cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.57780/esa-6hm2y58
title: 086147

description: We propose to observe the early X-ray emission of the ejecta of two novae in outburst comma  a classical or short-period recurrent nova comma  and a rarer symbiotic one openPari.e. comma  known to be a red giant binaryclosePar. They will be observed when comma  with the Swift XRT comma  we establish that they are sufficiently luminous for high quality RGS spectra and that the central comma  luminous supersoft X-ray source does not outshine the ejecta yet. The X-ray spectra of nova winds probe the nova kinematics comma  its chemistry and connections with the phenomena observed at other wavelengths comma including the intriguing gamma-ray emission. High resolution X-ray spectra of the outflowing material comma  without a major contribution yet of the central source comma  have seldom been obtained  we do need to broaden the sample to explore the complex physics.
DOI: 10.57780/esa-8td0cpm
title: 086540

description: The recent discovery of Pi Men c comma  a super-Earth transiting an outstandingly bright nearby star openParV = 5.67  18 pcclosePar comma  presents an unrivalled opportunity to study the atmosphere of a small planet just above the ..radius-period valley. While the expected transit signature of the atmosphere in the optical-infrared is very small comma  the high-energy environment of the planet is thought to be favourable for large transit absorption features in the far- ultraviolet due to an escaping comma  extended upper atmosphere. Using simultaneous XMM-Newton and HST observations comma  we propose to perform both a full reconstruction of the differential emission measure in order to characterise the high-energy irradiation impingent on the planet comma  and a sensitive search for evaporation signals due to these photons. In addit
DOI: 10.57780/esa-a3duvz6
title: 089381

description: #1 GRB211211A #2 SDSSJ1430+2303 #3 NGC5907 ULX1 #4 SDSSJ1430+2303 #5 2MASX J02344872-4419325 #6 GRB211211A #7 ASASSN-20qc #8 Mrk 501 #9 PKS1413+135   #11 Sgr A*
DOI: 10.15156/bio/sh1281258.09fu
title: SH1281258.09FU

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-bkcfv03
title: 085360

description: The goal is to understand the low-flux state and long-term behaviour of blazars at high-energies by studying Mrk 421 with a combination of observations from X-rays to TeV gamma rays comma  with two INTEGRAL observations of 370 ks each comma  one in each of the visibility periods in MayaquestionMarkquestionMarkJune and NovaquestionMarkquestionMarkDec. These observations will be enhanced with snapshots with XMM-Newton and Swift comma  and public monitoring programs by Fermi and Swift-XRT. The energy ranges covered by INTEGRAL and FACT are crucial for modelling the SED of blazars  we want to investigate the behaviour on timescales of months comma  to constrain blazar emission models. Comparing two observations comma  we want to investigate if Mrk 421 exhibits a peak shift and thus a tendency to extreme behaviour openParas Mrk 501 and 1ES 2344+51.4closePar.
DOI: 10.15156/bio/sh1281259.09fu
title: SH1281259.09FU

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-bpdfcs0
title: 086456

description: We propose a 130 ks XMM-Newton observation of RX J1301.9+2747 openParRX J1302closePar comma  the second AGN where X-ray Quasi-periodic Eruptions openParQPEsclosePar have been discovered comma  coordinated with 10 hours of VLA radio observations. First discovered in the galaxy GSN 069 openParMiniutti et al. 2019 comma  Nature 573 comma  381closePar comma  QPEs are unprecedented variability patterns formed by recurrent comma  rapid outbursts of X-ray light. While the QPEs in GSN 069 last about one hour and repeat about every nine hours comma  the QPEs in RX J1302 are much shorter comma  and their variability pattern is not clear. A new long XMM-Newton observation will allow to unveil what is the variability pattern of the QPEs in RX J1302  coordinated radio observations will help constraining the physical nature of this newly discovered phenomenon.
DOI: 10.57780/esa-d1sppw0
title: 085418

description: Obs.02doublePoint Draft to be copied
DOI: 10.15156/bio/sh1281260.09fu
title: SH1281260.09FU

