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Journal articles on the topic 'Monk detectives'

Author: Grafiati

Published: 4 June 2021

Last updated: 27 July 2025

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1

Jones, J. W. "Gay Detectives and Victims in German Mystery Novels." Monatshefte 104, no. 4 (2012): 570–92. http://dx.doi.org/10.1353/mon.2012.0102.

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Rosenstock, M. "Ernst Junger's Dangerous Encounter--the Detective Closes the Case on the Adventurer." Monatshefte 100, no. 3 (2008): 383–99. http://dx.doi.org/10.1353/mon.0.0053.

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3

Marinko, Vesna. "Gothic elements in contemporary detective story : Matthew Gregory Lewis and Minette Walters compared." Acta Neophilologica 42, no. 1-2 (2009): 35–43. http://dx.doi.org/10.4312/an.42.1-2.35-43.

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One of the most shocking Gothic novels was written by Matthew Gregory Lewis in 1796. His Gothic novel The Monk contains all the typical Gothic elements such as a ruined castle, aggressive villain, women in distress, the atmosphere of terror and horror and a lot more. This article analyses and compares to what extent the Gothic elements of the late 18th century survived in the contemporary detective story The Ice House (1993) written by Minette Walters and how these elements have changed.

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Perron-Cormier, Mathieu, Nathan Deg, Kristine Spekkens, et al. "WALLABY Pilot Survey and ASymba: Comparing H i Detection Asymmetries to the SIMBA Simulation." Astronomical Journal 169, no. 2 (2025): 114. https://doi.org/10.3847/1538-3881/ada567.

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Abstract An avenue for understanding cosmological galaxy formation is to compare morphometric parameters in observations and simulations of galaxy assembly. In this second paper of the ASymba: Asymmetries of H i in SIMBA Galaxies series, we measure atomic gas (H i) asymmetries in spatially resolved detections from the untargeted Widefield ASKAP L-band Legacy All-sky Blind surveY (WALLABY) survey, and compare them to realizations of WALLABY-like mock samples from the SIMBA cosmological simulations. We develop a Scanline Tracing method to create mock galaxy H i data cubes that minimizes shot noi

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Honca, Ciprian-Emanuel. "From “Patriot” to “Country Traitor”. The Espionage Accusation Brought to Monk Árkád Pásztory. Part I: The Reports of Detective Ede Sperling." Journal of Church History 2020, no. 1 (2020): 41–60. http://dx.doi.org/10.24193/jch.2020.1.3.

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Abstract: This study is an attempt for clarifying a less known episode in the life of the Brazilian Monk Árkád Pásztory, i.e. the motives and circumstances under which he became a suspect of country treason during the First World War. Thus, in this article we present a first part of a long events series of the trial whose documents have been kept in Budapest, at the National Archives of Hungary.

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Al-Aghberi, Munir Ahmed, and Hussein Saleh Ali Albahji. "Antiheroes in Mock-heroic Battles: Post 9/11 Alternatives in Jess Walter’s Novel The Zero." International Journal of Language and Literary Studies 5, no. 2 (2023): 24–36. http://dx.doi.org/10.36892/ijlls.v5i2.1268.

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Placing Jess Walter's The Zero within a post 9/11 counter discourse, the present study examines the novel as a modern mock-heroic fictional work. The novel is critically analyzed as a parody of both the detective fiction genre as well as the early post 9/11 fiction adopting the American official narrative. The argument proceeds through three sub-headings. The first part queries the novel's representation of antiheroism in response to the discourse of heroism prevalent in American culture. The second part ponders on the mock-heroic battles and situations taking place as part of the US war again

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An, Diya, Shui Yu, Tingting Jiang, Jianhui Zhang, Qun Liu, and Jing Liu. "Epidemiology and Molecular Characterization of Entamoeba spp. in Non-Human Primates in Zoos in China." Veterinary Sciences 11, no. 12 (2024): 590. http://dx.doi.org/10.3390/vetsci11120590.

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The genus Entamoeba infects both humans and NHPs. In zoos, visitors feeding significantly increases the frequency of human-to-NHP contact, thereby raising the risk of zoonotic transmission. In this study, six Entamoeba species were investigated and analyzed in the fecal samples of 14 NHP species from zoos in Beijing, Guiyang, Shijiazhuang, Tangshan, and Xingtai in China. A total of 19 out of 84 primate fecal samples tested positive for Entamoeba spp. by polymerase chain reaction (PCR). Among these, 14 samples contained mono-detections of E. coli (7/84), E. dispar (4/84), and E. polecki (3/84).

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Coudert, L. H., L. Margulès, C. Vastel, R. Motiyenko, E. Caux, and J. C. Guillemin. "Astrophysical detections and databases for the mono deuterated species of acetaldehyde CH2DCOH and CH3COD." Astronomy & Astrophysics 624 (April 2019): A70. http://dx.doi.org/10.1051/0004-6361/201834827.

