The American Astronomical Society is gravely concerned by the deep cuts to NASA science funding reported to be in the draft President’s Budget Request for Fiscal Year 2026. Read more here: aas.org/press/aas-st... and take action now: aas.org/urge-nasa-su...
Preview of the extension: VSDist.
Now the extension has been updated to v0.1.x with marge-stats added.
Shan, Hu et al. suggest that gravitational waves trigger wave-optics effects in microlensing, revealing host galaxies and opening a new window to the discovery of compact objects. https://bit.ly/3Y6V8gf #AstroSci
This is a preview of the extension.
As this is the first time I make extensions for VSCode, I only implemented basic features that I always use.
Please feel free to report issues or modify this extension.
If you are looking for tools to analyse MCMC chains generated by Cobaya in VSCode, you can try this extension: VSDist.
I develop the extension for quick preview of chain files on servers because I'm bothered with downloading them or writing scripts to visualise them. #cosmology
🆕 Suwei Wang and Lile Wang (Peking Univ) chat about new software instruments in the latest video from the AAS Journal Author Series: youtu.be/N-hvYXf6v-k
The AAS Journal Author Series connects authors with their article, their human story & the larger #astronomy community. 🔭
What if I told you there is no S8 tension?
youtu.be/PIQKe-tW1xQ
A two panel figure. The x-axis is omega_m, the fraction of matter in the Universe. The y-axis is S8 on the left and sigma_8 on the right. Both are measures of the 'clumpiness' of dark matter. The contours show that the KiDS data (two measurements using slightly different statistics, COSEBIs and Bandpowers) agree with the data from the Planck CMB survey.
🥳 It's paper day for the completed #ESO Kilo-Degree Survey. We end our journey with a consistent picture of #cosmology 😲
I've been co-leading KiDS for 12yrs & I'm so proud of what the team's achieved. If you're at the #Euclid meet, go to Angus Wright's talk @10am today!🔭
ℹ️: arxiv.org/pdf/2503.19441
☄️Today at the @icc-ub.bsky.social at Uni Barcelona we had one of the first presentations of the @desisurvey.bsky.social BAO DR2 results!🔭🧪
You can check it out on Youtube!
youtu.be/tuDzhR1SVDg?...
🔊 New BAO analysis from the 3-year observations (DR2). Long story short, as follows.
1. DESI alone is consistent with LCDM. 👉 Boring
2. DESI and Planck have a 2.3 discrepancy in Ωm-H0rd plane. 👉Interesting.
![A graph of the evolution of the dark energy (vertical axis) as a function of time (redshift on the horizontal axis) - showing an offset from the cosmological constant (a flat horizontal line). Here is the figure caption from the paper:
FIG. 12. Comparison of the constraints on the equation of
state of dark energy using the CPL parametrization and a bin-
ning reconstruction approach, using DESI+CMB+DESY5.
The solid green line shows the best-fit w(z) based on w0 and
wa inference and the green contours around it represent the
68% and 95% confidence intervals. We also show in blue the
constraints from the binning approach [47], with the hori-
zontal bars indicating the bin width (which is fixed) and the
vertical bars representing the 1σ error. Additionally, we in-
clude in gray the 1D posterior for each binning parameter.
The ΛCDM limit corresponds to the horizontal gray dashed
line.](https://cdn.bsky.app/img/feed_thumbnail/plain/did:plc:ok3ms3dzop7gcwejp7lswhpi/bafkreiaa64kyfu7u5ber7u6kwk2zzkuet66j6o3l4lr5ftl5sef67pzham)
A graph of the evolution of the dark energy (vertical axis) as a function of time (redshift on the horizontal axis) - showing an offset from the cosmological constant (a flat horizontal line). Here is the figure caption from the paper: FIG. 12. Comparison of the constraints on the equation of state of dark energy using the CPL parametrization and a bin- ning reconstruction approach, using DESI+CMB+DESY5. The solid green line shows the best-fit w(z) based on w0 and wa inference and the green contours around it represent the 68% and 95% confidence intervals. We also show in blue the constraints from the binning approach [47], with the hori- zontal bars indicating the bin width (which is fixed) and the vertical bars representing the 1σ error. Additionally, we in- clude in gray the 1D posterior for each binning parameter. The ΛCDM limit corresponds to the horizontal gray dashed line.
