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LSST survey: millions and millions of quasars

Published online by Cambridge University Press:  23 June 2017

Željko Ivezić
Željko Ivezić*
Affiliation:
Department of Astronomy, University of Washington, Box 351580, Seattle, WA 98195-1580, USA email: [email protected]
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Abstract

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The Large Synoptic Survey Telescope (LSST), the next-generation optical imaging survey sited at Cerro Pachon in Chile, will provide hundreds of detections for a sample of more than ten million quasars with redshifts up to about seven. The LSST design, with an 8.4m (6.7m effective) primary mirror, a 9.6 sq. deg. field of view, and a 3.2 Gigapixel camera, will allow about 10,000 sq. deg. of sky to be covered twice per night, every three to four nights on average, with typical 5-sigma depth for point sources of r=24.5 (AB). With about 1000 observations in ugrizy bands over a 10-year period, these data will enable a deep stack reaching r=27.5 (about 5 magnitudes deeper than SDSS) and faint time-domain astronomy. The measured properties of newly discovered and known astrometric and photometric transients will be publicly reported within 60 sec after closing the shutter. In addition to a brief introduction to LSST, I review optical quasar selection techniques, with emphasis on methods based on colors, variability properties, and astrometric behavior.

Keywords

surveysgalaxies: activequasars: generalstars: variablesstars: statistics
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S324: New Frontiers in Black Hole Astrophysics , September 2016 , pp. 330 - 337
Copyright
Copyright © International Astronomical Union 2017 

References

Becker, R. H., White, R. L. & Helfand, D. J. 1995, ApJ, 450, 559 Google Scholar
Bovy, J., Myers, A. D., Hennawi, J., et al. 2012, ApJ, 749, 41 Google Scholar
Butler, N. R. & Bloom, J. S. 2011 AJ, 141, 93 Google Scholar
Flaugher, B. 2008, In A Decade of Dark Energy: Spring Symposium, Proceedings of the conferences held May 5-8, 2008 in Baltimore, Maryland. (USA). Ed. by N. Pirzkal & H. Ferguson. Google Scholar
Hao, L., Strauss, M. A., Fan, X., et al. 2005, AJ, 129, 1795 Google Scholar
Hawkins, M.R.S. & Veron, P. 1995, MNRAS, 275, 1102 Google Scholar
Ivezić, Ž., Lupton, R. H., Johnston, D. E., et al. 2003, ArXiv:astro-ph/0310566 Google Scholar
Ivezić, Ž., Lupton, R. H., Jurić, M., et al. 2004, ArXiv:astro-ph/0404487 Google Scholar
Ivezić, Ž., Tyson, J. A., Acosta, E., et al. 2008, ArXiv:0805.2366 Google Scholar
Ivezić, Ž., Beers, T. C. & Jurić, M. 2012, ARAA, 50, 251 Google Scholar
Kaczmarczik, M. C., Richards, G. T., Mehta, S. S. & Schlegel, D. J. 2009, AJ, 138, 19 CrossRefGoogle Scholar
Kaiser, N., Burgett, W., Chambers, K., et al. 2010, Proc. SPIE 7733, Ground-based and Airborne Telescopes III, vol. 7733, 77330EGoogle Scholar
Kawaguchi, T., Mineshige, S., Umemura, M., & Turner, E. L. 1998, ApJ, 504, 671 Google Scholar
Kelly, B. C., Bechtold, J. & Siemiginowska, A. 2009, ApJ, 698, 895 CrossRefGoogle Scholar
Kimball, A., Ivezić, Ž., Wiita, P. J. & Schneider, D. P. 2011, AJ, 141, 182 Google Scholar
Kozłowski, S., Kochanek, C. S., Udalski, A., et al. 2010, ApJ, 708, 927 Google Scholar
LSST Science Collaboration 2009, LSST Science Book, http://www.lsst.org/lsst/SciBook, arXiv:0912.0201Google Scholar
MacLeod, C. L., Ivezić, Ž, Kochanek, C. S., et al. 2010, ApJ, 721, 1014 Google Scholar
MacLeod, C. L., Brooks, K., Ivezić, Ž, et al. 2011, ApJ, 728, 26 Google Scholar
MacLeod, C. L., Ivezić, Ž, Sesar, B., et al. 2012, ApJ, 753, 106 Google Scholar
Palanque-Delabrouille, N., Yéche, Ch., Myers, A. D., et al. 2011, A&A, 530, 122 Google Scholar
Palanque-Delabrouille, N., Magneville, Ch., Yéche, Ch., et al. 2013, A&A, 551, 29 Google Scholar
Pâris, I., Petitjean, P., Aubourg, É, et al. 2012, A&A, 548, 66 Google Scholar
Richards, G. T., Fan, X., Schneider, D. P., et al. 2001, AJ, 121, 2308 (see also arXiv:1311.4870)Google Scholar
Richards, G. T., Fan, X., Newberg, H. J., et al. 2002, AJ, 123, 2945 Google Scholar
Richards, G. T., Strauss, M. A., Fan, X., et al. 2006, AJ, 131, 2766 Google Scholar
Richards, G. T., Myers, A. D., Gray, A. G., et al. 2009, ApJS, 180, 67 Google Scholar
Ross, N. P., Myers, A. D., Sheldon, E. S., et al. 2012 ApJS, 199, 3 Google Scholar
Sesar, B., Ivezić, Ž., Lupton, R. H., et al. 2007, AJ, 134, 2236 Google Scholar
Schmidt, K. B., Marshall, P. J., Rix, H.-W., et al. 2010, ApJ, 714, 1194 Google Scholar
Schneider, D. P., Richards, G. T., Hall, P. B., et al. 2010, AJ, 139, 2360 Google Scholar
Strauss, M. A., Weinberg, D. H., Lupton, R. H., et al. 2002, AJ, 124, 1810 Google Scholar
Zakamska, N. L., Strauss, M. A., Krolik, J. H., et al. 2003, AJ, 126, 2125 Google Scholar
Zakamska, N. L., Strauss, M. A., Heckman, T. M., et al. 2004, AJ, 128, 1002 CrossRefGoogle Scholar
Zu, Y., Kochanek, C. S., Kozłowski, S. & Udalski, A. 2013, ApJ, 765, 106 Google Scholar