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Context. Detection of deuterated species may provide information on the evolving chemistry in the earliest phases of star-forming regions. For molecules with two isomeric forms of the same isotopic variant, gas-phase and solid-state formation pathways can be differentiated using their abundance ratio. Aims. Spectroscopic databases for astrophysical purposes are built for the two mono deuterated isomeric species CH2DCOH and CH3COD of the complex organic molecule acetaldehyde. These databases can be used to search and detect these two species in astrophysical surveys, retrieving their column den

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Freundlich, Jonathan, Benoit Famaey, Pierre-Antoine Oria, Michal Bílek, Oliver Müller, and Rodrigo Ibata. "Probing the radial acceleration relation and the strong equivalence principle with the Coma cluster ultra-diffuse galaxies." Astronomy & Astrophysics 658 (January 27, 2022): A26. http://dx.doi.org/10.1051/0004-6361/202142060.

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The tight radial acceleration relation (RAR) obeyed by rotationally supported disk galaxies is one of the most successful a priori predictions of the modified Newtonian dynamics (MOND) paradigm on galaxy scales. Another important consequence of MOND as a classical modification of gravity is that the strong equivalence principle (SEP) – which requires the dynamics of a small, free-falling, self-gravitating system not to depend on the external gravitational field in which it is embedded – should be broken. Multiple tentative detections of this so-called external field effect (EFE) of MOND have b

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Vasylenko, Vadym. "MODERNIZATION OF THE EPIC. UNFINISHED NOVELS AND STORIES BY IHOR KOSTETSKYI: GENRE, STYLE, AND STRUCTURE." Слово і Час, no. 6 (December 21, 2024): 42–60. https://doi.org/10.33608/0236-1477.2024.06.42-60.

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The paper analyzes several works of Ihor Kostetsky’s experimental prose, in particular his unfinished novels “The Three Look in the Mirror” and “There Are No More Dead,” as well as the stories “Saint’s Day” and “The Story of Monk Heinrich,” focusing on genre, style, literary technique, and ideas. There is a noticeable connection between the writer’s literary practices and the achievements of 1920s Ukrainian literature, especially the work of avant-garde writers, whose technical inventions Kostetsky developed while focusing on the latest trends in postwar writing. Exploring themes related to th

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Cavaglià, Marco, and Ashini Modi. "Two-Dimensional Correlation Function of Binary Black Hole Coalescences." Universe 6, no. 7 (2020): 93. http://dx.doi.org/10.3390/universe6070093.

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We compute the two-dimensional correlation functions of the binary black hole coalescence detections in LIGO-Virgo’s first and second observation runs. The sky distribution of binary black hole coalescence events is tested for correlations at different angular scales by comparing the observed correlation function to two reference functions that are obtained from mock datasets of localization error regions uniformly distributed in the sky. No excess correlation at any angular scale is found. The power-law slope of the correlation function is estimated to be γ = 2.24 ± 0.33 at the three- σ confi

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Agrawal, Shiva, Savankumar Bhanderi, and Gordon Elger. "Infra-3DRC-FusionNet: Deep Fusion of Roadside Mounted RGB Mono Camera and Three-Dimensional Automotive Radar for Traffic User Detection." Sensors 25, no. 11 (2025): 3422. https://doi.org/10.3390/s25113422.

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Mono RGB cameras and automotive radar sensors provide a complementary information set that makes them excellent candidates for sensor data fusion to obtain robust traffic user detection. This has been widely used in the vehicle domain and recently introduced in roadside-mounted smart infrastructure-based road user detection. However, the performance of the most commonly used late fusion methods often degrades when the camera fails to detect road users in adverse environmental conditions. The solution is to fuse the data using deep neural networks at the early stage of the fusion pipeline to us

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Kovacs, Geza. "Transit-period search from single-event space-based data: the role of wide-field surveys." Astronomy & Astrophysics 625 (May 2019): A145. http://dx.doi.org/10.1051/0004-6361/201935349.

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We investigate the optimization of dataset weighting in searching for the orbital period of transiting planets when high-precision space-based data with a single transit event are combined with (relatively) low-precision ground-based (wide-field) data. The optimization stems from the lack of multiple events in the high-precision data and the likely presence of such events in the low-precision data. With noise minimization, we combined two types of frequency spectra: (i) spectra that use two fixed transit parameters (moment of the center of the transit and duration of the event) derived from th

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Porth, Lucas, and Robert E. Smith. "Fast estimation of aperture-mass statistics – II. Detectability of higher order statistics in current and future surveys." Monthly Notices of the Royal Astronomical Society 508, no. 3 (2021): 3474–94. http://dx.doi.org/10.1093/mnras/stab2819.

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ABSTRACT We explore an alternative method to the usual shear correlation function approach for the estimation of aperture mass statistics in weak-lensing survey data. Our approach builds on the direct estimator method. In this paper, we extend our analysis to statistics of arbitrary order and to the multiscale aperture mass statistics. We show that there always exists a linear order algorithm to retrieve any of these generalized aperture mass statistics from shape catalogues when the direct estimator approach is adopted. We validate our approach through application to a large number of Gaussia

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Marshall, Madeline A., J. Stuart B. Wyithe, Rogier A. Windhorst, et al. "Observing the host galaxies of high-redshift quasars with JWST: predictions from the BlueTides simulation." Monthly Notices of the Royal Astronomical Society 506, no. 1 (2021): 1209–28. http://dx.doi.org/10.1093/mnras/stab1763.

