Speech community formation : a sociolinguistic profile of the Trio of Suriname

Overview of the Trio language. Brings together both extralinguistic factors, such as historical, economic, sociological and cultural factors that have and still contribute to the present-day status of the Trio Amerindians and their language and internal sociolinguistic factors, that is, factors that influence the choice of what the Trio speak to whom, how, and when. Shows that Trio sociolinguistically-speaking is in a strong position

Truth and knowledge markers in Wayana (Cariban), Suriname

"‘Truth and knowledge markers’ is the term used to group together a seemingly disparate set of grammatical markers that is pervasive in the Cariban, and also in some Arawakan languages of the Guianas in South America. Themarkers in question express epistemological ideas of realities and truths. In the existing grammatical descriptions, at best, a formal description of the morphemes in question as emphatic, similative, and frustrative markers may be found scattered through various parts of the morphology, where they are dealt with in a structural manner; however, what is needed, besides a structural analysis, is a systematic look at and detailed analysis of their semantic, pragmatic and indeed philosophical import, both as separate morphological items and also collectively as a systemof truth and realitymarkers. In this contribution,Wayana data are presented to exemplify at least parts of this system

The verbalizers in Trio (Cariban): a semantic description

"Trio has a range of verbalizers, many with aspectual meanings, which are suffixed to a nominal to form a verb. Some of the verbalizers are more productive than others; some result in a transitive, others in an intransitive verb. This paper deals in particular with the semantics of the verbalizers showing how much cultural information can be gleaned from the specific semantics of both the verbalizers and the resultant verbs

What’s in a verb? Studies in the verbal morphology of the languages of the Americas

Verbal morphology tends to be the most complex part of the grammatical structure of indigenous American languages. Studies in this volume look into the structural complexity that verbal forms can exhibit on the American continent and into the morphological categories that have attracted researchers’ special attention. Unlike most other volumes on indigenous American languages, the present collection overrides regional boundaries and addresses interesting morphological phenomena across North, Central, and South America. Moreover, it pays tribute to the long-standing tradition of Dutch and the Netherlands-based linguists working in the Americas and gives an overview of current Dutch involvement in the study of these languages. This volume is a collection of articles presenting original fieldwork or novel comparative or historical research, often on little-known languages and phenomena and illustrated with unique data. Each contribution provides a brief outline of the verbal morphology of the language under consideration and an in-depth analysis of a selected topic. This volume will be of particular interest to general linguists, typologists, linguistic experts as well as students with an interest in morphosyntax and morphophonology, and in the languages of the Americas in general

NANCY: Next-generation All-sky Near-infrared Community surveY

International audienceThe Nancy Grace Roman Space Telescope is capable of delivering an unprecedented all-sky, high-spatial resolution, multi-epoch infrared map to the astronomical community. This opportunity arises in the midst of numerous ground- and space-based surveys that will provide extensive spectroscopy and imaging together covering the entire sky (such as Rubin/LSST, Euclid, UNIONS, SPHEREx, DESI, SDSS-V, GALAH, 4MOST, WEAVE, MOONS, PFS, UVEX, NEO Surveyor, etc.). Roman can uniquely provide uniform high-spatial-resolution (~0.1 arcsec) imaging over the entire sky, vastly expanding the science reach and precision of all of these near-term and future surveys. This imaging will not only enhance other surveys, but also facilitate completely new science. By imaging the full sky over two epochs, Roman can measure the proper motions for stars across the entire Milky Way, probing 100 times fainter than Gaia out to the very edge of the Galaxy. Here, we propose NANCY: a completely public, all-sky survey that will create a high-value legacy dataset benefiting innumerable ongoing and forthcoming studies of the universe. NANCY is a pure expression of Roman's potential: it images the entire sky, at high spatial resolution, in a broad infrared bandpass that collects as many photons as possible. The majority of all ongoing astronomical surveys would benefit from incorporating observations of NANCY into their analyses, whether these surveys focus on nearby stars, the Milky Way, near-field cosmology, or the broader universe

