.09</min><percentile03>7.2812</percentile03><median>8.07</median><percentile97>8.55</percentile97><max>8.76</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>n_h</name><description>T_e-based nitrogen abundance given as 12+log(N/H)</description><ucd>phys.abund;arith.ratio</ucd><stats><min>5.63</min><percentile03>5.8939</percentile03><median>6.645</median><percentile97>7.8161</percentile97><max>8.57</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>t3</name><description>Electron temperature derived as given in t3src, reduced to t_3([O III])</description><unit>K</unit><ucd>phys.temperature.electron</ucd><stats><min>4100</min><percentile03>6539</percentile03><median>13100</median><percentile97>19461</percentile97><max>21500</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>t3src</name><description>Lines used for determination of t_3</description><ucd>meta.code;phys.temperature.electron</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>region_name</name><description>Name of the HII region.</description><ucd>meta.id;src</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>src</name><description>Reference to the source of the data quoted.</description><ucd>meta.bib.bibcode</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>hostalpha</name><description>ICRS RA of host object (from Simbad)</description><ucd>pos.eq.ra;meta.main</ucd><stats><min>0.492337</min><percentile03>5.0965</percentile03><median>164.446</median><percentile97>294.882</percentile97><max>354.561</max><fillFactor>0.833333</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>indexed</flag><flag>nullable</flag></column><column><name>hostdelta</name><description>ICRS Dec of host object (from Simbad)</description><ucd>pos.eq.dec;meta.main</ucd><stats><min>-66.4983</min><percentile03>-41.3763</percentile03><median>6.17278</median><percentile97>69.1924</percentile97><max>75.6278</max><fillFactor>0.833333</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>indexed</flag><flag>nullable</flag></column></table></schema></tableset></ri:Resource>