bluuebunny/crossref_metadata_2025_split huggingface dataset:
Manuscript Assessment and Editorial Decision-Making
Authors: Steinbrook Robert , Redberg Rita F. 
Published: October 2024

Abstract
Manuscript assessment and editorial decision-making are major responsibilities of journal editors. This chapter provides insight into how journal editors assess manuscripts, the key principles of editorial decision-making, and major criteria commonly used for evaluating manuscripts, including originality, scientific accuracy, presentation, and interest to readers. The life cycle of a manuscript is described, starting with submission of the manuscript to the journal, proceeding through editorial evaluation and possibly peer review and revision, and ending with either rejection or eventual acceptance. The usual editorial decisions, including provisional acceptance, revise and reconsider, and rejection, are discussed, along with the rationale and implications of each, providing authors with an inside-out look at the context within which journal editors evaluate submitted manuscripts.
Constraining planetary albedo of JWST targets in the TESS bandpass, using TESS, HST, and Spitzer eclipse depth observations
Authors: Arora Rahul , Goyal Jayesh 
Published: October 2024

ABSTRACT
Albedo is one of the important characteristics of hot Jupiter exoplanets. However, albedo constraints have been obtained for very few exoplanets. In this work, we present the Transiting Exoplanet Survey Satellite (TESS) phase curve observations of WASP-18b, WASP-19b, WASP-121b, WASP-43b, WASP-17b, and WASP-77b, all targets for atmospheric characterization and constrain their occultation depth as well as geometric albedo (A$_{\rm g}$). We use a grid of self-consistent model atmospheres to constrain the metallicity, C/O ratio, and heat re-distribution for these six targets by fitting to their HST and/or Spitzer observations and also compute the thermal contribution to total occultation depth in the TESS bandpass. We report the first value of TESS occultation depth for WASP-17b ($151_{-66}^{+83}$ ppm) and updated value for WASP-77Ab ($94_{-62}^{+53}$ ppm). We find self-consistent models constrain high values of thermal contribution to total occultation compared to Planck models. We find very low A$_{\rm g}$ values for WASP-18b (&lt;0.089), WASP-19b (&lt;0.022), WASP-121b ($0.0^{+0.055}_{-0.104}$), WASP-77Ab ($0.017^{+0.126}_{-0.147}$) and significantly higher value for WASP-43b ($0.109^{+0.086}_{-0.088}$), and WASP-17b ($0.401^{+0.526}_{-0.307}$). We find WASP-17b lies in the ideal spot of low gravity and low equilibrium temperature, conducive for cloud formation, leading to high A$_{\rm g}$. With the best-fitting models, we constrain low heat re-distribution for all planets, with WASP-18b having the least. We also constrain sub-solar metallicity for all planets except WASP-17b and WASP-19b. We find a highly sub-solar C/O ratio for WASP-77Ab and WASP-43b, solar for WASP-18b, and super-solar for WASP-121b. The best-fitting P–T profiles show thermal inversion for WASP-18b and WASP-121b and none for WASP-77b and WASP-43b, which is in agreement with previous works.
A Gaussian process model for stellar activity in 2D line profile time-series
Authors: Yu Haochuan , Aigrain Suzanne , Klein Baptiste , Cretignier Michael , Lienhard Florian , Roberts Stephen J 
Published: October 2024

ABSTRACT
Stellar active regions like spots and faculae can distort the shapes of spectral lines, inducing variations in the radial velocities that are often orders of magnitude larger than the signals from Earth-like planets. Efforts to mitigate these activity signals have hitherto focused on either the time or the velocity (wavelength) domains. We present a physics-driven Gaussian process (GP) framework to model activity signals directly in time series of line profiles or cross-correlation functions (CCFs). Unlike existing methods that correct activity signals in line profile time series, our approach exploits the time correlation between velocity (wavelength) bins in the line profile variations, and is based on a simplified but physically motivated model for the origin of these variations. When tested on both synthetic and real data sets with signal-to-noise ratios down to ∼100, our method was able to separate the planetary signal from the activity signal, even when their periods were identical. We also conducted injection/recovery tests using two years of realistically sampled HARPS-N solar data, demonstrating the ability of the method to accurately recover a signal induced by a 1.5-Earth mass planet with a semi-amplitude of 0.3 m s−1 and a period of 33 d during high solar activity.
Inferring system parameters from the bursts of the accretion-powered pulsar IGR J17498–2921
Authors: Galloway D K , Goodwin A J , Hilder T , Waterson L , Cupák M 
Published: October 2024

