Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/32049
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Otteson, Lillian | en_US |
dc.contributor.author | McCabe, Tyler | en_US |
dc.contributor.author | Ashcraft, Teresa A. | en_US |
dc.contributor.author | Windhorst, Rogier A. | en_US |
dc.contributor.author | Jansen, Rolf A. | en_US |
dc.contributor.author | Cohen, Seth H. | en_US |
dc.contributor.author | NONINO, Mario | en_US |
dc.contributor.author | PARIS, Diego | en_US |
dc.contributor.author | GRAZIAN, Andrea | en_US |
dc.contributor.author | FONTANA, Adriano | en_US |
dc.contributor.author | GIALLONGO, Emanuele | en_US |
dc.contributor.author | SPEZIALI, Roberto | en_US |
dc.contributor.author | TESTA, Vincenzo | en_US |
dc.contributor.author | Boutsia, Konstantina | en_US |
dc.contributor.author | Koekemoer, Anton | en_US |
dc.contributor.author | O’Connell, Robert W. | en_US |
dc.contributor.author | Rutkowski, Michael J. | en_US |
dc.contributor.author | Ryan, Russell E. | en_US |
dc.contributor.author | Scarlata, Claudia | en_US |
dc.contributor.author | Teplitz, Harry | en_US |
dc.date.accessioned | 2022-03-29T13:56:57Z | - |
dc.date.available | 2022-03-29T13:56:57Z | - |
dc.date.issued | 2021 | en_US |
dc.identifier.issn | 2515-5172 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/32049 | - |
dc.description.abstract | We present the optimal resolution and optimal depth U-filter mosaics using the seeing-sorted method of Ashcraft et al. on deep, ground-based U-bandimaging of the Great Observatories Origins Deep Survey South field as part of the near-UV imaging program UVCANDELS. We use the U-bandimages obtained with the VIsible Multi-Object Spectrograph on the European Southern Observatory Very Large Telescope by Nonino et al. Our best resolution mosaic includes images with a seeing full-width half maximum (FWHM) ≤ 0"8, and encompasses 50% of the data. Our best depth mosaic includes images with FWHM ≤ 1"5, corresponding to 100% of the data. Prior to being combined, the source fluxes in each individual background-subtracted image are corrected to match a 3D-HST photometric catalog of the same field to correct variations in the U-band zero-points. These mosaics provide deep U-banddata complementary to the UVCANDELS HST WFC3 F275W and ACS F435W images. We assess the depth of both U-bandmosaics. * Based on data acquired using the Very Large Telescope (VLT) of the European Southern Observatory (ESO). | en_US |
dc.language.iso | eng | en_US |
dc.title | Seeing-sorted Visible Multi-Object Spectrograph U-band Imaging of the GOODS-south Field* | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.3847/2515-5172/ac1db6 | en_US |
dc.identifier.url | https://iopscience.iop.org/article/10.3847/2515-5172/ac1db6 | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.volume | 5 | en_US |
dc.relation.issue | 8 | en_US |
dc.relation.firstpage | 190 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 20 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | USA | en_US |
dc.contributor.country | CHL | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | RESEARCH NOTES OF THE AAS | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2021RNAAS...5..190O | 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::PE9_8 Formation and evolution of galaxies | 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.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | O.A. Trieste | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.orcid | 0000-0001-6342-9662 | - |
crisitem.author.orcid | 0000-0002-7409-8114 | - |
crisitem.author.orcid | 0000-0002-5688-0663 | - |
crisitem.author.orcid | 0000-0003-3820-2823 | - |
crisitem.author.orcid | 0000-0003-0734-1273 | - |
crisitem.author.orcid | 0000-0003-3754-387X | - |
crisitem.author.orcid | 0000-0003-1033-1340 | - |
crisitem.journal.journalissn | 2515-5172 | - |
crisitem.journal.ance | E244721 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
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Seeing-sorted Visible Multi-Object Spectrograph U-band Imaging of the GOODS-south Field - IOPscience.pdf | Print of the HTML version | 367.16 kB | Adobe PDF | View/Open |
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