cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Research 101 : A process for developing local guidelines for ethical research in heavily researched communities
Creators: name: Neufeld, Scott D.
name: Chapman, Jule
name: Crier, Nicolas
name: Marsh, Samona
name: McLeod, Jim
name: Deane, Lindsay A.
Publisher: name: The University of British Columbia
Year: 2019

description: Background: Marginalized communities often attract more than their share of research. Too often, this research benefits researchers disproportionately and leaves such communities feeling exploited, misrepresented, and exhausted. The Downtown Eastside (DTES) neighborhood of Vancouver, Canada, has been the site of multiple public health epidemics related to injection drug use as well as the site of much community-led resistance and struggle that has led to the development of cutting-edge harm reduction interventions (e.g., North America’s first supervised injection facility, Insite) and a strong sense of community organization. This background has made the DTES one of the most heavily researched communities in the world. Amidst ongoing experiences of unethical or disrespectful research engagement in the neighborhood, a collaboration between local academic researchers and community representatives developed to explore how we could work together to encourage more respectful, community-responsive research and discourage exploitative or disrespectful research. Methods: We developed a series of six weekly workshops called “Research 101.” These workshops brought together approximately 13 representatives from peer-based organizations in the DTES with a variety of experiences with research. Research 101 created space for community members themselves to discuss the pitfalls and potential of research in their neighborhood and to express community expectations for more ethical and respectful research. Results: We summarized workshop discussions in a co-authored “Manifesto for Ethical Research in the Downtown Eastside.” This document serves as a resource to empower community organizations to develop more equitable partnerships with researchers and help researchers ground their work in the principles of locally developed “community ethics.” Manifesto guidelines include increased researcher transparency, community-based ethical review of projects, empowering peer researchers in meaningful roles within a research project, and taking seriously the need for reciprocity in the research exchange. Conclusions: Research 101 was a process for eliciting and presenting a local vision of “community ethics” in a heavily researched neighborhood to guide researchers and empower community organizations. Our ongoing work involves building consensus for these guidelines within the community and communicating these expectations to researchers and ethics offices at local universities
Cypridea nitidula Peck 1941
Creators: name: Bate, Raymond H.
name: Horne, David J.
name: Horne, Sarah E.
name: Douglas, Lyndsey
name: Miller, Giles
name: Lord, Alan R.
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Ostracoda
Podocopida
Cyprididae
Cypridea
Cypridea nitidula

description: Cypridea nitidula Peck, 1941 in Moos in Wicher, 1959
Fig. 1, 9a–c
1941 Cypridea nitidula n. sp. —Peck: p. 301, pl. 43, figs 1–5.
Figured specimen: Carapace, T.-K.-Nr. 3177.
Dimensions: length 0.97mm, height 0.58mm, width 0.44mm.
description: Published as part of Bate, Raymond H., Horne, David J., Horne, Sarah E., Douglas, Lyndsey, Miller, Giles & Lord, Alan R., 2022, Non-marine Ostracoda (Crustacea) of the Early Cretaceous ' Pre-Salt' sediments of Brazil: An illustrated catalogue of the type specimens of Wicher, Krömmelbein, Krömmelbein & Weber, and Bate, pp. 1-84 in Zootaxa 5098 (1) on page 9, DOI: 10.11646/zootaxa.5098.1.1, http://zenodo.org/record/6036685
title: Dead end: Right-wing populism Recognising diversity and immigration culture in Lusatia
Creators: name: Haas, Tobias
name: Staemmler, Johannes
Publisher: name: Institute for Advanced Sustainability Studies (IASS)
Year: 2021

description: The German government has resolved to phase out coal-fired power plants at the latest by 2038. The coal exit will inevitably mean the end of lignite mining in Lusatia, a central economic sector that has played a major role in shaping the region’s identity. However, against the backdrop of the worsening climate crisis, lignite is a hotly contested political issue. Although there are many people in Lusatia who reject the coal exit by 2038, lignite is not uncontroversial here either. (see Bischoff et. al. 2021). At the same time, in recent years the right-wing populist and to some extent radical right-wing party Alternative for Germany (AfD) has gained mass appeal among some of the Lusatian population. With their right-wing populist orientation and simplistic friend-foe argumentation, the AfD is driving social polarisation. The party rails against the coal exit, sheds doubt on man-made climate change and, more recently, has sought proximity to pandemic deniers. But why exactly is right-wing populism so popular in Lusatia? Why does this success pose a threat to structural change in the region? And how might we remove the breeding ground for right-wing populism and counteract social polarisation? This Discussion Paper addresses these questions and develops three approaches for countering social polarisation so that the coming structural change in Lusatia can be successful. Acknowledge diversity Lusatia is often presented as a homogeneous area with a homogeneous population. This in no way reflects the social reality on the ground. The population in Upper and Lower Lusatia is very heterogeneous in terms of their origins, political views, and religious beliefs. This diversity must be acknowledged and viewed as a resource for the region. Establish a culture of immigration Since 2000 alone, the population in Lusatia has declined by about 20 per cent, from 1.4 million to 1.1 million, and the average age has increased significantly (WRL 2019, 27). For the future, it is imperative to establish a culture of immigration to make the region attractive both for people who left as young adults and for people from other parts of Germany and abroad. Take fears about the future seriously, but do not exacerbate them The massive economic and social changes of the 1990s have stirred fear of change in the region. For this reason, it is important to establish spaces where dialogue can take place on what the future might look like without strengthening vague fears stemming from past experiences.
Multi-dimensional Jordan chain and Navier-Stokes Equation
Creators: name: Konopelchenko, B. G.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Mathematical Physics (math-ph)
subject: Exactly Solvable and Integrable Systems (nlin.SI)
subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: Multi-dimensional Jordan chain is presented. It is shown that it admits the finite-component reductions to the Navier-Stokes equation and other important equations of continuous media theory.
description: Some misprints are corrected
Cypridea brevicornis Peck 1941
Creators: name: Bate, Raymond H.
name: Horne, David J.
name: Horne, Sarah E.
name: Douglas, Lyndsey
name: Miller, Giles
name: Lord, Alan R.
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Ostracoda
Podocopida
Cyprididae
Cypridea
Cypridea brevicornis

