Early Enrichment Population Theory at High Redshift by Anne E. Blackwell, Joel N. Bregman

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Nebular and Nonthermal Radio Emissions for Young Stellar Populations with PARSEC v1.2s by Ikechukwu A. Obi, Pius N. Okeke, Bonaventure I. Okere

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Charged-Current Neutrino-Nucleus Scattering off the Even Molybdenum Isotopes by E. Ydrefors, J. Suhonen

“…Neutrinos from supernovae constitute important probes of both the currently unknown supernova mechanisms and of neutrino properties. …”
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Non-modifiable and Modifiable Risk Factors in Vascular Ageing Extremes: The African-PREDICT Study by Donavan Rooi, Ruan Kruger, Esmé Jansen van Vuren, Yolandi Breet

“…Black ethnicity was higher (p = 0.038) in the SUPERNOVA group. In exploratory factor analysis, a factor pattern including mean arterial pressure and fasting glucose showed beneficial odds (OR 0.62, p = 0.002) for SUPERNOVA and higher likelihood (OR 2.10, p < 0.001) for EVA. …”
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Cosmic rays escape from their sources by A. Marcowith

“…Cosmic rays (CRs) are accelerated in diverse astrophysical objects like supernova remnants, massive star clusters, or pulsars. …”
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Assembly of the salt-secreting mangrove Avicennia rumphiana. by Jeremy R Shearman, Chaiwat Naktang, Chutima Sonthirod, Wasitthee Kongkachana, Sonicha U-Thoomporn, Nukoon Jomchai, Chatree Maknual, Suchart Yamprasai, Poonsri Wanthongchai, Wirulda Pootakham, Sithichoke Tangphatsornruang

“…We sequenced and assembled the A. rumphiana genome into 24,094 Supernova-scaffolds totalling 499.6 Mb. Sequence comparison showed that 68.7% of the A. rumphiana genome aligned to A. marina sequence, covering 72% of the A. marina genome at an average nucleotide identity of 87.7%, showing that A. marina is closely related to A. rumphiana and, thus, suitable for reference based scaffolding of the A. rumphiana Supernova-scaffolds. …”
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Star shearing season: transient signals in wave-like dark matter experiments from black hole formation by Arturo de Giorgi, Joerg Jaeckel

“…When these objects are turned into black holes due to a supernova or a binary merger this “hair” could be “shorn” off. …”
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Neutral-Current Neutrino-Nucleus Scattering off Xe Isotopes by P. Pirinen, J. Suhonen, E. Ydrefors

“…Using suitable neutrino energy distributions, we compute estimates of total averaged cross sections for ​8B solar neutrinos and supernova neutrinos.…”
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Convoluted ν-Signals on 114Cd Isotope from Astrophysical and Laboratory Neutrino Sources by Vaitsa Tsakstara

“…Towards this purpose, the required folded cross section comes out of simulation techniques by employing several low, and intermediate-energy neutrino distributions of the astrophysical ν-sources, like the solar, supernova, and Earth neutrinos, as well as the laboratory neutrinos, the reactor neutrinos, the pion-muon stopped neutrinos, and the β-beam neutrinos.…”
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Revealing an unexpectedly low electron injection threshold via reinforced shock acceleration by Savvas Raptis, Ahmad Lalti, Martin Lindberg, Drew L. Turner, Damiano Caprioli, James L. Burch

“…Abstract Collisionless shock waves, found in supernova remnants, interstellar, stellar, and planetary environments, and laboratories, are one of nature’s most powerful particle accelerators. …”
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The Era of Kilometer-Scale Neutrino Detectors by Francis Halzen, Uli Katz

“…The scientific missions of these instruments include searching for sources of cosmic rays and for dark matter, observing Galactic supernova explosions, and studying the neutrinos themselves. …”
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Scheduling in Targeted Transient Surveys and a New Telescope for CHASE by Francisco Förster, Nicolás López, José Maza, Petr Kubánek, G. Pignata

“…In particular, we present example schedules designed for a future 50 cm telescope that will expand the capabilities of the CHASE survey, which aims to detect young supernova events in nearby galaxies. We also include a brief description of the telescope and the status of the project, which is expected to enter a commissioning phase in 2010.…”
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Pulsar Scattering as a Probe for Structures in the Interstellar Medium by Qiuyi He, Xun Shi, Guangxing Li

