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@ARTICLE{Rubin:491566,
      author       = {Rubin, David and Aldering, G. and Antilogus, P. and Aragon,
                      C. and Bailey, S. and Baltay, C. and Bongard, S. and Boone,
                      K. and Buton, C. and Copin, Y. and Dixon, S. and Fouchez, D.
                      and Gangler, E. and Gupta, R. and Hayden, B. and
                      Hillebrandt, W. and Kim, A. G. and Kowalski, M. and
                      Kuesters, Daniel and Leget, P.-F. and Mondon, F. and Nordin,
                      J. and Pain, R. and Pecontal, E. and Pereira, R. and
                      Perlmutter, S. and Ponder, K. A. and Rabinowitz, D. and
                      Rigault, M. and Runge, K. and Saunders, C. and Smadja, G.
                      and Suzuki, N. and Tao, C. and Taubenberger, S. and Thomas,
                      R. C. and Vincenzi, M. and Factory, Nearby Supernova},
      title        = {{U}niform {R}ecalibration of {C}ommon {S}pectrophotometry
                      {S}tandard {S}tars onto the {CALSPEC} {S}ystem {U}sing the
                      {S}uper{N}ova {I}ntegral {F}ield {S}pectrograph},
      reportid     = {PUBDB-2023-00258, arXiv:2205.01116},
      year         = {2022},
      note         = {ISSN 1538-4365 not unique: **2 hits**.Accepted for
                      publication in ApJS},
      abstract     = {We 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.},
      cin          = {ZEU-EXP/AT / ZEU-ICE},
      ddc          = {520},
      cid          = {$I:(DE-H253)ZEU-EXP_AT-20120731$ /
                      I:(DE-H253)ZEU-ICE-20160806},
      pnm          = {613 - Matter and Radiation from the Universe (POF4-613)},
      pid          = {G:(DE-HGF)POF4-613},
      experiment   = {EXP:(DE-MLZ)NOSPEC-20140101},
      typ          = {PUB:(DE-HGF)25},
      eprint       = {2205.01116},
      howpublished = {arXiv:2205.01116},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:2205.01116;\%\%$},
      url          = {https://bib-pubdb1.desy.de/record/491566},
}