description: Cypridea brevicornis Peck, 1941 in Moos in Wicher, 1959
Fig. 1, 10a–c
1941 Cypridea brevicornis n. sp. —Peck: p. 299–300, pl. 44, figs 22–24.
Figured specimen: Carapace, T.-K.-Nr. 3178.
Dimensions: length 1.05mm, height 0.64mm, width 0.43mm.
description: Published as part of Bate, Raymond H., Horne, David J., Horne, Sarah E., Douglas, Lyndsey, Miller, Giles & Lord, Alan R., 2022, Non-marine Ostracoda (Crustacea) of the Early Cretaceous ' Pre-Salt' sediments of Brazil: An illustrated catalogue of the type specimens of Wicher, Krömmelbein, Krömmelbein & Weber, and Bate, pp. 1-84 in Zootaxa 5098 (1) on page 9, DOI: 10.11646/zootaxa.5098.1.1, http://zenodo.org/record/6036685
The Appearance of Vortices in Protoplanetary Disks in Near-Infrared Scattered Light
Creators: name: Marr, Metea
name: Dong, Ruobing
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Azimuthally asymmetric structures have been discovered in millimeter continuum emission from many protoplanetary disks. One hypothesis is that they are vortices produced by the Rossby wave instability, for example at edges of planet-opened gaps or deadzones. Confirming the vortex nature of these structures will have profound implications to planet formation. One way to test the hypothesis is to compare the observed morphology of vortex candidates in near-infrared scattered light with theoretical expectations. To this end, we synthesize the appearance of vortices in H-band polarized light by combining hydrodynamic and radiative transfer simulations of the Rossby wave instability at a deadzone edge. In a disk at 140 pc, at the peak in its evolution a vortex at 65 au may appear as a radially narrow arc 50% - 70% brighter compared with an axisymmetric disk model. The contrast depends on the inclination of the disk and the position angle of the vortex only weakly. Such contrast levels are well detectable in imaging observations of bright disks using instruments such as VLT/SPHERE, Subaru/SCExAO, and Gemini/GPI. A vortex also casts a shadow in the outer disk, which may aid its identification. Finally, at modest to high inclinations (e.g., 60 degrees) a vortex may mimic a one-armed spiral. In the HD 34282 disk, such a one-armed spiral with a shadowed region on the outside has been found in scattered light. This feature roughly coincides with an azimuthal asymmetry in mm continuum emission, signifying the presence of a vortex.
description: 10 pages, 7 figures, ApJ accepted
title: Glossary of Ocean Governance Terms
Creators: name: Diz, Daniela
name: Hazin, Carolina
name: Boteler, Ben
name: Durussel, Carole
Publisher: name: Institute for Advanced Sustainability Studies (IASS)
Year: 2022

description: The STRONG High Seas project has published a Glossary of Ocean Governance Terms to provide decision-makers and other stakeholders, including the private sector, scientific communities, civil society, and traditional communities, with a reference lexicon on ocean governance related terms to facilitate understanding when engaging in negotiations and implementation of international and national policies and regulations. As in most areas of knowledge or activity, the field of ocean governance is associated with specialized terminology, or jargon. The use of specific terms is essential for clear communication, particularly among peers, but also to a wider audience. However, as one area becomes more specialized and consequently the use of jargons increases, the challenge for comprehensible communication also grows. A shared understanding of terms by stakeholders engaging in policy instruments is particularly critical. Texts of policy instruments and of decisions (or similar documents, such as Resolutions or measures) under these instruments are, in some cases, legally-binding, which makes States Parties generally abide by them. The same word could have different meaning to different audiences and at different times. Having a common understanding of a term will, therefore, ease communication and, ultimately, help decision-makers achieve agreement in a political context.
title: From coal to renewables in Mpumalanga: Employment effects, opportunities for local value creation, skills requirements, and gender-inclusiveness. Assessing the co-beneﬁts of decarbonising South Africa’s power sector. COBENEFITS Executive Report
Creators: name: Institute for Advanced Sustainability Studies (IASS)
name: International Energy Transition GmbH (IET)
name: Council for Scientiﬁc and Industrial Research (CSIR)
Publisher: name: Institute for Advanced Sustainability Studies (IASS)
Year: 2022

description: This study builds on a unique and hitherto confidential, unpublished set of employee data for Eskom and coal mines, provided by Eskom (under a non-disclosure agreement) and the Mining Quality Authority (MQA). The sourced data sets connect gender, qualification levels, and years of service, thereby enabling analysis of the skills and gender balance in the coal industry, and assessment of the potential for transferring expertise to the renewable energy sector. In addition, interviews were conducted with enterprise development (ED) managers to understand barriers and opportunities for women in the renewables sector. Based on these valuable data sets and economic modelling, the study analyses and quantiﬁes the socio-economic implications of repurposing coal-ﬁred plants in Mpumalanga via deployment of renewable energy. The analysis emphasises opportunities related to job creation, necessary skill development with a focus on gender questions, and regional value creation and industrial opportunities in Mpumalanga. The ﬁndings also highlight important framework conditions necessary for fully harnessing these beneﬁts.
Cypridea acuta Moos
Creators: name: Bate, Raymond H.
name: Horne, David J.
name: Horne, Sarah E.
name: Douglas, Lyndsey
name: Miller, Giles
name: Lord, Alan R.
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Ostracoda
Podocopida
Cyprididae
Cypridea
Cypridea acuta

