Materie … #Universum. Neue Analysen des #KiloDegreeSurvey zeigen, dass die #MaterieImAll weniger stark gebündelt ist als vom Standardmodell der Kosmologie vorhergesagt, was auf mögliche Lücken im Verständnis #dunklerMaterie oder der #AllgemeinenRelativitätstheorie hindeutet.🖖
Bluesky

Bluesky Social

The KiDS Legacy

What with all the cosmological goings-on of the past couple of weeks – see here, here and here – I quite forgot to mention another important set of results. These are from the final data release Kilo-Degree Survey known as KiDS for short and represent a final analysis of the complete dataset. For those of you not in the know, KiDs is a weak lensing shear tomography survey and its core science drivers are to map the large scale matter distribution in the Universe and constrain the equation of state of Dark Energy. The results can be found in three papers on arXiv, which you can add to your reading list:

As far as I’m concerned, the main result to leap out from the cosmological analysis, which primarily constrains the clumpiness of matter in the universe, expressed by the density parameter Ωm and a fluctuation amplitude σ8 in the combined parameter “S8“, which is constrained almost independently from Ωm. The value obtained for this parameter by KiDS has previously been “in tension” with values from other experiments (notably Planck) ; see here for a discussion. The new results, however, seem consistent with the standard cosmological model. Here is a figure from the last paper in the above list that illustrates the point:

As is often the case, there’s also one of those nice Cosmology Talks videos that discusses this and other aspects of the KiDS Legacy results to which I refer you for more details!

https://www.youtube.com/watch?v=PIQKe-tW1xQ

#arXiv250319440 #arXiv250319441 #arXiv250319442 #DarEnergy #GravitationalLensing #KIDS #KiloDegreeSurvey #KilodegreeSurvey #weakGravitationalLensing

Results from the Atacama Cosmology Telescope

Today is going to be a very busy day on the cosmology front – with the Euclid Q1 Data Release coming out at 11am GMT – but I’ll start off by sharing news of final data release (DR…

In the Dark

#RUB:
"
Kilo-Degree Survey bestätigt Standardmodell der Kosmologie

Daten von 41 Millionen Galaxien hat ein internationales Forschungsteam ausgewertet, um die Materieverteilung im Weltall zu bestimmen. Die Daten bestätigen ein lang existierendes Modell – zur Überraschung des Teams.
"
https://news.rub.de/presseinformationen/wissenschaft/2025-03-26-astrophysik-kilo-degree-survey-bestaetigt-standardmodell-der-kosmologie

26.3.2025

#Astronomie #Astrophysik #Galaxien #Gravitationslinse #KiDS #KiloDegreeSurvey #Kosmologie #Materie #Standardmodell #Universum

Kilo-Degree Survey bestätigt Standardmodell der Kosmologie

Daten von 41 Millionen Galaxien hat ein internationales Forschungsteam ausgewertet, um die Materieverteilung im Weltall zu bestimmen. Die Daten bestätigen ein lang existierendes Modell – zur Überraschung des Teams.

Newsportal - Ruhr-Universität Bochum

Kilo-Degree-Survey ontdekt nieuw stellair system

Astronomen hebben in de buitenwijken, als onderdeel van de Kilo-Degree Survey (KiDS) een nieuw stellair systeem gevonden in de buitenwijken van de Melkweg. Het pas gevonden systeem, Sextans II genaamd, is hoogstwaarschijnlijk een ultrazwak dwergsterrenstelsel.

https://www.kuuke.nl/kilo-degree-survey-ontdekt-nieuw-stellair-system/

#KiDS #KiloDegreeSurvey #melkweg #SeaxtansII #UDF #UltrazwakDwergsterrenstelsel

Kilo-Degree-Survey ontdekt nieuw stellair system

Astronomen hebben een nieuw stellair systeem gevonden in de buitenwijken van de Melkweg. Het systeem, Sextans II, is vermoedelijk een ultrazwak dwergsterrenstelsel.

Kuuke's Sterrenbeelden
KiDS in the sky: New stellar system discovered by the Kilo-Degree Survey

Astronomers have discovered a new stellar system in the outskirts of the Milky Way as part of the Kilo-Degree Survey (KiDS). The newfound system, named Sextans II, is most likely an ultra-faint dwarf galaxy. The finding is reported in a paper published November 10 on the pre-print server arXiv.

Phys.org