Active Galaxy Science in the LSST Deep-Drilling Fields: Footprints, Cadence Requirements, and Total-Depth Requirements. (arXiv:1811.06542v1 [astro-ph.IM])
<a href="http://arxiv.org/find/astro-ph/1/au:+Brandt_W/0/1/0/all/0/1">W.N. Brandt</a> (Penn State), <a href="http://arxiv.org/find/astro-ph/1/au:+Ni_Q/0/1/0/all/0/1">Q. Ni</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Yang_G/0/1/0/all/0/1">G. Yang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Anderson_S/0/1/0/all/0/1">S.F. Anderson</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Assef_R/0/1/0/all/0/1">R.J. Assef</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Barth_A/0/1/0/all/0/1">A.J. Barth</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bauer_F/0/1/0/all/0/1">F.E. Bauer</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bongiorno_A/0/1/0/all/0/1">A. Bongiorno</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Chen_C/0/1/0/all/0/1">C.-T. Chen</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Cicco_D/0/1/0/all/0/1">D. De Cicco</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Gezari_S/0/1/0/all/0/1">S. Gezari</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Grier_C/0/1/0/all/0/1">C.J. Grier</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hall_P/0/1/0/all/0/1">P.B. Hall</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hoenig_S/0/1/0/all/0/1">S.F. Hoenig</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Lacy_M/0/1/0/all/0/1">M. Lacy</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Li_J/0/1/0/all/0/1">J. Li</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Luo_B/0/1/0/all/0/1">B. Luo</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Paolillo_M/0/1/0/all/0/1">M. Paolillo</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Peterson_B/0/1/0/all/0/1">B.M. Peterson</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Popovic_L/0/1/0/all/0/1">L.C. Popović</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Richards_G/0/1/0/all/0/1">G.T. Richards</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Shemmer_O/0/1/0/all/0/1">O. Shemmer</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Shen_Y/0/1/0/all/0/1">Y. Shen</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Sun_M/0/1/0/all/0/1">M. Sun</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Timlin_J/0/1/0/all/0/1">J.D. Timlin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Trump_J/0/1/0/all/0/1">J.R. Trump</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Vito_F/0/1/0/all/0/1">F. Vito</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Yu_Z/0/1/0/all/0/1">Z. Yu</a>
This white paper specifies the footprints, cadence requirements, and
total-depth requirements needed to allow the most-successful AGN studies in the
four currently selected LSST Deep-Drilling Fields (DDFs): ELAIS-S1, XMM-LSS,
CDF-S, and COSMOS. The information provided on cadence and total-depth
requirements will also likely be applicable to enabling effective AGN science
in any additional DDFs that are chosen.
This white paper specifies the footprints, cadence requirements, and
total-depth requirements needed to allow the most-successful AGN studies in the
four currently selected LSST Deep-Drilling Fields (DDFs): ELAIS-S1, XMM-LSS,
CDF-S, and COSMOS. The information provided on cadence and total-depth
requirements will also likely be applicable to enabling effective AGN science
in any additional DDFs that are chosen.
http://arxiv.org/icons/sfx.gif
