The Pan-STARRS1 Surveys

K. C. Chambers; E. A. Magnier; N. Metcalfe; H. A. Flewelling; M. E. Huber; C. Z. Waters; L. Denneau; P. W. Draper; D. Farrow; D. P. Finkbeiner; C. Holmberg; J. Koppenhoefer; P. A. Price; R. P. Saglia; E. F. Schlafly; S. J. Smartt; W. Sweeney; R. J. Wainscoat; W. S. Burgett; T. Grav; J. N. Heasley; K. W. Hodapp; R. Jedicke; N. Kaiser; R.-P. Kudritzki; G. A. Luppino; R. H. Lupton; D. G. Monet; J. S. Morgan; P. M. Onaka; C. W. Stubbs; J. L. Tonry; E. Banados; E. F. Bell; R. Bender; E. J. Bernard; M. T. Botticella; S. Casertano; S. Chastel; W.-P. Chen; X. Chen; S. Cole; N. Deacon; C. Frenk; A. Fitzsimmons; S. Gezari; C. Goessl; T. Goggia; B. Goldman; E. K. Grebel; N. C. Hambly; G. Hasinger; A. F. Heavens; T. M. Heckman; R. Henderson; T. Henning; M. Holman; U. Hopp; W.-H. Ip; S. Isani; C. D. Keyes; A. Koekemoer; R. Kotak; K. S. Long; J. R Lucey; M. Liu; N. F. Martin; B. McLean; E. Morganson; D. N. A. Murphy; M. A. Nieto-Santisteban; P. Norberg; J. A. Peacock; E. A. Pier; M. Postman; N. Primak; C. Rae; A. Rest; A. Riess; A. Riffeser; H. W. Rix; S. Roser; E. Schilbach; A. S. B. Schultz; D. Scolnic; A. Szalay; S. Seitz; B. Shiao; E. Small; K. W. Smith; D. Soderblom; A. N. Taylor; A. R. Thakar; J. Thiel; D. Thilker; Y. Urata; J. Valenti; F. Walter; S. P. Watters; S. Werner; R. White; W. M. Wood-Vasey; R. Wyse

The Pan-STARRS1 Surveys

K. C. Chambers, E. A. Magnier, N. Metcalfe, H. A. Flewelling, M. E. Huber, C. Z. Waters, L. Denneau, P. W. Draper, D. Farrow, D. P. Finkbeiner, C. Holmberg, J. Koppenhoefer, P. A. Price, R. P. Saglia, E. F. Schlafly, S. J. Smartt, W. Sweeney, R. J. Wainscoat, W. S. Burgett, T. GravJ. N. Heasley, K. W. Hodapp, R. Jedicke, N. Kaiser, R.-P. Kudritzki, G. A. Luppino, R. H. Lupton, D. G. Monet, J. S. Morgan, P. M. Onaka, C. W. Stubbs, J. L. Tonry, E. Banados, E. F. Bell, R. Bender, E. J. Bernard, M. T. Botticella, S. Casertano, S. Chastel, W.-P. Chen, X. Chen, S. Cole, N. Deacon, C. Frenk, A. Fitzsimmons, S. Gezari, C. Goessl, T. Goggia, B. Goldman, E. K. Grebel, N. C. Hambly, G. Hasinger, A. F. Heavens, T. M. Heckman, R. Henderson, T. Henning, M. Holman, U. Hopp, W.-H. Ip, S. Isani, C. D. Keyes, A. Koekemoer, R. Kotak, K. S. Long, J. R Lucey, M. Liu, N. F. Martin, B. McLean, E. Morganson, D. N. A. Murphy, M. A. Nieto-Santisteban, P. Norberg, J. A. Peacock, E. A. Pier, M. Postman, N. Primak, C. Rae, A. Rest, A. Riess, A. Riffeser, H. W. Rix, S. Roser, E. Schilbach, A. S. B. Schultz, D. Scolnic, A. Szalay, S. Seitz, B. Shiao, E. Small, K. W. Smith, D. Soderblom, A. N. Taylor, A. R. Thakar, J. Thiel, D. Thilker, Y. Urata, J. Valenti, F. Walter, S. P. Watters, S. Werner, R. White, W. M. Wood-Vasey, R. Wyse

