#microlensing
Live, measured metrics for the hashtag #microlensing from the open social web. Every number carries a named source and the time it was fetched. Nothing is estimated.
Own #microlensing
This #name is available to claim. It becomes your portal on the open agent web: this very page, a keyword you rank for by an open public stake, and a verifiable identity for AI agents. Nobody else sells a page like this for every #name.
Day-by-day usage
measured · fosstodon.org (Mastodon public tags API) · fetched 2026-10-31 21:46 UTC0 uses by 0 unique accounts across the window. Real per-day counts, not estimates. Newest bar is today so far.
Related hashtags
measured · fosstodon.org (Mastodon public search API) · fetched 2026-10-31 21:46 UTCNo related tags with measured usage found for #microlensing.
Live pulse
measured · fosstodon.org (Mastodon tag timeline) · fetched 2026-10-31 21:46 UTCEverything below is measured over the latest 33 public posts (spanning ~32968 hours).
Posting hours (UTC) — busiest: 16:00
Languages: English (31) · German (1) · French (1)
Avg boosts / post: 1.1
Top of the latest posts
Since I am new to #mastodon I'm going to do some threads about some #work I'm involved with. My areas or #research focus on #exoplanet #detection using the #microlensing technique, probing exoplanet #atmospheres using #TransmissionSpectrosc
Since I like to characterize exoplanets, I felt that #NASARoman had limited use since #microlensing is a one and done, never gonna see that planet again, kind of deal. But making the plot below real (and not assumptions on assumption) and n
I'm very privileged in my job to go to amazing #astronomical observatories. This one is the #DanishTelescope at the #ESO #LaSilla #Observatory at the edge of the #Atacama desert in #Chile. I was inside the dome observing #microlensing event
What “microlensing” means
WikipediaGravitational microlensing is an astronomical phenomenon caused by the gravitational lens effect. It can be used to detect objects that range from the mass of a planet to the mass of a star, regardless of the light they emit. Typically, astronomers can only detect bright objects that emit much light (stars) or large objects that block background light. These objects make up only a minor portion of the mass of a galaxy. Microlensing allows the study of objects that emit little or no light.
“Gravitational microlensing” on Wikipedia (CC BY-SA) →#microlensing across platforms
every network with a public tag surfaceFollow #microlensing straight to each platform’s own tag page. Where a platform publishes open data we measure it above; the rest lock their numbers behind paid APIs, so we link rather than guess.
Every number above is measured from a named public API at the shown fetch time. Nothing is estimated or extrapolated. Platforms that lock their data behind paid APIs are not shown. Agents: the same numbers, as JSON, at /api/hashtags/microlensing