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ABSTRACT The bright emission from high-redshift quasars completely conceals their host galaxies in the rest-frame ultraviolet/optical, with detection of the hosts in these wavelengths eluding even the Hubble Space Telescope (HST) using detailed point spread function (PSF) modelling techniques. In this study, we produce mock images of a sample of z = 7 quasars extracted from the BlueTides simulation, and apply Markov chain Monte Carlo-based PSF modelling to determine the detectability of their host galaxies with the James Webb Space Telescope (JWST). While no statistically significant detection

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Broussard, Adam, Eric Gawiser, and Kartheik Iyer. "Improved Measurements of Galaxy Star Formation Stochasticity from the Intrinsic Scatter of Burst Indicators." Astrophysical Journal 939, no. 1 (2022): 35. http://dx.doi.org/10.3847/1538-4357/ac94c2.

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Abstract Measurements of short-timescale star formation variations (i.e., “burstiness” or star formation stochasticity) are integral to our understanding of star formation feedback mechanisms and the assembly of stellar populations in galaxies. We expand upon the work of Broussard et al. by introducing a new analysis of galaxy star formation burstiness that accounts for variations in the Q sg = E B − V stars / E B − V gas distribution, a major confounding factor. We use Balmer decrements from the MOSFIRE Deep Evolution Field (MOSDEF) survey to measure Q sg , which we use to construct mock cata

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Zywert, Aleksandra. "Pomiędzy Sherlockiem Holmesem a Eberhardem Mockiem: Hotel „Wielkie Prusy” Bohdana Kołomijczuka." Studia Ukrainica Posnaniensia 10, no. 2 (2022): 97–114. http://dx.doi.org/10.14746/sup.2022.10.2.7.

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The subject of the analysis in this paper is the novel by Bohdan Kolomiichuk entitled The Great Prussia Hotel. From the genre point of view, the piece fits seamlessly into the so-called retro detective story with elements of the noir novel. The author’s variant of the retro detective story is clearly inspired by the classics of the genre, such as Artur Conan Doyle or Agata Christie (also contemporary ones, already containing further original modifications, such as Marek Krajewski or Konrad Lewandowski). This translates, for example, into the construction of the main character. Thus, a hybrid c

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Hotchkiss, S., S. Nadathur, S. Gottlöber, et al. "The ISW imprints of voids and superclusters on the CMB." Proceedings of the International Astronomical Union 11, S308 (2014): 580–84. http://dx.doi.org/10.1017/s1743921316010619.

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AbstractWe examine the stacked integrated Sachs-Wolfe (ISW) imprints on the CMB along the lines of sight of voids and superclusters in galaxy surveys, using the Jubilee ISW simulation and mock luminous red galaxy (LRG) catalogues. We show that the expected signal in the concordance \Lam CDM model is much smaller than the primary anisotropies arising at the last scattering surface and therefore any currently claimed detections of such an imprint cannot be caused by the ISW effect in \Lam CDM. We look for the existence of such a signal in the Planck CMB using a catalogue of voids and supercluste

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19

Kang, Yacheng, Chang Liu, and Lijing Shao. "Prospects for Detecting Exoplanets around Double White Dwarfs with LISA and Taiji." Astronomical Journal 162, no. 6 (2021): 247. http://dx.doi.org/10.3847/1538-3881/ac23d8.

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Abstract Recently, Tamanini & Danielski discussed the possibility of detecting circumbinary exoplanets (CBPs) orbiting double white dwarfs (DWDs) with the Laser Interferometer Space Antenna (LISA). Extending their methods and criteria, we discuss the prospects for detecting exoplanets around DWDs not only by LISA, but also by Taiji, a Chinese space-borne gravitational-wave (GW) mission that has slightly better sensitivity at low frequencies. We first explore how different binary masses and mass ratios affect the abilities of LISA and Taiji to detect CBPs. Second, for certain known detached

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20

IWAI, T., C. W. HONG, and P. GREIL. "FAST PARTICLE PAIR DETECTION ALGORITHMS FOR PARTICLE SIMULATIONS." International Journal of Modern Physics C 10, no. 05 (1999): 823–37. http://dx.doi.org/10.1142/s0129183199000644.

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New algorithms with O(N) complexity have been developed for fast particle-pair detections in particle simulations like the discrete element method (DEM) and molecular dynamic (MD). They exhibit robustness against broad particle size distributions when compared with conventional boxing methods. Almost similar calculation speeds are achieved at particle size distributions from is mono-size to 1:10 while the linked-cell method results in calculations more than 20 times. The basic algorithm, level-boxing, uses the variable search range according to each particle. The advanced method, multi-level b

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Cai, Rong-Gen, and Tao Yang. "Space-borne atom interferometric gravitational wave detections. Part I. The forecast of bright sirens on cosmology." Journal of Cosmology and Astroparticle Physics 2021, no. 12 (2021): 017. http://dx.doi.org/10.1088/1475-7516/2021/12/017.

