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Microlensing mass measurement from images of rotating gravitational arcs
dc.abstract.en | Gravitational microlensing<SUP>1</SUP> is a powerful technique for measuring the mass of isolated and faint or non-luminous objects in the Milky Way<SUP>2,3</SUP>. In most cases, however, additional observations to the photometric light curve are required to measure accurately the mass of the microlens. Long-baseline optical/infrared interferometry provides a new and efficient way to deliver such independent constraints<SUP>4-7</SUP>, as demonstrated recently by first interferometric observations in microlensing event TCP J05074264+2447555 (`Kojima-1')<SUP>8</SUP>. Here we report real-time observations of gravitationally lensed arcs in rotation around a microlens, Gaia19bld<SUP>9</SUP>, made with the PIONIER instrument<SUP>10</SUP> at the Very Large Telescope Interferometer. Our data allowed us to determine the angular separation and length of the arcs, as well as their rotation rate. Combining these measurements with ground-based photometric data enabled the determination of the microlens mass, M = 1.147 ± 0.029 M<SUB>⊙</SUB>, to a very high accuracy. We anticipate interferometric microlensing to play an important future role in the mass and distance determination of isolated stellar-mass black holes<SUP>11-13</SUP> in the Galaxy, which cannot be addressed by any other technique. |
dc.affiliation | Uniwersytet Warszawski |
dc.contributor.author | Wyrzykowski, Łukasz |
dc.contributor.author | Wertz, Olivier |
dc.contributor.author | Cassan, Arnaud |
dc.contributor.author | Street, Rachel |
dc.contributor.author | Surdej, Jean |
dc.contributor.author | Hundertmark, Markus |
dc.contributor.author | Bouquin, Jean-Baptiste Le |
dc.contributor.author | Bachelet, Étienne |
dc.contributor.author | Absil, Olivier |
dc.contributor.author | Ranc, Clément |
dc.contributor.author | Tsapras, Yiannis |
dc.contributor.author | Rybicki, Krzysztof |
dc.contributor.author | Wambsganss, Joachim |
dc.date.accessioned | 2024-01-25T11:29:01Z |
dc.date.available | 2024-01-25T11:29:01Z |
dc.date.issued | 2022 |
dc.description.finance | Publikacja bezkosztowa |
dc.description.volume | 6 |
dc.identifier.doi | 10.1038/S41550-021-01514-W |
dc.identifier.uri | https://repozytorium.uw.edu.pl//handle/item/112425 |
dc.identifier.weblink | http://adsabs.harvard.edu/abs/2022NatAs...6..121C |
dc.language | eng |
dc.pbn.affiliation | astronomy |
dc.relation.ispartof | Nature Astronomy |
dc.relation.pages | 121-128 |
dc.rights | ClosedAccess |
dc.sciencecloud | nosend |
dc.title | Microlensing mass measurement from images of rotating gravitational arcs |
dc.type | JournalArticle |
dspace.entity.type | Publication |