True!
Hence, my second favourite black hole is the less massive component of GW241011!
@haster.bsky.social
Assistant Professor at UNLV+NevadaCfA looking for gravitational waves and the best music. Previously at LIGO, MITKavli, CITA_ICAT and UoBIGWaves.
True!
Hence, my second favourite black hole is the less massive component of GW241011!
Depends how well you will justify picking another one π
12.12.2025 00:56 β π 1 π 0 π¬ 1 π 0International conventions should not be held in the U.S.
11.12.2025 22:49 β π 142 π 52 π¬ 8 π 0For now, the more massive component of the GW241011 binary β«οΈ
12.12.2025 00:53 β π 1 π 0 π¬ 1 π 0Hubble Space Telescope in space orbiting above Earthβs limb. Words to the right read: Hubble Notebook Update.
Improvements ahead! A team at STScI recently launched a full suite of enhanced Jupyter Notebooks for scientific analyses with Hubble. The upgrades improve the functionality of the repository, as well as the DrizzlePac software suite: https://bit.ly/3XJAXVh π π§ͺ βοΈ
09.12.2025 18:14 β π 23 π 5 π¬ 0 π 0Heartbreaking. The University of Nebraska will terminate its entire Earth science department.
One of the country's most successful and respected geology & climate programs: gone.
When ideologues & politicians are threatened by the very act of studying climate change, I wonder: who of us is next?
It's easy to forget we live in a future with a fully operating space station with multiple docking ports for various spacecraft.
www.space.com/space-explor...
A black and white comic of the author talkin to themselves, they say βahhh a new year, a fresh startβ. They then look at the calendar in shock seeing itβs already May. βHUH? MAY??β they say. Then they say βthatβs fine, I have the whole summer ahead of me!β They look at the calendar, now itβs September. βWHAT?! HUH?β They hold their head in their hands, despairing. βNo, no, itβs okay, thereβs still timeβ they look at the calendar which now says December and shriek βSTOP!!β At it
Happy old year
01.12.2025 22:15 β π 4660 π 1319 π¬ 25 π 22A skill that might actually be quite useful while on the ISS!
26.11.2025 10:48 β π 3 π 0 π¬ 0 π 0Also featured is the Spherical Cow by @minouette.bsky.social π
25.11.2025 21:12 β π 2 π 0 π¬ 0 π 0The fun office corner π
25.11.2025 20:54 β π 2 π 0 π¬ 1 π 0A really nice Astrobites article about our recent discovery of two really interesting black hole binaries observed with @ligo.org and @egovirgo.bsky.social!
24.11.2025 00:27 β π 6 π 1 π¬ 0 π 0Are you fucking kidding me itβs like we are living in a cartoon
21.11.2025 08:33 β π 3995 π 1108 π¬ 43 π 45and it makes one corner of my office significantly more fun π
23.11.2025 07:46 β π 1 π 0 π¬ 1 π 0It is indeed a very pretty (and scientifically accurate) star!
23.11.2025 06:52 β π 1 π 0 π¬ 1 π 0Game for cool people
22.11.2025 01:37 β π 2 π 0 π¬ 0 π 0Have you ever wanted @astropy.org tutorials on:
βΒ spectroscopic data reduction from a raw FITS image,
βΒ computing galactic orbits from Gaia measurements,
βΒ cross-matching astronomical catalogs?
Check out the redesigned learn.astropy.org! Announcement from @numfocus.bsky.social below. π§ͺπ #astrocode
Infographic about GW241011 and GW241110 GW241011's source contained black holes about 13 and 8 times the mass of our Sun. The spin of the bigger black hole is high and bear aligned with the orbit. GW241110's source contained black holes about 17 and 8 times the mass of our Sun. The spin of the larger black hole is high and near anti-aligned with the orbit. Credit: Shanika Galaudage/Northwestern University/Adler Planetarium
We are pleased to announce our discovery of #GW241011 and #GW241110
Both come from binary black holes where one black hole is much larger than the other. The larger black holes have large spin. Could these black holes have formed in a previous merger?
ligo.org/science-summ...
#O4IsHere ππ§ͺβοΈβοΈ
A little less than a year ago, a large team of cosmologists reported evidence that dark energy (which drives the acceleration of the expansion of the Universe) evolves over time. This made a huge splash but has also been viewed with healthy skepticism. Today they report that evidence has weakened. π§ͺ
12.11.2025 12:00 β π 181 π 37 π¬ 5 π 4GWTC-4.0 Introduction & Open Data Webinar 13 November 2025 Webinar live from 15:00 UTC
Our next webinar will introduce our latest #GWTC4 release and the associated data (papers arxiv.org/abs/2508.18080 and arxiv.org/abs/2508.18079)
Tomorrow at 15:00 UTC, with the recording on YouTube after
Free registration wisconsin-edu.zoom.us/webinar/regi...
βοΈπ
A universal mystery πͺ Recently published research co-authored by UNLV astrophysicist Carl-Johan Haster gives insight into black holes and fundamental physics.
#UniversityResearch #Science #Physics #Astrophysics
www.unlv.edu/news/release...
Weβre closer to solving dark matter thanks to these black holes!
OzGrav PhD student at ANU, Aswathi, was part of the analysis team of the GW241011+GW241110 special event paper. Here she explains how these events helped refine our understanding of dark matter.
youtube.com/shorts/wW4yp...
A really nice article in AAS Nova about our article that was published today!
28.10.2025 18:14 β π 3 π 0 π¬ 0 π 0It's been very fun/frustrating sitting on these results for the last couple of months π
So I'm happy they're out for the rest of the world to see!
Finally, I want to thank the amazing team I've had the privilege to work with over the last couple of months in preparing this paper!
I couldn't find a better group of people to work with, and explore the amazing astrophysical potential our observations provide π
This precise spin measurements also allow us to do some pretty impressive tests of fundamental physics, in addition to the very informative astrophysical constraints.
Again, showing the amount GW observations will be able to help us understand our Universe better in so many different ways!
This is most evident in the very well measured spins of the more massive BH in our binaries.
28.10.2025 16:06 β π 1 π 0 π¬ 1 π 0These two binaries have some pretty exciting properties, with binary configurations nicely hinting towards a likely formation through *at least* a dynamical process, but also potentially with one of the Black Holes in our observed binaries being the remnant from a previous BBH merger!
28.10.2025 16:06 β π 1 π 0 π¬ 1 π 0I'm incredibly happy to share the amazing results we in the @ligo.org, @egovirgo.bsky.social, KAGRA collaborations have made public today.
iopscience.iop.org/article/10.3...
We are today announcing the observation of two new Binary Black Holes, GW241011 and GW241110.