Research output: Contribution to journal › Article

Abstract

Pan-STARRS1 has carried out a set of distinct synoptic imaging sky surveys including the $3\pi$ Steradian Survey and the Medium Deep Survey in 5 bands (\grizy). The mean 5$\sigma$ point source limiting sensitivities in the stacked 3$\pi$ Steradian Survey in \grizy are (23.3, 23.2, 23.1, 22.3, 21.4) respectively. The upper bound on the systematic uncertainty in the photometric calibration across the sky is 7-12 millimag depending on the bandpass. The systematic uncertainty of the astrometric calibration using the Gaia frame comes from a comparison of the results with Gaia: the standard deviation of the mean and median residuals ($ \Delta ra, \Delta dec $ ) are (2.3, 1.7) milliarcsec, and (3.1, 4.8) milliarcsec respectively. The Pan-STARRS system and the design of the PS1 surveys is described and an overview of the resulting image and catalog data products and their basic characteristics are described together with a summary of important results. The images, reduced data products, and derived data products from the Pan-STARRS1 surveys are available to the community from the Mikulski Archive for Space Telescopes (MAST) at STScI.

Original language	English
Journal	arXiv
Publication status	Unpublished - 01 Dec 2016

Keywords

Astrophysics - Instrumentation and Methods for Astrophysics
Astrophysics - Earth and Planetary Astrophysics
Astrophysics - Astrophysics of Galaxies
Astrophysics - Solar and Stellar Astrophysics

Access to Document

http://adsabs.harvard.edu/abs/2016arXiv161205560C

Cite this

Chambers, K. C., Magnier, E. A., Metcalfe, N., Flewelling, H. A., Huber, M. E., Waters, C. Z., Denneau, L., Draper, P. W., Farrow, D., Finkbeiner, D. P., Holmberg, C., Koppenhoefer, J., Price, P. A., Saglia, R. P., Schlafly, E. F., Smartt, S. J., Sweeney, W., Wainscoat, R. J., Burgett, W. S., ... Wyse, R. (2016). The Pan-STARRS1 Surveys. Unpublished. http://adsabs.harvard.edu/abs/2016arXiv161205560C

@article{7ce3409d0bc441a1955feecbafe05c11,

title = "The Pan-STARRS1 Surveys",

abstract = "Pan-STARRS1 has carried out a set of distinct synoptic imaging sky surveys including the $3\pi$ Steradian Survey and the Medium Deep Survey in 5 bands (\grizy). The mean 5$\sigma$ point source limiting sensitivities in the stacked 3$\pi$ Steradian Survey in \grizy are (23.3, 23.2, 23.1, 22.3, 21.4) respectively. The upper bound on the systematic uncertainty in the photometric calibration across the sky is 7-12 millimag depending on the bandpass. The systematic uncertainty of the astrometric calibration using the Gaia frame comes from a comparison of the results with Gaia: the standard deviation of the mean and median residuals ($ \Delta ra, \Delta dec $ ) are (2.3, 1.7) milliarcsec, and (3.1, 4.8) milliarcsec respectively. The Pan-STARRS system and the design of the PS1 surveys is described and an overview of the resulting image and catalog data products and their basic characteristics are described together with a summary of important results. The images, reduced data products, and derived data products from the Pan-STARRS1 surveys are available to the community from the Mikulski Archive for Space Telescopes (MAST) at STScI.",

keywords = "Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics",

author = "Chambers, {K. C.} and Magnier, {E. A.} and N. Metcalfe and Flewelling, {H. A.} and Huber, {M. E.} and Waters, {C. Z.} and L. Denneau and Draper, {P. W.} and D. Farrow and Finkbeiner, {D. P.} and C. Holmberg and J. Koppenhoefer and Price, {P. A.} and Saglia, {R. P.} and Schlafly, {E. F.} and Smartt, {S. J.} and W. Sweeney and Wainscoat, {R. J.} and Burgett, {W. S.} and T. Grav and Heasley, {J. N.} and Hodapp, {K. W.} and R. Jedicke and N. Kaiser and R.-P. Kudritzki and Luppino, {G. A.} and Lupton, {R. H.} and Monet, {D. G.} and Morgan, {J. S.} and Onaka, {P. M.} and Stubbs, {C. W.} and Tonry, {J. L.} and E. Banados and Bell, {E. F.} and R. Bender and Bernard, {E. J.} and Botticella, {M. T.} and S. Casertano and S. Chastel and W.-P. Chen and X. Chen and S. Cole and N. Deacon and C. Frenk and A. Fitzsimmons and S. Gezari and C. Goessl and T. Goggia and B. Goldman and Grebel, {E. K.} and Hambly, {N. C.} and G. Hasinger and Heavens, {A. F.} and Heckman, {T. M.} and R. Henderson and T. Henning and M. Holman and U. Hopp and W.-H. Ip and S. Isani and Keyes, {C. D.} and A. Koekemoer and R. Kotak and Long, {K. S.} and Lucey, {J. R} and M. Liu and Martin, {N. F.} and B. McLean and E. Morganson and Murphy, {D. N. A.} and Nieto-Santisteban, {M. A.} and P. Norberg and Peacock, {J. A.} and Pier, {E. A.} and M. Postman and N. Primak and C. Rae and A. Rest and A. Riess and A. Riffeser and Rix, {H. W.} and S. Roser and E. Schilbach and Schultz, {A. S. B.} and D. Scolnic and A. Szalay and S. Seitz and B. Shiao and E. Small and Smith, {K. W.} and D. Soderblom and Taylor, {A. N.} and Thakar, {A. R.} and J. Thiel and D. Thilker and Y. Urata and J. Valenti and F. Walter and Watters, {S. P.} and S. Werner and R. White and Wood-Vasey, {W. M.} and R. Wyse",