NANCY: Next-generation All-sky Near-infrared Community surveY

International audienceThe Nancy Grace Roman Space Telescope is capable of delivering an unprecedented all-sky, high-spatial resolution, multi-epoch infrared map to the astronomical community. This opportunity arises in the midst of numerous ground- and space-based surveys that will provide extensive spectroscopy and imaging together covering the entire sky (such as Rubin/LSST, Euclid, UNIONS, SPHEREx, DESI, SDSS-V, GALAH, 4MOST, WEAVE, MOONS, PFS, UVEX, NEO Surveyor, etc.). Roman can uniquely provide uniform high-spatial-resolution (~0.1 arcsec) imaging over the entire sky, vastly expanding the science reach and precision of all of these near-term and future surveys. This imaging will not only enhance other surveys, but also facilitate completely new science. By imaging the full sky over two epochs, Roman can measure the proper motions for stars across the entire Milky Way, probing 100 times fainter than Gaia out to the very edge of the Galaxy. Here, we propose NANCY: a completely public, all-sky survey that will create a high-value legacy dataset benefiting innumerable ongoing and forthcoming studies of the universe. NANCY is a pure expression of Roman's potential: it images the entire sky, at high spatial resolution, in a broad infrared bandpass that collects as many photons as possible. The majority of all ongoing astronomical surveys would benefit from incorporating observations of NANCY into their analyses, whether these surveys focus on nearby stars, the Milky Way, near-field cosmology, or the broader universe

NANCY: Next-generation All-sky Near-infrared Community surveY

International audienceThe Nancy Grace Roman Space Telescope is capable of delivering an unprecedented all-sky, high-spatial resolution, multi-epoch infrared map to the astronomical community. This opportunity arises in the midst of numerous ground- and space-based surveys that will provide extensive spectroscopy and imaging together covering the entire sky (such as Rubin/LSST, Euclid, UNIONS, SPHEREx, DESI, SDSS-V, GALAH, 4MOST, WEAVE, MOONS, PFS, UVEX, NEO Surveyor, etc.). Roman can uniquely provide uniform high-spatial-resolution (~0.1 arcsec) imaging over the entire sky, vastly expanding the science reach and precision of all of these near-term and future surveys. This imaging will not only enhance other surveys, but also facilitate completely new science. By imaging the full sky over two epochs, Roman can measure the proper motions for stars across the entire Milky Way, probing 100 times fainter than Gaia out to the very edge of the Galaxy. Here, we propose NANCY: a completely public, all-sky survey that will create a high-value legacy dataset benefiting innumerable ongoing and forthcoming studies of the universe. NANCY is a pure expression of Roman's potential: it images the entire sky, at high spatial resolution, in a broad infrared bandpass that collects as many photons as possible. The majority of all ongoing astronomical surveys would benefit from incorporating observations of NANCY into their analyses, whether these surveys focus on nearby stars, the Milky Way, near-field cosmology, or the broader universe

NANCY: Next-generation All-sky Near-infrared Community surveY

International audienceThe Nancy Grace Roman Space Telescope is capable of delivering an unprecedented all-sky, high-spatial resolution, multi-epoch infrared map to the astronomical community. This opportunity arises in the midst of numerous ground- and space-based surveys that will provide extensive spectroscopy and imaging together covering the entire sky (such as Rubin/LSST, Euclid, UNIONS, SPHEREx, DESI, SDSS-V, GALAH, 4MOST, WEAVE, MOONS, PFS, UVEX, NEO Surveyor, etc.). Roman can uniquely provide uniform high-spatial-resolution (~0.1 arcsec) imaging over the entire sky, vastly expanding the science reach and precision of all of these near-term and future surveys. This imaging will not only enhance other surveys, but also facilitate completely new science. By imaging the full sky over two epochs, Roman can measure the proper motions for stars across the entire Milky Way, probing 100 times fainter than Gaia out to the very edge of the Galaxy. Here, we propose NANCY: a completely public, all-sky survey that will create a high-value legacy dataset benefiting innumerable ongoing and forthcoming studies of the universe. NANCY is a pure expression of Roman's potential: it images the entire sky, at high spatial resolution, in a broad infrared bandpass that collects as many photons as possible. The majority of all ongoing astronomical surveys would benefit from incorporating observations of NANCY into their analyses, whether these surveys focus on nearby stars, the Milky Way, near-field cosmology, or the broader universe