cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.5281/zenodo.14922378
title: Dataset for the manuscript: "Decoding injury risk: Exploring the impact of asymptomatic hypermobility on lower limb injury risk factors in young female volleyball players"

description: This dataset includes all variables required to replicate the study. The dataset contains demographic characteristics, Beighton scores, Hypermobility group, Single leg dynamic balance data (Speed and range of motion of Centre of Presssure in anterio-posterior and medio-lateral direction for dominant and non-dominant leg), Limb Symmetry index for the single and triple hop, and Landing Error Scoring System scores.
DOI: 10.6084/m9.figshare.28329818
title: Supplementary Data for "MultiNovo: A universal deep learning-based framework for de novo peptide sequencing from multiple spectra"

description: Supplementary Data for "MultiNovo: A universal deep learning-based framework for de novo peptide sequencing from multiple spectra"
DOI: 10.57780/esa-01njcix
title: 2070017

description: INTEGRAL observation of GRB 231115A
DOI: 10.57780/esa-01qc2cy
title: 0299838

description: Galactic Plane Survey for AO 02 and Pattern 38
DOI: 10.15468/dl.rc2kyt
title: Occurrence Download

description: A dataset listing the 2632 species recorded in GBIF matching the query:
{
 "DatasetKey" : [
 "is MSB Mammal Collection (Arctos)"
 ]
}

 The dataset's 2632 records were derived from 1 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0008405-250310093411724/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.57780/esa-04twykc
title: 0820036

description: We propose a 2 Msec key program  to study a list of hard X-ray detected extragalactic jets from the TANAMI sample in coordination with radio Very Long Baseline Interferometry (VLBI)  gamma-ray Fermi/LAT and optical/UV/soft-X-ray Swift observations. Our target fields contain 10 TANAMI sources which are known to be bright hard X-ray emitters from the Swift/BAT survey. Only one of these sources (Cen A) has previously been observed with INTEGRAL and multiwavelength techniques. For all other objects we will measure the spectral energy distribution (SED) of these sources for the first time with quasi-simultaneous data from the radio band to gamma-ray energies and will produce the first high-SNR hard X-ray spectra during well-determined states of the radio jets [truncated! Please see actual data for full text]
DOI: 10.57780/esa-05f97h6
title: 1760001

description: INTEGRAL Crab monitoring every four revolutions whenever the source is visible
DOI: 10.57780/esa-0a2bjk5
title: 8860259

description: Crab 2012: JEM-X Staring rev 1213
DOI: 10.57780/esa-0aidgpp
title: 8860314

description: This is a public observation where the Earth will drift through the field of view of the INTEGRAL instruments. Results from this observation will help in separating the cosmic and instrumental backgrounds and so ultimately lead to improved background subtraction.Scientifically the main goals are to measure the spectral shape of the cosmic X-ray background emission above 20 keV and to study any high-energy emission from the Earth during storms in auroral regions. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-0avvim1
title: 0620001

description: The Galactic bulge region is a rich host of variable X-ray and gamma-ray point sources.In AO-3 AO-4 and AO-5 we have been monitoring this region with one hexagonal observation approximately every 3 days whenever it was visible by INTEGRAL. Because of the high scientific return and to preserve the continuity with respect to past observations of this ever-changing regionwe suggest to continue our successful observing program. As a service to the scientificcommunity we make the IBIS/ISGRI and JEM-X light curves both in two energy bands perscience window and per hexagonal observation as well as the mosaic images per hexagonalobservation publicly available through the web as soon as possible after theobservations have been performed. Any interesting source behaviour which emerges from ourobservations will be announced promptly so that rapid follow-up by the community ispossible. Our team consists of scientists with expertise on a large range of topics. We alsointend to do a more in-depth analysis (spectra bursts flares etc.) of sources of particular intereston short and long time scales. These sources include bright and relatively faint X-raytransients X-ray bursters persistent neutron star and black-hole candidate binarieshigh-mass X-ray binaries etc.. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-0dir86a
title: 8860327

