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<ri:Resource created="2017-10-18T15:11:44Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" 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/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.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>PESSTO catalog</title><shortName>J/A+A/579/A40</shortName><identifier>ivo://CDS.VizieR/J/A+A/579/A40</identifier><altIdentifier>doi:10.26093/cds/vizier.35790040</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Smartt S.J.</name></creator><creator><name>Valenti S.</name></creator><creator><name>Fraser M.</name></creator><creator><name>Inserra C.</name></creator><creator><name>Young D.R.</name></creator><creator><name>Sullivan M.,Pastorello A.</name></creator><creator><name>Benetti S.</name></creator><creator><name>Gal-Yam A.</name></creator><creator><name>Knapic C.</name></creator><creator><name>Molinaro M.,Smareglia R.</name></creator><creator><name>Smith K.W.</name></creator><creator><name>Taubenberger S.</name></creator><creator><name>Yaron O.</name></creator><creator><name>Anderson J.P.,Ashall C.</name></creator><creator><name>Balland C.</name></creator><creator><name>Baltay C.</name></creator><creator><name>Barbarino C.</name></creator><creator><name>Bauer F.E.</name></creator><creator><name>Baumont S.,Bersier D.</name></creator><creator><name>Blagorodnova N.</name></creator><creator><name>Bongard S.</name></creator><creator><name>Botticella M.T.</name></creator><creator><name>Bufano F.,Bulla M.</name></creator><creator><name>Cappellaro E.</name></creator><creator><name>Campbell H.</name></creator><creator><name>Cellier-Holzem F.</name></creator><creator><name>Chen T.-W.,Childress M.J.</name></creator><creator><name>Clocchiatti A.</name></creator><creator><name>Contreras C.</name></creator><creator><name>Dall'ora M.</name></creator><creator><name>Danziger J.,De Jaeger T.</name></creator><creator><name>De Cia A.</name></creator><creator><name>Della Valle M.</name></creator><creator><name>Dennefeld M.</name></creator><creator><name>Elias-Rosa N.,Elman N.</name></creator><creator><name>Feindt U.</name></creator><creator><name>Fleury M.</name></creator><creator><name>Gall E.</name></creator><creator><name>Gonzalez-Gaitan S.</name></creator><creator><name>Galbany L.,Morales Garoffolo A.</name></creator><creator><name>Greggio L.</name></creator><creator><name>Guillou L.L.</name></creator><creator><name>Hachinger S.</name></creator><creator><name>Hadjiyska E.,Hage P.E.</name></creator><creator><name>Hillebrandt W.</name></creator><creator><name>Hodgkin S.</name></creator><creator><name>Hsiao E.Y.</name></creator><creator><name>James P.A.,Jerkstrand A.</name></creator><creator><name>Kangas T.</name></creator><creator><name>Kankare E.</name></creator><creator><name>Kotak R.</name></creator><creator><name>Kromer M.</name></creator><creator><name>Kuncarayakti H.,Leloudas G.</name></creator><creator><name>Lundqvist P.</name></creator><creator><name>Lyman J.D.</name></creator><creator><name>Hook I.M.</name></creator><creator><name>Maguire K.</name></creator><creator><name>Manulis I.,Margheim S.J.</name></creator><creator><name>Mattila S.</name></creator><creator><name>Maund J.R.</name></creator><creator><name>Mazzali P.A.</name></creator><creator><name>Mccrum M.,Mckinnon R.</name></creator><creator><name>Moreno-Raya M.E.</name></creator><creator><name>Nicholl M.</name></creator><creator><name>Nugent P.</name></creator><creator><name>Pain R.</name></creator><creator><name>Pignata G.,Phillips M.M.</name></creator><creator><name>Polshaw J.</name></creator><creator><name>Pumo M.L.</name></creator><creator><name>Rabinowitz D.</name></creator><creator><name>Reilly E.,Romero-Canizales C.</name></creator><creator><name>Scalzo R.</name></creator><creator><name>Schmidt B.</name></creator><creator><name>Schulze S.</name></creator><creator><name>Sim S.,Sollerman J.</name></creator><creator><name>Taddia F.</name></creator><creator><name>Tartaglia L.</name></creator><creator><name>Terreran G.</name></creator><creator><name>Tomasella L.,Turatto M.</name></creator><creator><name>Walker E.</name></creator><creator><name>Walton N.A.</name></creator><creator><name>Wyrzykowski L.</name></creator><creator><name>Yuan F.</name></creator><creator><name>Zampieri L.