Semianalytical Fokker–Planck Models for Nuclear Star Clusters by Karamveer Kaur, Barak Rom, Re’em Sari

Subjects: “…Galaxy nuclei…”
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Non-Gaussianity from Large-Scale Structure Surveys by Licia Verde

“…With the advent of galaxy surveys which provide large samples of galaxies or galaxy clusters over a volume comparable to the horizon size (SDSS-III, HETDEX, Euclid, JDEM, LSST, Pan-STARRS, CIP, etc.) or mass-selected large cluster samples over a large fraction of the extra-galactic sky (Planck, SPT, ACT, CMBPol, B-Pol), it is timely to investigate what constraints these surveys can impose on primordial non-Gaussianity. …”
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Recoiling Black Holes: Electromagnetic Signatures, Candidates, and Astrophysical Implications by S. Komossa

“…Long-lived oscillations of the SMBHs in galaxy cores, and in rare cases even SMBH ejections from their host galaxies, are the consequence. …”
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Clustering of X-Ray-Selected AGN by N. Cappelluti, V. Allevato, A. Finoguenov

“…In particular, one of the key results is that X-ray AGNs are hosted by dark matter halos of mass similar to that of galaxy groups. This result, together with model predictions, has lead to the hypothesis that galaxy mergers may constitute the main AGN-triggering mechanism. …”
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Testing General Relativity Using Large-scale Structure Photometric Redshift Surveys and the Cosmic Microwave Background Lensing Effect by Shang Li, Jun-Qing Xia

“…The E _G statistic provides a valuable tool for evaluating the predictions of general relativity (GR) by probing the relationship between gravitational potential and galaxy clustering on cosmological scales within the observable Universe. …”
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Analytical Predictions of Fragment Penetration through Hollow Concrete Masonry Units by David Bogosian, Bence Gerber

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Bose-Einstein Condensate Dark Matter Halos Confronted with Galactic Rotation Curves by M. Dwornik, Z. Keresztes, E. Kun, L. Á. Gergely

“…In the second class the rotational velocity of HSB and LSB galaxies exhibits long flat plateaus, resulting in better fit with the NFW model for HSB galaxies and comparable fits for LSB galaxies. …”
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High-energy Neutrino Source Cross-correlations with Nearest-neighbor Distributions by Zhuoyang Zhou, Jessi Cisewski-Kehe, Ke Fang, Arka Banerjee

“…We conduct a statistical power analysis of an associated likelihood ratio test with estimations of its sensitivity and discovery potential with synthetic neutrino data samples and a WISE–2MASS galaxy sample. We apply the method to IceCube’s public ten-year point-source data and find no statistically significant evidence for spatial cross-correlations with the selected galaxy sample. …”
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Molecular mechanisms and correlation of CMTM6 and PD-L1 inhibitors in colorectal cancer treatment by Liang Gao, Sai Ma

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The Low-Mass End of the MBH/Mhost Relation in Quasars by Roberto Decarli, Renato Falomo, Jari K. Kotilainen, Tomi Hyvönen, Michela Uslenghi, Aldo Treves

“…Host galaxy luminosities and stellar masses are computed, under reasonable assumptions on their star formation histories. …”
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Using DIMet for Differential Analysis of Labeled Metabolomics Data: A Step-by-step Guide Showcasing the Glioblastoma Metabolism by Johanna Galvis, Joris Guyon, Thomas Daubon, Macha Nikolski

“…Accessible to all researchers through Galaxy, DIMet is free, user-friendly, and open source, making it a valuable resource for advancing metabolic research.…”
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Hysterectomy: Current Methods and Alternatives by Liselotte Mettler, Harry Reich, Limin Feng, Shailesh Puntambekar, Adolf Gallinat, Michael Stark

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Astronomaly Protege: Discovery through Human-machine Collaboration by Michelle Lochner, Lawrence Rudnick

“…We train PROTEGE on images from the MeerKAT Galaxy Cluster Legacy Survey, leveraging the self-supervised deep learning algorithm Bootstrap Your Own Latent to find a low-dimensional representation of the radio galaxy cutouts. …”
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Les Quotas by Marie-Laure Schultze, Sujarei Tali

“…What you will see happens aboard a shabby spaceship, at the edge of a galaxy. The Intergalactic, the totalitarian power in place, stalks those who don’t obey to its rules. …”
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The Astronomical Pulse of Global Extinction Events by David F.V. Lewis, Jean-Lou C.M. Dorne

“…In particular, the apparent 26 million year cycle of global extinctions may be related to the motion of the solar system around the galaxy, especially perpendicular to the galactic plane. …”
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Can the New Neutrino Telescopes Reveal the Gravitational Properties of Antimatter? by Dragan Slavkov Hajdukovic

“…Our simplified calculations suggest that the antineutrinos emitted by supermassive black holes in the centre of the Milky Way and Andromeda Galaxy could be detected by the new generation of neutrino telescopes.…”
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Intermediate Mass Black Holes: Their Motion and Associated Energetics by C. Sivaram, Kenath Arun

“…There is a lot of current astrophysical evidence and interest in intermediate mass black holes (IMBH), ranging from a few hundred to several thousand solar masses. The active galaxy M82 and the globular cluster G1 in M31, for example, are known to host such objects. …”
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Signature of Plausible Accreting Supermassive Black Holes in Mrk 261/262 and Mrk 266 by Gagik Ter-Kazarian, Lusine Sargsyan

“…We address the neutrino radiation of plausible accreting supermassive black holes closely linking to the 5 nuclear components of galaxy samples of Mrk 261/262 and Mrk 266. We predict a time delay before neutrino emission of the same scale as the age of the Universe. …”
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Null Geodesics and Strong Field Gravitational Lensing of Black Hole with Global Monopole by M. Sharif, Sehrish Iftikhar

“…We then find Einstein rings, magnifications, and observables of the relativistic images for supermassive black hole at the center of galaxy NGC4486B. We also examine time delays for different galaxies and present our results numerically. …”
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Doppler cross-correlation spectroscopy as a path to the detection of Earth-like planets by Mayor, Michel

“…In the middle of the 20th century, a paradigm shift appeared concerning the expected frequency of planetary systems in the galaxy ...a shift induced by the observation of the rotational velocities of low main sequence stars (Struve 1952)!…”
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