cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.15156/bio/sh1283975.09fu
title: SH1283975.09FU

description: UNITE provides a unified way for delimiting, identifying, communicating, and working with DNA-based Species Hypotheses (SH). All fungal ITS sequences in the international nucleotide sequence databases are clustered to approximately the species level by applying a set of dynamic distance values (<0.5 - 3.0%). All species hypotheses are given a unique, stable name in the form of a DOI, and their taxonomic and ecological annotations are verified through distributed, web-based third-party annotation efforts. SHs are connected to a taxon name and its classification as far as possible (phylum, class, order, etc.) by taking into account identifications for all sequences in the SH. An automatically or manually designated sequence is chosen to represent each such SH. These sequences are released (https://unite.ut.ee/repository.php) for use by the scientific community in, for example, local sequence similarity searches and next-generation sequencing analysis pipelines. The system and the data are updated automatically as the number of public fungal ITS sequences grows.
DOI: 10.57780/esa-8mmp22b
title: 16068

description: We propose to make a Chandra observation of a newly discovered high mass comma  low density globular cluster. This cluster has properties largely similar to that of Omega Centauri in terms of its stellar mass and its ratio of tidal to core radius comma  but its characteristic radii are a factor of about 3 larger than Omega Cen.s. As a result comma  this is the first Milky Way cluster for which the stellar density is small enough that dynamical formation and destruction of close binaries will be unimportant comma  while having a large enough stellar mass that it can be expected to show some interacting binaries anyway. It will be the first object that can be used to characterize the baseline rate of production of these systems in a low metallicity comma  old stellar population.
DOI: 10.15156/bio/sh1283976.09fu
title: SH1283976.09FU

description: UNITE provides a unified way for delimiting, identifying, communicating, and working with DNA-based Species Hypotheses (SH). All fungal ITS sequences in the international nucleotide sequence databases are clustered to approximately the species level by applying a set of dynamic distance values (<0.5 - 3.0%). All species hypotheses are given a unique, stable name in the form of a DOI, and their taxonomic and ecological annotations are verified through distributed, web-based third-party annotation efforts. SHs are connected to a taxon name and its classification as far as possible (phylum, class, order, etc.) by taking into account identifications for all sequences in the SH. An automatically or manually designated sequence is chosen to represent each such SH. These sequences are released (https://unite.ut.ee/repository.php) for use by the scientific community in, for example, local sequence similarity searches and next-generation sequencing analysis pipelines. The system and the data are updated automatically as the number of public fungal ITS sequences grows.
DOI: 10.57780/esa-8oa2366
title: 16226

description: Environment is thought to play a central role in quenching low-mass dwarf galaxies. However comma  an increasing number of dwarf galaxies discovered in isolation suggest that mechanisms other than environment can quench dwarf galaxies. Here comma  we propose deep WFC3-F395N (Ca H  and  K) imaging to measure metallicites (virgul0.1-0.2 dex) for hundreds of individual stars in Cetus and Tucana comma  the two nearest examples of isolated quenched dwarf galaxies. Our Ca H  and  K photometry will provide an order-of-magnitude increase in the number of stars in each systems with reliable metallicities (from virgul40 to 400) comma  enabling the first detailed study of the metallicity distribution functions (MDFs) comma  and the physics they encode comma  in isolated quenched dwarf galaxies. Specifically comma  we will (1) construct and characterize detailed MDFs for Cetus and Tucana from a number of stars comparable to MW satellites  (2) use our MDFs to differentiate between signatures of external vs internal quenching in low-mass galaxies  and (3) combine our MDFs comma  HST-based SFHs comma  and HST-based proper motions (and orbital histories) to complete our knowledge of these enigmatic galaxies. formation histories.      This program will provide qualitatively new insight into how and why isolated low-mass galaxies stop forming stars. The construction of MDFs in such distant systems is only possible due to the excellent blue-sensitivity and angular resolution of HST -- no other ground- or space-based facility can acquire this data. This novel use of HST will establish it as a leader for measuring stellar metallicities in galaxies located at large distances from the Milky Way.
DOI: 10.57780/esa-8sdp7eb
title: 16591

