The NANOGrav 15 yr Data Set: Looking for Signs of Discreteness in the Gravitational-wave Background by Gabriella Agazie, Akash Anumarlapudi, Anne M. Archibald, Zaven Arzoumanian, Jeremy George Baier, Paul T. Baker, Bence Bécsy, Laura Blecha, Adam Brazier, Paul R. Brook, Lucas Brown, Sarah Burke-Spolaor, J. Andrew Casey-Clyde, Maria Charisi, Shami Chatterjee, Tyler Cohen, James M. Cordes, Neil J. Cornish, Fronefield Crawford, H. Thankful Cromartie, Kathryn Crowter, Megan E. DeCesar, Paul B. Demorest, Heling Deng, Timothy Dolch, Elizabeth C. Ferrara, William Fiore, Emmanuel Fonseca, Gabriel E. Freedman, Nate Garver-Daniels, Peter A. Gentile, Joseph Glaser, Deborah C. Good, Kayhan Gültekin, Jeffrey S. Hazboun, Ross J. Jennings, Aaron D. Johnson, Megan L. Jones, Andrew R. Kaiser, David L. Kaplan, Luke Zoltan Kelley, Matthew Kerr, Joey S. Key, Nima Laal, Michael T. Lam, William G. Lamb, Bjorn Larsen, T. Joseph W. Lazio, Natalia Lewandowska, Tingting Liu, Duncan R. Lorimer, Jing Luo, Ryan S. Lynch, Chung-Pei Ma, Dustin R. Madison, Alexander McEwen, James W. McKee, Maura A. McLaughlin, Natasha McMann, Bradley W. Meyers, Patrick M. Meyers, Chiara M. F. Mingarelli, Andrea Mitridate, Priyamvada Natarajan, Cherry Ng, David J. Nice, Stella Koch Ocker, Ken D. Olum, Timothy T. Pennucci, Benetge B. P. Perera, Nihan S. Pol, Henri A. Radovan, Scott M. Ransom, Paul S. Ray, Joseph D. Romano, Jessie C. Runnoe, Shashwat C. Sardesai, Ann Schmiedekamp, Carl Schmiedekamp, Kai Schmitz, Brent J. Shapiro-Albert, Xavier Siemens, Joseph Simon, Magdalena S. Siwek, Sophia V. Sosa Fiscella, Ingrid H. Stairs, Daniel R. Stinebring, Kevin Stovall, Abhimanyu Susobhanan, Joseph K. Swiggum, Stephen R. Taylor, Jacob E. Turner, Caner Unal, Michele Vallisneri, Sarah J. Vigeland, Haley M. Wahl, London Willson, Caitlin A. Witt, David Wright, Olivia Young

“…The cosmic merger history of supermassive black hole binaries (SMBHBs) is expected to produce a low-frequency gravitational wave background (GWB). …”
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Wide and Fast: Monitoring the Sky in Subsecond Domain with the FAVOR and TORTORA Cameras by Sergey Karpov, Grigory Beskin, Sergey Bondar, Adriano Guarnieri, Corrado Bartolini, Giuseppe Greco, Adalberto Piccioni

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Simultaneous Multiwavelength Observations of the Repeating Fast Radio Burst FRB 20190520B with Swift and FAST by Zhen Yan, Wenfei Yu, Kim L. Page, Jie Lin, Di Li, Chenhui Niu, Casey Law, Bing Zhang, Shami Chatterjee, Xian Zhang, Reshma Anna-Thomas

“…We detect no multiwavelength counterpart to the PRS. The 3 σ luminosity upper limits are 1.04 × 10 ^47 (15–150 keV), 8.81 × 10 ^42 (0.3–10 keV), 9.26 × 10 ^42 (UVW1), and 2.54 × 10 ^42 erg s ^−1 ( U ), respectively. …”
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Roped Solidarity by Burak Sezer

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Mythopoetics of Space in the Novels by Yuri Rytkheu by Albina S. Zhuleva

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Mass of Cepheid V350 Sgr Incorporating Interferometry and the Companion Mass by Nancy Remage Evans, Alexandre Gallenne, Pierre Kervella, H. Moritz Günther, Joanna Kuraszkiewicz, Richard I. Anderson, Charles Proffitt, Antoine Mérand, Boris Trahin, Giordano Viviani, Shreeya Shetye

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Synchronous and Asynchronous X-Ray Monitoring of FRB 20190520B with the Chandra X-Ray Observatory by Jessica Sydnor, Sarah Burke-Spolaor, Kshitij Aggarwal, Reshma Anna-Thomas, Casey J. Law, Harsha Blumer, Liam Connor

