cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.15156/bio/sh1284094.09fu
title: SH1284094.09FU

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-h97jaqo
title: 16432

description: ----SPECIAL REQUESTS FOR ARCHIVEdoublePoint----- 1. Please turn off calibration for the COS-FUV exposures. 2. Please disassociate all exposures. SQL is used to meet the above requests. In case 1 qexposure.control_id is modified. In case 2 qeassociation re
DOI: 10.15156/bio/sh1284095.09fu
title: SH1284095.09FU

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-hecmi1l
title: 16665

description: We propose to obtain deep WFC3-UVIS FQ937N narrow band imaging of a sample of six quasars at zvirgul6.7 with extant high resolution ALMA sub-mm observations and deep optical-to-infrared spectra. These quasar fields will also be observed with deep JWST-NIRCam imaging in rest-frame UV (F115W and F200W) and optical (F356W) as well as slitless spectroscopy at 3-4 um to detect the Hbeta+CORCHETE_OPENOIIICORCHETE_CLOSE lines of galaxies in the quasar fields. The proposed HST observations will detect the Lyman alpha emission in zvirgul6.7 galaxies comma  and together with the JWST observations and deep optical dropout band imaging comma  will enable us to measure the distribution and the clustering of Lyman alpha emitters (LAEs) in the quasar vicinity and thus measure the dark matter halo mass of these earliest supermassive black holes (SMBHs). Compared with the distribution and clustering of more massive Hbeta+CORCHETE_OPENOIIICORCHETE_CLOSE emitters in quasar vicinity comma  we will gain insights on how the strong quasar UV radiation affects the formation of galaxies at different masses. The HST narrow band observations will detect close companion galaxies and the extended Lyman alpha halos around the quasars to pinpoint whether the fast black hole growth are triggered by galaxy merger or cold stream accretion. The combination of the HST narrow band observations and JWST observations will also provide unparalleled measurements of the Lyman alpha emitting galaxy fraction and the distribution of the Lyman alpha line equivalent width and luminosity in the highly ionized quasar vicinity and constrain the reionization topology by comparing with such measurements in blank fields without strong ionization radiation from quasar and-or overdensity of galaxies.
DOI: 10.57780/esa-hfhixde
title: 16518

description: This program will be used to cross-calibrate the HST focus in two WFC3-UVIS filters using interleaved exposures in F410M and F606W. It will supplement the existing CAL-OTA Focus  and  Optical Monitor program comma  which executes every 2 months in F410M comma  and will allow us to tie the observations to the WFC3 PSF database and phylogram-type plots (Anderson and Bedin 2017 comma  MNRAS 470 comma  p. 948) comma  which include far more observations in F606W than in F410M. It will supplement the results obtained from interleaved exposures in F410M and F606W in program 15585.
DOI: 10.15156/bio/sh1284096.09fu
title: SH1284096.09FU

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-hhb1229
title: 16951

description: This purpose of this activity is to repair radiation induced hot pixel damage to the STIS CCD by warming the CCD to the ambient instrument temperature and annealing radiation damaged pixels. Radiation damage creates hot pixels in the STIS CCD Detector. Many of these hot pixels can be repaired by warming the CCD from its normal operating temperature near -83 C to the ambient instrument temperature (virgul +5 C) for several hours. The number of hot pixels repaired is a function of annealing temperature. The effectiveness of the CCD hot pixel annealing process is assessed by measuring the dark current behavior before and after annealing and by searching for any window contamination effects.
DOI: 10.57780/esa-hiasbuz
title: 16291

description: A key question in galaxy formation is how active galactic nuclei (AGN) interact with their host galaxies. Extremely Red Quasars (ERQs) are ideal objects to study this interaction since they are believed to be quasars caught in a short-lived phase where they are actively clearing gas from their host galaxy.s central regions.  Most known ERQs are at z=2-3 comma  making it challenging to resolve details of their winds and host galaxies comma  even with HST.  Here we propose to study the lowest redshift ERQ  discovered to date (zvirgul0.94) with the aim of directly resolving the high ionization outflow using narrow-band imaging of the CORCHETE_OPENNe VCORCHETE_CLOSE line.  The narrow band observations will provide a first look at the size and spatial distribution of a powerful quasar outflow during this key phase. The broad band observations will enable measurement of the host galaxy properties including Sersic index comma  evidence of merging comma  and recent (100 Myr) star formation. J0048-0046 provides the best possible chance to constrain the ionized gas outflow size of an ERQ comma  both due to its low redshift and its high level of nuclear obscuration.  With the derived outflow size measurements comma  we can test our theories of galaxy formation and measure whether ERQ winds have enough kinetic power to blow the gas out of their hosts. These observations will also help contribute to building up a sample of ERQ hosts and outflow measurements that can be used to assess how ERQs outflows are driven and how the hosts of these galaxies evolve.
DOI: 10.15156/bio/sh1284097.09fu
title: SH1284097.09FU