“…By comparing this smooth distribution with observational data, we identify two ISM structures responsible for pulsar scattering, one is associated with the Vela supernova remnant region within the Gum Nebula, while the other is a newly discovered structure—a distant superbubble, G38, located at a distance of 2.3 kpc with a size of ~50 pc. …”
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Total Oil Content and Fatty Acid Profile of some Almond (Amygdalus Communis L.) Cultivars by Yildirim Adnan Nurhan, Akinci-Yildirim Fatma, Şan Bekir, Sesli Yılmaz

“…Total oil contents were changed from 50.90% (Picantili) to 62.01% (Supernova) in 2008 and from 52.44% (Lauranne) to 63.18% (Cristomorto) in 2009. …”
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Kinematics of Young Stellar Objects under Various Stellar Feedback by Longhui Yang, Dejian Liu, Chaojie Hao, Zehao Lin, YingJie Li, Yiwei Dong, Zu-Jia Lu, En-Wei Liang, Y. Xu

“…In feedback environments dominated by outflows, massive stars, and supernova feedback, the corresponding velocity differences range from [0, 1.4], [0.1, 0.4], and [0.1, 1] km s ^−1 , respectively. …”
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Pulse-profile Modeling and Spin–Orbit Alignment in a Suzaku Sample of Accreting X-Ray Binary Pulsars by Silas G. T. Laycock, Rigel C. Cappallo, Pragati Pradhan, Dimitris M. Christodoulou, Biswajit Paul

“…The implications of our study are as follows: (a) apparently, accretion torques have had time to erase spin–orbit misalignment caused by supernova kicks in two-thirds of the systems; (b) many X-ray binary pulsars have dominant dipolar surface magnetic fields, in contrast to the recently reported exotic configurations in millisecond pulsars; and (c) if the binary inclinations can be determined by pulse-profile modeling, even for a subset of the ∼200 known X-ray binary pulsars, most of which orbital inclinations are as yet poorly constrained, it raises the prospect of tightening dramatically ongoing neutron-star mass determinations. …”
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Stability of compact stars in a uniform density background cloud by Ksh. Newton Singh, S. K. Maurya, A. Errehymy, O. Donmez, K. Myrzakulov, T. T. Smitha

“…Abstract We are discussing a scenario where a compact star (neutron star, NS) is embedded in a thin, uniform density background cloud (a remnant cloud after a supernova or a cloud generated from the late stages of a star e.g., a planetary nebula or asymptotic red giant phases) and its effect on the stability of the compact star. …”
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Quantifying Baryonic Feedback on the Warm–Hot Circumgalactic Medium in CAMELS Simulations by Isabel Medlock, Chloe Neufeld, Daisuke Nagai, Daniel Anglés-Alcázar, Shy Genel, Benjamin D. Oppenheimer, Xavier Sims, Priyanka Singh, Francisco Villaescusa-Navarro

“…Additionally, the AGN feedback efficiency parameters affect the CGM gas fraction at low halo masses in SIMBA, hinting at complex, nonlinear interactions between the AGN and supernova feedback modes. Overall, we demonstrate that stellar and AGN feedback are intimately interwoven, especially at low redshift, due to subgrid implementation, resulting in halo property effects that might initially seem counterintuitive.…”
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Newest Measurements of Hubble Constant from DESI 2024 Baryon Acoustic Oscillation Observations by Wuzheng Guo, Qiumin Wang, Shuo Cao, Marek Biesiada, Tonghua Liu, Yujie Lian, Xinyue Jiang, Chengsheng Mu, Dadian Cheng

“…This result is still in a 4.3 σ tension with the results of the Supernova H0 for the Equation of State.…”
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Diffuse Ionized Gas in the Anticenter of the Milky Way by Shiming Wen, Wei Zhang, Lin Ma, Yunning Zhao, Man I. Lam, Chaojian Wu, Juanjuan Ren, Jianjun Chen, Yuzhong Wu, Guozhen Hu, Yonghui Hou, Yongheng Zhao, Hong Wu

“…Using data from the Large Area Multi-Object fiber Spectroscopic Telescope Medium-Resolution Spectroscopic Survey of Nebulae, we create a sample of 17,821 diffuse ionized gas spectra in the anticenter region of the Milky Way by excluding fibers in the directions of H ii regions and supernova remnants. We then analyze the radial and vertical distributions of three line ratios ([N ii ]/H α , [S ii ]/H α , and [S ii ]/[N ii ]), as well as the oxygen abundance. …”
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