cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.57780/esa-3gjrioq
title: 8860351

description: New OMC FF sequence ISOC v42 onwards: sequence of ff measurements with LED on/off then a narrow 3x3 dither followed by a DC cal.
DOI: 10.57780/esa-3hszv6b
title: 0320033

description: We request dedicated INTEGRAL observations of two INTEGRAL selected AGN: IGR J21247+5058 and LEDA170194. Both objects have been discovered in the IBIS survey (first and forthcoming versions).  Among a set of 7 similar objects these are the only with poor exposure.  Aim of the present proposal is to provide a higher signal to noise ratio as well as broad band spectroscopy by means of all INTEGRAL instruments and/or hopefully in conjunction with an XMM observation for which time has been requested in the latest XMM AO. We also plan to combine all information obtained in the X-ray and gamma-ray domain with observations at other wavebands in order to construct the Spectral Energy Distribution of each source and so establish if they are atypical in some ways with respect to the local AGN X-ray population. In order to achieve our goals we request 300 ks exposure on each source possibly at two different epochs in order to probe source variability. [truncated! Please see actual data for full text]
DOI: 10.23708/4bd06a6b-11c6-4029-b0a3-862ea530ed20
title: Villages - Île d'Atauro - Timor oriental - Asie
title: Villages- Atauro Island - East Timor - Asia

description: Numérisation et identification des villages de l'ïle d'Atauro, Timor oriental. Données issues de terrain réalisés sur l'ïle d'Atauro entre 2013 et 2020 par Jean-Christophe Galipaud (ANR 18-CE27-020)
description: Digitization and identification of villages on Atauro Island, East Timor. Data from fieldwork carried out on Atauro Island between 2013 and 2020 by Jean-Christophe Galipaud (ANR 18-CE27-020)
DOI: 10.57780/esa-3lnwj2p
title: 8860189

description: OMC FF sequence ISOC V10 onwards: sequence of ff measurements with LED on/off followed by a DC cal.
DOI: 10.57780/esa-3mxat7u
title: 0199911

description: Galactic Centre Deep Exposure for cycle 1 pattern 1
DOI: 10.23708/15eb3fa5-6439-456c-abcf-f269831d352b
title: Toponymie - Île d'Atauro - Timor oriental - Asie
title: Place names - Atauro Island - East Timor - Asia

description: Toponymie - Villages de Uaru Ana et Akrema - Ile d'Atauro, École d'été, 2019, Timor oriental (ANR 18-CE27-020). Les toponymes ont été collectés dans les villages d'Akrema et Uaroana au cours d'une école d'été sur le patrimoine local qui s'est tenue du 17 au 29 août 2019. Trois jours de théorie et quatre jours de travail sur le terrain ont été organisés dans les villages d'Akrema et d'Uaroana (Fig. 1). Les deux derniers jours de travail sur le terrain, les étudiants ont travaillé leurs données et préparé des présentations en guise de retour d'information préliminaire pour les communautés locales. Des cartes d'Akrema et d'Uaruana ont été imprimées et remises aux communautés.
description: Toponymy - Villages of Uaru Ana and Akrema - Atauro Island, Summer school, 2019, East Timor (ANR 18-CE27-020). Toponyms were collected in the villages of Akrema and Uaroana during a local heritage summer school held from 17 to 29 August 2019. Three days of theory and four days of fieldwork were organised in the villages of Akrema and Uaroana (Fig. 1). On the last two days of fieldwork, the students worked on their data and prepared presentations as preliminary feedback to the local communities. Maps of Akrema and Uaruana were printed and given to the communities.
DOI: 10.57780/esa-3o21hv0
title: 0399826

description: Galactic Plane Survey for AO 03 and Pattern 26
DOI: 10.57780/esa-3ovp077
title: 0399824

description: Galactic Plane Survey for AO 03 and Pattern 24
DOI: 10.23708/287c36ec-cade-4e74-86c9-3c40f5a099e1
title: Sites fortifiés - Île d'Atauro - Timor oriental - Asie
title: Fortified sites - Atauro Island - East Timor - Asia