ABSTRACT
Thermonuclear (type-I) bursts exhibit properties that depend both on the local surface conditions of the neutron stars on which they ignite, as well as the physical parameters of the host binary system. However, constraining the system parameters requires a comprehensive method to compare the observed bursts to simulations. We have further developed the beansp code for this purpose and analysed the bursts observed from IGR J17498$-$2921, a 401-Hz accretion-powered pulsar, discovered during it’s 2011 outburst. We find good agreement with a model having H-deficient fuel with $X=0.15\pm 0.4$, and CNO metallicity $Z=0.0014^{+0.0004}_{-0.0003}$, about a tenth of the solar value. The model has the system at a distance of $5.7^{+0.6}_{-0.5}$ kpc, with a massive (${\approx} 2\ \mathrm{ M}_\odot$) neutron star and a likely inclination of $60^\circ$. We also re-analysed the data from the 2002 outburst of the accretion-powered millisecond pulsar SAX J1808.4$-$3658. For that system we find a substantially closer distance than previously inferred, at $2.7\pm 0.3$ kpc, likely driven by a larger degree of burst emission anisotropy. The other system parameters are largely consistent with the previous analysis. We briefly discuss the implications for the evolution of these two systems.
The supermassive black hole merger-driven evolution of high-redshift red nuggets into present-day cored early-type galaxies
Authors: Rantala Antti , Rawlings Alexander , Naab Thorsten , Thomas Jens , Johansson Peter H 
Published: October 2024

ABSTRACT
Very compact ($R_\mathrm{e}\lesssim 1$ kpc) massive quiescent galaxies (red nuggets) are more abundant in the high-redshift Universe ($z\sim 2$–3) than today. Their size evolution can be explained by collisionless dynamical processes in galaxy mergers which, however, fail to reproduce the diffuse low-density central cores in the local massive early-type galaxies (ETGs). We use sequences of major and minor merger N-body simulations starting with compact spherical and disc-like progenitor models to investigate the impact of supermassive black holes (SMBHs) on the evolution of the galaxies. With the ketju code we accurately follow the collisional interaction of the SMBHs with the nearby stellar population and the collisionless evolution of the galaxies and their dark matter haloes. We show that only models including SMBHs can simultaneously explain the formation of low-density cores up to sizes of $R_\mathrm{b} \sim 1.3$ kpc with mass deficits in the observed range and the rapid half-mass size evolution. In addition, the orbital structure in the core region (tangentially biased orbits) is consistent with observation-based results for local cored ETGs. The displacement of stars by the SMBHs boost the half-mass size evolution by up to a factor of 2 and even fast rotating progenitors (compact quiescent discs) lose their rotational support after 6–8 mergers. We conclude that the presence of SMBHs is required for merger-driven evolution models of high-redshift red nuggets into local ETGs.
Surviving the waves: evidence for a dark matter cusp in the tidally disrupting Small Magellanic Cloud
Authors: De Leo Michele , Read Justin I , Noël Noelia E D , Erkal Denis , Massana Pol , Carrera Ricardo 
Published: October 2024

