Spurious shear in weak lensing with the Large Synoptic Survey Telescope

The complete 10-yr survey from the Large Synoptic Survey Telescope (LSST) will image ∼20 000 deg2 of the sky in six filter bands every few nights, bringing the final survey depth to r ∼ 27.5, with over four billion well-measured galaxies. To take full advantage of this unprecedented statistical powe...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2013-01, Vol.428 (3), p.2695-2713
Hauptverfasser:	Chang, C., Kahn, S. M., Jernigan, J. G., Peterson, J. R., AlSayyad, Y., Ahmad, Z., Bankert, J., Bard, D., Connolly, A., Gibson, R. R., Gilmore, K., Grace, E., Hannel, M., Hodge, M. A., Jee, M. J., Jones, L., Krughoff, S., Lorenz, S., Marshall, P. J., Marshall, S., Meert, A., Nagarajan, S., Peng, E., Rasmussen, A. P., Shmakova, M., Sylvestre, N., Todd, N., Young, M.
Format:	Artikel
Sprache:	eng
Schlagworte:	Algorithms Astrophysics Mathematical functions Measurement errors Simulation Stars & galaxies Telescopes
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