description: Cypridea acuta Moos in Wicher, 1959
Fig. 1, 11a–c
1959 Cypridea acuta n. sp. —Moos in Wicher, p. 46–47, pl. 9, fig. 3.
Diagnosis: A smooth-shelled Cypridea which is more than twice as long as it is high and whose posterior ventral corner is drawn out to a point.
Holotype: Carapace, T.-K.-Nr. 3179.
Dimensions: Holotype, length c. 1.40mm, height 0.72mm, width c. 0.57mm.
description: Published as part of Bate, Raymond H., Horne, David J., Horne, Sarah E., Douglas, Lyndsey, Miller, Giles & Lord, Alan R., 2022, Non-marine Ostracoda (Crustacea) of the Early Cretaceous ' Pre-Salt' sediments of Brazil: An illustrated catalogue of the type specimens of Wicher, Krömmelbein, Krömmelbein & Weber, and Bate, pp. 1-84 in Zootaxa 5098 (1) on page 9, DOI: 10.11646/zootaxa.5098.1.1, http://zenodo.org/record/6036685
Polarization from Aligned Dust Grains in the $β$ Pic Debris Disk
Creators: name: Hull, Charles L. H.
name: Yang, Haifeng
name: Cortés, Paulo C.
name: Dent, William R. F.
name: Kral, Quentin
name: Li, Zhi-Yun
name: Gouellec, Valentin J. M. Le
name: Hughes, A. Meredith
name: Milli, Julien
name: Teague, Richard
name: Wyatt, Mark C.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present 870 $μ$m ALMA polarization observations of thermal dust emission from the iconic, edge-on debris disk $β$ Pic. While the spatially resolved map does not exhibit detectable polarized dust emission, we detect polarization at the $\sim$3$σ$ level when averaging the emission across the entire disk. The corresponding polarization fraction is $P_\textrm{frac}$ = $0.51 \pm 0.19$%. The polarization position angle $χ$ is aligned with the minor axis of the disk, as expected from models of dust grains aligned via radiative alignment torques (RAT) with respect to a toroidal magnetic field ($B$-RAT) or with respect to the anisotropy in the radiation field ($k$-RAT). When averaging the polarized emission across the outer versus inner thirds of the disk, we find that the polarization arises primarily from the SW third. We perform synthetic observations assuming grain alignment via both $k$-RAT and $B$-RAT. Both models produce polarization fractions close to our observed value when the emission is averaged across the entire disk. When we average the models in the inner versus outer thirds of the disk, we find that $k$-RAT is the likely mechanism producing the polarized emission in $β$ Pic. A comparison of timescales relevant to grain alignment also yields the same conclusion. For dust grains with realistic aspect ratios (i.e., $s > 1.1$), our models imply low grain-alignment efficiencies.
description: 22 pages, 13 figures, 2 tables. Accepted for publication in the Astrophysical Journal. Materials accessible in the online version of the ApJ article include the FITS files used to make the ALMA images
title: Nachhaltigkeit im Brandenburger Strukturwandel. Wie die Lausitz zu einer Modellregion für die Transformation werden könnte
Creators: name: Löw Beer, David
name: Gürtler, Konrad
Publisher: name: Research Institute for Sustainability (RIFS)
Year: 2023

description: Der Strukturwandel in den ehemaligen Braunkohlerevieren wird mit erheb- lichen Bundes- und Landesmitteln gefördert. Sie fließen zum einen als Kompensation für einen vorzeitigen Kohleausstieg. Damit verbunden ist zum anderen der Anspruch, dass Transformationen Erfolg haben können, indem neue Arbeitsplätze sowie lebenswerte und zukunftsfähige Regionen entstehen. Es geht um Nachhaltigkeit im Strukturwandel und nicht nur um den Kohleausstieg. Da es bisher kein Nachhaltigkeitsmonitoring für die Lausitz gibt, lassen sich aufgrund der vorliegen- den Projekte und Projektanträge sowie zahlreicher Gespräche vor Ort nur erste vorsichtige Schlüsse zie- hen. Diese beziehen sich auf die verabschiedeten und vorgeschlagenen Projekte, bei denen das Land Brandenburg die Verantwortung hat (sog. Arm 1-Projekte): Antragsstellende müssen erläutern, wie ihre Projek- te einen positiven Beitrag zu einem ökologischen und einem weiteren der 17 nachhaltigen Entwicklungsziele der Vereinten Nationen leisten. Diese Auflage führte bislang kaum dazu, dass die Projekte einen hohen Nachhaltigkeitsanspruch verfolgen. Hohe Förderquoten würden es bereits jetzt ermög- lichen ambitioniertere Nachhaltigkeitsinvestitionen zu vertretbaren Kosten umzusetzen. Eher günstige geographische und makroökonomische Bedingungen führen dazu, dass viele Projekte auf eine Reduktion von Treibhausgasemissionen bzw. zur Erforschung entsprechender Technologi- en ausgerichtet sind. Mit seinem bisherigen Verfahren verfolgt Brandenburg einen anderen Ansatz als Sachsen, das Nachhaltigkeit in einem Scoring-Verfahren berücksichtigt. Sowohl die Nachhaltigkeitserklärungen als auch die Scoring-Verfahren setzen geringe Nachhaltigkeitsanreize im Vergleich etwa zu EU-Vorgaben. In diesem Policy Brief liefern wir drei umsetzbare und kostengünstige Vorschläge, wie sich die Nach- haltigkeit des Strukturwandels in der brandenburgischen Lausitz verbessern ließe.
title: Technical requirements in public auctions to make solar plants shine
Creators: name: Marian, Adela
name: Münch, Florian Anselm
name: Ammel, Elena
name: Ferdinand, Niels
name: Kumar, Saurabh
name: Ukar, Asier
name: López, Maialen
name: Blind, Knut
name: Quitzow, Rainer
Publisher: name: Institute for Advanced Sustainability Studies (IASS)
Year: 2022

