Investigating the population of Galactic star formation regions and star clusters within a Wide-Fast-Deep Coverage of the Galactic Plane. (arXiv:1812.03025v1 [astro-ph.SR])

Investigating the population of Galactic star formation regions and star clusters within a Wide-Fast-Deep Coverage of the Galactic Plane. (arXiv:1812.03025v1 [astro-ph.SR])
<a href="http://arxiv.org/find/astro-ph/1/au:+Prisinzano_L/0/1/0/all/0/1">L. Prisinzano</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Magrini_L/0/1/0/all/0/1">L. Magrini</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Damiani_F/0/1/0/all/0/1">F. Damiani</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Sacco_G/0/1/0/all/0/1">G. Sacco</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bonito_R/0/1/0/all/0/1">R. Bonito</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Venuti_L/0/1/0/all/0/1">L. Venuti</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Casali_G/0/1/0/all/0/1">G. Casali</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Roccatagliata_V/0/1/0/all/0/1">V. Roccatagliata</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Randich_S/0/1/0/all/0/1">S. Randich</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Inno_L/0/1/0/all/0/1">L. Inno</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Cantat_Gaudin_T/0/1/0/all/0/1">T. Cantat-Gaudin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Minniti_D/0/1/0/all/0/1">D. Minniti</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bragaglia_A/0/1/0/all/0/1">A. Bragaglia</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Innocenti_S/0/1/0/all/0/1">S. Degli Innocenti</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Moroni_P/0/1/0/all/0/1">P. G. Prada Moroni</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Tognelli_E/0/1/0/all/0/1">E. Tognelli</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Sollima_A/0/1/0/all/0/1">A. Sollima</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Vallenari_A/0/1/0/all/0/1">A. Vallenari</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Guarcello_M/0/1/0/all/0/1">M. Guarcello</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Messina_S/0/1/0/all/0/1">S. Messina</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Micela_G/0/1/0/all/0/1">G. Micela</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Sciortino_S/0/1/0/all/0/1">S. Sciortino</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Spagna_A/0/1/0/all/0/1">A. Spagna</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Sanna_N/0/1/0/all/0/1">N. Sanna</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kastner_J/0/1/0/all/0/1">J. Kastner</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Roman_A/0/1/0/all/0/1">A. Roman</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Szabo_R/0/1/0/all/0/1">R. Szabo</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Dias_B/0/1/0/all/0/1">B. Dias</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Feigelson_E/0/1/0/all/0/1">E. Feigelson</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Jeffries_R/0/1/0/all/0/1">R. Jeffries</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Friel_E/0/1/0/all/0/1">E. Friel</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Stauffer_J/0/1/0/all/0/1">J. Stauffer</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Swaelmen_M/0/1/0/all/0/1">M. Van der Swaelmen</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Sordo_R/0/1/0/all/0/1">R. Sordo</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bossini_D/0/1/0/all/0/1">D. Bossini</a>

One of the aims of LSST is to perform a systematic survey of star clusters
and star forming regions (SFRs) in our Galaxy. In particular, the observations
obtained with LSST will make a big difference in Galactic regions that have
been poorly studied in the past, such as the anticenter and the disk beyond the
Galactic center, and they will have a strong impact in discovering new distant
SFRs. These results can be achieved by exploiting the exquisite depth that will
be attained if the wide-fast-deep (WFD) observing strategy of the main survey
is also adopted for the Galactic plane, in the g, r, and i filters.

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