description: The Space Telescope Science Institute (STScI) Director has decided to devote up to 1000 orbits of Director.s Discretionary time in observing Cycles 27-29 to a new Hubble Ultraviolet Legacy program focused on star formation and associated stellar physics. This new program comma  ULLYSES (UV Legacy Library of Young Stars as Essential Standards) comma  will provide a UV spectroscopic reference sample of young (< 10 Myr) high- and low-mass stars. It will target virgul165 OB stars in the Magellanic Clouds and lower metallicity galaxies in the Local Group comma  and virgul67 T Tauri stars and brown dwarfs in the Milky Way. In addition comma  ULLYSES will monitor 4 typical T Tauri stars over different rotational phases through at least three rotation periods comma  and over timescales of months to years. The resulting library will provide template spectra of massive stars at metallicities substantially below the well studied comma  while the low mass sample will cover a wide range of ages comma  accretion rates comma  and masses comma  including objects down to well below 0.5 M_sun. The legacy of this large UV dataset on the first 10 Myr of stellar evolution will be enhanced by complementary datasets obtained by the scientific community. In addition to the core goals of the program related to stellar astrophysics of low and high mass stars comma  this data will also enable exciting science in the fields of ISM comma  CGM comma  jets comma  and exoplanets. ULLYSES will be modeled after the Frontier Fields programdoublePoint all data obtained will be non-proprietary. The implementation team at STScI is developing high-level science data products and a sophisticated database and website for disseminating data from the ULLYSES program and ancillary datasets for the ULLYSES target sample from space and ground-based facilities.
DOI: 10.15156/bio/sh1283977.09fu
title: SH1283977.09FU

description: UNITE provides a unified way for delimiting, identifying, communicating, and working with DNA-based Species Hypotheses (SH). All fungal ITS sequences in the international nucleotide sequence databases are clustered to approximately the species level by applying a set of dynamic distance values (<0.5 - 3.0%). All species hypotheses are given a unique, stable name in the form of a DOI, and their taxonomic and ecological annotations are verified through distributed, web-based third-party annotation efforts. SHs are connected to a taxon name and its classification as far as possible (phylum, class, order, etc.) by taking into account identifications for all sequences in the SH. An automatically or manually designated sequence is chosen to represent each such SH. These sequences are released (https://unite.ut.ee/repository.php) for use by the scientific community in, for example, local sequence similarity searches and next-generation sequencing analysis pipelines. The system and the data are updated automatically as the number of public fungal ITS sequences grows.
DOI: 10.57780/esa-8t9t09n
title: 16958

description: Test the repeatibility of the slit wheel by taking a sequence of comparison lamp spectra with grating G230MB (2697) and the three smallest long slits (52X0.2 comma  52X0.1 comma  and 52X0.05). This is a clone of Cycle 29 Program 16557.
DOI: 10.15156/bio/sh1283978.09fu
title: SH1283978.09FU

description: UNITE provides a unified way for delimiting, identifying, communicating, and working with DNA-based Species Hypotheses (SH). All fungal ITS sequences in the international nucleotide sequence databases are clustered to approximately the species level by applying a set of dynamic distance values (<0.5 - 3.0%). All species hypotheses are given a unique, stable name in the form of a DOI, and their taxonomic and ecological annotations are verified through distributed, web-based third-party annotation efforts. SHs are connected to a taxon name and its classification as far as possible (phylum, class, order, etc.) by taking into account identifications for all sequences in the SH. An automatically or manually designated sequence is chosen to represent each such SH. These sequences are released (https://unite.ut.ee/repository.php) for use by the scientific community in, for example, local sequence similarity searches and next-generation sequencing analysis pipelines. The system and the data are updated automatically as the number of public fungal ITS sequences grows.
DOI: 10.57780/esa-8tlz7hi
title: 16642

