cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.15156/bio/sh1284209.09fu
title: SH1284209.09FU

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-pt0x63j
title: 16180

description: Eclipse mapping is an observational technique that uniquely measures an exoplanet.s thermal structure as a function of both latitude and longitude. Multiwavelength eclipse maps provide an unprecedented view of a planet.s three-dimensional dynamics comma  thermal structure comma  chemistry comma  and energetics. Here we propose to produce the first spectroscopic eclipse map of an exoplanet via observations of the best-studied hot Jupiter comma  HD 189733b comma  from 1.1-1.7 microns with WFC3-G141. These observations will measure the geographic distribution of dayside emission over these wavelengths comma  thereby constraining the global circulation patterns and relevant atmospheric timescales in HD 189733b with latitude comma  longitude and altitude. When combined with published Spitzer-IRAC mid-IR photometric phase curves and eclipse maps comma  our proposed WFC3 spectroscopic eclipse maps will paint the most detailed and complete picture to date of weather deep in a hot Jupiter atmosphere comma  refining general circulation models that aim to predict their climate. In addition comma  our proposed eclipse mapping observations will serve as the foundation upon which future observational and theoretical frameworks will interpret future spectroscopic eclipse maps with HST and of considerably smaller and cooler planets with JWST.
DOI: 10.15156/bio/sh1284210.09fu
title: SH1284210.09FU

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-ptuyqwi
title: 17021

description: This is a continuation of programs 11433 (SMOV) comma  11915 (Cy 17) comma  12338 (Cy 18) comma  12712 (Cy 19) comma  13098 (Cy 20) comma  13587 (Cy 21) comma  14029 (Cy 22) comma  14391 (Cy23) comma  14548 (Cy24) comma  14998 (Cy25) comma  15591 (Cy26) comma  15731 (Cy27) comma  16411 (Cy28) comma  and 16586 (Cy29). We study the stability and structure of the IR channel flat field images through all filter elements.  Flats are monitored comma  to capture any temporal trends and delta flats are produced.  High signal observations will provide a map of the pixel-to-pixel flat field structure comma  as well as identify the positions of any dust particles.  This version contains a full set of IR filter exposures once in the middle of the cycle. In addition we will acquire 3 exposures in each of the broadband filters F105W comma  F110W comma  F125W comma  F140W comma  and F160W twice during the cycle.  This work builds on the ISR of Ryan  and  Baggett (2015-011) and Ryan (2019-06).    ------ Calibration Justification -------  The target electrons per pixel is 40 comma 000 - 60 comma 000 comma  so that the Poisson noise of an individual pixel and a single exposure will be 0.5% comma  comparable to or smaller than any individual astronomical image made by WFC3 IR.  With 2 well-exposed flats per medium- and narrow-band filter comma  the Poisson-limited noise after combining 2 individuals will be virgul1.4x smaller.  For the broad-band filters comma  we can combine 3 exposures to produce bi-monthly flats comma  or combine a total of 18 exposures for a extremely low noise flats in the case temporal variations are limited.  Analysis results will be detailed in an ISR.
DOI: 10.57780/esa-pu39jq4
title: 17254

description: On 2022 September 8 comma  Pan-STARRS detected a dust tail - trail associated with a new main-belt asteroid candidate.  Confirming follow-up observations with the 3.6m Canada-France-Hawaii Telescope on September 22 show a tail corresponding to at least 25 comma 000 km length in space.  A search of the Pan-STARRS image archive shows no matching object in pre-discovery images comma  nor could the recent astrometry be linked to any existing asteroid comma  or isolated tracklets comma  implying that this is a new discovery that was not previously visible.  Something happened recently to trigger significant activity comma  resulting in an increase in brightness by at least 2 orders of magnitude.  We propose a DD programme of WFC3 imaging over two orbits.  Only HST will allow us to study the changing morphology of the dust structures and thus differentiate between continuous mass-loss and an impulsive event.
DOI: 10.15156/bio/sh1284211.09fu
title: SH1284211.09FU

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-pudqwqv
title: 16173

description: The Close AGN Reference Survey (CARS  www.cars-survey.org) has assembled a rich comma  hyperdimensional dataset for 33 nearby Type 1 AGN comma  anchored by VLT-MUSE IFU datacubes for every target comma  along with pan-chromatic complementary datasets including ALMA for a large subset of the sample. We now propose an orders-of-magnitude increase in the spatial and temporal resolution of young stars  and  their  ages  (respectively)  for the entire sample.  The proposed WFC3-UVIS UV imaging will map sites of very recent star formation along multiphase quasar-driven outflows comma  instability-driven gas inflows comma  and merger-driven tidal interactions comma  testing whether each might lead to the suppression or even triggering of star formation.  It is comma  therefore comma  a direct test of both negative and positive black hole feedback models.
DOI: 10.15156/bio/sh1284212.09fu
title: SH1284212.09FU

