SDSS data management and photometric quality assessment

Ž Ivezić; R. H. Lupton; D. Schlegel; B. Boroski; J. Adelman-McCarthy; B. Yanny; S. Kent; C. Stoughton; D. Finkbeiner; N. Padmanabhan; C. M. Rockosi; J. E. Gunn; G. R. Knapp; M. A. Strauss; G. T. Richards; D. Eisenstein; T. Nicinski; S. J. Kleinman; J. Krzesinski; P. R. Newman; S. Snedden; A. R. Thakar; A. Szalay; J. A. Munn; J. A. Smith; D. Tucker; B. C. Lee

doi:10.1002/asna.200410285

SDSS data management and photometric quality assessment

Ž Ivezić
, R. H. Lupton
, D. Schlegel
, B. Boroski
, J. Adelman-McCarthy
, B. Yanny
, S. Kent
, C. Stoughton
, D. Finkbeiner
, N. Padmanabhan
, C. M. Rockosi
, J. E. Gunn
, G. R. Knapp
, M. A. Strauss
, G. T. Richards
, D. Eisenstein
, T. Nicinski
, S. J. Kleinman
, J. Krzesinski
, P. R. Newman

S. Snedden, A. R. Thakar, A. Szalay, J. A. Munn, J. A. Smith, D. Tucker, B. C. Lee

Research output: Contribution to journal › Article › peer-review

428 Scopus citations

Abstract

We summarize the Sloan Digital Sky Survey data acquisition and processing steps, and describe runQA, a pipeline designed for automated data quality assessment. In particular, we show how the position of the stellar locus in color-color diagrams can be used to estimate the accuracy of photometric zeropoint calibration to better than 0.01 mag in 0.03 deg ² patches. Using this method, we estimate that typical photometric zeropoint calibration errors for SDSS imaging data are not larger than ∼ 0.01 mag in the g, r, and i bands, 0.02 mag in the z band, and 0.03 mag in the u band (root-mean-scatter for zeropoint offsets).

Original language	English (US)
Pages (from-to)	583-589
Number of pages	7
Journal	Astronomische Nachrichten
Volume	325
Issue number	6-8
DOIs	https://doi.org/10.1002/asna.200410285
State	Published - 2004

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

Keywords

Methods: data analysis
Stars: fundamental parameters
Stars: statistics
Surveys
Techniques: photometric

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10.1002/asna.200410285

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Ivezić, Ž., Lupton, R. H., Schlegel, D., Boroski, B., Adelman-McCarthy, J., Yanny, B., Kent, S., Stoughton, C., Finkbeiner, D., Padmanabhan, N., Rockosi, C. M., Gunn, J. E., Knapp, G. R., Strauss, M. A., Richards, G. T., Eisenstein, D., Nicinski, T., Kleinman, S. J., Krzesinski, J., ... Lee, B. C. (2004). SDSS data management and photometric quality assessment. Astronomische Nachrichten, 325(6-8), 583-589. https://doi.org/10.1002/asna.200410285

@article{77a658b1350f4ba4b5f16dd69958b136,

title = "SDSS data management and photometric quality assessment",

abstract = "We summarize the Sloan Digital Sky Survey data acquisition and processing steps, and describe runQA, a pipeline designed for automated data quality assessment. In particular, we show how the position of the stellar locus in color-color diagrams can be used to estimate the accuracy of photometric zeropoint calibration to better than 0.01 mag in 0.03 deg 2 patches. Using this method, we estimate that typical photometric zeropoint calibration errors for SDSS imaging data are not larger than ∼ 0.01 mag in the g, r, and i bands, 0.02 mag in the z band, and 0.03 mag in the u band (root-mean-scatter for zeropoint offsets).",

keywords = "Methods: data analysis, Stars: fundamental parameters, Stars: statistics, Surveys, Techniques: photometric",

author = "{\v Z} Ivezi{\'c} and Lupton, \{R. H.\} and D. Schlegel and B. Boroski and J. Adelman-McCarthy and B. Yanny and S. Kent and C. Stoughton and D. Finkbeiner and N. Padmanabhan and Rockosi, \{C. M.\} and Gunn, \{J. E.\} and Knapp, \{G. R.\} and Strauss, \{M. A.\} and Richards, \{G. T.\} and D. Eisenstein and T. Nicinski and Kleinman, \{S. J.\} and J. Krzesinski and Newman, \{P. R.\} and S. Snedden and Thakar, \{A. R.\} and A. Szalay and Munn, \{J. A.\} and Smith, \{J. A.\} and D. Tucker and Lee, \{B. C.\}",

