Extragalactic microlensing through Ultra Diffuse Galaxies
Sung Kei Li, Thomas Broadhurst, Jose M. Diego, Jeremy Lim, Jose M. Palencia + 1 more
TLDR
This paper explores extragalactic microlensing through Ultra Diffuse Galaxies, finding it possible but rare for NGC1052-DF2, with future prospects using Euclid and LSST.
Key contributions
- Explores extragalactic microlensing through Ultra Diffuse Galaxies (UDGs) for the first time.
- Finds UDG microlensing detection possible but rare for NGC1052-DF2 with current JWST/LSST observations.
- Suggests Euclid for identifying ideal targets, estimating O(1-10) events/year across the sky with LSST monitoring.
- Highlights UDG microlensing's potential to independently estimate stellar IMF and multiplicity in low-mass regimes.
Why it matters
This paper introduces a novel method to study extragalactic microlensing using Ultra Diffuse Galaxies, a previously unexplored avenue. It highlights the potential for future large-scale surveys like Euclid and LSST to detect these rare events. The findings could provide crucial insights into the stellar populations and dark matter content of UDGs.
Original Abstract
Stellar microlensing is a powerful method to constrain compact dark matter models, uncover binary stars, and exoplanets during caustic crossing events. At cosmological distances, {\it James-Webb Space Telescope} ({\it JWST}) is routinely detecting microlensed giant stars in highly magnified galaxies behind massive lensing clusters. Here, we explore for the first time microlensing in modest redshift galaxies commonly seen through local Ultra Diffuse Galaxies (UDGs). Using the UDG NGC1052-DF2 as a case study, we found that detecting UDG microlensing events through UDGs is possible. However, a low total UDG microlensing event rate of $\sim 5.6\times10^{-2}\,\textrm{yr}^{-1}$ over its five background galaxies is expected for typical {\it JWST} $\sim 29\,$mag visits, and a low Vera Rubin Legacy Survey of Space and Time (LSST) detection rate of $\sim 2\times10^{-8}\,\textrm{yr}^{-1}$ such that NGC1052-DF2 might not be a prime target given its lack of low-redshift background galaxies. {\it Euclid} is ideal for identifying samples of low-redshift star-forming galaxies seen through local galaxies for deeper cadenced follow-up, where our zeroth-order calculation estimates that $\mathcal{O}(1-10)$ events per year are expected over the whole sky under the monitoring of LSST. Finally, we postulate that UDG microlensing will allow an independent estimate of the initial mass function (IMF) and the stellar multiplicity in the low mass regime, of considerable interest for UDG galaxies, where stellar mass has been claimed to predominate over dark matter in some cases, including NGC1052-DF2.
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