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Title: Gravitational Microlensing Event Statistics for the Zwicky Transient Facility

Abstract

Microlensing surveys have discovered thousands of events, with almost all events discovered within the Galactic bulge or toward the Magellanic Clouds. The Zwicky Transient Facility (ZTF), while not designed to be a microlensing campaign, is an optical time-domain survey that observes the entire northern sky, including the Galactic plane, every few nights. The ZTF observes ~109 stars in the g and r bands and can significantly contribute to the observed microlensing population. In this paper, we predict that the ZTF will observe ~1100 microlensing events in 3 yr of observing within 10° latitude of the Galactic plane, with ~500 events in the outer Galaxy (ℓ ≥ 10°). This yield increases to ~1400 (~800) events by combining every three ZTF exposures, ~1800 (~900) events if the ZTF observes for a total of 5 yr, and ~2400 (~1300) events for a 5 yr survey with postprocessing image stacking. Using the microlensing modeling software PopSyCLE, we compare the microlensing populations in the Galactic bulge and the outer Galaxy. We also present an analysis of the microlensing event ZTF18abhxjmj to demonstrate how to leverage these population statistics in event modeling. The ZTF will constrain Galactic structure, stellar populations, and primordial black holes through photometricmore » microlensing.« less

Authors:
ORCiD logo [1]; ORCiD logo [2]; ORCiD logo [3]; ORCiD logo [2]; ORCiD logo [3]; ORCiD logo [3]; ORCiD logo [4]
  1. Univ. of California, Berkeley, CA (United States); Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
  2. Univ. of California, Berkeley, CA (United States)
  3. Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
  4. Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
Publication Date:
Research Org.:
Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States); Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
Sponsoring Org.:
USDOE National Nuclear Security Administration (NNSA); USDOE Laboratory Directed Research and Development (LDRD) Program; National Science Foundation (NSF); USDOE Office of Science (SC)
OSTI Identifier:
1660505
Alternate Identifier(s):
OSTI ID: 1780743
Report Number(s):
LLNL-JRNL-806658
Journal ID: ISSN 1538-4357; 1011998; TRN: US2203521
Grant/Contract Number:  
AC52-07NA27344; LGF-19-600357; AST-1909641; AC02-05CH11231
Resource Type:
Accepted Manuscript
Journal Name:
The Astrophysical Journal (Online)
Additional Journal Information:
Journal Name: The Astrophysical Journal (Online); Journal Volume: 897; Journal Issue: 2; Journal ID: ISSN 1538-4357
Publisher:
Institute of Physics (IOP)
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; Stellar astronomy; Stellar populations; Black holes; Bayesian statistics; Time domain astronomy; Transient sources; Milky Way dark matter halo; Galactic bulge; Milky Way disk; Astronomy data modeling; Gravitational microlensing; Microlensing event rate

Citation Formats

Medford, Michael S., Lu, Jessica R., Dawson, William A., Lam, Casey Y., Golovich, Nathan R., Schlafly, Edward F., and Nugent, Peter. Gravitational Microlensing Event Statistics for the Zwicky Transient Facility. United States: N. p., 2020. Web. doi:10.3847/1538-4357/ab9a4f.
Medford, Michael S., Lu, Jessica R., Dawson, William A., Lam, Casey Y., Golovich, Nathan R., Schlafly, Edward F., & Nugent, Peter. Gravitational Microlensing Event Statistics for the Zwicky Transient Facility. United States. https://doi.org/10.3847/1538-4357/ab9a4f
Medford, Michael S., Lu, Jessica R., Dawson, William A., Lam, Casey Y., Golovich, Nathan R., Schlafly, Edward F., and Nugent, Peter. Mon . "Gravitational Microlensing Event Statistics for the Zwicky Transient Facility". United States. https://doi.org/10.3847/1538-4357/ab9a4f. https://www.osti.gov/servlets/purl/1660505.
@article{osti_1660505,
title = {Gravitational Microlensing Event Statistics for the Zwicky Transient Facility},
author = {Medford, Michael S. and Lu, Jessica R. and Dawson, William A. and Lam, Casey Y. and Golovich, Nathan R. and Schlafly, Edward F. and Nugent, Peter},
abstractNote = {Microlensing surveys have discovered thousands of events, with almost all events discovered within the Galactic bulge or toward the Magellanic Clouds. The Zwicky Transient Facility (ZTF), while not designed to be a microlensing campaign, is an optical time-domain survey that observes the entire northern sky, including the Galactic plane, every few nights. The ZTF observes ~109 stars in the g and r bands and can significantly contribute to the observed microlensing population. In this paper, we predict that the ZTF will observe ~1100 microlensing events in 3 yr of observing within 10° latitude of the Galactic plane, with ~500 events in the outer Galaxy (ℓ ≥ 10°). This yield increases to ~1400 (~800) events by combining every three ZTF exposures, ~1800 (~900) events if the ZTF observes for a total of 5 yr, and ~2400 (~1300) events for a 5 yr survey with postprocessing image stacking. Using the microlensing modeling software PopSyCLE, we compare the microlensing populations in the Galactic bulge and the outer Galaxy. We also present an analysis of the microlensing event ZTF18abhxjmj to demonstrate how to leverage these population statistics in event modeling. The ZTF will constrain Galactic structure, stellar populations, and primordial black holes through photometric microlensing.},
doi = {10.3847/1538-4357/ab9a4f},
journal = {The Astrophysical Journal (Online)},
number = 2,
volume = 897,
place = {United States},
year = {Mon Jul 13 00:00:00 EDT 2020},
month = {Mon Jul 13 00:00:00 EDT 2020}
}

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