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-er1up5y
title: 086302

description: We propose XMM-Newton observations of 2 Galactic high-mass X-ray binary openParHMXBclosePar candidates with relatively low absorption column densities openParNH < 1e22 cmelev-2closePar. These targets lack detailed X-ray studies comma  and have low X-ray fluxes or limits in quiescence. The nature of the accreting object is not clear in these cases  are they white dwarfsquestionMark neutron starsquestionMark black holesquestionMark XMM-Newton observations will confirm whether the Be star counterparts are truly X- ray sources comma  and if so comma  characterize their spectra and possibly pulsations comma  helping to identify the nature of the accretor.
DOI: 10.15156/bio/sh1281261.09fu
title: SH1281261.09FU

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-f8hfkyi
title: 088199

description: Radio and X-ray observations of supernovae openParSNeclosePar acquired in the poorly sampled phase of years to decades post-explosion are necessary to drive progress in several fundamental areas of explosive transient research. Bright emission virgulyears to decades post explosion of extragalactic SNe may be due to AclosePar shock-interaction with the circumstellar medium  or BclosePar the emergence of radiation from a pulsar wind nebula. A solid identification of the scenarios above would lead to significant advances in our understanding of the physics of stellar explosions comma  their progenitors comma  and their remnants. We propose the first systematic late-time X-ray survey of SNe with bright detected radio emission.
DOI: 10.15156/bio/sh1281262.09fu
title: SH1281262.09FU

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-jcry2dd
title: 085219

description: There are four massive quasars discovered at z>5. These sources present a puzzle  how black holes grow to 10elev9 solar masses in the limited age of the universe. We would like to address this by estimating the population of such objects. The population estimation requires good constraints on their jet properties comma  in particular comma  the Doppler factor. We propose to observe the high-redshift blazar SDSSJ013127.34-032100.1 with XMM and NuSTAR for 40 ks and 100 ks comma  respectively comma  in order to model the broadband SED accurately. The broadband X-ray observation will allow us to measure the Doppler factor for the source comma  constraining the high-a supermassive BH population in the early universe. These measurements will be used to infer the number of similar BHs at high redshifts.
DOI: 10.57780/esa-kh0ohxm
title: 086378

description: We propose to observe a recently discovered radio-loud quasar at redshift z=6.82  this quasar is both the most radio-loud and the most radio-luminous quasar known at z>6 comma  and appears to be powered by a supermassive black hole experiencing super-Eddington accretion. VLA images have revealed an additional structure 25 arc seconds openParvirgul125 kpc comma  projectedclosePar away comma  potentially indicating large jets associated with the extreme accretion rate. If these jets are interacting with the Cosmic Microwave Background comma  which has an energy density that scales as openPar1+zcloseParelev4 comma  we expect to see significant extended X-ray emission around the quasar. Our proposal will provide the first X-ray observations of a radio-loud quasar at z>6.
DOI: 10.57780/esa-mz0fmom
title: 086159

description: We propose to carry out EPIC imaging spectroscopy of two Wolf-Rayet binaries with very short period openParP < 1 dayclosePar. Thanks to the excellent EPIC sensitivity comma  we willdoublePoint openPariclosePar obtain good quality spectra of these objects yet unobserved with the modern X-ray observatories openParChandra comma  XMM-NewtonclosePar  openPariiclosePar deduce the plasma parameters in their X-ray emitting region  openPariiiclosePar derive valuable information on their origin.
DOI: 10.15156/bio/sh1281263.09fu
title: SH1281263.09FU

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-q12wxh8
title: 086276

description: We propose a broadband observation of the transient ULX comma  NGC 925 ULX-3 comma  for 40ks with XMM-Newton quasi-simultaneous with a 100ks observation with NuSTAR. This source exhibits extreme levels of long-term variability of over a factor of 36 comma  a feature also seen in several ULXs identified as neutron stars to date and linked to different possible mechanisms that are not well understood. We plan to trigger this observation when the source exceeds a flux of 6x10elev and #8722 13 ergs-s-cm2 comma  determined from an existing Swift monitoring campaign comma  allowing us to constrain its high-flux broadband spectrum. Coupled with this monitoring and a complementary proposal at a low flux comma  we will be able to build an understanding of the geometry and physical processes in play in this extreme accreting system.
DOI: 10.15156/bio/sh1281264.09fu
title: SH1281264.09FU

