Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/26283
DC Field | Value | Language |
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dc.contributor.author | Treu, T. | en_US |
dc.contributor.author | Brammer, G. | en_US |
dc.contributor.author | Diego, J. M. | en_US |
dc.contributor.author | Grillo, C. | en_US |
dc.contributor.author | Kelly, P. L. | en_US |
dc.contributor.author | Oguri, M. | en_US |
dc.contributor.author | Rodney, S. A. | en_US |
dc.contributor.author | Rosati, P. | en_US |
dc.contributor.author | Sharon, K. | en_US |
dc.contributor.author | Zitrin, A. | en_US |
dc.contributor.author | Balestra, I. | en_US |
dc.contributor.author | Bradac, M. | en_US |
dc.contributor.author | Broadhurst, T. | en_US |
dc.contributor.author | Caminha, G. B. | en_US |
dc.contributor.author | Halkola, A. | en_US |
dc.contributor.author | Hoag, A. | en_US |
dc.contributor.author | Ishigaki, M. | en_US |
dc.contributor.author | Johnson, T. L. | en_US |
dc.contributor.author | Karman, W. | en_US |
dc.contributor.author | Kawamata, R. | en_US |
dc.contributor.author | MERCURIO, AMATA | en_US |
dc.contributor.author | Schmidt, K. B. | en_US |
dc.contributor.author | Strolger, L. -G. | en_US |
dc.contributor.author | Suyu, S. H. | en_US |
dc.contributor.author | Filippenko, A. V. | en_US |
dc.contributor.author | Foley, R. J. | en_US |
dc.contributor.author | Jha, S. W. | en_US |
dc.contributor.author | Patel, B. | en_US |
dc.date.accessioned | 2020-07-02T07:38:52Z | - |
dc.date.available | 2020-07-02T07:38:52Z | - |
dc.date.issued | 2016 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/26283 | - |
dc.description.abstract | Since the discovery of SN Refsdal on 2014 November 11, the MACSJ1149.5+2223 field has been observed in great detail, with HST imaging in optical and infrared bands, and deep spectroscopy from HST, Keck, and the VLT. <P />The HST grism spectroscopy comprises two data sets. The GLASS data consist of 10 orbits of exposures taken through the G102 grism and 4 orbits of exposures taken through the G141 grism, spanning the wavelength range 0.81-1.69um. The GLASS data were taken at two approximately orthogonal position angles (PAs) to mitigate contamination by nearby sources (the first one on 2014 February 23-25, the second PA on 2014 November 3-11). The SN Refsdal follow-up spectra were taken between 2014 December 23 and 2015 January 4. For more details the reader is referred to Schmidt et al. (2014ApJ...782L..36S) and Treu et al. (2015, J/ApJ/812/114) for GLASS, and G. B. Brammer et al. (2015, in preparation) and P. L. Kelly et al. (2015, in preparation) for the deeper follow-up data. <P />Integral-field spectroscopy was obtained with the MUSE instrument on the VLT between 2015 February 14 and 2015 April 12, as part of a Director Discretionary Time program to observe SN Refsdal (PI Grillo). Details of the data acquisition and processing are given in a separate paper (Grillo et al. 2015, arXiv:1511.04093). Spectroscopy of the field was obtained using the DEIMOS spectrograph on the 10m Keck II telescope on 2014 December 20. (3 data files). | en_US |
dc.language.iso | eng | en_US |
dc.title | VizieR Online Data Catalog: Multiply imaged supernova Refsdal (Treu+, 2016) | en_US |
dc.type | Database | - |
dc.identifier.doi | 10.26093/cds/vizier.18170060 | en_US |
dc.identifier.url | http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/ApJ/817/60 | en_US |
dc.relation.firstpage | J/ApJ/817/60 | en |
dc.description.numberofauthors | 28 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | USA | en_US |
dc.contributor.country | DEU | en_US |
dc.contributor.country | DNK | en_US |
dc.contributor.country | NLD | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | VizieR Online Data Catalog | en |
dc.type.miur | 295 Banca dati | - |
dc.identifier.adsbibcode | 2016yCat..18170060T | 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.oa | 3 - prodotto già presente in altro archivio Open Access, es. VizieR (allegare file read.me al passo 5-Carica) | en_US |
item.grantfulltext | open | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.languageiso639-1 | en | - |
item.openairetype | Database | - |
item.cerifentitytype | Publications | - |
crisitem.author.dept | O.A. Capodimonte | - |
crisitem.author.orcid | 0000-0001-9261-7849 | - |
Appears in Collections: | 4.06 Banche Dati |
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File | Description | Size | Format | |
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J_ApJ_817_60.pdf | ReadMe | 145 kB | Adobe PDF | View/Open |
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