</name></creator><date role="Updated">2017-11-13T13:07:03Z</date><date role="Created">2017-10-18T15:11:44Z</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>supernovae</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>Wide-band photometry</subject><subject>sloan-photometry</subject><description>The Public European Southern Observatory Spectroscopic Survey of Transient Objects (PESSTO) began as a public spectroscopic survey in April 2012. PESSTO classifies transients from publicly available sources and wide-field surveys, and selects science targets for detailed spectroscopic and photometric follow-up. PESSTO runs for nine months of the year, January - April and August - December inclusive, and typically has allocations of 10 nights per month. We describe the data reduction strategy and data products that are publicly available through the ESO archive as the Spectroscopic Survey data release 1 (SSDR1). PESSTO uses the New Technology Telescope with the instruments EFOSC2 and SOFI to provide optical and NIR spectroscopy and imaging. We target supernovae and optical transients brighter than 20.5^m^ for classification. Science targets are selected for follow-up based on the PESSTO science goal of extending knowledge of the extremes of the supernova population. We use standard EFOSC2 set-ups providing spectra with resolutions of 13-18{AA} between 3345-9995{AA}. A subset of the brighter science targets are selected for SOFI spectroscopy with the blue and red grisms (0.935-2.53{mu}m and resolutions 23-33{AA}) and imaging with broadband JHK_s_ filters. This first data release (SSDR1) contains flux calibrated spectra from the first year (April 2012-2013). A total of 221 confirmed supernovae were classified, and we released calibrated optical spectra and classifications publicly within 24h of the data being taken (via WISeREP). The data in SSDR1 replace those released spectra. They have more reliable and quantifiable flux calibrations, correction for telluric absorption, and are made available in standard ESO Phase 3 formats. We estimate the absolute accuracy of the flux calibrations for EFOSC2 across the whole survey in SSDR1 to be typically ~15%, although a number of spectra will have less reliable absolute flux calibration because of weather and slit losses. Acquisition images for each spectrum are available which, in principle, can allow the user to refine the absolute flux calibration. The standard NIR reduction process does not produce high accuracy absolute spectrophotometry but synthetic photometry with accompanying JHK_s_ imaging can improve this. Whenever possible, reduced SOFI images are provided to allow this. Future data releases will focus on improving the automated flux calibration of the data products. 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Landolt U magnitude in Vega system (U_VEGA_MAG)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Umag</name><description>? rms uncertainty on Umag (U_VEGA_MAGERR)</description><unit>mag</unit><ucd>stat.error;phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Bmag</name><description>? Landolt B magnitude in Vega system (B_VEGA_MAG)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Bmag</name><description>? rms uncertainty on Bmag (B_VEGA_MAGERR)</description><unit>mag</unit><ucd>stat.error;phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Vmag</name><description>? 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Swift V magnitude (V_SWIFT_MAG)</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_VSmag</name><description>? rms uncertainty on VSmag (V_SWIFT_MAGERR)</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/A+A/579/A40/pessto</name><description>PESSTO Public ESO Spectroscopic Survey of Transient Objects</description><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="29*">char</dataType></column><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>LC</name><description>Show the light curves</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>Source</name><description>Transient discovery ID (TRANSIENT_DISCOVERY_ID)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>RAJ2000</name><description>Transient right ascension (J2000) (TRANSIENT_RAJ2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Transient declination (J2000) (TRANSIENT_DECJ2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Class</name><description>Transient classification (TRANSIENT_CLASSIFICATION) (1)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>f_Class</name><description>[0/1] Transient