description: The deployment of solar photovoltaic (PV) technology is accelerating across the globe, as prices continue to fall and countries begin their transition from fossil to renewable energy. Public auctions have become the dominant policy tool for solar PV deployment: 106 countries held renewable energy auctions (dominated by solar) by the end of 2018 (IRENA a, 2019). One third of the 55 countries that held renewable auctions in 2017 – 2018 did so for the first time (ibid.). Little solar-specific experience and capacity in newly adopting countries can result in technical failures and lower solar plant performance (IRENA 2017). For instance, it was reported that 30 percent of nearly 100 analysed projects in different countries indicate severe defects that impact performance (TÜV Rheinland 2015). This makes investment in solar plants in newcomer countries risky, hindering the development of the solar sector and undermining political targets of solar energy deployment in these countries. In this context, international organisations have suggested that policymakers in adopting countries include international quality standards1 as technical requirements in the design of public auctions. This policy brief outlines the potential benefits and challenges of doing so, highlighting the crucial role of the Quality Infrastructure (QI) system in newcomer countries. Key lessons learnt are synthesised from international experiences with technical requirements in solar PV auctions. On this basis, entry points are identified for the development of strategies for their introduction in newly adopting countries. The two key things policymakers should consider are the adoption of appropriate standards based on the specific country context and the implementation of real-time data monitoring.
Ion-scale transition of plasma turbulence: Pressure-strain effect
Creators: name: Hellinger, Petr
name: Montagud-Camps, Victor
name: Franci, Luca
name: Matteini, Lorenzo
name: Papini, Emanuele
name: Verdini, Andrea
name: Landi, Simone
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Plasma Physics (physics.plasm-ph)
subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: We investigate properties of solar wind-like plasma turbulence using direct numerical simulations. We analyze the transition from large, magnetohydrodynamic (MHD) scales to the ion characteristic ones using two-dimensional hybrid (fluid electrons, kinetic ions) simulations. To capture and quantify turbulence properties, we apply the Karman-Howarth-Monin (KHM) equation for compressible Hall MHD (extended by considering the plasma pressure as a tensor quantity) to the numerical results. The KHM analysis indicates that the transition from MHD to ion scales (the so called ion break in the power spectrum) results from a combination of an onset of Hall physics and of an effective dissipation owing to the pressure-strain energy-exchange channel and resistivity. We discuss the simulation results in the context of the solar wind.
description: 7 pages, 3 figures
Cypridea (Pseudocypridina) piedmonti Moos
Creators: name: Bate, Raymond H.
name: Horne, David J.
name: Horne, Sarah E.
name: Douglas, Lyndsey
name: Miller, Giles
name: Lord, Alan R.
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Ostracoda
Podocopida
Cyprididae
Cypridea
Cypridea piedmonti

description: Cypridea (Pseudocypridina) piedmonti (Roth, 1933) in Moos in Wicher, 1959
Fig. 1, 12a–c
1933 Pseudocypridina piedmonti n. sp. —Roth, p. 404–405, pl. 48, figs 7a–h.
1935 Cypridea piedmonti (Roth) —Harper & Sutton, p. 625–626, pl. 76, figs 12–15.
1946 Cypridea (Pseudocypridina) piedmonti (Roth) —Swain, p. 550, pl. 83, figs 10–12.
Figured specimen: Carapace, T.-K.-Nr. 3180.
Dimensions: Carapace, T.-K.-Nr. 3180, length 0.70mm, height 0.12, width 0.45mm.
Remarks (Bate et al. herein): No diagnosis was provided and no dimensions were given for specimen Nr 3180 although from the illustration in Wicher (1959, pl. 9, fig. 6) this species appears to be slightly larger than Cypridea kegeli.
description: Published as part of Bate, Raymond H., Horne, David J., Horne, Sarah E., Douglas, Lyndsey, Miller, Giles & Lord, Alan R., 2022, Non-marine Ostracoda (Crustacea) of the Early Cretaceous ' Pre-Salt' sediments of Brazil: An illustrated catalogue of the type specimens of Wicher, Krömmelbein, Krömmelbein & Weber, and Bate, pp. 1-84 in Zootaxa 5098 (1) on page 9, DOI: 10.11646/zootaxa.5098.1.1, http://zenodo.org/record/6036685
Polarization-resolving graphene-based mid-infrared detector
Creators: name: Semkin, Valentin
name: Mylnikov, Dmitry
name: Titova, Elena
name: Zhukov, Sergey
name: Svintsov, Dmitry
Publisher: name: arXiv
Year: 2022
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Applied Physics (physics.app-ph)
subject: FOS: Physical sciences

