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<ri:Resource created="2019-02-12T06:52:35Z" status="active" updated="2025-06-13T15:25:00Z" 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/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>Comet C/2017 E4 composition with iSHELL at NASA/IRTF</title><shortName>J/AJ/156/68</shortName><identifier>ivo://CDS.VizieR/J/AJ/156/68</identifier><altIdentifier>doi:10.26093/cds/vizier.51560068</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Faggi S.</name></creator><creator><name>Villanueva G.L.</name></creator><creator><name>Mumma M.J.</name></creator><creator><name>Paganini L.</name></creator><date role="Updated">2019-03-11T08:34:27Z</date><date role="Created">2019-02-12T06:52:35Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>solar-system</subject><subject>comets</subject><subject>molecular-physics</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><description>In 2017 April, we acquired comprehensive high-resolution spectra of newly discovered comet C/2017 E4 (Lovejoy) as it approached perihelion, and before its disintegration. We detected many cometary emission lines in the range (2.8-5.3) {mu}m, in four customized instrument settings (L1-c, L3, Lp1-c, and M1) of iSHELL - the new near-IR high-resolution immersion echelle spectrograph at NASA/IRTF (Maunakea, Hawaii). We identified 12 molecular species: nine primary volatiles (H_2_O, HCN, NH_3_, CO, C_2_H_2_, C_2_H_6_, CH_4_, CH_3_OH, H_2_CO) and three product species (CN, NH_2_, OH). We detected 85 H_2_O emission lines from 12 water vibrational bands across L1-c and M1 settings. The many detected water emission lines enabled retrieval of accurate measures for ortho- and para-H_2_O independently, thereby reducing systematic uncertainty in the derived ortho-para ratio and nuclear spin temperature. Excitation analyses and emission profile analyses were performed for all species, and molecular abundance ratios relative to water are compared with values found for other Oort Cloud comets in our infrared database. Abundance ratios are consistent for most species, with the exception of underabundant methanol and overabundant ammonia in E4.</description><source format="bibcode">2018AJ....156...68F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/156/68</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/B/comets">B/comets : Database of the orbital elements of comets (Rocher, 2007)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/156/68</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/156/68</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/156/68</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/156/68</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/156/68</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/156/68</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/156/68/table3</name><description>Mean flux calibration factors</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Set</name><description>Instrument setting (G1)</description><ucd>instr.setup</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Order</name><description>[18/184] Order number per each setting</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Freq</name><description>[1933.8252/3534.9645] Mean frequency across the orders</description><unit>cm**-1</unit><ucd>em.freq</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Gamma</name><description>[1.1642e-17/2.7809e-17] Mean {Gamma} calibration factor per order (1)</description><unit>W.m**-2.cm.count**-1.s**-1</unit><ucd>arith.factor</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Through</name><description>[4.38/10.63] Throughputs of individuals orders</description><unit>%</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/AJ/156/68/table4</name><description>Detected individual emission lines of volatile species in C/2017 E4 (Lovejoy)</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Mol</name><description>Molecule name</description><ucd>meta.id;phys.mol</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>ID</name><description>Molecular identifier</description><ucd>meta.id;phys.mol</ucd></column><column><name>Trot</name><description>[75/81] Rotational temperature</description><unit>K</unit><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_Trot</name><description>[3/11]? Uncertainty in Trot</description><unit>K</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Multi</name><description>[1e-08/1e-05] g-factor multiplier; e.g. g-fac*Multi</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Set</name><description>iSHELL/IRTF setting (G1)</description><ucd>instr.setup</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>f_Set</name><description>[1/12] Flag on Set giving the orders (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Trans</name><description>Transition quantum numbers; up-low</description><ucd>phys.atmol.qn;phys.atmol.transition</ucd></column><column><name>Freq</name><description>[1949.8073/3539.52]? Mean frequency</description><unit>cm**-1</unit><ucd>em.freq</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Flux</name><description>[0.06/112.59]? Flux of the cometary line at top of the Earth atmosphere</description><unit>1e-19W.m**-2</unit><ucd>phot.flux;spect.line</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_Flux</name><description>[0.28/8.2182]? Uncertainty in Flux</description><unit>1e-19W.m**-2</unit><ucd>stat.error;phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>g-fac</name><description>[0.361/207.5]? Molecular g-factor (fluorescence efficiency)</description><unit>ph.s**-1.mol**-1</unit><ucd>phys.atmol</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Erot</name><description>[0/607.61]? Rotational energy</description><unit>cm**-1</unit><ucd>phys.energy;phys.mol.rotation</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Transm</name><description>[0.1111/0.9963]? Atmospheric transmittance at the Doppler-shifted position of the cometary line</description><ucd>phys.atmol</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>