J/ApJ/720/480ivo://CDS.VizieR/J/ApJ/720/480doi:10.26093/cds/vizier.17200480CDSOberg K.I.Qi C.Fogel J.K.J.Bergin E.A.Andrews S.M.Espaillat C.,van Kempen T.A.Wilner D.J.Pascucci I.2012-08-23T07:28:07Z2012-08-23T07:27:56ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frinterferometryradio-astronomyinterstellar-mediumyoung-stellar-objectsradio-spectroscopyChemistry plays an important role in the structure and evolution of protoplanetary disks, with implications for the composition of comets and planets. This is the first of a series of papers based on data from DISCS (Disk Imaging Survey of Chemistry with SMA), a Submillimeter Array survey of the chemical composition of protoplanetary disks. The six Taurus sources in the program (DM Tau, AA Tau, LkCa 15, GM Aur, CQ Tau, and MWC 480) range in stellar spectral type from M1 to A4 and offer an opportunity to test the effects of stellar luminosity on the disk chemistry. The disks were observed in 10 different lines at ~3" resolution and an rms of ~100mJy/beam at ~0.5km/s.2010ApJ...720..480Ohttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/720/480CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+A/463/1017 : B and V light curves of AA Tau (Bouvier+, 2007)J/A+A/409/169 : UBVRI light curves of AA Tau in 1999 (Bouvier+, 2003)J/A+A/349/619 : UBVRI light curves of AA Tau in 1995 (Bouvier+, 1999)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/720/480https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/720/480http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/720/480https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/720/480https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/720/480http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/720/480GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapRadiodefaultJ/ApJ/720/480/table7Integrated spectrarecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameSource namemeta.id;meta.maincharV-CO2-1? CO 2-1 velocitykm/sspect.dopplerVelocfloatnullableF-CO2-1? CO 2-1 flux density (\wGraph{J/ApJ/720/480/DM_Tau}{F-CO2-1}{spectrum})Jyphot.fluxfloatnullableV-HCO+3-2? HCO+ 3-2 velocitykm/sspect.dopplerVelocfloatnullableF-HCO+3-2? HCO+ 3-2 flux density (\wGraph{J/ApJ/720/480/DM_Tau}{F-HCO+3-2}{spectrum})Jyphot.fluxfloatnullableV-DCO+3-2? DCO+ 3-2 velocitykm/sspect.dopplerVelocfloatnullableF-DCO+3-2? DCO+ 3-2 flux density (\wGraph{J/ApJ/720/480/DM_Tau}{F-DCO+3-2}{spectrum})Jyphot.fluxfloatnullableV-N2H+3-2? N2H+ 3-2 velocitykm/sspect.dopplerVelocfloatnullableF-N2H+3-2? N2H+ 3-2 flux density (\wGraph{J/ApJ/720/480/DM_Tau}{F-N2H+3-2}{spectrum})Jyphot.fluxfloatnullableV-H2CO4-3? H2CO 4-3 velocitykm/sspect.dopplerVelocfloatnullableF-H2CO4-3? H2CO 4-3 flux density (\wGraph{J/ApJ/720/480/DM_Tau}{F-H2CO4-3}{spectrum})Jyphot.fluxfloatnullableV-H2CO3-2? H2CO 3-2 velocitykm/sspect.dopplerVelocfloatnullableF-H2CO3-2? H2CO 3-2 flux density (\wGraph{J/ApJ/720/480/DM_Tau}{F-H2CO3-2}{spectrum})Jyphot.fluxfloatnullableV-HCN3-2? HCN 3-2 velocitykm/sspect.dopplerVelocfloatnullableF-HCN3-2? HCN 3-2 flux density (\wGraph{J/ApJ/720/480/DM_Tau}{F-HCN3-2}{spectrum})Jyphot.fluxfloatnullableV-DCN3-2? DCN 3-2 velocitykm/sspect.dopplerVelocfloatnullableF-DCN3-2? DCN 3-2 flux density (\wGraph{J/ApJ/720/480/DM_Tau}{F-DCN3-2}{spectrum})Jyphot.fluxfloatnullableV-CN23-12? CN 2_3_-1_2_ velocitykm/sspect.dopplerVelocfloatnullableF-V-CN23-12? CN 2_3_-1_2_ flux density (\wGraph{J/ApJ/720/480/DM_Tau}{F-V-CN23-12}{spectrum})Jyphot.fluxfloatnullableV-CN22-11? CN 2_2_-1_1_ velocitykm/sspect.dopplerVelocfloatnullableF-CN22-11? CN 2_2_-1_1_ flux density (\wGraph{J/ApJ/720/480/DM_Tau}{F-CN22-11}{spectrum})Jyphot.fluxfloatnullable