Since the 1970s, hundreds of khipus—Andean knotted-string recording devices—have been named after academic researchers. This practice disassociates individual khipus from their places of origin and reifies scientific inequity. Here, a new convention of the form KH#### (e.g., KH0125) is proposed, which we believe represents a more neutral, direct, and accurate nomenclature. The change is implemented in the Open Khipu Repository (OKR), the largest khipu database.

Our knowledge of the institutional features of local government in Canadian cities is surprisingly fragmentary. The academic literature has long identified dominant tendencies in Canadian local institutions, but systematic empirical data has been missing. In this article, we address this gap in knowledge in two ways. We introduce the Canadian Municipal Attributes Portal (CMAP), a new open-access database that contains information on dozens of institutional features of local government for nearly 100 of the most populous municipalities in Canada. We then propose a new multidimensional index of authority concentration, which is designed to capture variation in the local structure of decision-making authority in a systematic and nuanced manner. We apply this index to a systematic pan-Canadian subsample of 65 CMAP municipalities. The result is a rich portrait of institutional variety, one that both corroborates and substantially extends our current understanding of the shape of municipal institutions in Canadian cities.

The aim of this paper is to identify scientific content and compilations related to circus arts available in subscription databases and in renowned and free academic information systems. After providing terminological definitions for circus and circus arts, the article describes the search strategies applied and the issues which emerged during the searches, and then introduces quantitative results, thereby also identifying the major periodicals and the most often referenced articles of the topic. The analysis provides useful input for representatives of other arts related to circus arts (e.g., performing arts, theatre arts, visual arts, musical arts) and of other academic fields (e.g., literary studies, history, media science); but first of all, it serves as an unparalleled library information service guide for navigating between electronic information sources.

This paper corresponds to an invited oral contribution to the session 5A organised by the IAU inter-commission B2-B5 working group (WG) “Laboratory Astrophysics Data Compilation, Validation and Standardization: from the Laboratory to FAIR usage in the Astronomical Community” at the IAU 2022 General Assembly (GA) Rengel (2022). This WG provides a platform where to discuss the Findability, Accessibility,Interoperability, Reuse (FAIR) usage of laboratory Atomic and Molecular (A&M) data in astronomy and astrophysics.

A&M data play a key role in the understanding of the physics and chemistry of processes in several research topics, including planetary science and interdisciplinary research in particular the atmospheres of planets and planetary explorations, etc. Databases, compilation of spectroscopic parameters, and facility tools are used by computer codes to interpret spectroscopic observations and simulate them. In this talk I presented existing A&M databases of interest to the planetary community focusing on access, organisation, infrastructures, limitations and issues, etc.

Daily data collection during archaeological fieldwork forms the basis for later interpretation and analysis. Across the world, we observe a wide variety of digital data collection methods and tools employed during fieldwork. Here, we detail the daily practices at four recent survey and excavation projects in the South Caucasian country of Armenia. As archaeology continues to become ever more digital, it is useful to consider these day-to-day recording processes at a typical field project. We provide details on both the types of data collected and the ways they are collected so as to foreground these topics. Finally, we reflect on how our work is currently impacted by digital changes and how it may continue to change in the future.

We review Big Data in Astronomy and its role in Astronomy Education. At present all-sky and large-area astronomical surveys and their catalogued data span over the whole range of electromagnetic spectrum, from gamma-ray to radio, as well as most important surveys giving optical images, proper motions, variability and spectroscopic data. Most important astronomical databases and archives are presented as well. They are powerful sources for many-sided efficient research using the Virtual Observatory (VO) environment. It is shown that using and analysis of Big Data accumulated in astronomy lead to many new discoveries. Using these data gives a significant advantage for Astronomy Education due to its attractiveness and due to big interest of young generation to computer science and technologies. The Computer Science itself benefits from data coming from the Universe and a new interdisciplinary science Astroinformatics has been created to manage these data.

The development of chronologies relies on integrating information from a number of different sources. In addition to direct dating evidence, such as radiocarbon dates, researchers will have contextual information which might be an environmental sequence or the context in an archaeological site. This information can be combined through Bayesian or other types of age-model. Once a chronology has been developed, this information can be used to estimate, for example, chronological uncertainties, rates of change, or the age of material which has not been directly dated.

Dealing with the information associated with chronology building is complicated and re-evaluation of chronologies often requires structured information which is hard to access. Although there are many databases with primary dating information, these often do not contain all of the information needed for a chronology. The Chronological Query Language (CQL) developed for OxCal was intended to be a convenient way of pulling such information together for Bayesian analysis. However, even this does not include much of the associated information required for reusing data in other analyses.

The IntChron initiative builds on the framework set up for the INTIMATE (Integrating Ice core, Marine and Terrestrial Records) chronological database (Bronk Ramsey et al. 2014) and is primarily an information exchange format and data visualization tool which enables users to pull together the types of information needed for chronological analysis. It is intended for use with multiple dating methodologies and while it will be integrated with OxCal, is intended to be an open format suitable for use with other software tools. The file format is JSON which is easily readable in software such as R, Python and MatLab. IntChron is not primarily intended to be a data depository but rather an index of sites where information is stored in the relevant format. As an initial step, databases of radiocarbon dates from the Oxford Radiocarbon Accelerator Unit (including those for the NERC radiocarbon facility), the RESET tephra database, the INTIMATE chronological database and regional radiocarbon databases for Egypt and Southern Africa are all linked. The intention is that users of OxCal will also be able to make published data accessible to others and to store working data, visible only to the user, to be used with the associated analysis tools. The IntChron site allows data from third party sources to be accessed through a representational state transfer (REST) application programming interface (API) in a number of different formats (JSON, csv, txt, oxcal) and associated bibliographic information in BibTeX format.

The aim of the IntChron initiative is to make it easy for users to provide data (in the single JSON format with limited minimum requirements) as well as to access data and tools, while promoting robust chronologies including realistic estimates of uncertainties. It is hoped that this will help to bring the chronological research communities to a point where data access is as easy as it is in some other fields. This is particularly important for Early Career Researchers and for those seeking to use large datasets in novel ways.

Since the beginning of the century, the digitization of medieval manuscripts has been a major concern of institutions in the possession of such material. This has led to the massive production of digital surrogates for online display. Preservation condition and temporal and spatial limitations are no longer restrictions for accessing these objects, making them easily available to a potentially larger public than before. The databases created for hosting the surrogates are designed for different categories of audience, with various standards in mind and different levels of technical sophistication. Although primarily accessed for the texts they bear, the digital surrogates of manuscripts are also the object of study of a specialized group of users interested in their physical features. This review will discuss whether databases that comprise digital surrogates of Greek New Testament manuscripts built by different types of institutions are efficient in addressing the needs of this admittedly small audience. I examine questions of content, interface, organization, and rationales behind the choices of their creators.