description: The ability to resolve the polarization of light with on-chip devices represents an urgent problem in optoelectronics. The detectors with polarization resolution demonstrated so far mostly require multiple oriented detectors or movable external polarizers. Here, we experimentally demonstrate the feasibility to resolve the polarization of mid-infrared light with a single chemical-vapor-deposited graphene-channel device with dissimilar metal contacts. This possibility stems from an unusual dependence of photoresponse at graphene-metal junctions on gate voltage and polarization angle. Namely, there exist certain gate voltages providing the polarization-insensitive signal; operation at these voltages can be used for power calibration of the detector. At other gate voltages, the detector features very strong polarization sensitivity, with the ratio of signals for two orthogonal polarizations reaching ~10. Operation at these voltages can provide information about polarization angles, after the power calibration. We show that such unusual gate- and polarization-dependence of photosignal can appear upon competition of isotropic and anisotropic photovoltage generation pathways and discuss the possible physical candidates.
description: 6 pages, 4 figures
Black holes at cosmic dawn in the redshifted 21cm signal of HI
Creators: name: Mirabel, I. Felix
name: Rodriguez, Luis F.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: Indirect insights of Pop III stars and Black Holes (BHs) at Cosmic Dawn (CD) may be imprinted as an absorption signal in the 21cm line of HI against the CMB, when the Universe was less than 200 Myr old. To explain the additional large amplitude of the 21cm HI absorption reported by EDGES there have been proposed models based on an additional synchrotron Cosmic Radio Background (CRB) from BH-jet sources that boost the HI absorption signal at CD. The recent observations of radio loud supermassive BHs (SMBHs) in high-z quasars up to z=7 suggest the existence of a CRB from growing BHs at z > 15, of unknown intensity. To match the onset of the EDGES signal a CRB of comparable intensity to that of the CMB is required. Here we provide approximate calculations to analyze this type of absorption signals, taking that of EDGES as an example. Assuming a BH mass to radio luminosity ratio as observed in radio-loud SMBHs of ~10^9 solar masses in quasars at z = 6-7, we find that rapidly growing radio luminous BHs of Intermediate Mass (IMBHs) in their way to become SMBHs, are the only type of astrophysical radio sources of a CRB that could explain the amplitude of the HI absorption reported by EDGES in the interval of z = 18-20. At those redshifts the EDGES signal would imply that the global mass density of IMBHs must be dominant over that of stars, more than 70% of the maximum Stellar Mass Density (SMD) expected at those high redshifts. This suggests that those IMBHs are formed before and grow faster than the bulk of stars, with no large mass contribution from stellar-mass BH remnants of typical Pop III stars. The highly redshifted signals from these IMBHs may be detected at long radio wavelengths with ultrasensitive interferometers such as the SKA, in the infrared with the JWST, and in the X-rays with future space missions.
description: 34 pages, 2 figures, 1 table. Accepted for publication in New Astronomy Reviews
Gomphocythere forbesii
Creators: name: Bate, Raymond H.
name: Horne, David J.
name: Horne, Sarah E.
name: Douglas, Lyndsey
name: Miller, Giles
name: Lord, Alan R.
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Ostracoda
Podocopida
Limnocytheridae
Gomphocythere
Gomphocythere forbesii

description: Gomphocythere forbesii (Jones, 1885) in Wicher, 1959
Fig. 2, 1a–c
1959 Gomphocythere forbesii (Jones, 1885) subsp.—Wicher, p. 43, pl. 7, fig. 8.
Diagnosis: A subspecies of Gomphocythere forbesii, which partly includes the nodose type.
Holotype: Carapace ♂. T.-K.-Nr. 3174.
Paratypes: Carapaces ♀. T.-K.-Nr 3184, 3185.
Dimensions: Carapace ♂. T.-K.-Nr. 3181, length 0.78mm, height 0.43mm, width 0.38mm (Moos in Wicher, p. 48).
description: Published as part of Bate, Raymond H., Horne, David J., Horne, Sarah E., Douglas, Lyndsey, Miller, Giles & Lord, Alan R., 2022, Non-marine Ostracoda (Crustacea) of the Early Cretaceous ' Pre-Salt' sediments of Brazil: An illustrated catalogue of the type specimens of Wicher, Krömmelbein, Krömmelbein & Weber, and Bate, pp. 1-84 in Zootaxa 5098 (1) on page 9, DOI: 10.11646/zootaxa.5098.1.1, http://zenodo.org/record/6036685
Cultroribula microdentata Krivolutsky 1962
Creators: name: Revelo-Tobar, Harol
name: Ojeda, Margarita
name: García-Ayala, Leonardo J.
name: Palacios-Vargas, José G.
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Sarcoptiformes
Astegistidae
Cultroribula
Cultroribula microdentata

description: Cultroribula microdentata Krivolutsky, 1962
 Distribution: Paleartic and Mexico.
 Records in Mexico: Quintana Roo.
 Biogeographic province: Yucatan Peninsula.
 Habitat: Low flooded forest.
 References: Vázquez & Prieto (2001): 78–79.
description: Published as part of Revelo-Tobar, Harol, Ojeda, Margarita, García-Ayala, Leonardo J. & Palacios-Vargas, José G., 2024, Checklist Of Oribatid Mites (Acari: Oribatida) From Mexico, pp. 1-178 in Zootaxa 5465 (1) on page 83, DOI: 10.11646/zootaxa.5465.1.1, http://zenodo.org/record/11613709
title: Agriculture, Ammonia, and Air Pollution
Creators: name: Von Schneidemesser, Erika
name: Kutzner, Rebecca
name: Muenster, Amrei
name: Staudt, Elisabeth
name: Saar, Dorothee
name: Schaap, Martijn
name: Banzhaf, Sabine
Publisher: name: Institute for Advanced Sustainability Studies (IASS)
Year: 2016