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-hjbi8x6
title: 16579

description: Using high signal-to-noise observations of spectrophotometric standard stars in staring mode comma  this program serves as a monitor of the UVIS and IR channel throughput and stability. The data will be used to compute inverse sensitivities (i.e. zeropoints) comma  encircled energies comma  and any required color term corrections for both WFC3 channels as a function of time comma  wavelength comma  and position on the detector.
DOI: 10.15156/bio/sh1284098.09fu
title: SH1284098.09FU

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-hlkpfyr
title: 17011

description: This program acquires a variety of WFC3-IR darks to support the removal and study of dark current comma  which is critical to the success of WFC3. Similar to previous  IR dark monitor programs comma  about a quarter of the orbits are used to periodically  obtain SPARS200-full-frame dark observations. These long observations are used  to monitor trends in the bad pixels (hot comma  unstable comma  or dead) comma  zeroth read level comma  and  dark current. The remaining orbits collect dark ramps for generating stacked IR  dark calibration files for use by the MAST pipeline. The ramps will be collected  for each observing mode at a cadence roughly scaled with the newness of the  observing mode as well as its popularity in approved recent proposals.
DOI: 10.57780/esa-hnyprpr
title: 16275

description: The discovery of a gamma-ray flash and kilonova (KN  aka. macronova) comma  AT2017gfo comma  associated with the first binary neutron star (BNS) merger detected by aLIGO-AdV comma  GW170817 comma  heralded the era of GW+EM multi-messenger astronomy.  This landmark event confirmed both the association of short GRBs with binary mergers comma  and that neutron star material can be ejected in sufficient quantities to power a detectable radioactive transient.   It opened a new window on several long-standing problems in astrophysics comma  cosmology and fundamental physics comma  including the possibility that BNS and NSBH compact binary mergers represent the dominant source of heavy r-process elements in the universe.  However comma  the lack of success in identifying similar events in the O3 run of the gravitational wave detector network so far has highlighted that their rate is low in the nearby universe (e.g. d<200 Mpc) comma  thus opportunities for intensive study of kilonovae comma  crucial to understanding their heavy element yields comma  for example comma  will be infrequent. Here we propose a ToO campaign targeting a kilonova discovered during cycle 28. This is between the GW network science runs comma  but KNe may still be found in blind surveys comma  accompanying short-GRBs comma  or during GW engineering runs.  HST has already made unique contributions to the follow-up of AT2017gfo and its off-axis relativistic jet comma  and also provided the primary evidence for the most compelling cases of KNe following SGRBs.  Our program is flexible to adapt for different possible scenarios comma  and will be crucial for understanding the diversity of EM signatures from neutron star compact binary mergers comma  and providing the data to test increasingly sophisticated KN models.
DOI: 10.15156/bio/sh1284099.09fu
title: SH1284099.09FU

