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Atmospheric extinction properties above Mauna Kea from the Nearby SuperNova Factory spectro-photometric data set

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dc.contributor.authorButon, C
dc.contributor.authorCopin, Y
dc.contributor.authorAldering, G
dc.contributor.authorAntilogus, Pierre
dc.contributor.authorAragon, C
dc.contributor.authorBailey, S
dc.contributor.authorBaltay, C
dc.contributor.authorBongard, S
dc.contributor.authorCanto, A
dc.contributor.authorCellier-Holzem, F
dc.contributor.authorChildress, M
dc.contributor.authorChotard, N
dc.contributor.authorFakhouri, H K
dc.contributor.authorGangler, E
dc.contributor.authorGuy, J
dc.contributor.authorScalzo, Richard
dc.date.accessioned2015-12-10T23:35:06Z
dc.date.issued2013
dc.date.updated2016-02-24T08:54:08Z
dc.description.abstractWe present a new atmospheric extinction curve for Mauna Kea spanning 3200-9700. It is the most comprehensive to date, being based on some 4285Â standard star spectra obtained on 478Â nights spread over a period of 7 years obtained by the Nearby SuperNov
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/1885/69708
dc.publisherSpringer
dc.sourceAstronomy and Astrophysics
dc.subjectKeywords: Atmospheric effects; Atmospheric extinction; Atmospheric science; Calibration uncertainty; Data sets; Extinction curves; Imaging data; Instrumentation: spectrographs; Integral field spectrograph; Mauna Loa; Methods:observational; Physical components; Tech Atmospheric effects; Instrumentation: spectrographs; Methods: observational; Techniques: imaging spectroscopy
dc.titleAtmospheric extinction properties above Mauna Kea from the Nearby SuperNova Factory spectro-photometric data set
dc.typeJournal article
local.bibliographicCitation.lastpage21
local.bibliographicCitation.startpageA8 1
local.contributor.affiliationButon, C, Universität Bonn
local.contributor.affiliationCopin, Y, Université de Lyon
local.contributor.affiliationAldering, G, Lawrence Berkeley National Laboratory
local.contributor.affiliationAntilogus, Pierre, Laboratoire de Physique Nucleaire des Hautes Energies
local.contributor.affiliationAragon, C, Lawrence Berkeley National Laboratory
local.contributor.affiliationBailey, S, Lawrence Berkeley National Laboratory
local.contributor.affiliationBaltay, C, Yale University
local.contributor.affiliationBongard, S, Université Pierre et Marie Curie Paris 6
local.contributor.affiliationCanto, A, Université Pierre et Marie Curie Paris 6,
local.contributor.affiliationCellier-Holzem, F, Universite Pierre et Marie Curie Paris
local.contributor.affiliationChildress, M, Lawrence Berkeley National Laboratory
local.contributor.affiliationChotard, N, Tsinghua University
local.contributor.affiliationFakhouri, H K, University of California
local.contributor.affiliationGangler, E, Université de Lyon
local.contributor.affiliationGuy, J, Universite Pierre et Marie Curie Paris 6
local.contributor.affiliationScalzo, Richard, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidScalzo, Richard, u4956999
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.ariespublicationf5625xPUB2099
local.identifier.ariespublicationu4630950xPUB165
local.identifier.citationvolume549
local.identifier.doi10.1051/0004-6361/201219834
local.identifier.scopusID2-s2.0-84870834063
local.identifier.thomsonID000313745000008
local.type.statusPublished Version

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