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-puu40j7
title: 16838

description: The Fermi Large Area Telescope (LAT) has found a sample of highly relativistic gamma-ray bursts (GRBs) comma  which may be among the most energetic bursts ever discovered. Here we propose to use Chandra and HST to follow the late time X-ray and optical light curves of a LAT detected burst that also has excellent early multiwavelength coverage. Our observations comma  in conjunction with the Fermi data comma  will allow us to measure the energy comma  bulk Lorentz factor comma  and probe the jet physics of the explosion. Recent work on some of the most powerful GRBs has begun to substantially constrain physical models of the central engine. Our observations may greatly strengthen these constraints as well as provide new insight into the relativistic physics of the bursts.
DOI: 10.57780/esa-pv0not7
title: 16725

description: On the cusp of the JWST era comma  we are still lacking mass measurements for the coldest brown dwarfs comma  even though mass is crucial for testing substellar models. We propose a 3-year orbit monitoring program to obtain the first sample of dynamical masses at temperatures of 400-800 K. With projected separations of only 1-3 AU comma  our targets are among the tightest and faintest substellar visual binaries ever found comma  discovered at the extreme limits of existing facilities. Resolved astrometry comma  combined with existing parallax data comma  is needed to measure their orbits comma  and only HST can deliver the high-precision monitoring required. These systems comma  composed entirely of T8-Y0 dwarfs comma  are likely to be the only such binaries amenable to direct mass measurements within the decade.
DOI: 10.15156/bio/sh1284213.09fu
title: SH1284213.09FU

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-pz6afyj
title: 16553

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=1 program is alternated with a gain=4 program annually.  All  exposures are internals.
DOI: 10.15156/bio/sh1284214.09fu
title: SH1284214.09FU

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-q099p85
title: 16561

description: This calibration program is for obtaining STIS NUV MAMA Dark on a regular basis. The basic monitor takes two 1300s TIME-TAG darks bi-weekly.  The pairs of exposures are linked so that they are taken about 6 hours apart in the same SAA free interval.  This pairing of exposures will make it easier to separate long and short term temporal variability from temperature dependent changes.
DOI: 10.15156/bio/sh1284215.09fu
title: SH1284215.09FU

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-q0y1aoq
title: 16366

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: 10.57780/esa-q33ax2s
title: 16538

description: This program monitors the stability of the constant terms in the NUV dispersion solutions. To monitor for any changes comma  the program observes HD 6655 at selected cenwaves for the three NUV gratings that have seen use since Cycle 21. Via cross-correlation comma  spectra are compared to those obtained in previous iterations of the program and to STIS spectra obtained in-orbit.
DOI: 10.15156/bio/sh1284216.09fu
title: SH1284216.09FU

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-q38rlqz
title: 16644

description: Pinning down the processes at work during the last phase-change of our universe - the epoch of reionization comma  EoR - remains of paramount importance. While enormous progress has been made on many fronts comma  we still do not know the nature of the population of objects that was responsible. Recent results suggest that the rapid conclusion of the EoR should have been driven by an ensemble of very compact star-forming galaxies. The major missing piece of this puzzle comma  however comma  is knowledge of their emergent ionizing luminosity comma  and how this varies with galaxy type. How Lyman continuum radiation (LyC) escapes from galaxies presents an ongoing challenge that requires empirical confrontation.   Recent surveys at low redshift comma  where the ionizing flux can be measured comma  have implicated feedback from star-formation in the emission of LyCdoublePoint winds are likely necessary to clear dense gas from the ISM. However no strong conclusions can currently be drawn comma  due to a limited dynamic range in existing surveys. Here we propose to test this feedback-based hypothesis by stretching it to its absolute limit along one axis of the parameter spacedoublePoint we will observe the direct LyC output of galaxies undergoing the most extreme feedback. The proposed starbursts have star-formation densities and outflow velocities an order of magnitude higher than any currently surveyed in LyC. We expect that if there is any population that is stripping its own interstellar medium comma  leaving channels clear for LyC escape comma  then it is this one. We will use the results of this very efficient program (six galaxies in just 14 orbits) to empirically evaluate the role to similar compact starbursts in cosmic reionization.
DOI: 10.15156/bio/sh1284217.09fu
title: SH1284217.09FU

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-q51afdo
title: 16296

description: To date three brown dwarfs in the L-T transition show signs of planetary-wave light-curve beating. Here comma  the differential rotation of wave-derived structure in various latitudinal bands causes their individual light curves alternately to constructively and destructively interfere. Luhman 16AB is an intriguing target comma  with both components exhibiting peculiar behaviors that hint to the existence of bands in their atmospheres. Recently comma  indirect evidence for bands on Luhman 16A were found using polarization. However comma  no data exists to date that is able to verify the existence of bands on 16A or B. We propose to observe Luhman 16AB with WFC3 to test the existence of bands in these two L-T transition brown dwarfs. Our observations will 1) test the hypothesis that there are planetary-scale waves and bands in L-T transition atmospheres comma  2) verify the ability of polarization to detect bands in exoatmospheres comma  and 3) nearly double the sample of long-temporal-baseline observations available to detect planetary-scale waves in L-T transition brown dwarfs.