description: OMC FF sequence ISOC V10 onwards: sequence of ff measurements with LED on/off followed by a DC cal.
DOI: 10.57780/esa-0ew8jec
title: 1220045

description: This proposal is aimed on obtaining legacy-level observational datasets on the Milky Way Galactic disk. The ultimate goal of the entire project is to have model independent and systematics free measurements of the fluxes in nuclear lines (511 keV annihilation emission 1.8 MeV Al26 and 1.17 MeV and 1.33 MeV Fe60 lines) and a broad band spectrum of the Galactic background emission which at different energies is provided either by cumulative emission of faint Galactic source or by interaction of low energy cosmic rays with interstellar medium. Taking into account the unique combination of properties of INTEGRAL instruments - broad band coverage large fields of view and possibilities to eliminate the contribution of discrete sources from the total measured photon flux the proposed strategy is the best possible usage of the valuable INTEGRAL time. Wide mapping of the Milky Way during the campaign of Galactic latitude scans also contributes to the legacy of the INTEGRAL observatory giving the opportunity to study the population of Galactic sources at high latitudes. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-0g18li9
title: 0720044

description: This proposal is a one of three accompanying proposals aimed on obtaining legacy-level observational datasets on the Milky Way Galactic disk. The ultimate goal of the entire project (which started in AO4 and which we plan to continue it in subsequent AOs) is to have model  independent and systematics free measurements of the fluxes in nuclear lines (511 keV annihilation emission 1.8 MeV 26Al and 1.17 MeV and 1.33 MeV 60Fe lines) and a broad band spectrum of the Galactic background emission which at different energies is provided either by cumulative emission of faint Galactic source or by  interaction of low energy cosmic rays with interstellar medium. Our strategy was supported by INTEGRAL TACs during previous AOs and now we propose to continue the coverage of the Galactic disk with scanning observations.  Taking into account the unique combination of properties of INTEGRAL instruments - broad band coverage large fields of view and possibilities to eliminate the contribution of descrete sources from the total measured photon flux the proposed strategy is the best possible usage of the valuable INTEGRAL time. In this proposal we ask for 1.5 Msec observations of outer galactic region at l=215 deg which will be complimentary to the already performed observations of the inner Galaxy at l~40 22.5 and -45 deg. This is one of the two underexposed regions of the Galaxy. Here we were driven largely by the INTEGRAL Legasy consideration. It is important that the whole galactic plane is mapped with INTEGRAL. With these observations we will continue the mapping of the GRXE namely put upper limits to hard X-ray emission generating by accreting White Dwarfs in the Galaxy. It is possible that gamma-ray continuum emission of the Galactic disk will not be detected at such large distances from the Galactic Center however any measurement of the Galactic emission will be useful for constraining the models of the cosmic ray induc [truncated! Please see actual data for full text]
DOI: 10.57780/esa-0gcr3ly
title: 1070002

description: Observations of Mkn 501 (ToO outside TAC)As per request of E. Pian on July 12
DOI: 10.57780/esa-0h7wseu
title: 0320092

description: As a follow-up of the 2 Msec observation in AO-1 and 2.5 Msecobservation in AO-2 we propose a new deep 3.4 Msec exposure of thefield of the Galactic Center which corresponds to 27% share time inthe total available for this target in AO3. Observations of the GCregion make the best use of the unique INTEGRAL capabilities andundoubtedly are the most efficient investment of its preciousobserving time. It is especially important in the study of Galacticdiffuse nuclear and positron annihilation lines.  With the proposedobservation the total INTEGRAL exposure of the GC field will exceed 15Msec by the end of AO-3 which will increase the sensitivity ofINTEGRAL instruments in this very interesting region.  As confirmed bythe analysis of available first ~4 Msec of the AO-1 and AO-2observations the guaranteed science includes detailed study of thediffuse gamma-ray line and continuum emission monitoring of Sgr A*and of dozens of X-ray binaries study of transient phenomena.  Shouldthis proposal be accepted the data will be made available during theproprietary period to scientists of major astrophysical institutionsof Russia. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-0hv81h9
title: 0740016

