Results 11 to 20 of about 3,073 (217)
Forward Modeling of Galaxy Populations for Cosmological Redshift Distribution Inference
The Astrophysical Journal Supplement Series, 2023 We present a forward-modeling framework for estimating galaxy redshift distributions from photometric surveys. Our forward model is composed of: a detailed population model describing the intrinsic distribution of the physical characteristics of galaxies,
Justin Alsing +4 more
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Physical Properties and Environments of Nearby Galaxies [PDF]
Annual Review of Astronomy and Astrophysics, 2009 We review the physical properties of nearby, relatively luminous galaxies, using results from newly available massive data sets together with more detailed observations. First, we present the global distribution of properties, including the optical and ultraviolet (UV) luminosity, stellar mass, and atomic gas mass functions.
Blanton, Michael R., Moustakas, John
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Targeted decrease of portal hepatic pressure gradient improves ascites control after TIPS
Hepatology, EarlyView., 2022 The river diagram demonstrates that after transjugular intrahepatic portosystemic shunt insertion (TIPS) the majority of patients without ascites and 50% of the patients with ascites detectable at ultrasound, show the best response in the long term follow‐up.
Alexander Queck +14 more
wiley +1 more source
The Astrophysical Journal, 2023 This paper represents an effort to provide robust constraints on the galaxy–halo connection and simultaneously test the Planck ΛCDM cosmology using a fully numerical model of small-scale galaxy clustering.
Gillian D. Beltz-Mohrmann +3 more
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Multimessenger Probes for New Physics in Light of A. Sakharov’s Legacy in Cosmoparticle Physics
Universe, 2021 A.D. Sakharov’s legacy in now standard model of the Universe is not reduced to baryosynthesis but extends to the foundation of cosmoparticle physics, which studies the fundamental relationship of cosmology and particle physics.
Maxim Khlopov
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Physical Classification of Galaxies with MOPED∕VESPA [PDF]
AIP Conference Proceedings, 2008 Invited talk at the class2008 meeting in ...
Raul Jimenez +4 more
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Probing the Physics of Interacting Galaxies
Astrophysics and Space Science, 2003 Both Arp 140 and Arp 104 reveal extended tidal tails in the HI. The Halpha and FIR fluxes of Arp 140 yield similar SFR of ~0.8 solar masses per year. In contrast the Halpha flux of Arp 104 yields a SFR of ~0.05 solar masses per year, ~ 20 times smaller than that obtained from the FIR flux.
Cullen, Harriet +2 more
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The physics of galaxy evolution with SPICA observations [PDF]
Proceedings of the International Astronomical Union, 2019 AbstractThe evolution of galaxies at Cosmic Noon (1 < z < 3) passed through a dust-obscured phase, during which most stars formed and black holes in galactic nuclei started to shine, which cannot be seen in the optical and UV, but it needs rest frame mid-to-far IR spectroscopy to be unveiled. At these frequencies, dust extinction is minimal and a
Luigi Spinoglio +2 more
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Cluster Physics with Merging Galaxy Clusters
Frontiers in Astronomy and Space Sciences, 2016 Collisions between galaxy clusters provide a unique opportunity to study matter in a parameter space which cannot be explored in our laboratories on Earth.
Sandor M. Molnar
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The Open Journal of Astrophysics, 2023 The recent launch of JWST has ushered in a new era of high-redshift astronomy by providing detailed insights into the gas and stellar populations of galaxies in the epoch of reionization.
Harley Katz +9 more
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