description: IASS Fact Sheet
Seven Years of SN 2014C: a Multi-Wavelength Synthesis of an Extraordinary Supernova
Creators: name: Thomas, Benjamin P.
name: Wheeler, J. Craig
name: Dwarkadas, Vikram V.
name: Stockdale, Christopher
name: Vinko, Jozsef
name: Pooley, David
name: Xu, Yerong
name: Zeimann, Greg
name: MacQueen, Phillip
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: SN 2014C was originally classified as a Type Ib supernova, but at phase ϕ = 127 d post-explosion strong Hα emission was observed. SN 2014C has since been observed in radio, infrared, optical and X-ray bands. Here we present new optical spectroscopic and photometric data spanning ϕ = 947 - 2494 d post-explosion. We address the evolution of the broadened Hα emission line, as well as broad [O III] emission and other lines. We also conduct a parallel analysis of all publicly available multi-wavelength data. From our spectra, we find a nearly constant Hα FWHM velocity width of {\sim}2000 km/s that is significantly lower than that of other broadened atomic transitions ({\sim}3000 - 7000 km/s) present in our spectra ([O I] λ6300; [O III] λλ4959,5007; He I λ7065; [Ca II] λλ7291,7324). The late radio data demand a fast forward shock ({\sim}10,000 km/s at ϕ = 1700 d) in rarified matter that contrasts with the modest velocity of the Hα. We propose that the infrared flux originates from a toroidal-like structure of hydrogen surrounding the progenitor system, while later emission at other wavelengths (radio, X-ray) likely originates predominantly from the reverse shock in the ejecta and the forward shock in the quasi-spherical progenitor He wind. We propose that the Hα emission arises in the boundary layer between the ejecta and torus. We also consider the possible roles of a pulsar and a binary companion.
description: 33 pages, 12 figures
title: Monitoring der globalen Wasserstoffwirtschaft. Konzeptentwurf und Datenquellen
Creators: name: Quitzow, Rainer
name: Jahn, Joschka
name: Marian, Adela
name: Blind, Knut
name: Cremonese, Lorenzo
name: Mbungu, Grace Kageni
name: Neuner, Felix
name: Thielges, Sonja
name: Wietschel, Martin
Publisher: name: Institute for Advanced Sustainability Studies (IASS)
Year: 2022

description: This report presents a framework for the systematic monitoring of the global hydrogen economy. It suggests data sources and indicators to systematically survey the most important trends and developments of a future global hydrogen economy. Monitoring based on this framework could provide an important knowledge base for the continuous review of policy measures related to the German and European hydrogen policy.
description: Im folgenden Bericht wird ein Konzept für ein systematisches Monitoring der globalen Wasserstoffwirtschaft vorgestellt. Der Bericht stellt Datenquellen und Indikatoren zur systematischen Erfassung der wichtigsten Trends und Entwicklungen im Rahmen einer globalen Wasserstoffwirtschaft vor. Ein entsprechendes Monitoring könnte einen wichtigen Beitrag zur kontinuierlichen Überprüfung von Politikmaßnahmen im Rahmen der deutschen und europäischen Wasserstoffpolitik leisten.
Supplementary document for Full Poincaré polarimetry enabled through physical inference - 6025529.pdf
Creators: name: He, Chao
name: Lin, Jianyu
name: Chang, Jintao
name: Antonello, Jacopo
name: Dai, Ben
name: Wang, Jingyu
name: Cui, Jiahe
name: qi, ji
name: Wu, Min
name: Elson, Daniel
Publisher: name: Optica Publishing Group
Year: 2025
Subjects: Uncategorized

description: Supplementary information
Future skills and job creation through renewable energy in Vietnam. Assessing the co-benefits of decarbonising the power sector
Creators: name: Okunlola, Ayodeji
name: Nagel, Laura
name: Helgenberger, Sebastian
name: Thi Khanh, Nguy
name: Thi Mai Dung, Nguyen
name: Kovac, Sarah
name: Green Innovation And Development Centre (GreenID)
Publisher: name: Institute for Advanced Sustainability Studies (IASS)
Year: 2019

description: IASS Study
Mutual Inclination of Ultra-Short-Period Planets with Time Varying Stellar J2-moment
Creators: name: Chen, Chen
name: Li, Gongjie
name: Petrovich, Cristobal
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Systems with ultra-short-period planets (USPs) tend to possess larger mutual inclinations compared to those with planets located farther from their host stars. This could be explained due to precession caused by stellar oblateness at early times when the host star was rapidly spinning. However, stellar oblateness reduces over time due to the decrease in the stellar rotation rate, and this may further shape the planetary mutual inclinations. In this work, we investigate in detail how the final mutual inclination varies under the effect of a decreasing $J_2$. We find that different initial parameters (e.g., the magnitude of $J_2$ and planetary inclinations) will contribute to different final mutual inclinations, providing a constraint on the formation mechanisms of USPs. In general, if the inner planets start in the same plane as the stellar equator (or co-planar while misaligned with the stellar spin-axis), the mutual inclination decreases (or increases then decreases) over time due to the decay of the $J_2$ moment. This is because the inner orbit typically possesses less orbital angular momentum than the outer ones. However, if the outer planet is initially aligned with the stellar spin while the inner one is misaligned, the mutual inclination nearly stays the same. Overall, our results suggest that either the USP planets formed early and acquired significant inclinations (e.g., $\gtrsim30^\circ$ with its companion or $\gtrsim10^\circ$ with its host star spin-axis for Kepler-653c) or they formed late ($\gtrsim$Gyr) when their host stars rotate slower.
description: Accepted for publication in ApJ
title: Carbon Dioxide Removal
Creators: name: Boettcher, Miranda
name: Schäfer, Stefan
name: Honegger, Matthias
name: Low, Sean
name: Lawrence, Mark G.
Publisher: name: Institute for Advanced Sustainability Studies (IASS)
Year: 2017

description: IASS Fact Sheet
description: Despite extensive efforts, greenhouse gases continue to be emitted in vast amounts, with potentially devastating consequences around the world. This is why targeted interventions in the climate system, known collectively as ‘climate engineering’, are receiving increased attention. Proposed approaches are often divided into two groups: those intended to remove carbon dioxide from the atmosphere and those intended to reduce the amount of solar energy that reaches the Earth’s surface or is trapped in the atmosphere. There are some similarities between the two classes of activities, but they often raise different physical, political, and governance concerns. This series provides an introduction to each set of approaches.
Paracypridea Swain 1946
Creators: name: Bate, Raymond H.
name: Horne, David J.
name: Horne, Sarah E.
name: Douglas, Lyndsey
name: Miller, Giles
name: Lord, Alan R.
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Ostracoda
Podocopida
Cyprideidae
Paracypridea