ABSTRACT
We use spectroscopic data for ${\sim }6000$ red giant branch stars in the Small Magellanic Cloud (SMC), together with proper motion data from Gaia Early Data Release 3, to build a mass model of the SMC. We test our Jeans mass modelling method (binulator + gravsphere) on mock data for an SMC-like dwarf undergoing severe tidal disruption, showing that we are able to successfully remove tidally unbound interlopers, recovering the dark matter density and stellar velocity anisotropy profiles within our 95 per cent confidence intervals. We then apply our method to real SMC data, finding that the stars of the cleaned sample are isotropic at all radii (at 95 per cent confidence) and that the inner dark matter density profile is dense, $\rho _{\rm DM}(150\ {\rm pc}) = 1.58_{-0.58}^{+0.80}\times 10^8 \ {\rm M}_{\odot }\, \rm kpc^{-3}$, consistent with a $\Lambda$ cold dark matter cusp. Our model gives a new estimate of the SMC’s total mass within 3 kpc $(M_{\rm tot} \le 3\ {\rm kpc})$ of $2.29\pm 0.46 \times 10^9 \ {\rm M}_{\odot }$. We also derive an astrophysical ‘J-factor’ of $18.99\pm 0.16$ GeV$^2$ cm$^{-5}$ and a ‘D-factor’ of $18.73\pm 0.04$ GeV$^2$ cm$^{-5}$, making the SMC a promising target for dark matter annihilation and decay searches. Finally, we combine our findings with literature measurements to test models in which dark matter is ‘heated up’ by baryonic effects. We find good qualitative agreement with the Di Cintio et al. model but we deviate from the Lazar et al. model at high $M_*/M_{200} &gt; 10^{-2}$. We provide a new, analytical, density profile that reproduces dark matter heating behaviour over the range $10^{-4} &lt; M_*/M_{200} &lt; 10^{-1}$.
Bayesian inference of initial conditions from non-linear cosmic structures using field-level emulators
Authors: Doeser Ludvig , Jamieson Drew , Stopyra Stephen , Lavaux Guilhem , Leclercq Florent , Jasche Jens 
Published: October 2024

ABSTRACT
Analysing next-generation cosmological data requires balancing accurate modelling of non-linear gravitational structure formation and computational demands. We propose a solution by introducing a machine learning-based field-level emulator, within the Hamiltonian Monte Carlo-based Bayesian Origin Reconstruction from Galaxies (BORG) inference algorithm. Built on a V-net neural network architecture, the emulator enhances the predictions by first-order Lagrangian perturbation theory to be accurately aligned with full N-body simulations while significantly reducing evaluation time. We test its incorporation in BORG for sampling cosmic initial conditions using mock data based on non-linear large-scale structures from N-body simulations and Gaussian noise. The method efficiently and accurately explores the high-dimensional parameter space of initial conditions, fully extracting the cross-correlation information of the data field binned at a resolution of $1.95\,h^{-1}$ Mpc. Percent-level agreement with the ground truth in the power spectrum and bispectrum is achieved up to the Nyquist frequency $k_\mathrm{N} \approx 2.79h \,\, \mathrm{Mpc}^{-1}$. Posterior resimulations – using the inferred initial conditions for N-body simulations – show that the recovery of information in the initial conditions is sufficient to accurately reproduce halo properties. In particular, we show highly accurate $M_{200\mathrm{c}}$ halo mass function and stacked density profiles of haloes in different mass bins $[0.853,16]\times 10^{14}\,{\rm M}_{\odot }\,h^{-1}$. As all available cross-correlation information is extracted, we acknowledge that limitations in recovering the initial conditions stem from the noise level and data grid resolution. This is promising as it underscores the significance of accurate non-linear modelling, indicating the potential for extracting additional information at smaller scales.
Industrial Genotoxicology Group: 36th Annual Meeting Report
Authors: Kidd Darren , Crooks Ian , Saccardo Angela , Ponting David J , Kocks Grace , Gandhi Raj , Thomas Dean , Pass Emily , Lynch Anthony , Johnson George , Fowler Paul , Wilson Amy 
Published: October 2024

Abstract
The proceedings of the 36th annual meeting of the Industrial Genotoxicology Group (IGG) are shared here. The meeting held at Lhasa Limited, Leeds, UK on 28 November 2023, focussed on two aspects; new approach methodologies (NAMs), including those for the assessment of non-standard modalities such as gas-vapour assessments and nanomaterials, and addressing the regulatory challenges associated with understanding the genotoxic and carcinogenic potential of N-nitrosamines and N-nitrosamine impurities. New approach methodologies, such as error-corrected sequencing and enhanced Ames tests that may help address these challenges were also discussed.
Phoenix Rises
Authors: Finch Andrew J. 
Published: October 2024

