Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/25928
DC Field | Value | Language |
---|---|---|
dc.contributor.author | RIPEPI, Vincenzo | en_US |
dc.contributor.author | Cignoni, M. | en_US |
dc.contributor.author | TOSI, Monica | en_US |
dc.contributor.author | MARCONI, Marcella | en_US |
dc.contributor.author | MUSELLA, ILARIA | en_US |
dc.contributor.author | Coppola, G. | en_US |
dc.contributor.author | GRADO, ANIELLO | en_US |
dc.contributor.author | Limatola, L. | en_US |
dc.contributor.author | CLEMENTINI, Gisella | en_US |
dc.contributor.author | BROCATO, Enzo | en_US |
dc.contributor.author | CANTIELLO, Michele | en_US |
dc.contributor.author | Capaccioli, M. | en_US |
dc.contributor.author | CAPPELLARO, Enrico | en_US |
dc.contributor.author | Cioni, M. -R. L. | en_US |
dc.contributor.author | CUSANO, FELICE | en_US |
dc.contributor.author | DALL'ORA, Massimo | en_US |
dc.contributor.author | Gallagher, J. S. | en_US |
dc.contributor.author | Grebel, E. K. | en_US |
dc.contributor.author | Nota, A. | en_US |
dc.contributor.author | Palla, F. | en_US |
dc.contributor.author | ROMANO, Donatella | en_US |
dc.contributor.author | RAIMONDO, Gabriella | en_US |
dc.contributor.author | Sabbi, E. | en_US |
dc.contributor.author | GETMAN, FEDOR | en_US |
dc.contributor.author | NAPOLITANO, NICOLA ROSARIO | en_US |
dc.contributor.author | SCHIPANI, Pietro | en_US |
dc.contributor.author | ZAGGIA, Simone | en_US |
dc.date.accessioned | 2020-06-05T09:44:35Z | - |
dc.date.available | 2020-06-05T09:44:35Z | - |
dc.date.issued | 2016 | en_US |
dc.identifier.isbn | 978-3-319-19329-8 | en_US |
dc.identifier.issn | 1570-6591 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/25928 | - |
dc.description.abstract | STEP (Small Magellanic Cloud in Time: Evolution of a Prototype interacting late-type dwarf galaxy) is a Guaranteed Time Observation survey being carried out at the VLT Survey Telescope. STEP will obtain homogeneous photometry in the g-, r-, i- and Hα-bands over an area of 74 deg<SUP>2</SUP> covering the main body of the Small Magellanic Cloud, the Bridge that connects it to the Large Magellanic Cloud and a small part of the Magellanic Stream (2 deg<SUP>2</SUP>). Our photometry will allow us to detect and measure the magnitudes of individual stars well below the main sequence turnoff of the oldest populations. Here we briefly describe the observing strategy, the photometric techniques, and the upcoming data products of the STEP survey. | en_US |
dc.language.iso | eng | en_US |
dc.title | The VST Survey of the SMC and the Magellanic Bridge (STEP): First Results | en_US |
dc.type | Conference paper | - |
dc.identifier.doi | 10.1007/978-3-319-19330-4_23 | en_US |
dc.identifier.scopus | 2-s2.0-84978942605 | en_US |
dc.identifier.isi | 000389802600024 | en_US |
dc.identifier.url | https://link.springer.com/chapter/10.1007%2F978-3-319-19330-4_23 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 42 | en_US |
dc.relation.firstpage | 145 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.relation.ispartofbook | The Universe of Digital Sky Surveys: a Meeting to Honour the 70th Birthday of Massimo Capaccioli | en_US |
dc.relation.conferencename | The Universe of Digital Sky Surveys: a Meeting to Honour the 70th Birthday of Massimo Capaccioli | en_US |
dc.relation.conferenceplace | Napoli, Italy | en_US |
dc.relation.conferencedate | 25-28 November, 2014 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.type.miur | 273 Contributo in Atti di convegno | - |
dc.relation.series | ASTROPHYSICS AND SPACE SCIENCE PROCEEDINGS | en_US |
dc.identifier.adsbibcode | 2016ASSP...42..145R | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering | 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 | Conference paper | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | reserved | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | O.A. Capodimonte | - |
crisitem.author.dept | O.A. Capodimonte | - |
crisitem.author.dept | O.A. Capodimonte | - |
crisitem.author.dept | O.A. Capodimonte | - |
crisitem.author.dept | O.A. Abruzzo | - |
crisitem.author.dept | O.A. Abruzzo | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | O.A. Capodimonte | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | O.A. Abruzzo | - |
crisitem.author.dept | O.A. Capodimonte | - |
crisitem.author.dept | O.A. Capodimonte | - |
crisitem.author.dept | O.A. Capodimonte | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.orcid | 0000-0003-1801-426X | - |
crisitem.author.orcid | 0000-0002-0986-4759 | - |
crisitem.author.orcid | 0000-0002-1330-2927 | - |
crisitem.author.orcid | 0000-0001-5909-6615 | - |
crisitem.author.orcid | 0000-0002-0501-8256 | - |
crisitem.author.orcid | 0000-0001-9206-9723 | - |
crisitem.author.orcid | 0000-0001-7988-8177 | - |
crisitem.author.orcid | 0000-0003-2072-384X | - |
crisitem.author.orcid | 0000-0001-5008-8619 | - |
crisitem.author.orcid | 0000-0003-2910-6565 | - |
crisitem.author.orcid | 0000-0001-8209-0449 | - |
crisitem.author.orcid | 0000-0002-0845-6171 | - |
crisitem.author.orcid | 0000-0002-5577-7023 | - |
crisitem.author.orcid | 0000-0003-1550-0182 | - |
crisitem.author.orcid | 0000-0003-0911-8884 | - |
crisitem.author.orcid | 0000-0003-0197-589X | - |
crisitem.author.orcid | 0000-0001-6081-379X | - |
crisitem.journal.journalissn | 1570-6591 | - |
crisitem.journal.ance | E210911 | - |
Appears in Collections: | 3.01 Contributi in Atti di convegno |
Files in This Item:
File | Description | Size | Format | Existing users please |
---|---|---|---|---|
Ripepi2016_Chapter_TheVSTSurveyOfTheSMCAndTheMage.pdf | [Administrators only] | 263.33 kB | Adobe PDF |
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