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Unique Science from a Coordinated LSST-WFIRST Survey of the Galactic Bulge

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arxiv 1812.04445 v1 pith:MAZM6DDD submitted 2018-12-07 astro-ph.IM astro-ph.EPastro-ph.SR

R.A. Street , M.B. Lund , M. Donachie , S. Khakpash , N. Golovich , M. Penny , D. Bennett , W.A. Dawson
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J. Pepper M. Rabus P. Szkody W.I. Clarkson R. Di Stefano N. Rattenbury M.P.G. Hundertmark Y. Tsapras S. Ridgway K. Stassun V. Bozza A. Bhattacharya S. Calchi Novati Y. Shvartzvald (LSST Transient Variable Stars Collaboration)
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classification astro-ph.IMastro-ph.EPastro-ph.SR
keywords surveybulgeexploregalacticlsstmicrolensingmissionscience
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NASA's WFIRST mission will perform a wide-field, NIR survey of the Galactic Bulge to search for exoplanets via the microlensing techniques. As the mission is due to launch in the mid-2020s, around half-way through the LSST Main Survey, we have a unique opportunity to explore synergistic science from two landmark programs. LSST can survey the entire footprint of the WFIRST microlensing survey in a single Deep Drilling Field. Here we explore the great scientific potential of this proposal and recommend the most effective observing strategies.

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  1. WFIRST and EUCLID: enabling the microlensing parallax measurement from space

    astro-ph.EP 2019-08 conditional novelty 6.0 of 10

    High-cadence Euclid observations made simultaneously with WFIRST could measure microlens parallax and mass for about twenty free-floating planets over 120 days of coordinated observing.

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