description: Identification par relevés GPS des sites fortifiés de l'ïle d'Atauro, lors d'une mission de terrain réalisées en avril et mai 2023. Secrétariat d’État à l’Art et à la Culture (SEAC), UMR PALOC, 2023, Timor oriental (ANR 18-CE27-020)
description: GPS identification of fortified sites on the island of Atauro, during a field mission in April and May 2023. State Secretariat for Art and Culture (SEAC), UMR PALOC, 2023, East Timor (ANR 18-CE27-020)
DOI: 10.57780/esa-3qbzz27
title: 0399833

description: Galactic Plane Survey for AO 03 and Pattern 33
DOI: 10.57780/esa-3tvlcaj
title: 0630000

description: AO-6 Key Programme 1: Galactic CentreWe underline the importance of deep and continued observations of the  central molecular zone (CMZ) of the Galaxy with INTEGRAL as crucial  to gaining a more complete understanding of the origin and nature of  the energetic X-rays and gamma-rays detected from this unique part of  the Galaxy. We require long cumulative exposure on the CMZ ( +-200 pc  or +-1.5 deg from Sgr A* and request 2 Ms per year for 4 years. We  point out that given INTEGRALs large field of view (FOV) an  observation programme in the standard dithering mode for which the  nuclear region is the main target and hencewithin IBIS fully coded  FOV will satisfy the interests of many as these central 30 degrees abound  in sources of all kinds including that which is responsible for the  intense 511 keV line emission. Our primary interests remain the  extended emission from the molecularcomplexes of the CMZ including  the central compact emission region known as IGR J17456-2901. [truncated! Please see actual data for full text]
DOI: 10.23708/4672b6cc-b48e-4857-9124-ef37a68e5f45
title: Patrimoine culturel - Île d'Atauro - Timor oriental - Asie
title: Cultural heritage- Atauro Island - East Timor - Asia

description: Identification et numérisation du patrimoine culturel de l'ïle d'Atauro, Timor oriental. Les données sont issues de terrain réalisés sur l'ïle d'Atuaro entre 2019 et 2023 par Dominique Guillaud dans le cadre du Programme ANR 18-CE27-020. Après mise en place des autorisations de recherche et la collecte des accords des populations, l’équipe a pu totaliser 270 jours de terrain au cours de 8 missions. L’approche participative a impliqué de travailler avec plusieurs informateurs et avec un collectif d'habitants.
description: Identification and digitisation of cultural heritage - Atauro Island. The data comes from fieldwork carried out on the island of Atuaro between 2019 and 2023 by Dominique Guillaud as part of the ANR 18-CE27-020 Program. After setting up research authorizations and collecting agreements from local populations, the team was able to spend a total of 270 days in the field over the course of 8 missions. The participatory approach involved working with several informants and with a collective of local residents.
DOI: 10.57780/esa-3u4p0yl
title: 8860286

description: OMC FF sequence ISOC V10 onwards: sequence of ff measurements with LED on/off followed by a DC cal.
DOI: 10.57780/esa-3vhdk2v
title: 8860079

description: Miscellaneous pointing for rev 345
DOI: 10.23708/015195a0-ae5b-455e-9ca4-4cab44274fcd
title: Sites archéologiques - Île d'Atauro - Timor oriental - Asie
title: Archaeological sites- Atauro Island - East Timor - Asia

description: Identification et numérisation des sites archéologiques de l'ïle d'Atauro, Timor oriental. Les données collectées sont issues de terrain réalisés sur l'ïle d'Atauro entre 2013 et 2020 par Jean-Christophe Galipaud dans le cadre de missions financées par l'IRD puis par le programme ANR 18-CE27-020.
description: Identification and digitization of archaeological sites on Atauro Island, East Timor. The data collected comes from fieldwork carried out on the island of Atauro between 2013 and 2020 by Jean-Christophe Galipaud as part of missions funded by the IRD and then by the ANR 18-CE27-020 program.
DOI: 10.57780/esa-3vwib12
title: 1620017