description: We  ask  for up  to  3 INTEGRAL TOO observations of one blazar in outburst for a total of 600~ks conditional to stringent  triggering  criteria  based on X-ray or  gamma-ray brightening as detected by the current high energy missions including INTEGRAL itself Swift/BAT and Fermi GST or by Cherenkov telescopes. Coordinated INTEGRAL and multiwavelength observations will guarantee the coverage of a broad energy range and allow us to follow the evolution of the overall spectral energy distribution (SED) during one or more flaring episodes. We will thus map accurately the high energy spectrum and constrain the time-dependent parameters of the emission models. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-0icaptc
title: 0399944

description: Galactic lattitude scan Proposal for AO 03 Cycle 4
DOI: 10.57780/esa-0j0jaoa
title: 0299927

description: Galactic Centre Deep Exposure for AO 02 and Pattern 27 Cycle 7
DOI: 10.57780/esa-0jcvxxy
title: 1420013

description: The survey of the Galactic Plane has continued as one of the main INTEGRAL scientific objectives because of the scientificpotential of both new source discovery and detailed monitoring of already known sources. We propose for a total of 3.0 Ms of observations in AO14 and 3 Ms in AO15 to continue our Key Program covering areas of the Plane with regular scans every orbit. For these AOs we selected a section of the Plane incorporating 2 sky regions that are rich in galactic sources (HMXB and SFXT in particular) and potential MeV/TeV sources.Our purpose is to regularly monitor known systems as well as to dramatically enhance the chances of discovering new systems or new outbursts from known sources. This program will allow a rapid response to bright events and a detailed study of fainttransients and their long term activity. Such a programme will be of high value to a very large fraction of the high-energyastronomy community stimulating science immediately and furthermore contributing greatly to the INTEGRAL legacy.In order to maximise the engagement of the scientific community we will continue to make the observations publicimmediately. The team will make as it has through AO8-12 and now in AO13 the scw-resolution IBIS and JEM-X lightcurves (in two energy bands) and per revolution mosaic images publicly available through the web as soon as possible afterthe observations have been performed. Any interesting source behaviour that emerges from our observations will beannounced promptly so that rapid follow-up by the community is possible as it has been already demonstrated. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-0jje53k
title: 1420021

description: This proposal is aimed on obtaining legacy-level observational datasets on the Milky Way Galactic disk.  The ultimate goal of the entire project is to have model independent and systematics free measurements of the fluxes in nuclear lines (511 keV annihilation emission and 1.8 MeV Al26) and a broad band spectrum of the Galactic background emission which at different energies is provided either by cumulative emission of faint Galactic source or by interaction of low energy cosmic rays with interstellar medium. Taking into account the unique combination of properties of INTEGRAL instruments - broad band coverage large fields of view and possibilities to eliminate the contribution of discrete sources from the total measured photon flux the proposed strategy is the best possible usage of the valuable INTEGRAL time. Wide mapping of the Milky Way during the campaign of Galactic latitude scans also contributes to the legacy of the INTEGRAL observatory giving the opportunity to study the population of Galactic sources at high latitudes. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-0k9hwtw
title: 1970013

description: INTEGRAL TOO observations of GRB221009A
DOI: 10.17631/rd-2025-0008-ddat
title: Interviews with survivors of conflict in Kosovo

description: This dataset contains de-identified transcripts of semi structured interviews that took place between August 2016 and June 2017. These interviews were conducted as part of a project entitled 'Transitional justice, wellbeing and intergroup relations'. There are 19 transcripts from interviews with survivors of conflict in Kosovo in the original language together with documentation, including the interview schedule and informed consent procedures.
DOI: 10.57780/esa-0p0zwmj
title: 8860018