year = "2004",

doi = "10.1002/asna.200410285",

language = "English (US)",

volume = "325",

pages = "583--589",

journal = "Astronomische Nachrichten",

issn = "0004-6337",

publisher = "Wiley-VCH Verlag",

number = "6-8",

}

Ivezić, Ž, Lupton, RH, Schlegel, D, Boroski, B, Adelman-McCarthy, J, Yanny, B, Kent, S, Stoughton, C, Finkbeiner, D, Padmanabhan, N, Rockosi, CM, Gunn, JE, Knapp, GR, Strauss, MA, Richards, GT, Eisenstein, D, Nicinski, T, Kleinman, SJ, Krzesinski, J, Newman, PR, Snedden, S, Thakar, AR, Szalay, A, Munn, JA, Smith, JA, Tucker, D & Lee, BC 2004, 'SDSS data management and photometric quality assessment', Astronomische Nachrichten, vol. 325, no. 6-8, pp. 583-589. https://doi.org/10.1002/asna.200410285

TY - JOUR

T1 - SDSS data management and photometric quality assessment

AU - Ivezić, Ž

AU - Lupton, R. H.

AU - Schlegel, D.

AU - Boroski, B.

AU - Adelman-McCarthy, J.

AU - Yanny, B.

AU - Kent, S.

AU - Stoughton, C.

AU - Finkbeiner, D.

AU - Padmanabhan, N.

AU - Rockosi, C. M.

AU - Gunn, J. E.

AU - Knapp, G. R.

AU - Strauss, M. A.

AU - Richards, G. T.

AU - Eisenstein, D.

AU - Nicinski, T.

AU - Kleinman, S. J.

AU - Krzesinski, J.

AU - Newman, P. R.

AU - Snedden, S.

AU - Thakar, A. R.

AU - Szalay, A.

AU - Munn, J. A.

AU - Smith, J. A.

AU - Tucker, D.

AU - Lee, B. C.

PY - 2004

Y1 - 2004

N2 - We summarize the Sloan Digital Sky Survey data acquisition and processing steps, and describe runQA, a pipeline designed for automated data quality assessment. In particular, we show how the position of the stellar locus in color-color diagrams can be used to estimate the accuracy of photometric zeropoint calibration to better than 0.01 mag in 0.03 deg 2 patches. Using this method, we estimate that typical photometric zeropoint calibration errors for SDSS imaging data are not larger than ∼ 0.01 mag in the g, r, and i bands, 0.02 mag in the z band, and 0.03 mag in the u band (root-mean-scatter for zeropoint offsets).

AB - We summarize the Sloan Digital Sky Survey data acquisition and processing steps, and describe runQA, a pipeline designed for automated data quality assessment. In particular, we show how the position of the stellar locus in color-color diagrams can be used to estimate the accuracy of photometric zeropoint calibration to better than 0.01 mag in 0.03 deg 2 patches. Using this method, we estimate that typical photometric zeropoint calibration errors for SDSS imaging data are not larger than ∼ 0.01 mag in the g, r, and i bands, 0.02 mag in the z band, and 0.03 mag in the u band (root-mean-scatter for zeropoint offsets).

KW - Methods: data analysis

KW - Stars: fundamental parameters

KW - Stars: statistics

KW - Surveys

KW - Techniques: photometric

UR - https://www.scopus.com/pages/publications/9944245412

UR - https://www.scopus.com/pages/publications/9944245412#tab=citedBy

U2 - 10.1002/asna.200410285

DO - 10.1002/asna.200410285

M3 - Article

AN - SCOPUS:9944245412

SN - 0004-6337

VL - 325

SP - 583

EP - 589

JO - Astronomische Nachrichten

JF - Astronomische Nachrichten

IS - 6-8

ER -

SDSS data management and photometric quality assessment

Abstract

All Science Journal Classification (ASJC) codes

Keywords

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