J/A+A/709/A241ivo://CDS.VizieR/J/A+A/709/A241CDSGuarneri F.Schindler J.T.Meyer R.A.Yang D.Hennawi J.F.,Lucie-Smith L.Bosman S.E.I.Davies F.B.2026-06-01T06:19:08Z2026-05-19T12:30:29ZCDS support team

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

cds-question@unistra.frsurveysquasarsspectroscopyultraviolet-astronomyvisible-astronomyQuasars at the redshift frontier (z>7.0) are fundamental probes of black hole growth and evolution but notoriously difficult to identify. At these redshifts, machine learning-based selection methods have proven to be efficient, but require appropriate training sets to express their full potential. Here, we present QUEST, a Variational Auto-Encoder capable of generating realistic quasar spectra that can be post-processed for the generation of synthetic photometry and for spectral imputation. We start from the SDSS DR16Q catalogue, pre-process the spectra, and vet the sample to obtain a clean data set. After training the model, we investigate the properties of its latent space to understand whether it has learnt relevant physics. Furthermore, we provide a pipeline to generate photometry from the sampled spectra, compare it with actual quasar photometry, and showcase the capabilities of the model in reconstructing and extending quasar spectra. The trained network faithfully reproduces the input spectrum, both in terms of sample median and variance. By examining the latent space, we find correlations with, among others, continuum and bolometric luminosity, black hole mass, redshift, continuum slope, and emission line properties. When used to generate photometry, we find results in excellent agreement with the control sample. The model provides satisfactory results in reconstructing emission lines: estimates of the black hole mass from the reconstructed spectra are in good agreement with those from the original SDSS spectra. Furthermore, when spectra with broad absorption line features are reconstructed, the model successfully interpolates over the absorption systems. Compared with previous work, we find excellent agreement between the spectra sampled from our model and the output of their results. However, QUEST does not require any ad-hoc tuning, and is capable of reproducing the full variety of spectra available in the training set.2026A&A...709A.241Ghttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/709/A241CatalogResearchIsServedByTAP VizieR generic servicerelated-toVII/289 : SDSS quasar catalog, sixteenth data release (Lyke+, 2020)J/A+A/585/A87 : Quasar composite made from bright QSOs (Selsing+, 2016)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/709/A241https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/709/A241http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/709/A241https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/709/A241https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/709/A241http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/709/A241GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapUVOpticaldefaultJ/A+A/709/A241/tablea1Median composite of the general purpose training datasetrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlambdaRest-fame wavelength0.1nmem.wldoubleMedFluxMedian flux array (1)phot.fluxdoubleNspNumber of contributing spectra in a pixelmeta.numberfloat1stperc01st percentile array (1)stat.fit.paramdouble16thperc16th percentile array (1)stat.fit.paramdouble84thperc84th percentile array (1)stat.fit.paramdouble99thperc99th percentile array (1)stat.fit.paramdoubleJ/A+A/709/A241/tablee1SDSS identifiers for objects in each cluster (Fig. 9), and boolean indicating which cluster they belong torecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSDSSSDSS identifier (SDSS_JHHMMSS.ss+DDMMSS.s)meta.id;meta.maincharClusterRed[0/1] Part of red cluster?meta.codeintClusterBlue[0/1] Part of blue cluster?meta.codeintClusterGreen[0/1] Part of green cluster?meta.codeint