description: In just 25 years comma  we went from not knowing if the solar system is a fluke of Nature to realising that it is totally normal for stars to have planets. More remarkably comma  it is now clear that planet formation is a  robust process comma  as rich multi-planet systems are found around stars more massive and less massive than the Sun. More recently comma  planetary systems  have been identified in increasingly complex architectures comma  including circumbinary planets comma  wide binaries with planets orbiting one or both stellar components comma  and planets in triple stellar systems.  We have also learned that many planetary systems will survive the evolution of their host stars into the white dwarf phase. Small bodies are scattered by unseen planets into the gravitational field of the white dwarfs comma  tidally disrupt comma  form dust discs comma  and eventually accrete onto the white dwarf comma  where they can be spectroscopically detected. HST-COS has played a critical role in the study these evolved planetary systems comma  demonstrating that overall the bulk composition of the debris is rocky and resembles in composition the inner the solar system comma  including evidence for water-rich planetesimals.   Past observations of planetary systems at white dwarfs were limited to biased and incomplete samples. Here we propose a legacy HST survey of all white dwarfs within 100pc identified with Gaia to answer the following questionsdoublePoint  * How efficient is planet formation around 2-10Msun starsquestionMark  * What are the metallicities of the progenitors of debris-accreting white dwarfsquestionMark * What is the fate of circumbinary planetsquestionMark * Can star-planet interactions generate magnetic fields in the white dwarf hostquestionMark
DOI: 10.57780/esa-8yu1r14
title: 16369

description: The Space Telescope Science Institute (STScI) Director has decided to devote up to 1000 orbits of Director.s Discretionary time in observing Cycles 27-29 to a new Hubble Ultraviolet Legacy program focused on star formation and associated stellar physics. This new program comma  ULLYSES (UV Legacy Library of Young Stars as Essential Standards) comma  will provide a UV spectroscopic reference sample of young (< 10 Myr) high- and low-mass stars. It will target over virgul150 OB stars in the Magellanic Clouds and lower metallicity galaxies in the Local Group comma  and virgul40 T Tauri stars and brown dwarfs in the Milky Way. In addition comma  ULLYSES will monitor 4 typical T Tauri stars over different rotational phases through at least three rotation periods comma  and over timescales of months to years. The resulting library will provide template spectra of massive stars at metallicities substantially below the well studied comma  while the low mass sample will cover a wide range of ages comma  accretion rates comma  and masses comma  including objects down to well below 0.5 M_sun. The legacy of this large UV dataset on the first 10 Myr of stellar evolution will be enhanced by complementary datasets obtained by the scientific community. In addition to the core goals of the program related to stellar astrophysics of low and high mass stars comma  this data will also enable exciting science in the fields of ISM comma  CGM comma  jets comma  and exoplanets. ULLYSES will be modeled after the Frontier Fields programdoublePoint all data obtained will be non-proprietary. The implementation team at STScI is developing high-level science data products and a sophisticated database and website for disseminating data from the ULLYSES program and ancillary datasets for the ULLYSES target sample from space and ground-based facilities.
DOI: 10.15156/bio/sh1283979.09fu
title: SH1283979.09FU

description: UNITE provides a unified way for delimiting, identifying, communicating, and working with DNA-based Species Hypotheses (SH). All fungal ITS sequences in the international nucleotide sequence databases are clustered to approximately the species level by applying a set of dynamic distance values (<0.5 - 3.0%). All species hypotheses are given a unique, stable name in the form of a DOI, and their taxonomic and ecological annotations are verified through distributed, web-based third-party annotation efforts. SHs are connected to a taxon name and its classification as far as possible (phylum, class, order, etc.) by taking into account identifications for all sequences in the SH. An automatically or manually designated sequence is chosen to represent each such SH. These sequences are released (https://unite.ut.ee/repository.php) for use by the scientific community in, for example, local sequence similarity searches and next-generation sequencing analysis pipelines. The system and the data are updated automatically as the number of public fungal ITS sequences grows.
DOI: 10.5281/zenodo.7852343
title: Data set Quality of Life Autism

description: Data set for Quality of life of Families of Children with Autism Spectrum Disorders in Jordan.
DOI: 10.57780/esa-8z02i40
title: 16825