classification peculiar flag (TRANSIENT_CLASSIFICATION_PECULIAR_FLAG) (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>r_Class</name><description>Transient classification source (TRANSIENT_CLASSIFICATION_SOURCE)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>ClassA</name><description>? Transient classification ATel number reporting the classification (TRANSIENT_CLASSIFICATION_ATEL)</description><ucd>meta.bib</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>MJD</name><description>MJD at the point of classification (TRANSIENT_CLASSIFICATION_MJD)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>z</name><description>Transient redshift measured from the classification spectra (TRANSIENT_CLASSIFICATION_REDSHIFT)</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Phase</name><description>Phase of the transient at classification with respect to maximum light (TRANSIENT_CLASSIFICATION_PHASE)</description><unit>d</unit><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>b_Phase</name><description>? Estimated lower limit of the phase of the transient (TRANSIENT_CLASSIFICATION_PHASE_LOWER_LIMIT)</description><unit>d</unit><ucd>time.phase;stat.min</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>B_Phase</name><description>? Estimated upper limit of the phase of the transient (TRANSIENT_CLASSIFICATION_PHASE_UPPER_LIMIT)</description><unit>d</unit><ucd>time.phase;stat.max</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>DMJD</name><description>MJD at the point of discovery, reported from the originating discovery survey (TRANSIENT_DISCOVERY_MJD)</description><ucd>phot.mag;arith.zp</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Dmag</name><description>Magnitude of the transient at the point of discovery, reported from the originating discovery survey (TRANSIENT_DISCOVERY_MAG)</description><ucd>phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DFilt</name><description>Transient discovery magnitude filter (TRANSIENT_DISCOVERY_MAG_FILTER)</description><ucd>instr.bandpass</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>FT</name><description>[0/1] Target followup (FOLLOWUP_TARGET) (3)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>HStage</name><description>[1/5]? Stage of the transient-galaxy cross-match method at which the host galaxy was matched (HOST_SEARCH_STAGE)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Host</name><description>Host galaxy name (HOST_ID)</description><ucd>meta.id.parent</ucd><dataType xsi:type="vs:VOTableType" arraysize="30*">char</dataType></column><column><name>HRAdeg</name><description>? Host galaxy right ascension (J2000) (HOST_RAJ2000)</description><unit>deg</unit><ucd>pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>HDEdeg</name><description>? Host galaxy declination (J2000) (HOST_DECJ2000)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>OffN</name><description>? N-S transient-host separation (Positive means the transient is North of the host) (HOST_OFFSET_N)</description><unit>deg</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>OffE</name><description>? E-W transient-host separation (Positive means the transient is East of the host) (HOST_OFFSET_E)</description><unit>deg</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>r_Hzsp</name><description>Source for Hzsp (HOST_REDSHIFT_SPEC_SOURCE)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>Hzsp</name><description>? Host galaxy spectroscopic redshift (HOST_REDSHIFT_SPEC)</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>r_Hzph</name><description>Source for Hzph (HOST_REDSHIFT_PHOT_SOURCE)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>Hzph</name><description>? Host galaxy photometric redshift (HOST_REDSHIFT_PHOT)</description><ucd>src.redshift.phot</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_Hzph</name><description>? rms uncertainty on Hzph (HOST_REDSHIFT_PHOT_ERR)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Name</name><description>Transient IAU id, SNYYYYaa (TRANSIENT_IAU_ID)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>OName</name><description>Transient alternative ids (TRANSIENT_ALTERNATIVE_IDS)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="65*">char</dataType></column><column><name>PName</name><description>Name used in mphot.dat file</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column></table></schema></tableset></ri:Resource>