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-qbanx8a
title: 086277

description: eROSITA comma  successfully launched in mid-2019 comma  will perform multiple all-sky X-ray surveys. Monitoring roughly half a million AGN-quasars comma  eROSITA will identify rare comma  accretion ignition-depletion events as they occur. To explore how the X-ray corona and accretion disk respond to a sudden comma  major change in accretion rate comma  the identified sources need medium signal to noise XMM-Newton ToO openParEPIC+OMclosePar observations to derive meaningful spectral constraints. Thus comma  we propose 10 ToOs openParfive with 10 ks -- ignition event  five with 60 ks -- depletion eventclosePar each joint with VLT FORS2 imaging and spectroscopy openParfor each ToO 1 hourclosePar for optical counterpart localization and tracking the Broad Line Region.s responses.
DOI: 10.57780/esa-rhjgs6m
title: 086441

description: Galaxy clusters grow hierarchically through the merger-accretion of smaller substructures along filaments. The dynamically young cluster A1367 is one of the best examples to study the cluster evolution because of its proximity and with abundant multi-wavelength data. Additional to the main merger along the NW-SE direction and a merger shock-radio relic at the NW comma  we also find evidences of another counter-shock at the SE and the accretion of group-filament along the Coma-A1367 supercluster. We propose XMM observations to complete a coverage of the R500 radius of A1367 to 1closePar explore the unique case of an extended shock radio-tail interaction  2closePar study the dynamics of the cluster-filament transition region  and 3closePar search for X-ray tails-clumps associated with Halpha emission.
DOI: 10.15156/bio/sh1281265.09fu
title: SH1281265.09FU

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-t6dqg7j
title: 084119

description: We propose to obtain the first complete X-ray CCD image of the newly discovered supernova remnant openParSNRclosePar G53.41+0.03. The spectral image study of this rare and relatively young openPar1000 8000 yrclosePar SNR will allow us todoublePoint iclosePar better constraint the element abundances comma  which are crucial for pinpointing the SNR origin  iiclosePar significantly improve the age estimation by better measuring the plasma parameters  iiiclosePar search for active acceleration sites producing synchrotron radiation and ivclosePar for a compact object which could be either a normal pulsar comma  CCO or a magnetar. In addition we will compare the X-ray morphology to our previous radio study.
DOI: 10.15156/bio/sh1281266.09fu
title: SH1281266.09FU

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-t9q42nd
title: 089180

description: #1 ASASSN-20qc #2 ASASSN-20qc openParCAL CLOSEDclosePar #3 RX J1605.3+3249 #4 NGC 1052 #5 BL Lac #6 XMMSL1 J024916.6-041244 #7 4FGL J1408.6-2917 #8 V767 Cen   #11 WISEA J045649.8-2037 #12 PSR J1740-5340B   #13 AD Leo   #14 TC0221 #15 NGC 5907 ULX1  #16 EX 04570-5206 #19 CN Leo #21 2MASX J01110461-4558435 #30-35 C-2021 A1 #36-37 ASASSN-20qc  #40-43 RBS1124
DOI: 10.57780/esa-ud59sxt
title: 090263

description: Abell 746 is a unique system hosting a spectacular double radio relic comma  a possible radio halo comma  and two radio bright diffuse regions to the east of the cluster. With our proposed XMM-Newton and JVLA observations comma   along with existing low frequency radio data comma  we will openPar1closePar understand the origin of complex diffuse radio sources  openPar2closePar probe the underlying particle acceleration mechanism  openPar3closePar characterize the properties of the shocks responsible for these sources  openPar4closePar determine the merger scenario by comparison with simulations  and openPar5closePar study polarization properties of the relics and the magnetization of the intracluster medium through Faraday analysis.
DOI: 10.15156/bio/sh1281267.09fu
title: SH1281267.09FU

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.