description: The Space Telescope Science Institute (STScI) Director has decided to devote up to 1000 orbits of Director.s Discretionary time in observing Cycles 27-29 to a new Hubble Ultraviolet Legacy program focused on star formation and associated stellar physics. This new program comma  ULLYSES (UV Legacy Library of Young Stars as Essential Standards) comma  will provide a UV spectroscopic reference sample of young (< 10 Myr) high- and low-mass stars. It will target over virgul150 OB stars in the Magellanic Clouds and lower metallicity galaxies in the Local Group comma  and virgul40 T Tauri stars and brown dwarfs in the Milky Way. In addition comma  ULLYSES will monitor 4 typical T Tauri stars over different rotational phases through at least three rotation periods comma  and over timescales of months to years. The resulting library will provide template spectra of massive stars at metallicities substantially below the well studied comma  while the low mass sample will cover a wide range of ages comma  accretion rates comma  and masses comma  including objects down to well below 0.5 M_sun. The legacy of this large UV dataset on the first 10 Myr of stellar evolution will be enhanced by complementary datasets obtained by the scientific community. In addition to the core goals of the program related to stellar astrophysics of low and high mass stars comma  this data will also enable exciting science in the fields of ISM comma  CGM comma  jets comma  and exoplanets. ULLYSES will be modeled after the Frontier Fields programdoublePoint all data obtained will be non-proprietary. The implementation team at STScI is developing high-level science data products and a sophisticated database and website for disseminating data from the ULLYSES program and ancillary datasets for the ULLYSES target sample from space and ground-based facilities.
DOI: 10.15156/bio/sh1283980.09fu
title: SH1283980.09FU

description: UNITE provides a unified way for delimiting, identifying, communicating, and working with DNA-based Species Hypotheses (SH). All fungal ITS sequences in the international nucleotide sequence databases are clustered to approximately the species level by applying a set of dynamic distance values (<0.5 - 3.0%). All species hypotheses are given a unique, stable name in the form of a DOI, and their taxonomic and ecological annotations are verified through distributed, web-based third-party annotation efforts. SHs are connected to a taxon name and its classification as far as possible (phylum, class, order, etc.) by taking into account identifications for all sequences in the SH. An automatically or manually designated sequence is chosen to represent each such SH. These sequences are released (https://unite.ut.ee/repository.php) for use by the scientific community in, for example, local sequence similarity searches and next-generation sequencing analysis pipelines. The system and the data are updated automatically as the number of public fungal ITS sequences grows.
DOI: 10.5281/zenodo.7852342
title: Data set Quality of Life Autism

description: Data set for Quality of life of Families of Children with Autism Spectrum Disorders in Jordan.
DOI: 10.57780/esa-90vddj0
title: 17094

description: Highly irradiated gas-giant exoplanets vigorously lose their atmospheres.  This makes them excellent laboratories for extreme atmospheric physics - where we can study the effect of high levels of irradiation and stellar wind. Despite decades of observations with HST comma  the scientific value of the Lyman-alpha detections remains surprisingly under-exploited. In particular comma  the observations have not yet been able to precisely quantify planetary mass-loss rates. To address the gap between Lyman-alpha models and observations comma  a new observational pathway has been proposed to untangle the web of parameter interdependency.  Originally identified in the 3D radiative-hydrodynamic simulations comma  this method requires measuring the second Lyman-alpha transits that are predicted to occur for hot Jupiters after the main transit. Second Lyman-alpha transits have never yet been probed or observed comma  despite this theoretical prediction. By measuring the time-delay of the secondary transit comma  the strength of the acceleration mechanism and the inertia of the outflowing gas can be measured comma  which is set by the mass loss rate. Thus comma  a measurement of a hot Jupiter.s secondary transit will allow us to break the degeneracies that have plagued interpretation of Lyman-alpha transits comma  bringing firm physical constraints which will finally allow us to observationally comma  qualitatively constrain the mass-loss rate of an exoplanet.
DOI: 10.57780/esa-913cscd
title: 17080

