Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/27767
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | Clark, C. J. R. | en_US |
dc.contributor.author | Verstocken, S. | en_US |
dc.contributor.author | BIANCHI, SIMONE | en_US |
dc.contributor.author | Fritz, J. | en_US |
dc.contributor.author | Viaene, S. | en_US |
dc.contributor.author | Smith, M. W. L. | en_US |
dc.contributor.author | Baes, M. | en_US |
dc.contributor.author | CASASOLA, VIVIANA | en_US |
dc.contributor.author | CASSARA, LETIZIA PASQUA | en_US |
dc.contributor.author | Davies, J. I. | en_US |
dc.contributor.author | De Looze, I. | en_US |
dc.contributor.author | De Vis, P. | en_US |
dc.contributor.author | Evans, R. | en_US |
dc.contributor.author | Galametz, M. | en_US |
dc.contributor.author | Jones, A. P. | en_US |
dc.contributor.author | Lianou, S. | en_US |
dc.contributor.author | Madden, S. | en_US |
dc.contributor.author | Mosenkov, A. V. | en_US |
dc.contributor.author | Xilouris, M. | en_US |
dc.date.accessioned | 2020-10-13T14:20:02Z | - |
dc.date.available | 2020-10-13T14:20:02Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.issn | 0004-6361 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/27767 | - |
dc.description.abstract | Aims: The DustPedia project is capitalising on the legacy of the Herschel Space Observatory, using cutting-edge modelling techniques to study dust in the 875 DustPedia galaxies - representing the vast majority of extended galaxies within 3000 km s<SUP>-1</SUP> that were observed by Herschel. This work requires a database of multiwavelength imagery and photometry that greatly exceeds the scope (in terms of wavelength coverage and number of galaxies) of any previous local-Universe survey. Methods: We constructed a database containing our own custom Herschel reductions, along with standardised archival observations from GALEX, SDSS, DSS, 2MASS, WISE, Spitzer, and Planck. Using these data, we performed consistent aperture-matched photometry, which we combined with external supplementary photometry from IRAS and Planck. <BR /> Results: We present our multiwavelength imagery and photometry across 42 UV-microwave bands for the 875 DustPedia galaxies. Our aperture-matched photometry, combined with the external supplementary photometry, represents a total of 21 857 photometric measurements. A typical DustPedia galaxy has multiwavelength photometry spanning 25 bands. We also present the Comprehensive & Adaptable Aperture Photometry Routine (CAAPR), the pipeline we developed to carry out our aperture-matched photometry. CAAPR is designed to produce consistent photometry for the enormous range of galaxy and observation types in our data. In particular, CAAPR is able to determine robust cross-compatible uncertainties, thanks to a novel method for reliably extrapolating the aperture noise for observations that cover a very limited amount of background. Our rich database of imagery and photometry is being made available to the community. <P />Photometry data tables are only available at the CDS via anonymous ftp to <A href="http://cdsarc.u-strasbg.fr">http://cdsarc.u-strasbg.fr</A> (<A href="http://130.79.128.5">http://130.79.128.5</A>) or via <A href="http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/609/A37">http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/609/A37 | en_US |
dc.language.iso | eng | en_US |
dc.title | DustPedia: Multiwavelength photometry and imagery of 875 nearby galaxies in 42 ultraviolet-microwave bands | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1051/0004-6361/201731419 | en_US |
dc.identifier.scopus | 2-s2.0-85040307851 | en_US |
dc.identifier.url | https://www.aanda.org/articles/aa/full_html/2018/01/aa31419-17/aa31419-17.html | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 609 | en_US |
dc.relation.firstpage | A37 | en_US |
dc.type.referee | REF_1 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | ASTRONOMY & ASTROPHYSICS | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2018A&A...609A..37C | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Article | - |
item.languageiso639-1 | en | - |
item.fulltext | With Fulltext | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
crisitem.journal.journalissn | 0004-6361 | - |
crisitem.journal.ance | E016240 | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.orcid | 0000-0002-9384-846X | - |
crisitem.author.orcid | 0000-0002-3879-6038 | - |
crisitem.author.orcid | 0000-0001-5760-089X | - |
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