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Abstract Atom interferometers (AIs) as gravitational-wave (GW) detectors have been proposed a decade ago. Both ground and space-based projects will be in construction and preparation in the near future. In this paper, for the first time, we investigate the potential of the space-borne AIs on detecting GW standard sirens and hence the applications on cosmology. We consider AEDGE as our fiducial AI GW detector and estimate the number of bright sirens that would be obtained within a 5-years data-taking period of GW and with the follow-up observation of electromagnetic (EM) counterparts. We then c

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Zhu 朱, Liang-Gui 良贵, Hui-Min 会敏 Fan 范, Xian 弦. Chen 陈, Yi-Ming 一鸣 Hu 胡, and Jian-dong 建东 Zhang 张. "Improving Cosmological Constraints by Inferring the Formation Channel of Extreme-mass-ratio Inspirals." Astrophysical Journal Supplement Series 273, no. 2 (2024): 24. http://dx.doi.org/10.3847/1538-4365/ad5446.

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Abstract Extreme-mass-ratio inspirals (EMRIs) could be detected by space-borne gravitational-wave (GW) detectors, such as the Laser Interferometer Space Antenna (LISA), TianQin, and Taiji. Localizing EMRIs by GW detectors can help us select candidate host galaxies, which can be used to infer the cosmic expansion history. In this paper, we demonstrate that the localization information can also be used to infer the formation channel of EMRIs, and can hence allow us to extract more precisely the redshift probability distributions. By conducting mock observations of the EMRIs that can be detected

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Davies, James E., Rupert A. C. Croft, Tiziana Di-Matteo, Bradley Greig, Yu Feng, and J. Stuart B. Wyithe. "Stacking redshifted 21 cm images of H ii regions around high-redshift galaxies as a probe of early reionization." Monthly Notices of the Royal Astronomical Society 501, no. 1 (2020): 146–56. http://dx.doi.org/10.1093/mnras/staa3531.

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ABSTRACT A number of current and future experiments aim to detect the reionization of neutral hydrogen by the first stars and galaxies in the Universe via the redshifted 21 cm line. Using the bluetides simulation, we investigate the measurement of an average ionized region towards the beginning of reionization by stacking redshifted 21 cm images around optically identified bright galaxies using mock observations. We find that with an SKA 1000 h observation, assuming perfect foreground subtraction, a 5σ detection of a stacked H ii region can be made with 30 images around some of the brightest g

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Hou, Wan-Ting, Jing-Zhao Qi, Tao Han, Jing-Fei Zhang, Shuo Cao, and Xin Zhang. "Prospects for constraining interacting dark energy models from gravitational wave and gamma ray burst joint observation." Journal of Cosmology and Astroparticle Physics 2023, no. 05 (2023): 017. http://dx.doi.org/10.1088/1475-7516/2023/05/017.

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Abstract With the measurement of the electromagnetic (EM) counterpart, a gravitational wave (GW) event could be treated as a standard siren. As a novel cosmological probe, GW standard sirens will bring significant implications for cosmology. In this paper, by considering the coincident detections of GW and associated γ ray burst (GRB), we find that only about 400 GW bright standard sirens from binary neutron star mergers could be detected in a 10-year observation of the Einstein Telescope and the THESEUS satellite mission. Based on this mock sample, we investigate the implications of GW standa

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25

Știubianu, Mihaela. "Ipostaze balcanice în proza lui Ioan Groșan: înțelepții rătăcitori." Comunicare interculturală și literatură 29, no. 2 (2024): 108–10. https://doi.org/10.35219/cil.2022.2.15.

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The present analysis has as a starting point the existence of human models representative of literary Balkanism, thus theorized by Mircea Muthu: the tragic type, the wandering sage, the outlaw and the upstart. The type of the wandering sage is illustrated, among others, in Ioan Groșan's novel, "One Hundred Years at the Gates of the Orient", a representative work for the 1980’s prose. Groșan's work, published in 1992, has the merit of anticipating - mutatis mutandis - Umberto Eco's novel, "The Mysterious Flame of Queen Loana" (published in 2004), the common element being the game of intertextua

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Cozzumbo, Andrea, Ulyana Dupletsa, Rodrigo Calderón, Riccardo Murgia, Gor Oganesyan та Marica Branchesi. "Model-independent cosmology with joint observations of gravitational waves and γ-ray bursts". Journal of Cosmology and Astroparticle Physics 2025, № 05 (2025): 021. https://doi.org/10.1088/1475-7516/2025/05/021.