“…We place a direct limit on the presence of a massive black hole (MBH) in this system, limiting mass and the Eddington ratio λ _E to ${M}_{\mathrm{BH}}\lt 4.3\times 1{0}^{3}({\lambda }_{{\rm{E}}}^{-1})\,{M}_{\odot }$ (in a low-density line-of-sight limit) and ${M}_{\mathrm{BH}}\lt 1.8\times 1{0}^{4}({\lambda }_{{\rm{E}}}^{-1})\,{M}_{\odot }$ (high-density limit). …”
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A New Approach to the Low-frequency Stochastic Gravitational-wave Background: Constraints from Quasars and the Astrometric Hellings–Downs Curve by Jeremy Darling

“…This astrometric analysis does not yet reach the sensitivity needed to detect the pulsar timing–based red gravitational-wave spectrum extrapolated to the quasar gravitational-wave sensitivity window, assuming that the turnover in the spectrum occurs at ∼1 nHz for massive black hole binaries. The limits presented here may exclude some exotic interpretations of the stochastic gravitational-wave background.…”
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Discourses of “religion” in public health research: Constructing religious facilitators, barriers, and subjects of health as exercises of power by Tyler J. Fuller

“…These discourses reinforce binaries of “good religion” and “bad belief,” contributing to epistemic injustice and shaping health subjectivities in ways that can undermine equity. …”
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Impossible Justice and the Allure of the Absolute: A Psychoanalytic Reading of Radicalization by Sadeq Rahimi

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The He(A)rt of the Witness: Remembering Australian Prisoners of War in Richard Flanagan’s The Narrow Road to the Deep North by Rūta Šlapkauskaitė

Invisible Theatre: militarized space and the staging of affective atmospheres by Leah Lovett

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Gaia-4b and 5b: Radial Velocity Confirmation of Gaia Astrometric Orbital Solutions Reveal a Massive Planet and a Brown Dwarf Orbiting Low-mass Stars by Gudmundur Stefánsson, Suvrath Mahadevan, Joshua N. Winn, Marcus L. Marcussen, Shubham Kanodia, Simon Albrecht, Evan Fitzmaurice, Onė Mikulskytė, Caleb I. Cañas, Juan I. Espinoza-Retamal, Yiri Zwart, Daniel M. Krolikowski, Andrew Hotnisky, Paul Robertson, Jaime A. Alvarado-Montes, Chad F. Bender, Cullen H. Blake, J. R. Callingham, William D. Cochran, Megan Delamer, Scott A. Diddams, Jiayin Dong, Rachel B. Fernandes, Mark R. Giovinazzi, Samuel Halverson, Jessica Libby-Roberts, Sarah E. Logsdon, Michael W. McElwain, Joe P. Ninan, Jayadev Rajagopal, Varghese Reji, Arpita Roy, Christian Schwab, Jason T. Wright

“…Here we present RV follow-up observations of 28 M and K stars with candidate astrometric substellar companions, which led to the confirmation of two systems, Gaia-4b and Gaia-5b, identification of five systems that are single lined but require additional data to confirm as substellar companions, and the refutation of 21 systems as stellar binaries. Gaia-4b is a massive planet ( M  = 11.8 ± 0.7 M _J ) in a P  = 571.3 ± 1.4 day orbit with a projected semimajor axis a _0  = 0.312 ± 0.040 mas orbiting a 0.644 ± 0.02 M _⊙ star. …”
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Revisiting the Activity–Rotation Relation for Evolved Stars by Henggeng Han, Song Wang, Xue Li, Chuanjie Zheng, Jifeng Liu

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Asālīb Ta’līm Mahārati An-Nuthqi Ash-Shahih Lillugatil Arabiyyah ( Dirāsah Tahlīliyyah ‘Alā Shautiyyāt Kitāb Al-Arabiyyah Baina Yadaik) by Ruhul Kudus, Fatkhul Ulum, Mohd Shauki Bik Bin Mohd Kasim

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How to Avoid the Paradigm of Censorship: Self-Consciousness, Mimetic Desire and the Empathic Style of Anita Desai by Manodip Chakraborty

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Reimagining Blackness through posthumanist sculpture: an analysis of the works of Ghanaian artist, Sulemana Armiyaw by Armiyaw Sulemana, Jiang Tieli, Ebenezer Fiifi Mensah, Kwame Opoku-Bonsu

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Waithood, Music, Fakes, and Well-Being: Exploring the Mobile Lives of South African Township Youth Through the Mobile Diary Method by Priscilla Boshoff, Chikezie E. Uzuegbunam, Bimbo Fafowora, Nonhlanhla Ndlovu, Alette Schoon

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Generation of Magnetic Fields around Black Hole Accretion Disks due to Nonconservative Radiation Fields by Mukesh Kumar Vyas, Asaf Pe’er

“…The predicted field strengths could affect the thermal emission, synchrotron radiation, and polarization properties of black hole accretion systems, with implications for X-ray binaries, active galactic nuclei, and jet formation. …”
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Applying the Adomian Method to Solve the Fokker–Planck Equation: A Case Study in Astrophysics by Melina Silva de Lima, José Vicente Cardoso Santos, José Humberto de Souza Prates, Celso Barreto Silva, Davidson Moreira, Marcelo A. Moret

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