Congrats to @desisurvey.bsky.social - it's looking more & more like dark energy isn't Einstein's cosmological constant! If you've woken up to the news & are searching for the publications, they don't appear to be on arxiv 🤷♀️ but they are online. 🔭 #cosmology 🧪
ℹ️: data.desi.lbl.gov/public/paper...
“The Science of the Einstein Telescope”: An overview of what the next-generation gravitational wave observatory will enable. The sheer volume speaks for itself—550 pages full of science! 🔭🧪⚛️☄️
Freely accessible on arxiv.org/abs/2503.12263
🚨 BIG NEWS ALERT! 🚨
We’re just 24 HOURS AWAY from a MAJOR DESI release! 🌉🔭
Tomorrow at 3 PM PT, DESI is unveiling DR1, our first official Data Release—the largest dataset of its kind, packed with information on 18.7 million galaxies, quasars, and stars! But that’s not all…
The left of a mosaic of photographs from Euclid’s Early Release Observations in the background, containing stars, galaxies and glowing dust. “ONE WEEK UNTIL…” is written in large font in the foreground.
The right of a mosaic of photographs from Euclid’s Early Release Observations in the background, containing stars, galaxies and glowing dust. “Q1 DATA RELEASE” is written in large font in the foreground. Also shown is the Euclid Consortium logo and “#EUCLIDUK”.
Are you ready for it…?
Make room in your calendar for 19th March at 11:00, when stunning results with contributions from UK scientists will be revealed. 🚨 🗓️
#Euclid #Q1Release #Astronomy #Cosmology
A person holding a sign which says “I am here so my little sister can dream of becoming a scientist.”
🥹
Very cool. Here's the paper: dx.doi.org/10.1038/s415...
arXiv: dx.doi.org/10.48550/arx...
#Science #Astronomy #Physics #Cosmology 🧪🔭⚛️
A thin ring of a perfect circular shape and a piercingly bright white disc in its middle are the protagonists of this image. They stand out against a uniformly coloured background of a hazy dark grey. The ring appears as if it was a faint brush stroke, where at four evenly spaced spots more pressure was applied on the brush. These stand out in the ring as four brighter and thicker spots. The white disc within the ring gives the impression of a gaping hole in the image, through its stark contrast to the dark background.
This is the first time that the ring of light surrounding the centre of NGC 6505 is detected, thanks to Euclid’s high-resolution instruments.
🔭🧪
#cosmology
Happy Chinese New Year！🎉🎉🎉
A snake lady in a Chinese dress, celebrating her year (2025)
Wishing everyone a Happy Chinese New Year!!!
#katdraws
Cosmology Researcher Talks database 2024 stats:
1132 talks by 899 speakers re 1180 arXiv papers
Top 10 sources:
94 Cosmology fr Home
93 Perimeter Inst
92 Kyoto U, YITP
80 CosmoVerse
76 Misc
57 KITP
52 ICTP-SAIFR
42 CERN
31 Neutrinos fr Home
30 Parity Violation fr Home
jrdmb.netlify.app/crt.html
more books to read
The constraints on logfR0 from this work are compared with those from previous works. The best result from this work is shown in red, while other constraints using cosmic shear are presented in blue. Results from previous studies are depicted in black.
This is a comparison of results between our work and previous studies.
While our results are not the strongest, they are comparable to constraints from previous studies.
It seems that galaxy clustering information will be critical for constraints, so this will be involved in our future work.
Paper day! 🎉
My second work is now available on arXiv!
In this work, we test f(R) gravity with the state-of-the-art measurements of cosmic shear combined with CMB and BAO data.
We find an upper limit on the f(R) parameter, with log(fR0) constrained to be less than -4.79 (95% C.L.).
🧪🔭⚛️ #cosmology
Wow! Thank you so much!
Cheers!
Hi Physgal, I'm now studying cosmology at BNU and this is my website: astrobai.github.io.
Could you please add me there? Thanks!
Hi I am Physgal and I will be adding physicists to the Science feed. Please respond below with evidence that you are a physicist to be added to the feed.
teammates: @physgal.bsky.social / @quarkcharme.bsky.social
Today's random code is fkpt: Compute LCDM and modified gravity perturbation theory using fk-kernels
ascl.net/2403.006
fkpt computes the 1-loop redshift space power spectrum for tracers in LCDM and Modified Gravity models using perturbation theory.#astronomy
I just submitted my second paper.
Cheers!