Abstract
The Montgomery County Board of Education approved a pilot program to address drug use in December 1978, and they asked that it be modeled on Brian Berthiaume’s Other Way school. April 1979 was set as the opening date, giving Berthiaume about ninety days to plan. This chapter explains how staff were identified and a location was selected in Silver Spring, causing a reaction by parents who did not want the school in their neighborhood. Staff received training in family systems therapy. The staff also named the school “Phoenix,” after the mythical bird. Enrollment criteria were devised, and students were recruited. The chapter includes a case description of a typical Phoenix School student in its early days. Initially, students with less severe behavior issues appeared to be doing better. The Phoenix School programming is described, and an account of the first graduation concludes the chapter.
Normalized Alternatives
Authors: Finch Andrew J. 
Published: October 2024

Abstract
Minnesota became the epicenter of growth for recovery high schools in the 1980s and 1990s. The expansion was rooted in both the alternative school and adolescent treatment sectors dating to the early 1970s. This chapter describes the growth of alternative schools and adolescent treatment in Minnesota, and it introduces Carol Robson, a Minneapolis social worker who could not find a suitable school for her son, Joshua, who had cerebral palsy, so she started the school that finally propelled recovery high schools into a national movement. A key element of the expansion of alternative schools was legislation facilitating school choice. In time, Minnesota had fully embraced school choice so much that recovery high schools blossomed there more than in any other state.
Becoming Sobriety High
Authors: Finch Andrew J. 
Published: October 2024

Abstract
Carol Robson met former advertising executive Ralph Neiditch at a mutual aid meeting near the Hazelden treatment center in Minnesota in the mid-1980s. Together, they refashioned New Dimensions into a recovery high school, which was eventually renamed Sobriety High in 1988. This chapter explores how Robson’s marriage dissolved and how Neiditch took control of the organization. Under Neiditch’s leadership, Sobriety High recruited influential donors to its board of directors, revised its bylaws, and began major fundraising and marketing campaigns that would transform the school into a program that would inspire multiple new recovery high schools in Minnesota and other states.
Second Wave Pocket
Authors: Thompson Gordon Ross 
Published: October 2024

Abstract
With the rise of feminism in the late 1960s, women began to gain a sense of agency. Veteran singer Jackie Lee’s performance of the theme song to the television show White Horses appealed to young women, as did the infantilized members of the group the Paper Dolls. London’s reputation also attracted singers from Europe, including Rita Pavone, Mireille Mathieu, and Françoise Hardy. Cilla Black complained that the press lumped her, Sandie Shaw, Lulu, and Dusty Springfield together as “British girl pop singers with star quality,” despite their differences. Springfield, Shaw, and Lulu all sought and achieved some control over their careers. Younger performers were less successful. Welsh singer Mary Hopkin became a vehicle for Paul McCartney’s venture as a producer and an unhappy participant in the Eurovision competition. Others, such as Beryl Marsden and Christine Perfect, however, defied gendered stereotypes that presented women musicians as separate from the band.
The Ideology of Automata
Authors: Seaford Richard 
Published: October 2024

Abstract
The power of a Mesopotamian deity in its temple may preclude an identity separate from its image. This facilitates the act of offering, e.g., of food brought to the temple to be eaten by the deity. In the one Homeric instance of an offering brought to a deity in a temple (Athena in Troy in Iliad 6), her image seems to move, to be alive. Similarly, the immortal gold and silver dogs guarding the doors of royal house in the fabulous land of Phaeacia (Odyssey 7) surely derive from reports of the living images of dogs guarding Assyrian entrances. But in the public space (political and commercial) and egalitarian animal sacrifice that will generate the Greek polis there is no place for an omnipotent image. The myth of Prometheus establishes both the communal consumption of the sacrificial meat and therefore also—this is of unrecognized importance—the withdrawal of the gods to the sky, gods who (in a narrative with Near-Eastern elements) in revenge leave with mortals a living artifact, an immortal image, Pandora. Also characteristic of the (monetized) polis is the development of the dualisms of (a) image (or symbol) and reality (pioneered in Herakleitos’ condemnation of the ignorance involved in praying to statues: B5), and (b) body and soul (also pioneered in Herakleitos). These dualisms tend to make a Greek living image (artifact) into an anomaly or thauma.
Automatic Puppets, Toy Carts, and Robots
Authors: Galluzzo Gabriele 
Published: October 2024