description: This Crab offset staring observation is used to determine the off-axis imaging properties of IBIS and to provide an absolute calibration of  the off-axis PSF.  The off-axis position of the Crab in this staring observation (zenith 9.6 degree azimuth 0. degree)  is defined in the instrumental coordinate system and depends on the start date of the observation. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-0pkeots
title: 0299847

description: Galactic Plane Survey for AO 02 and Pattern 47
DOI: 10.57780/esa-0qcojie
title: 2020014

description: This proposal is aimed on obtaining legacy-level observational datasets on the Milky Way Galactic disk.  The ultimate goal of the entire project is to have model independent and systematics free measurements of the fluxes in nuclear lines (511 keV annihilation emission and 1.8 MeV Al26) and a broad band spectrum of the Galactic background emission which at different energies is provided either by cumulative emission of faint Galactic source or by interaction of low energy cosmic rays with interstellar medium. Taking into account the unique combination of properties of INTEGRAL instruments - broad band coverage large fields of view and possibilities to eliminate the contribution of discrete sources from the total measured photon flux the proposed strategy is the best possible usage of the valuable INTEGRAL time. Wide mapping of the Milky Way during the campaign of Galactic latitude scans also contributes to the legacy of the INTEGRAL observatory giving the opportunity to study the population of Galactic sources at high latitudes. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-0tf99uw
title: 1940011

description: Since early 2016 the IceCube collaboration is promptly distributing alerts of high-energy neutrino detections in order to allow follow-up searches for possible counterparts at the neutrino position. Finding such counterparts would provide important clues on the origin of the high-energy neutrinos and by proxy on the nature of the high-energy cosmic ray accelerators one of the most important and long-standing puzzles of high-energy astrophysics. We ask for pointed ToO observation of the HESE (High Energy Starting Events) and EHE (Extremely High Energy) neutrinos detected by IceCube and reported either in pub-lic or in private GCNs. We will employ the best available knowledge of the INTEGRAL instruments and our expertise in multimessenger transient searches to hunt for a possible hard X-ray and gamma-ray counterparts. In absence of a detection we will set the most stringent upper limits.We intend to promptly communicate the results of our ToOs to the general community thus supporting additional multiwavelength follow-ups and increasing the visibility of the INTEGRAL contribution to the searches of multimessenger transients. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-0ualcca
title: 0620002

description: We request two INTEGRAL observations of 250 ksec each of the bright Seyfert 2 galaxy NGC 2110. Previous observations by BeppoSAX showed a complex X-ray spectrum but did not extend significantly above 100 keV in order to study the continuum and determine the turnover (cut-off) in the hard X-ray band. INTEGRAL offers the unique possibility to study the physics involved in absorbed AGN and even enables us to study the connection between flux variation high-energy cut-off reflection component and iron fluorescence line. The variation in flux over the time of the observation in various energy bands can reveal the geometry of this source. The two separate observations will most likely catch the source in two different states allowing to further constrain the connection between high energy spectrum and reprocessing. Analysing all INTEGRAL data covering NGC 2110 even though being at large off-axis angles led to a 11 sigma (20 - 40 keV) detection in ISGRI within 97 ksec ensuring that this source is indeed bright enough to perform detailed spectral studies. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-0v3jun1
title: 1420008