year = "2016",

month = dec,

day = "1",

language = "English",

journal = "arXiv",

}

Chambers, KC, Magnier, EA, Metcalfe, N, Flewelling, HA, Huber, ME, Waters, CZ, Denneau, L, Draper, PW, Farrow, D, Finkbeiner, DP, Holmberg, C, Koppenhoefer, J, Price, PA, Saglia, RP, Schlafly, EF, Smartt, SJ, Sweeney, W, Wainscoat, RJ, Burgett, WS, Grav, T, Heasley, JN, Hodapp, KW, Jedicke, R, Kaiser, N, Kudritzki, R-P, Luppino, GA, Lupton, RH, Monet, DG, Morgan, JS, Onaka, PM, Stubbs, CW, Tonry, JL, Banados, E, Bell, EF, Bender, R, Bernard, EJ, Botticella, MT, Casertano, S, Chastel, S, Chen, W-P, Chen, X, Cole, S, Deacon, N, Frenk, C, Fitzsimmons, A, Gezari, S, Goessl, C, Goggia, T, Goldman, B, Grebel, EK, Hambly, NC, Hasinger, G, Heavens, AF, Heckman, TM, Henderson, R, Henning, T, Holman, M, Hopp, U, Ip, W-H, Isani, S, Keyes, CD, Koekemoer, A, Kotak, R, Long, KS, Lucey, JR, Liu, M, Martin, NF, McLean, B, Morganson, E, Murphy, DNA, Nieto-Santisteban, MA, Norberg, P, Peacock, JA, Pier, EA, Postman, M, Primak, N, Rae, C, Rest, A, Riess, A, Riffeser, A, Rix, HW, Roser, S, Schilbach, E, Schultz, ASB, Scolnic, D, Szalay, A, Seitz, S, Shiao, B, Small, E, Smith, KW, Soderblom, D, Taylor, AN, Thakar, AR, Thiel, J, Thilker, D, Urata, Y, Valenti, J, Walter, F, Watters, SP, Werner, S, White, R, Wood-Vasey, WM & Wyse, R 2016, 'The Pan-STARRS1 Surveys', arXiv. <http://adsabs.harvard.edu/abs/2016arXiv161205560C>

TY - JOUR

T1 - The Pan-STARRS1 Surveys

AU - Chambers, K. C.

AU - Magnier, E. A.

AU - Metcalfe, N.

AU - Flewelling, H. A.

AU - Huber, M. E.

AU - Waters, C. Z.

AU - Denneau, L.

AU - Draper, P. W.

AU - Farrow, D.

AU - Finkbeiner, D. P.

AU - Holmberg, C.

AU - Koppenhoefer, J.

AU - Price, P. A.

AU - Saglia, R. P.

AU - Schlafly, E. F.

AU - Smartt, S. J.

AU - Sweeney, W.

AU - Wainscoat, R. J.

AU - Burgett, W. S.

AU - Grav, T.

AU - Heasley, J. N.

AU - Hodapp, K. W.

AU - Jedicke, R.

AU - Kaiser, N.

AU - Kudritzki, R.-P.

AU - Luppino, G. A.

AU - Lupton, R. H.

AU - Monet, D. G.

AU - Morgan, J. S.

AU - Onaka, P. M.

AU - Stubbs, C. W.

AU - Tonry, J. L.

AU - Banados, E.

AU - Bell, E. F.

AU - Bender, R.

AU - Bernard, E. J.

AU - Botticella, M. T.

AU - Casertano, S.

AU - Chastel, S.