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Abstract Multi-messenger (MM) observations of binary neutron star (BNS) mergers provide a promising approach to trace the distance-redshift relation, crucial for understanding the expansion history of the Universe and, consequently, testing the nature of Dark Energy (DE). While the gravitational wave (GW) signal offers a direct measure of the distance to the source, high-energy observatories can detect the electromagnetic counterpart and drive the optical follow-up providing the redshift of the host galaxy. In this work, we exploit up-to-date catalogs of γ-ray bursts (GRBs) supposedly coming f

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Kodi Ramanah, Doogesh, Nikki Arendse, and Radosław Wojtak. "AI-driven spatio-temporal engine for finding gravitationally lensed type Ia supernovae." Monthly Notices of the Royal Astronomical Society 512, no. 4 (2022): 5404–17. http://dx.doi.org/10.1093/mnras/stac838.

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ABSTRACT We present a spatio-temporal AI framework that concurrently exploits both the spatial and time-variable features of gravitationally lensed supernovae in optical images to ultimately aid in future discoveries of such exotic transients in wide-field surveys. Our spatio-temporal engine is designed using recurrent convolutional layers, while drawing from recent advances in variational inference to quantify approximate Bayesian uncertainties via a confidence score. Using simulated Young Supernova Experiment (YSE) images of lensed and non-lensed supernovae as a showcase, we find that the us

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Huang, Liang Xian, Qiu Feng An, Jing Men, and Qian Jin Wang. "Film Morphology and Film-Forming Ability of Supramolecular Compound Self-Assembled with Amino Polysiloxane Emulsion and Carboxyl Polysiloxane Emulsion." Advanced Materials Research 503-504 (April 2012): 358–62. http://dx.doi.org/10.4028/www.scientific.net/amr.503-504.358.

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Using cation amino polysiloxane emulsion(ASE) and anion carboxyl polysiloxane emulsion (CSE) as materials, mixing ASE and CSE together to self-assemble or aggregate by electrostatic interaction, supramolecular compound emulsion (ASE-CSE) was formed. TEM and particle size analyzer observation showed that the particle of ASE-CSE is sphericity, and its particle diameter is bigger than that of mono-composition emulsion and has single-peak distribution. SEM, atomic force microscope (AFM) and other instruments detections indicated that the ASE-CSE possesses good form-film property. The ASE-CSE film

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Rusta, Elka, Stefania Salvadori, Viola Gelli, Ioanna Koutsouridou, and Alessandro Marconi. "Linking High-z and Low-z: Are We Observing the Progenitors of the Milky Way with JWST?" Astrophysical Journal Letters 974, no. 2 (2024): L35. http://dx.doi.org/10.3847/2041-8213/ad833d.

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Abstract The recent JWST observation of the Firefly Sparkle at z = 8.3 offers a unique opportunity to link the high- and the low-z Universe. Indeed, the claim of it being a Milky Way (MW) type of assembly at the cosmic dawn opens the possibility of interpreting the observation with locally calibrated galaxy-formation models. Here, we use the a state-of-the-art MW-evolution model to perform forward modeling of our Galaxy's progenitors at high-z. We build a set of mock spectra for the MW building blocks to make predictions for JWST and to interpret the Firefly Sparkle observation. First, we find

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Hung, D., B. C. Lemaux, R. R. Gal, et al. "Establishing a new technique for discovering large-scale structure using the ORELSE survey." Monthly Notices of the Royal Astronomical Society 491, no. 4 (2019): 5524–54. http://dx.doi.org/10.1093/mnras/stz3164.

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ABSTRACT The Observations of Redshift Evolution in Large-Scale Environments (ORELSE) survey is an ongoing imaging and spectroscopic campaign initially designed to study the effects of environment on galaxy evolution in high-redshift (z ∼ 1) large-scale structures. We use its rich data in combination with a powerful new technique, Voronoi tessellation Monte Carlo (VMC) mapping, to search for serendipitous galaxy overdensities at 0.55 &lt; z &lt; 1.37 within 15 ORELSE fields, a combined spectroscopic footprint of ∼1.4 deg2. Through extensive tests with both observational data and our own

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Hanel, A., A. Mitschke, R. Boerner, et al. "METRIC SCALE CALCULATION FOR VISUAL MAPPING ALGORITHMS." ISPRS - International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences XLII-2 (May 30, 2018): 433–40. http://dx.doi.org/10.5194/isprs-archives-xlii-2-433-2018.

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Visual SLAM algorithms allow localizing the camera by mapping its environment by a point cloud based on visual cues. To obtain the camera locations in a metric coordinate system, the metric scale of the point cloud has to be known. This contribution describes a method to calculate the metric scale for a point cloud of an indoor environment, like a parking garage, by fusing multiple individual scale values. The individual scale values are calculated from structures and objects with a-priori known metric extension, which can be identified in the unscaled point cloud. Extensions of building struc

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Macher, Till-Hendrik, Robin Schütz, Atakan Yildiz, Arne J. Beermann, and Florian Leese. "Evaluating five primer pairs for environmental DNA metabarcoding of Central European fish species based on mock communities." Metabarcoding and Metagenomics 7 (September 5, 2023): e103856. https://doi.org/10.3897/mbmg.7.103856.

