2021AJ....161..262Z


Query : 2021AJ....161..262Z

2021AJ....161..262Z - Astron. J., 161, 262-262 (2021/June-0)

Real-time likelihood-free inference of Roman binary microlensing events with amortized neural posterior estimation.

ZHANG K., BLOOM J.S., GAUDI B.S., LANUSSE F., LAM C. and LU J.R.

Abstract (from CDS):

Fast and automated inference of binary-lens, single-source (2L1S) microlensing events with sampling-based Bayesian algorithms (e.g., Markov Chain Monte Carlo, MCMC) is challenged on two fronts: the high computational cost of likelihood evaluations with microlensing simulation codes, and a pathological parameter space where the negative-log-likelihood surface can contain a multitude of local minima that are narrow and deep. Analysis of 2L1S events usually involves grid searches over some parameters to locate approximate solutions as a prerequisite to posterior sampling, an expensive process that often requires human-in-the-loop domain expertise. As the next-generation, space-based microlensing survey with the Roman Space Telescope is expected to yield thousands of binary microlensing events, a new fast and automated method is desirable. Here, we present a likelihood-free inference approach named amortized neural posterior estimation, where a neural density estimator (NDE) learns a surrogate posterior \hatp(θ| x) as an observation-parameterized conditional probability distribution, from pre-computed simulations over the full prior space. Trained on 291,012 simulated Roman-like 2L1S simulations, the NDE produces accurate and precise posteriors within seconds for any observation within the prior support without requiring a domain expert in the loop, thus allowing for real-time and automated inference. We show that the NDE also captures expected posterior degeneracies. The NDE posterior could then be refined into the exact posterior with a downstream MCMC sampler with minimal burn-in steps.

Abstract Copyright: © 2021. The American Astronomical Society. All rights reserved.

Journal keyword(s): Binary lens microlensing - Gravitational microlensing exoplanet detection

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NAME EWS 2018-BLG-0677b Pl? 17 55 00.270 -32 00 59.51           ~ 8 0

Query : 2021AJ....161..262Z

Basic data :
NAME EWS 2018-BLG-0677b -- Extra-solar Planet Candidate
Other object types:
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Pl? (2020AJ)
ICRS coord. (ep=J2000) :
17 55 00.270 -32 00 59.51 [ ] D 2020AJ....159..256H
FK4 coord. (ep=B1950 eq=1950) :
17 51 44.730 -32 00 30.51 [ ]
Gal coord. (ep=J2000) :
358.388525 -03.313746 [ ]
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NAME EWS 2018-BLG-0677b

References (8 between 1850 and 2026) (Total 8)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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