description: Diffuse line emission from radioactive 26Al has been observed throughout the Galaxy and is one of the key science goals and assets of the INTEGRAL mission. INTEGRAL has provided a new image of the Galaxy in 26Al gamma-rays and has provided high-resolution spectra as a new astronomical measurement. This has led to a multi-wavelength test of massive-star nucleosynthesis for groups of stars comparing the INTEGRAL measurement to the richness of massive star clusters and their effects on surroundings other than the radioactive nucleosynthesis ejecta which are ionization of surrounding gas and cavities created in the ambient interstellar medium. Much has been learned from the brightest such nearby massive-star groups. Also on the Galactic scale the measured Doppler shifts from large scale Galactic rotation have led to a proposition of massive-star ejecta recycling preferentially through large superbubbles located between spiral arms. This was derived from the discrepancy of 26Al gas velocities to other objects participating in Galactic large-scale rotation.  60Fe radioactivity is assumed to arise from the same massive star groups except that it only is ejected from the later core collapse explosions rather than from Wolf-Rayet phase winds and supernovae as 26Al is. The ratio of 26Al to 60Fe emission for groups of stars provides us with a test of the models for massive-star interiors.Here we request data rights for all observations that cover different regions throughout the Galaxy with respect to analysis for 26Al emission and also for the fainter emission in 60Fe gamma-rays that is expected to correlate with 26Al. Additionally we propose that if the exposure of the disk is to be made more homogeneous the Carina region would be a suitable place to do so. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-0xc6o6f
title: 2040001

description: Black hole X-ray binaries (BHXBs) cycle through different accretion states rapidly providing a time- resolved view of how matter behaves in a strong gravity environment.  Simultaneous multi-wavelength observations are the optimal tool that exposes this view.  However these campaigns (connecting the evolving accretion inflow and jet outflow) have been rarely achieved. We request a TOO consisting of two INTEGRAL revolutions (340ks) of a BHXB as it transitions from the hard to the soft state to complement our Astrosat accepted coverage.  Our target list contains 15 candidates.  We target the transition to reveal both the rapid orbit-to-orbit X-ray variability and the slower X-ray variability that characterize the significantly changing accretion disk (derived from X-ray spectra and timing) and directly measure the broad-band SED in connection with multi-wavelength coverage. The INTEGRAL data will be crucial to extend the coverage at high energies and obtain complete spectral information. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-0z22jhn
title: 1520011

description: Massive stars and their impacts on their surrounding interstellar medium comprise the feedback scenario which is one of the main astrophysical issues in the context of galaxy and cosmic chemical evolution. Radioactivity from 26Al adds a unique diagnostic tool for studying this scenario in nearby massive-star regions. The Orion region hosts one of the closest such regions at ~400 pc. COMPTELs measurement of 1809 keV emission from this region had shown an interesting offset of the 26Al emission source from its likely sources and emission appears rather extended. This suggests champagne-like outflow into the Eridanus cavity as has recently also been seen with XMM-Newton. If true this opens unique possibilities to study the ISM as it is shaped by massive stars and the interaction of massive stars with their surrounding ISM in a new way: Due to their proximity and location on the near side of molecular clouds and at the edge of a large cavity we can compare the locations of massive stars to the morphology of the ISM and the emission pattern of 26Al radioactivity in order to constrain 26Al ejection from massive stars in mass and velocity. Previous observations led to ~3 Ms of exposure merely enough for a marginal hint of the expected signal. With our proposed deepening of exposure we aim to measure the intensity and kinematics of this nearby 26Al source with INTEGRAL. With these observations we can also search for annihilation radiation and for the intensity of nuclear deexcitation gamma-rays in the MeV range both valuable diagnostics of the structure of superbubble interiors and more than 30 Fermi sources are within our target region. But mainly this will give us unique measurements of ISM dynamics and massive stars as its driving engines within INTEGRALs lifetime  there is hardly a more suitable and closer target region. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-0zajzuh
title: 8860054

description: OMC FF sequence ISOC V10 onwards: sequence of ff measurements with LED on/off followed by a DC cal.
DOI: 10.57780/esa-0zif9t9
title: 1870008

description: INTEGRAL ToO observations of V4641 Sgr
DOI: 10.57780/esa-10kadso
title: 8860258

description: Crab 2012: IBIS Mask Corner rev 1213-14
DOI: 10.57780/esa-11nykgs
title: 0529700

description: This is an artificial proposal