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Environmental DNA (eDNA) metabarcoding has become a powerful tool for examining fish communities. Prior to the introduction of eDNA-based assessments into regulatory monitoring contexts (e.g., EU Water Framework Directive), there is a demand for methodological standardization. To ensure methodical accuracy and to meet regulatory standards, various sampling, laboratory and bioinformatic workflows have been established. However, a crucial prerequisite for comprehensive fish monitoring is the choice of suitable primer pairs to accurately identify the fishes present in a given water body. Various

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McGregor, Kyle, and Duncan R. Lorimer. "Modeling Current and Future High-cadence Surveys of Repeating Fast Radio Burst Populations." Astrophysical Journal 961, no. 1 (2024): 10. http://dx.doi.org/10.3847/1538-4357/ad1184.

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Abstract In recent years, the Canadian Hydrogen Intensity Mapping Experiment (CHIME) interferometer has revealed a large number of fast radio bursts (FRBs), including a sizable population that demonstrates repeating behavior. This transit facility, employing a real-time FRB search pipeline, continually scans the sky with declinations between −10° and 90° for events with fluences ⪆0.4 Jy ms. We simulate a population of repeating FRBs by performing Monte Carlo simulations of underlying source populations processed through a mock CHIME/FRB observing pipeline. Assuming intrinsic repeater rates fol

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Li, Yin-Jie, Shao-Peng Tang, Yuan-Zhu Wang, et al. "Population Properties of Neutron Stars in the Coalescing Compact Binaries." Astrophysical Journal 923, no. 1 (2021): 97. http://dx.doi.org/10.3847/1538-4357/ac34f0.

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Abstract We perform a hierarchical Bayesian inference to investigate the population properties of the coalescing compact binaries involving at least one neutron star (NS). With the current gravitational-wave (GW) observation data, we can rule out none of the double Gaussian, single Gaussian, and uniform NS mass distribution models, though a specific double Gaussian model inferred from the Galactic NSs is found to be slightly more preferred. The mass distribution of black holes (BHs) in the neutron star–black hole (NSBH) population is found to be similar to that in the Galactic X-ray binaries.

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Amorisco, Nicola C., James Nightingale, Qiuhan He, et al. "Halo concentration strengthens dark matter constraints in galaxy–galaxy strong lensing analyses." Monthly Notices of the Royal Astronomical Society 510, no. 2 (2021): 2464–79. http://dx.doi.org/10.1093/mnras/stab3527.

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ABSTRACT A defining prediction of the cold dark matter cosmological model is the existence of a very large population of low-mass haloes. This population is absent in models in which the dark matter particle is warm (WDM). These alternatives can, in principle, be distinguished observationally because haloes along the line of sight can perturb galaxy–galaxy strong gravitational lenses. Furthermore, the WDM particle mass could be deduced because the cut-off in their halo mass function depends on the mass of the particle. We systematically explore the detectability of low-mass haloes in WDM model

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Szulágyi, J., and A. Garufi. "Observability of forming planets and their circumplanetary discs – III. Polarized scattered light in near-infrared." Monthly Notices of the Royal Astronomical Society 506, no. 1 (2021): 73–83. http://dx.doi.org/10.1093/mnras/stab1723.

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ABSTRACT There is growing amount of very high resolution polarized scattered light images of circumstellar discs. Nascent giant planets are surrounded by their own circumplanetary discs that may scatter and polarize both the planetary and stellar light. Here, we investigate whether we could detect circumplanetary discs with the same technique and what can we learn from such detections. Here, we created scattered light mock observations at 1.245 microns (J band) for instruments like SPHERE and GPI, for various planetary masses (0.3, 1.0, 5.0, and 10.0 $\rm {\mathrm{ M}_{Jup}}$), disc inclinatio

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Hu, Qian, and John Veitch. "Accumulating Errors in Tests of General Relativity with Gravitational Waves: Overlapping Signals and Inaccurate Waveforms." Astrophysical Journal 945, no. 2 (2023): 103. http://dx.doi.org/10.3847/1538-4357/acbc18.

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Abstract Observations of gravitational waves (GWs) from compact binary coalescences provide powerful tests of general relativity (GR), but systematic errors in data analysis could lead to incorrect scientific conclusions. This issue is especially serious in the third-generation GW detectors in which the signal-to-noise ratio (S/N) is high and the number of detections is large. In this work, we investigate the impacts of overlapping signals and inaccurate waveform models on tests of GR. We simulate mock catalogs for Einstein Telescope and Cosmic Explorer and perform parametric tests of GR using

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Serrana, Joeselle, and Kozo Watanabe. "Haplotype-level DNA metabarcoding from freshwater macroinvertebrate community samples." ARPHA Conference Abstracts 4 (March 4, 2021): e64738. https://doi.org/10.3897/aca.4.e64738.