AU - Chen, W.-P.

AU - Chen, X.

AU - Cole, S.

AU - Deacon, N.

AU - Frenk, C.

AU - Fitzsimmons, A.

AU - Gezari, S.

AU - Goessl, C.

AU - Goggia, T.

AU - Goldman, B.

AU - Grebel, E. K.

AU - Hambly, N. C.

AU - Hasinger, G.

AU - Heavens, A. F.

AU - Heckman, T. M.

AU - Henderson, R.

AU - Henning, T.

AU - Holman, M.

AU - Hopp, U.

AU - Ip, W.-H.

AU - Isani, S.

AU - Keyes, C. D.

AU - Koekemoer, A.

AU - Kotak, R.

AU - Long, K. S.

AU - Lucey, J. R

AU - Liu, M.

AU - Martin, N. F.

AU - McLean, B.

AU - Morganson, E.

AU - Murphy, D. N. A.

AU - Nieto-Santisteban, M. A.

AU - Norberg, P.

AU - Peacock, J. A.

AU - Pier, E. A.

AU - Postman, M.

AU - Primak, N.

AU - Rae, C.

AU - Rest, A.

AU - Riess, A.

AU - Riffeser, A.

AU - Rix, H. W.

AU - Roser, S.

AU - Schilbach, E.

AU - Schultz, A. S. B.

AU - Scolnic, D.

AU - Szalay, A.

AU - Seitz, S.

AU - Shiao, B.

AU - Small, E.

AU - Smith, K. W.

AU - Soderblom, D.

AU - Taylor, A. N.

AU - Thakar, A. R.

AU - Thiel, J.

AU - Thilker, D.

AU - Urata, Y.

AU - Valenti, J.

AU - Walter, F.

AU - Watters, S. P.

AU - Werner, S.

AU - White, R.

AU - Wood-Vasey, W. M.

AU - Wyse, R.

PY - 2016/12/1

Y1 - 2016/12/1

N2 - Pan-STARRS1 has carried out a set of distinct synoptic imaging sky surveys including the $3\pi$ Steradian Survey and the Medium Deep Survey in 5 bands (\grizy). The mean 5$\sigma$ point source limiting sensitivities in the stacked 3$\pi$ Steradian Survey in \grizy are (23.3, 23.2, 23.1, 22.3, 21.4) respectively. The upper bound on the systematic uncertainty in the photometric calibration across the sky is 7-12 millimag depending on the bandpass. The systematic uncertainty of the astrometric calibration using the Gaia frame comes from a comparison of the results with Gaia: the standard deviation of the mean and median residuals ($ \Delta ra, \Delta dec $ ) are (2.3, 1.7) milliarcsec, and (3.1, 4.8) milliarcsec respectively. The Pan-STARRS system and the design of the PS1 surveys is described and an overview of the resulting image and catalog data products and their basic characteristics are described together with a summary of important results. The images, reduced data products, and derived data products from the Pan-STARRS1 surveys are available to the community from the Mikulski Archive for Space Telescopes (MAST) at STScI.

AB - Pan-STARRS1 has carried out a set of distinct synoptic imaging sky surveys including the $3\pi$ Steradian Survey and the Medium Deep Survey in 5 bands (\grizy). The mean 5$\sigma$ point source limiting sensitivities in the stacked 3$\pi$ Steradian Survey in \grizy are (23.3, 23.2, 23.1, 22.3, 21.4) respectively. The upper bound on the systematic uncertainty in the photometric calibration across the sky is 7-12 millimag depending on the bandpass. The systematic uncertainty of the astrometric calibration using the Gaia frame comes from a comparison of the results with Gaia: the standard deviation of the mean and median residuals ($ \Delta ra, \Delta dec $ ) are (2.3, 1.7) milliarcsec, and (3.1, 4.8) milliarcsec respectively. The Pan-STARRS system and the design of the PS1 surveys is described and an overview of the resulting image and catalog data products and their basic characteristics are described together with a summary of important results. The images, reduced data products, and derived data products from the Pan-STARRS1 surveys are available to the community from the Mikulski Archive for Space Telescopes (MAST) at STScI.

KW - Astrophysics - Instrumentation and Methods for Astrophysics

KW - Astrophysics - Earth and Planetary Astrophysics

KW - Astrophysics - Astrophysics of Galaxies

KW - Astrophysics - Solar and Stellar Astrophysics

M3 - Article

JO - arXiv

JF - arXiv

ER -

The Pan-STARRS1 Surveys

Abstract

Keywords

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