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-3w8zm27
title: 0220094

description: We propose a Target of Opportunity Observation of the recurrent pulsating transient X0115+63 in Outburst.We propose two observations of 200 ksec each (total 400 ksec) to be performed at two different luminosity states according to a strategy that depends on the type of the outburst. The key scientific objectives of the proposal are: measurement of the position width and depth of multiple harmonics across the pulse phase  measurement of the shapes of the harmonic so to test the different models for line formation  study of the dependence of the cyclotron structures on the luminosity and possibly measure the physical heights of the scattering region  measurement of the QPO and testing of the rotating warp/lump model. We will also search for red-shifted gamma-ray lines particularly 2.2 MeV photons from deuterium formation from nuclear processes at the neutron star polar cap. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-3wq9t8q
title: 1940021

description: While INTEGRAL instruments typically observe Galactic sources on the hundreds to thousands of pc scale the closest vicinity to Earth the solar system has received almost no attention from INTEGRAL in its more than 18 yr mission life time. So far the Earth had been used as an occulting object to measure the cosmic X-ray background. During one such observation IBIS could observe auroral X-ray emission from Earth in real time showing the interactions of the solar wind with the magnetic field of Earth. Such auroral emission has also been measured from Jupiter and found to not only be powered by solar activity but by the planet itself. Venus is also a known X-ray source. Lacking strong magnetic field and subsequently a pronounced magnetosphere Venus produces X-ray emission with atmospheric fluorescence as it is illuminated by Solar X-rays by Solar Wind Charge Exchange Mechanism (SWCX) or possibly by other currently poorly understood unknown processes. Most of the phenomena are restricted to photon energies of few keV but electron bremsstrahlung can be expected up to the hard X-ray regime as suggested from a population of relativistic electrons in the Jupiter system. A significant contribution to the diffuse emission above 100 keV comes from the interaction of cosmic rays (CRs) with asteroids in the Main Belt (MB) between Mars and Jupiter as well as from Kuiper Belt Objects (KBOs) Especially at the 511 keV line such a contribution from the ecliptic may result in false inferences for the size of and flux from the bulge halo and disk. We propose an observation program of the ecliptic to constrain the hard X-ray emission from Venus and Jupiter and to better estimate the foreground emission from the solar system M-NM-3-ray albedo. This proposal is a replacement and an extension of a multi-year proposal accepted in AO18 (PI: T. Siegert) and AO19. The present proposal differs primarily by adding Venus. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-3yvciy1
title: 2020017

description: We ask for the continuation of the INTEGRAL Key Programme observations of the area of the Galaxy bounded by -20<=  l <= +20 and -15 <= b <= +15 with a total of 2 Msec of observations. The aim is to study the inner region of the Galaxy including the hard X-ray variability of Sgr A*  and to enable significant serendipitous science in the Galactic center region. We do not ask for data rights for any of the sources except for the Galactic Center. [truncated! Please see actual data for full text]
DOI: 10.23708/bc3ab1e4-5386-4eee-9576-0015e901e7de
title: Routes - Île d'Atauro - Timor oriental - Asie
title: Roads - Atauro Island - East Timor - Asia

description: Routes de l'ïle d'Atauro, Timor oriental numérisées à partir de l'image satellite Pléiades 157 km2, Bundle à.5, Panchro + 2 m Color, datée du 19 mai 2016.
description: Roads on Atauro Island, East Timor digitized from Pleiades satellite image 157 km2, Bundle à.5, Panchro + 2 m Color, dated May 19, 2016.
DOI: 10.57780/esa-3yx6072
title: 0399819

description: Galactic Plane Survey for AO 03 and Pattern 19
DOI: 10.57780/esa-43f5i6h
title: 8860167

description: Crab-2007 Spring: JEM-X grey filter test
DOI: 10.23708/c92115d3-f58e-42e2-b7b4-3d84529fd26f
title: Paysage - Île d'Atauro - Timor oriental - Asie
title: Landscape- Atauro Island - East Timor - Asia