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DNA metabarcoding is a robust method for environmental impact assessments of freshwater ecosystems that enables the simultaneous multi-species identification of complex mixed community samples from different origins using extracellular and total genomic DNA. The development and evaluation of DNA metabarcoding protocols for haplotype level resolution require attention, specifically for basic population genetic applications, i.e., analysis to allow genetic diversity estimations and dispersal abilities of the species present in the bulk community samples. Various literature has proposed using DNA

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Sesana, Alberto, Astrid Lamberts, and Antoine Petiteau. "Finding binary black holes in the Milky Way with LISA." Monthly Notices of the Royal Astronomical Society: Letters 494, no. 1 (2020): L75—L80. http://dx.doi.org/10.1093/mnrasl/slaa039.

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ABSTRACT We determine the main properties of the Galactic binary black hole (BBH) population detectable by Laser Interferometer Space Antenna (LISA) and strategies to distinguish them from the much more numerous white dwarf binaries. We simulate BBH populations based on cosmological simulations of Milky Way-like galaxies and binary evolution models. We then determine their gravitational wave emission as observed by LISA and build mock catalogues. According to our model, LISA will detect ≈4 (6) BBHs assuming 4 (10) yr of operations. Those figures grow to ≈6 (9) when models are re-normalized to

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Despali, Giulia, Mark Lovell, Simona Vegetti, Robert A. Crain, and Benjamin D. Oppenheimer. "The lensing properties of subhaloes in massive elliptical galaxies in sterile neutrino cosmologies." Monthly Notices of the Royal Astronomical Society 491, no. 1 (2019): 1295–310. http://dx.doi.org/10.1093/mnras/stz3068.

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ABSTRACT We use high-resolution hydrodynamical simulations run with the EAGLE model of galaxy formation to study the differences between the properties of – and subsequently the lensing signal from – subhaloes of massive elliptical galaxies at redshift 0.2, in Cold and Sterile Neutrino (SN) Dark Matter models. We focus on the two 7 keV SN models that bracket the range of matter power spectra compatible with resonantly produced SN as the source of the observed 3.5 keV line. We derive an accurate parametrization for the subhalo mass function in these two SN models relative to cold dark matter (C

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Merryfield, Marcus, Shriharsh P. Tendulkar, Kaitlyn Shin, et al. "An Injection System for the CHIME/FRB Experiment." Astronomical Journal 165, no. 4 (2023): 152. http://dx.doi.org/10.3847/1538-3881/ac9ab5.

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Abstract Dedicated surveys searching for fast radio bursts (FRBs) are subject to selection effects that bias the observed population of events. Software injection systems are one method of correcting for these biases by injecting a mock population of synthetic FRBs directly into the real-time search pipeline. The injected population may then be used to map intrinsic burst properties onto an expected signal-to-noise ratio (S/N), so long as telescope characteristics such as the beam model and calibration factors are properly accounted for. This paper presents an injection system developed for th

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Thongkham, Khunanon, Anthony H. Gonzalez, Mark Brodwin, et al. "The Massive and Distant Clusters of WISE Survey 2: Second Data Release." Astrophysical Journal 976, no. 2 (2024): 186. http://dx.doi.org/10.3847/1538-4357/ad888c.

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Abstract We present the second data release of the Massive and Distant Clusters of WISE Survey 2 (MaDCoWS2). We expand from the equatorial first data release to most of the Dark Energy Camera Legacy Survey area, covering a total area of 6498 deg2. The catalog consists of 133,036 signal-to-noise ratio (S/N) ≥ 5 galaxy cluster candidates at 0.1 ≤ z ≤ 2, including 6790 candidates at z > 1.5. We train a convolutional neural network (CNN) to identify spurious detections and include CNN-based cluster probabilities in the final catalog. We also compare the MaDCoWS2 sample with literature catalogs

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Kalashnikova, V. A., T. P. Egorova, A. V. Demerchyan, et al. "Gut microbiota and bacterial associations in monkeys with gastrointestinal diseases in the setting of helminth infestation." Veterinary Science Today 13, no. 2 (2024): 154–63. http://dx.doi.org/10.29326/2304-196x-2024-13-2-154-163.

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One of the topical issues of current primatology is spontaneous pathology in monkeys, primarily gastrointestinal infections, which are the leading ones in the morbidity and mortality patterns of the animals raised in captivity. Gastrointestinal pathology in monkeys involves complicated infectious processes, most often of associative type, with the formation of various bacterial and parasitic associations. The study demonstrates the results of gastrointestinal disease and helminth infestation monitoring as well as of the microbial flora spectrum analysis in monkeys in 2017–2022. Mortality of mo

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Adam, R., M. Vannier, S. Maurogordato, et al. "Euclid preparation." Astronomy & Astrophysics 627 (June 26, 2019): A23. http://dx.doi.org/10.1051/0004-6361/201935088.

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Galaxy cluster counts in bins of mass and redshift have been shown to be a competitive probe to test cosmological models. This method requires an efficient blind detection of clusters from surveys with a well-known selection function and robust mass estimates, which is particularly challenging at high redshift. The Euclid wide survey will cover 15 000 deg2 of the sky, avoiding contamination by light from our Galaxy and our solar system in the optical and near-infrared bands, down to magnitude 24 in the H-band. The resulting data will make it possible to detect a large number of galaxy clusters

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Yoshida, Shohei, Keisuke Okamoto, Tomoyuki Kurioka, et al. "Catalytic Activity of Atomic Metals Clusters Decorated Polyaniline Electrodes in Electrochemical Oxidation of 1-Propanol." ECS Meeting Abstracts MA2023-02, no. 52 (2023): 2493. http://dx.doi.org/10.1149/ma2023-02522493mtgabs.