description: Located at 2.2 pc comma  the virgul250K Y2 (sub-)brown dwarf WISE J085510.83-071442.5 is the fourth closest known system to Earth. Studying this object provides unique insights into brown dwarf (and exoplanet) atmospheric properties comma  thermal evolution comma  multiplicity comma  and planet-hosting prospects.  We propose to use HST to obtain one the most accurate annual parallax of this - or any - planetary-mass brown dwarf to date comma  achieving an unprecedented accuracy of 200 micro-arcseconds comma  and constraining its absolute space motion to equivalent accuracy. More importantly comma  we will be able to search for faint companions co-moving with the target comma  either resolved or through astrometric perturbations of its linear motion comma  the latter probing down to a few Earth masses.  HST is the optimal facility for precision astrometric measurement of WISE 0855-0714 comma  as this source is too cool and faint at optical and near-infrared wavelengths to observe with ground-based facilities or Gaia. Our observations will improve current astrometric precision of this source by a factor of 40 and anchor future JWST measurements of this and other cold brown dwarfs comma  while providing high-precision distance and motion measurements and tight constraints on planetary-mass companions for one of the closest ''stellar object.. to the Sun.
DOI: 10.15156/bio/sh1283981.09fu
title: SH1283981.09FU

description: UNITE provides a unified way for delimiting, identifying, communicating, and working with DNA-based Species Hypotheses (SH). All fungal ITS sequences in the international nucleotide sequence databases are clustered to approximately the species level by applying a set of dynamic distance values (<0.5 - 3.0%). All species hypotheses are given a unique, stable name in the form of a DOI, and their taxonomic and ecological annotations are verified through distributed, web-based third-party annotation efforts. SHs are connected to a taxon name and its classification as far as possible (phylum, class, order, etc.) by taking into account identifications for all sequences in the SH. An automatically or manually designated sequence is chosen to represent each such SH. These sequences are released (https://unite.ut.ee/repository.php) for use by the scientific community in, for example, local sequence similarity searches and next-generation sequencing analysis pipelines. The system and the data are updated automatically as the number of public fungal ITS sequences grows.
DOI: 10.57780/esa-91sg996
title: 16689

description: Here comma  we propose to conduct a campaign to obtain HST STIS ultraviolet spectroscopy of 15 confirmed ultracompact binary systems discovered using the Zwicky Transient Facility. These observations will be used as a sensitive tool to measure the temperature and other physical properties in these systems comma  and will serve as a sensitive probe of accretion.
DOI: 10.15156/bio/sh1283982.09fu
title: SH1283982.09FU

description: UNITE provides a unified way for delimiting, identifying, communicating, and working with DNA-based Species Hypotheses (SH). All fungal ITS sequences in the international nucleotide sequence databases are clustered to approximately the species level by applying a set of dynamic distance values (<0.5 - 3.0%). All species hypotheses are given a unique, stable name in the form of a DOI, and their taxonomic and ecological annotations are verified through distributed, web-based third-party annotation efforts. SHs are connected to a taxon name and its classification as far as possible (phylum, class, order, etc.) by taking into account identifications for all sequences in the SH. An automatically or manually designated sequence is chosen to represent each such SH. These sequences are released (https://unite.ut.ee/repository.php) for use by the scientific community in, for example, local sequence similarity searches and next-generation sequencing analysis pipelines. The system and the data are updated automatically as the number of public fungal ITS sequences grows.
DOI: 10.57780/esa-9366yqu
title: 16976

description: The stability of the CCD flat fields will be monitored using the calibration lamps. One set of observations for all the filters and another at a different epoch for a subset of filters will be taken during this cycle. High signal observations will be used to assess the stability of the pixel-to-pixel flat field structure comma  to analyze image artifacts such as the newly discovered flecks comma  and to monitor the position of the dust motes.
DOI: 10.57780/esa-93hqc58
title: 16346

description: CTE measurements are made using the d_commainternal sparse field testd_comma comma  along the  parallel axis. The d_commaPOS=d_comma optional parameter comma  introduced during cycle 11 comma  is  used to provide off-center MSM positioning of some slits.  Various optical elements and exposure times are used to achieve 6 different flux levels.  This gain=4 program is alternated with a gain=1 program annually.  All  exposures are internals.