description: PARACYPRIDEA Swain, 1946
Type species: Cypridea (Paracypridea) obovata Swain, 1946
description: Published as part of Bate, Raymond H., Horne, David J., Horne, Sarah E., Douglas, Lyndsey, Miller, Giles & Lord, Alan R., 2022, Non-marine Ostracoda (Crustacea) of the Early Cretaceous ' Pre-Salt' sediments of Brazil: An illustrated catalogue of the type specimens of Wicher, Krömmelbein, Krömmelbein & Weber, and Bate, pp. 1-84 in Zootaxa 5098 (1) on page 10, DOI: 10.11646/zootaxa.5098.1.1, http://zenodo.org/record/6036685
Centrally Concentrated H I Distribution Enhances Star Formation in Galaxies
Creators: name: Yu, Niankun
name: Ho, Luis C.
name: Wang, Jing
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We use a sample of 13,511 nearby galaxies from the ALFALFA and SDSS spectroscopic surveys to study the relation between the spatial distribution of H I 21 cm emission and star formation rate (SFR). We introduce a new non-parametric quantity $K$, measured from the curve-of-growth of the line, to describe the shape of the integrated H I profile. The value of $K$ increases from double-horned to single-peaked profiles, depending on projection effects and the spatial and velocity distribution of the gas. Using carefully chosen samples to control for the competing factors that influence the integrated line profile, we argue that useful inferences can be made on the spatial distribution of the gas. We find that galaxies with a high value of $K$ tend to have more centrally concentrated H I distribution within the optical disk of the galaxy at fixed conditions, and that larger values of $K$ are associated with higher levels of total and central SFR. The results suggest that the global concentration of H I plays an important role in facilitating the conversion of neutral atomic hydrogen to molecular hydrogen gas, which, in turn, affects the star formation activity throughout the optical disk. Our sample is biased against quiescent galaxies, and thus the conclusions may not hold for galaxies with low SFR or low H I content.
description: Accepted by ApJ
title: Kollaborative Klima-Governance in Marburg. Chancen und Hemmnisse auf dem Weg zur Klimaneutralität
Creators: name: Hüncke, Anna
name: Plessing, Julia
name: Ratzmann, Nora
Publisher: name: Institute for Advanced Sustainability Studies (IASS)
Year: 2022

description: Als Teil der kollaborativen Aktionsforschung des Deutsch-Französischen Zukunftswerkes beleuchtet diese Studie die aktuellen Entwicklungen der Universitätsstadt Marburg in ihren Bestrebungen, bis 2030 klimaneutral zu werden. Die Analyse skizziert die Chancen und Herausforderungen lokaler Klimapolitik. Sie zeigt auf, wie trotz einer hohen Motivation seitens der lokalen politischen Führung und der Zivilgesellschaft, die Klimaneutralität zu erreichen, strukturelle Hemmnisse – wie zum Beispiel eine versäulte Verwaltung, Mangel an Kapazitäten und Ressourcen für die Messung des Fortschritts und für strukturierte Beteiligungs- und Kollaborationsmöglichkeiten – die Umsetzung des lokalen Klima-Aktionsplans ausbremsen können. Anhand der Daten über einen Beobachtungszeitraum von einem Jahr erläutert die Analyse ebenso, wie transformative Forschungsansätze, in Form von regelmäßigen Reflektionen mit Akteur:innen vor Ort, lokale Bestrebungen der Klimapolitik unterstützen und vorantreiben können.
description: This paper reflects on how, and under what conditions local transformative change towards climate neutrality can flourish, based on the case of the German city of Marburg, which has committed to become a climate neutral city by 2030. The research findings are drawn from the work of the Franco-German Forum for the Future established in 2020. The Forum seeks to accelerate social and ecological transformation through collaborative action research with pioneering municipalities in France and Germany, through the fostering of dialogue among these initiatives and through the development of political recommendations for the respective national governments. We show how despite a strong political will in Marburg among both political leadership and civil society to act decisively for the achievement of climate neutrality, institutional constraints, such as a lack of flexibility within the local administration, shortage of capacity and resources for the monitoring of progress and the absence of institutionalised mechanisms for citizen participation and collaboration can hamper progress towards achieving the ambitious goals.
Spatially resolved mass-metallicity relation at z~0.26 from the MUSE-Wide Survey
Creators: name: Yao, Yao
name: Chen, Guangwen
name: Liu, Haiyang
name: Chen, Xinkai
name: Lin, Zesen
name: Zhang, Hong-Xin
name: Gao, Yulong
name: Kong, Xu
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Aims: There is a spatially resolved star-forming main sequence (rSFMS) and mass-metallicity relation (rMZR) of galaxies in local universe. We know that the global mass-metallicity relation (MZR) results from the integral of rMZR, and it will evolve with the redshift. However, the evolution of rMZR with redshift is still unclear due to the low spatial resolution and signal-to-noise ratio. There are currently too few observations beyond local universe, and only simulations can reproduce the evolution of rMZR with redshift. Methods: In this work, we select ten emission-line galaxies with an average redshift of $z\sim 0.26$ from MUSE-Wide DR1. We obtain the spatially resolved star formation rate (SFR) and metallicity from the integral field spectroscopy (IFS), as well as the stellar mass surface density from the 3D-HST photometry. We derive the rSFMS and rMZR at $z\sim 0.26$ and compare them with local galaxies. Results: We find the rSFMS of galaxies at $z\sim 0.26$ has a slope of $\sim$0.771. The rMZR exists at $z\sim 0.26$, showing a similar shape to the local universe but a lower average metallicity about $\sim$0.11 dex than the local one. In addition, we also study their spatially resolved fundamental metallicity relation (rFMR). However, there is no obvious evidence that rFMR exists at $z\sim$0.26 and it is not an extension of rMZR at a high SFR. Conclusions: Similar to their global versions, the rSFMS and rMZR of galaxies also evolve with redshift. Given the fixed stellar mass, galaxies at higher redshift show higher SFR and lower metallicity. These suggest that the evolution of the global galaxy properties with redshift may result from integrating the evolution of spatially resolved properties of galaxies.
description: 9 pages, 8 figures, accepted for publication in A&A
title: Zukunftsfonds: Ein Instrument zur klimaverträglichen Gestaltung von Infrastruktur und Unternehmen
Creators: name: Löw Beer, David
name: Schellnhuber, Hans-Joachim
name: Leggewie, Claus
Publisher: name: Institute for Advanced Sustainability Studies (IASS)
Year: 2018

