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dc.contributor.authorSnyder, Gregory F.
dc.contributor.authorVogelsberger, Mark
dc.contributor.authorHayward, Christopher C.
dc.contributor.authorGenel, Shy
dc.contributor.authorSijacki, Debora
dc.contributor.authorSpringel, Volker
dc.contributor.authorHernquist, Lars
dc.contributor.authorNelson, Dylan
dc.contributor.authorKriek, Mariska
dc.contributor.authorPillepich, Annalisa
dc.contributor.authorSales, Laura V.
dc.contributor.authorMcBride, Cameron K.
dc.contributor.authorTorrey, Paul A.
dc.date.accessioned2015-09-11T13:00:48Z
dc.date.available2015-09-11T13:00:48Z
dc.date.issued2015-01
dc.date.submitted2014-11
dc.identifier.issn0035-8711
dc.identifier.issn1365-2966
dc.identifier.urihttp://hdl.handle.net/1721.1/98458
dc.description.abstractWe present our methods for generating a catalogue of 7000 synthetic images and 40 000 integrated spectra of redshift z = 0 galaxies from the Illustris simulation. The mock data products are produced by using stellar population synthesis models to assign spectral energy distributions (SED) to each star particle in the galaxies. The resulting synthetic images and integrated SEDs therefore properly reflect the spatial distribution, stellar metallicity distribution, and star formation history of the galaxies. From the synthetic data products, it is possible to produce monochromatic or colour-composite images, perform SED fitting, classify morphology, determine galaxy structural properties, and evaluate the impacts of galaxy viewing angle. The main contribution of this paper is to describe the production, format, and composition of the image catalogue that makes up the Illustris Simulation Observatory. As a demonstration of this resource, we derive galactic stellar mass estimates by applying the SED fitting code fast to the synthetic galaxy products, and compare the derived stellar masses against the true stellar masses from the simulation. We find from this idealized experiment that systematic biases exist in the photometrically derived stellar mass values that can be reduced by using a fixed metallicity in conjunction with a minimum galaxy age restriction.en_US
dc.language.isoen_US
dc.publisherOxford University Pressen_US
dc.relation.isversionofhttp://dx.doi.org/10.1093/mnras/stu2592en_US
dc.rightsCreative Commons Attribution-Noncommercial-Share Alikeen_US
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/4.0/en_US
dc.sourcearXiven_US
dc.titleSynthetic galaxy images and spectra from the Illustris simulationen_US
dc.typeArticleen_US
dc.identifier.citationTorrey, P., G. F. Snyder, M. Vogelsberger, C. C. Hayward, S. Genel, D. Sijacki, V. Springel, et al. “Synthetic Galaxy Images and Spectra from the Illustris Simulation.” Monthly Notices of the Royal Astronomical Society 447, no. 3 (January 5, 2015): 2753–2771.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.departmentMIT Kavli Institute for Astrophysics and Space Researchen_US
dc.contributor.mitauthorTorrey, Paulen_US
dc.contributor.mitauthorVogelsberger, Marken_US
dc.relation.journalMonthly Notices of the Royal Astronomical Societyen_US
dc.eprint.versionAuthor's final manuscripten_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsTorrey, P.; Snyder, G. F.; Vogelsberger, M.; Hayward, C. C.; Genel, S.; Sijacki, D.; Springel, V.; Hernquist, L.; Nelson, D.; Kriek, M.; Pillepich, A.; Sales, L. V.; McBride, C. K.en_US
dc.identifier.orcidhttps://orcid.org/0000-0001-8593-7692
dc.identifier.orcidhttps://orcid.org/0000-0002-5653-0786
mit.licenseOPEN_ACCESS_POLICYen_US
mit.metadata.statusComplete


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