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000491566 005__ 20230214113614.0
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000491566 0247_ $$2arXiv$$aarXiv:2205.01116
000491566 0247_ $$2altmetric$$aaltmetric:127666433
000491566 037__ $$aPUBDB-2023-00258
000491566 041__ $$aEnglish
000491566 088__ $$2arXiv$$aarXiv:2205.01116
000491566 082__ $$a520
000491566 1001_ $$0P:(DE-HGF)0$$aRubin, David$$b0$$eCorresponding author
000491566 245__ $$aUniform Recalibration of Common Spectrophotometry Standard Stars onto the CALSPEC System Using the SuperNova Integral Field Spectrograph
000491566 260__ $$c2022
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000491566 500__ $$aISSN 1538-4365 not unique: **2 hits**.Accepted for publication in ApJS
000491566 520__ $$aWe calibrate spectrophotometric optical spectra of 32 stars commonly used as standard stars, referenced to 14 stars already on the Hubble Space Telescope–based CALSPEC flux system. Observations of CALSPEC and non-CALSPEC stars were obtained with the SuperNova Integral Field Spectrograph over the wavelength range 3300–9400 Å as calibration for the Nearby Supernova Factory cosmology experiment. In total, this analysis used 4289 standard-star spectra taken on photometric nights. As a modern cosmology analysis, all presubmission methodological decisions were made with the flux scale and external comparison results blinded. The large number of spectra per star allows us to treat the wavelength-by-wavelength calibration for all nights simultaneously with a Bayesian hierarchical model, thereby enabling a consistent treatment of the Type Ia supernova cosmology analysis and the calibration on which it critically relies. We determine the typical per-observation repeatability (median 14 mmag for exposures ≳5 s), the Maunakea atmospheric transmission distribution (median dispersion of 7 mmag with uncertainty 1 mmag), and the scatter internal to our CALSPEC reference stars (median of 8 mmag). We also check our standards against literature filter photometry, finding generally good agreement over the full 12 mag range. Overall, the mean of our system is calibrated to the mean of CALSPEC at the level of ∼3 mmag. With our large number of observations, careful cross-checks, and 14 reference stars, our results are the best calibration yet achieved with an integral-field spectrograph, and among the best calibrated surveys.
000491566 536__ $$0G:(DE-HGF)POF4-613$$a613 - Matter and Radiation from the Universe (POF4-613)$$cPOF4-613$$fPOF IV$$x0
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000491566 7001_ $$aAldering, G.$$b1
000491566 7001_ $$00000-0002-0389-5706$$aAntilogus, P.$$b2
000491566 7001_ $$00000-0002-9502-0965$$aAragon, C.$$b3
000491566 7001_ $$0S.Bailey.1$$aBailey, S.$$b4
000491566 7001_ $$00000-0003-0424-8719$$aBaltay, C.$$b5
000491566 7001_ $$0S.Bongard.1$$aBongard, S.$$b6
000491566 7001_ $$00000-0002-5828-6211$$aBoone, K.$$b7
000491566 7001_ $$00000-0002-3780-7516$$aButon, C.$$b8
000491566 7001_ $$00000-0002-5317-7518$$aCopin, Y.$$b9
000491566 7001_ $$00000-0003-1861-0870$$aDixon, S.$$b10
000491566 7001_ $$00000-0002-7496-3796$$aFouchez, D.$$b11
000491566 7001_ $$00000-0001-6728-1423$$aGangler, E.$$b12
000491566 7001_ $$aGupta, R.$$b13
000491566 7001_ $$00000-0001-9200-8699$$aHayden, B.$$b14
000491566 7001_ $$0W.Hillebrandt.1$$aHillebrandt, W.$$b15
000491566 7001_ $$aKim, A. G.$$b16
000491566 7001_ $$0P:(DE-H253)PIP1006050$$aKowalski, M.$$b17
000491566 7001_ $$0P:(DE-H253)PIP1032717$$aKuesters, Daniel$$b18
000491566 7001_ $$00000-0002-8357-3984$$aLeget, P.-F.$$b19
000491566 7001_ $$0F.Mondon.1$$aMondon, F.$$b20
000491566 7001_ $$aNordin, J.$$b21
000491566 7001_ $$00000-0003-4016-6067$$aPain, R.$$b22
000491566 7001_ $$0E.Pecontal.2$$aPecontal, E.$$b23
000491566 7001_ $$aPereira, R.$$b24
000491566 7001_ $$00000-0002-4436-4661$$aPerlmutter, S.$$b25
000491566 7001_ $$00000-0002-8207-3304$$aPonder, K. A.$$b26
000491566 7001_ $$00000-0003-4961-7653$$aRabinowitz, D.$$b27
000491566 7001_ $$aRigault, M.$$b28
000491566 7001_ $$aRunge, K.$$b29
000491566 7001_ $$00000-0002-4094-2102$$aSaunders, C.$$b30
000491566 7001_ $$00000-0002-9093-8849$$aSmadja, G.$$b31
000491566 7001_ $$aSuzuki, N.$$b32
000491566 7001_ $$aTao, C.$$b33
000491566 7001_ $$00000-0002-4265-1958$$aTaubenberger, S.$$b34
000491566 7001_ $$aThomas, R. C.$$b35
000491566 7001_ $$0M.Vincenzi.1$$aVincenzi, M.$$b36
000491566 7001_ $$0P:(DE-HGF)0$$aFactory, Nearby Supernova$$b37
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000491566 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1032717$$aExternal Institute$$b18$$kExtern
000491566 9131_ $$0G:(DE-HGF)POF4-613$$1G:(DE-HGF)POF4-610$$2G:(DE-HGF)POF4-600$$3G:(DE-HGF)POF4$$4G:(DE-HGF)POF$$aDE-HGF$$bForschungsbereich Materie$$lMatter and the Universe$$vMatter and Radiation from the Universe$$x0
000491566 9141_ $$y2022
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