Abstract
The chapter examines the issue of how automata sit within Aristotle’s complex metaphysics of artifacts. In particular, the question will be raised as to whether the case of automata poses a challenge to Aristotle’s sharp distinction between artificial and natural things and, more specifically, between artificial and living things, which are for Aristotle paradigmatic and eminent instances of natural things. The answer will be that Aristotle’s distinction stands. What is more, the case of automata shows one crucial point of demarcation between organisms and artifacts, i.e., the complete absence in the case of artifacts of an intrinsic or internal teleology. An artifact’s purpose, end, and function essentially depend on the interests and ends of its creator. And this applies even to such complex artifacts as automata. The analysis focuses on three main texts and contexts, which describe an increasing level of engagement on Aristotle’s part with the metaphysical import of automata and automatic analogies: Aristotle’s explanation of the motion of animals in On the Movement of Animals; his account of embryological development in On the Generation of Animals, Book 2; and finally Aristotle’s suggestive fantasy, in Book 1 of the Politics, of a world in which slaves are replaced by robot-style artifacts.
Transliteration and Translation
Authors: Gill Ann-Katrin , Smith Mark 
Published: October 2024

Abstract
This chapter presents the complete line-by-line transliteration and translation for all sixteen spells of the Glorification Recited on Each Due Occasion of the Embalming Place. The best-preserved manuscript of the composition, P. Louvre N. 3129, forms the type witness. This papyrus also provides the most accurate and reliable version of the text, to which all other versions are compared in this chapter and the commentary. Textual notes on problematic readings are included in the footnotes of this chapter, as are remarks which concern the hieroglyphic transcription or peculiarities in hieratic writings of words in the type version P. Louvre N. 3129. An effort has been made to provide an easily understandable translation, suitable for the layman as well as specialists, with more literal renderings provided in the footnotes when deemed necessary.
Introduction
Authors: Gamble Steven 
Published: October 2024

Abstract
This introductory chapter sets the scene for a study of hip hop and the internet. It demonstrates the significance of hip hop and the internet in everyday life for over half the global population. After defining key terms, it identifies the Anglophone scope of the research into social media cultures and explains the combination of qualitative and quantitative methods adopted throughout the book. The author provides a positionality statement and reflects on his approach to online hip hop as an aca-fan. The chapter elaborates on crucial concepts in internet studies and underlying assumptions about hip hop. It closes by outlining the remaining chapters of the book.
Addressing Anti-Asian Racism with Social Work Advocacy and Action
Authors: 9780197672266  
Published: October 2024

Abstract
Beginning in the 18th century, Asian Americans have experienced persistent racism, marginalizing stereotyping, microaggressions, verbal and physical attacks, hate crimes, and harassments driven by individual-level racism and institutional reinforcement. This volume systemically examines the experience and impact of racism from the perspective of Asian American, Native Hawaiian, and Pacific Islander (AANHPI) and delves into the need to seek out evidence-based micro, meso, and macro solutions. Contributors to this volume comprise many of the seminal social work scholars, activists, and educators addressing anti-Asian racism and cover a range of perspectives and methodological approaches across the social work discipline. This volume provides a comprehensive and in-depth investigation to address anti-Asian racism through social work action. It intends to serve as a timely resource for social work educators, researchers, and practitioners committed to eliminating racism experienced by a population that will no longer accept the label of being “invisible.”
The History of Anti-Asian Racism and Violence in the United States
Authors: Liu Meirong , Lee Nayoun , Si Zhanjie , Aquino Olivia 
Published: October 2024

Abstract
This chapter begins with a review of the history of anti-Asian racism in the United States. Beginning in the mid-19th century, Asian immigrants played a vital role in the development of the country. However, Asian Americans have faced a long legacy of exclusion and inequality, particularly during periods of economic recession, disease outbreaks, or war throughout US history. Adopting the framework of “othering,” this chapter analyzes the major events in US history related to Asian Americans, such as the Chinese Exclusion Act of 1882, the Immigration Act of 1924, the Japanese internment camps during World War II, and the anti-Asian immigration policies adopted by the Trump administration. Through this, the authors illustrate how historic racism and xenophobia at both individual and institutional levels have operated to marginalize Asian Americans and reproduce inequality, and they demonstrate the common roots of racism that lie in White supremacy.