description: IASS Policy Brief
Paracypridea quadrirugosa subsp. quadrirugosa quadrirugosa (Wicher 1959
Creators: name: Bate, Raymond H.
name: Horne, David J.
name: Horne, Sarah E.
name: Douglas, Lyndsey
name: Miller, Giles
name: Lord, Alan R.
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Ostracoda
Podocopida
Cyprideidae
Paracypridea
Paracypridea quadrirugosa
Paracypridea quadrirugosa quadrirugosa (wicher, 1959)

description: Paracypridea quadrirugosa quadrirugosa (Wicher, 1959)
Remarks (Bate et al. herein): Krömmelbein (1961, p. 356) elevates Wicher’s subspecies quadrirugosa to specific rank, placing it in Paracypridea; and then recognizes two subspecies P. quadrirugosa quadrirugosa and P. quadrirugosa weberi; the former is figured in plate 1, figs 1–6 of Krömmelbein’s paper (Form a, SMF Xe 3568; Form b, SMF Xe 3569).
description: Published as part of Bate, Raymond H., Horne, David J., Horne, Sarah E., Douglas, Lyndsey, Miller, Giles & Lord, Alan R., 2022, Non-marine Ostracoda (Crustacea) of the Early Cretaceous ' Pre-Salt' sediments of Brazil: An illustrated catalogue of the type specimens of Wicher, Krömmelbein, Krömmelbein & Weber, and Bate, pp. 1-84 in Zootaxa 5098 (1) on page 10, DOI: 10.11646/zootaxa.5098.1.1, http://zenodo.org/record/6036685
Paracypridea quadrirugosa subsp. weberi Krommelbein 1961
Creators: name: Bate, Raymond H.
name: Horne, David J.
name: Horne, Sarah E.
name: Douglas, Lyndsey
name: Miller, Giles
name: Lord, Alan R.
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Ostracoda
Podocopida
Cyprideidae
Paracypridea
Paracypridea quadrirugosa
Paracypridea quadrirugosa weberi krömmelbein, 1961

description: Paracypridea quadrirugosa weberi Krömmelbein, 1961
1961 Paracypridea quadrirugosa weberi n. ssp. — Krömmelbein, p. 357–358, pl. 2, figs 7–12.
Diagnosis: A large subspecies of Paracypridea quadrirugosa with weak, irregular wrinkled sculpture. Without strongly prominent coarse sculpture like nodes, etc.
Fig. 2, 2a–c
Holotype: Carapace, Form b dimorph, SMF Xe 3661.
Dimensions: Holotype, length 1.82mm, height 1.04mm.
Fig. 2, 3a–c
Paratypes: Carapace, Form a dimorph, SMF Xe.3660; plus 8 carapaces under SMF Xe 3662.
Dimensions: Paratype, Form a dimorph, SMF Xe.3660, length 1.45mm, height 0.93mm.
description: Published as part of Bate, Raymond H., Horne, David J., Horne, Sarah E., Douglas, Lyndsey, Miller, Giles & Lord, Alan R., 2022, Non-marine Ostracoda (Crustacea) of the Early Cretaceous ' Pre-Salt' sediments of Brazil: An illustrated catalogue of the type specimens of Wicher, Krömmelbein, Krömmelbein & Weber, and Bate, pp. 1-84 in Zootaxa 5098 (1) on page 10, DOI: 10.11646/zootaxa.5098.1.1, http://zenodo.org/record/6036685
Landing in Hot Water : Burn Prevention for Young Children
Creators: name: B.C. Injury Research And Prevention Unit
Publisher: name: The University of British Columbia
Year: 2021

description: Burns and scalds are common injuries among young children, often happening in the home environment. These injuries can result from contact with hot water, drinks, or food, or from contact with hot surfaces, such as stoves, ovens, or small appliances. By implementing a few simple strategies in the household, injuries can be prevented.
Gustavia microcephala Nicolet 1855
Creators: name: Revelo-Tobar, Harol
name: Ojeda, Margarita
name: García-Ayala, Leonardo J.
name: Palacios-Vargas, José G.
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Sarcoptiformes
Gustaviidae
Gustavia
Gustavia microcephala

description: Gustavia microcephala Nicolet, 1855
 Distribution: Palearctic, Eastern and Mexico.
 Habitat: Sphagnum sp.
 References: Hammer (1969): 70; Hoffmann & López-Campos (2000): 154; Hoffmann & López-Campos (2002): 274.
 Remarks: The determination of this species is not totally reliable. The authors did not provide the exact location of the collection site for his species reports.
description: Published as part of Revelo-Tobar, Harol, Ojeda, Margarita, García-Ayala, Leonardo J. & Palacios-Vargas, José G., 2024, Checklist Of Oribatid Mites (Acari: Oribatida) From Mexico, pp. 1-178 in Zootaxa 5465 (1) on page 83, DOI: 10.11646/zootaxa.5465.1.1, http://zenodo.org/record/11613709