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Electrochemical sensors are capable to fast-detect chemicals with a high sensitivity at a low cost. Thanks to these advantages, electrochemical sensors are promising for detections of biomolecules, such as glucose, dopamine, uric acid, etc. The catalytic electrode in a electrochemical sensor is composed of noble noble metals, such as Au and Pd,and a suppoorting material. Polyaniline (PANI)[ 1]is an ideal supporting material for noble metal clusters because of its good electrical conductivity, high stability, large active surface area, and simple preparation process. Recently, PANI decorated wi

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Snyder, Matthew R., and Carol A. Stepien. "Increasing confidence for discerning species and population compositions from metabarcoding assays of environmental samples: case studies of fishes in the Laurentian Great Lakes and Wabash River." Metabarcoding and Metagenomics 4 (August 26, 2020): e53455. https://doi.org/10.3897/mbmg.4.53455.

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Community composition data are essential for conservation management, facilitating identification of rare native and invasive species, along with abundant ones. However, traditional capture-based morphological surveys require considerable taxonomic expertise, are time consuming and expensive, can kill rare taxa and damage habitats, and often are prone to false negatives. Alternatively, metabarcoding assays can be used to assess the genetic identity and compositions of entire communities from environmental samples, comprising a more sensitive, less damaging, and relatively time- and cost-effici

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Schreiber, C., D. Elbaz, M. Pannella, L. Ciesla, T. Wang, and M. Franco. "Dust temperature and mid-to-total infrared color distributions for star-forming galaxies at 0 < z < 4." Astronomy & Astrophysics 609 (December 22, 2017): A30. http://dx.doi.org/10.1051/0004-6361/201731506.

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We present a new, publicly available library of dust spectral energy distributions (SEDs). These SEDs are characterized by only three parameters: the dust mass (Mdust), the dust temperature (Tdust), and the mid-to-total infrared color (IR8 ≡ LIR/L8). The latter measures the relative contribution of polycyclic aromatic hydrocarbon (PAH) molecules to the total infrared luminosity. We used this library to model star-forming galaxies at 0.5 < z < 4 in the deep CANDELS fields, using both individual detections and stacks of Herschel and ALMA imaging, and extending this sample to z = 0 using th

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Grould, M., F. H. Vincent, T. Paumard, and G. Perrin. "General relativistic effects on the orbit of the S2 star with GRAVITY." Astronomy & Astrophysics 608 (December 2017): A60. http://dx.doi.org/10.1051/0004-6361/201731148.

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Context. The first observations of the GRAVITY instrument obtained in 2016, have shown that it should become possible to probe the spacetime close to the supermassive black hole Sagittarius A* (Sgr A*) at the Galactic center by using accurate astrometric positions of the S2 star. Aims. The goal of this paper is to investigate the detection by GRAVITY of different relativistic effects affecting the astrometric and/or spectroscopic observations of S2 such as the transverse Doppler shift, the gravitational redshift, the pericenter advance and higher-order general relativistic (GR) effects, in par

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Voionmaa, Daniel Noemi. "Radical Justice: Spain and the Southern Cone beyond Market and State, Luis Martín Cabrera (2011)." Persona y Sociedad 26, no. 3 (2012): 141. http://dx.doi.org/10.53689/pys.v26i3.29.

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Justicia radical estudia novelas policiales y documentales que refieren y elaboran sobre el período de las posdictaduras en España, Argentina y Chile. Esta perspectiva transnacional no desconoce las especificidades de cada país, pero enfatiza el hecho de que los eventos acaecidos son “parte del desarrollo global del capitalismo y de sus redes de terror” (4).1 El texto, en sus cuatro capítulos más introducción, desarrolla un triple trabajo: la elaboración de un marco y aparato teórico –cuyo centro es el concepto de ‘no-lugar’–; el análisis y lectura detallada de cuatro novelas y cuatro document

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Elphick, Camilla, Richard Philpot, Min Zhang, et al. "Digital Detectives: Websleuthing Reduces Eyewitness Identification Accuracy in Police Lineups." Frontiers in Psychology 12 (April 15, 2021). http://dx.doi.org/10.3389/fpsyg.2021.640513.

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Eyewitnesses to crimes sometimes search for a culprit on social media before viewing a police lineup, but it is not known whether this affects subsequent lineup identification accuracy. The present online study was conducted to address this. Two hundred and eighty-five participants viewed a mock crime video, and after a 15–20 min delay either (i) viewed a mock social media site including the culprit, (ii) viewed a mock social media site including a lookalike, or (iii) completed a filler task. A week later, participants made an identification from a photo lineup. It was predicted that searching

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