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-ht5w6ka
title: 16734

description: The escape fraction of ionizing radiation (f_esc) comma  a fundamental parameter in modeling of reionization comma  is impossible to measure at z>6. Therefore comma  a number of HST studies are calibrating indirect indicators of f_esc comma  using large samples of local galaxies (zvirgul0.3). What is missing is a comparable sample of galaxies at the highest redshifts where all the necessary observables (covering the full spectrum from 950AA to the rest frame optical) can be measured.   We propose a coordinated HST-NOIRLab program to observe a unique sample of 8 strongly lensed  Lyman alpha (Lya) emitters at 2.1<z<2.6. THese observations will enable the measurement of their escape fraction of ionizing radiation and test for evolution in its  indirect estimators. WFC3 UVIS imaging will  directly measure  the emission at ionizing wavelengths (LyC comma  lambda<912AA). Longer wavelength imaging will constrain the  properties of the young stars comma  including the dust content and the sizes of the star-forming regions. The coordinated NOIRLab Gemini observations comma  consisting of rest-frame UV+optical IFU spectroscopy comma   will provide the diagnostics required to quantify the intrinsic ionizing radiation field comma  nebular dust content comma  and  kinematics of the ISM.  Only the combination of the strong magnification and redshifts of these galaxies allow us to perform these measurements comma  probing a completely unexplored regime of physical sizes (virgul100svirgulpc) and intrinsic luminosities (virgul1-1000 L*UV) at z>0.5. Our sample complement planned JWST programs that are targeting the rest-frame optical for known zvirgul3 bright emitters.
DOI: 10.15156/bio/sh1284100.09fu
title: SH1284100.09FU

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-htscpkg
title: 16977

description: This program monitors the SBC dark current and detector temperature as a function of turn-on time.  SBC darks will be taken over a continuous 4 orbit period so that the effect of temperature with turn-on time can be monitored. Normally this procedure will be performed 4 times a year comma  but because Cycle 30 is longer than normal comma  it will contain 5 visits.
DOI: 10.15156/bio/sh1284101.09fu
title: SH1284101.09FU

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-hu8pn33
title: 16796

description: We propose to create a legacy map of the southern half of M31 in the optical and near ultraviolet (NUV).  The Panchromatic Hubble Andromeda Southern Treasury (PHAST) will add virgul100 million stars to M31.s stellar photometry archive and cover regions of M31 that are structurally unique and more sensitive to the merger history than the northern disk mapped in the Panchromatic Hubble Andromeda Treasury (PHAT).   These newly mapped regions include the intersections with M32 and the giant southern stream comma  the split portion of the star forming ring comma  and the southern bar.  By providing age comma  metallicity comma  stellar mass comma  and follow-up kinematics comma  the resolved stellar photometry of these regions will be used for detailed comparisons to simulations comma  including star formation history and population asymmetries as well as the orbits of M32 and the giant southern stream comma  allowing us to distinguish between competing merger scenarios.  Thus comma  these measurements tightly constrain models of M31.s merger history and disk evolution.  Furthermore comma  the legacy value for such observations is undeniable  M31 has been and will continue to be a centerpiece target for many NASA and ESA missions comma  as well as for ground-based time-domain observations that could find extremely valuable events that require HST resolution for identifying precursors.  These current and future data sets cover the entire galaxy comma  and thus comma  our coverage will increase the value of all past and future M31 observations.  PHAST will complete a lasting baseline data set for this high-demand target that no other current or planned facility will be able to produce.
DOI: 10.57780/esa-hulu995
title: 16535

description: Perform routine monitoring of NUV MAMA detector dark rate. The main purpose is  to look for evidence of a change in the dark rate comma  both to track on-orbit time  dependence and to check for a detector problem developing. Variations of count rates   as a function of orbital positions will be analyzed to study the effect of SAA.   Stacked images will help us study the spatial distribution of dark rates on the detector.
DOI: 10.15156/bio/sh1284102.09fu
title: SH1284102.09FU

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-hvv6fgb
title: 16485

description: Nearly all galaxies harbor supermassive black holes and galaxy mergers are common in hierarchical galaxy formation. Therefore comma  the study of dual (virgul1kpc separation) or binary (virgul1pc separation) supermassive black hole (SMBH) is very important to understand the co-evolution of SMBH and its host galaxy. However comma  the number of confirmed dual or binary AGNs is small because most of the follow-up observations of the dual or binary SMBH candidates rely on a single observing band and therefore have a low success rate when one of the two (or both) AGNs is not visible in the chosen band. Based on the recent discovery of the radio-optical dual AGN demonstrating the importance of the multiband confirmation comma  we propose a pilot study of dual-binary AGN search using both highresolution radio and NIR images from VLBA and HST in order not to miss AGN that is visible only in either one of the observing bands. This program will provide high-resolution radio and NIR images to measure the separation of the two AGNs with the estimate of the galaxy stellar mass and black hole mass comma  and will demonstrate the power of using VLBA and HST(JWST in future) for a large scale systematic search for binary SMBHs.