description: Les données sont issues d’un séjour de terrain mené par Dominique Guillaud en novembre-décembre 2019, dans le cadre du projet Politiques culturelles, patrimoines locaux et approches collaboratives dans l’Est insulindien—ANR-18-CE27-020 POPEI-COLL. Les données sur le paysage sont centrées sur le village de Makili situé au sud-est de l'ïle d'Atauro (Timor-Leste). Forêt et champs sont cartographiés afin de mieux comprendre les difficultés de la population à faire face aux crises passées et présentes.
description: The data come from a field trip conducted by Dominique Guillaud in November-December 2019, as part of the project Politiques culturelles, patrimoines locaux et approches collaboratives dans l'Est insulindien-ANR-18-CE27-020 POPEI. The data collected focuses on the village of Makili in the south-east of the island of Atauro (Timor-Leste). The landscape data focuses on the village of Makili in the south-east of the island of Atauro (Timor-Leste). Forest and fields are mapped in order to better understand the population's difficulties in coping with past and present crises.
DOI: 10.57780/esa-45arhsm
title: 0120014

description: In the 30 years of satellite observations at least six black hole X-ray transients have been seen to undergo recurrent outbursts. The typical timescale is probably between 10-50 years although one system shows regular outbursts every ~1.6 years. We wish to study outbursts from any known BHC transient using INTEGRAL to complement already approved XMM-Newton observations.  The high X-ray sensitivity of XMM-Newton combined with the high-energy coverage of INTEGRAL will allow the complex ultra-soft (at low energies) ultra-hard (at high energies) spectra of the majority of these systems to be simultaneously studied with unprecedented precision. Observations with SPI will allow the properties of any high-energy line features similar to that seen from Nova Muscae to be determined with unprecedented precision. JEM-X data will also be important for helping to understand the X-ray continua since many outbursts are too bright for the CCD cameras on XMM-Newton to operate without significant pile-up. [truncated! Please see actual data for full text]
DOI: 10.23708/e8512a35-1e56-4ace-ad93-fb861a2ace35
title: Maisons coutumières - Île d'Atauro - Timor oriental - Asie
title: Customary houses - Atauro Island - East Timor - Asia

description: Les données sont issues d’un séjour de terrain mené par Gabriel Facal, anthropologue, en novembre-décembre 2019, dans le cadre du projet Politiques culturelles, patrimoines locaux et approches collaboratives dans l’Est insulindien—ANR-18-CE27-020 POPEI-COLL. Les entretiens ont été menés avec 32 membres et chefs de maisons et clans, en langue indonésienne ou par l’intermédiaire d’un habitant de Makili qui traduisait depuis la langue hresuk (parlée à Makili par environ 2 500 locuteurs) vers l’indonésien. Les interlocuteurs principaux, José Lopes (Kau Sahe) et Patricio de Jesus Cabesas (Kurukose), ainsi que tous les représentants de clans ont accepté de partager leurs récits d’origine. Des autorisations de recherche et des accords avec les populations locales ont été mis en place pour ce projet participatif.
description: The data come from a field trip conducted by Gabriel Facal in November-December 2019, as part of the project Politiques culturelles, patrimoines locaux et approches collaboratives dans l'Est insulindien-ANR-18-CE27-020 POPEI-COLL. Interviews were conducted with 32 members and heads of houses and clans, in Indonesian or through a Makili resident who translated from Hresuk (spoken in Makili by around 2,500 speakers) into Indonesian. The main interlocutors, José Lopes (Kau Sahe) and Patricio de Jesus Cabesas (Kurukose), as well as all the clan representatives, agreed to share their origin stories. Research permits and agreements with local populations have been put in place for this participatory project.
DOI: 10.57780/esa-45rci08
title: 0920008

description: Monitoring of microquasars such as GRS 1915+105 and Cygnus X-1 during the previous INTEGRAL AOs has revealed a wealth of new observational information. The monitoring has revealed the dynamical behavior of these sources above 20 keV on all timescales as opposed to the snapshot observations available before. We propose to continue the monitoring of these canonical black holes with a dedicated Key Programme in INTEGRAL AO8 which will also include the soft X-rays through a strategy that allows the source to remain in the field of view of JEM-X. The proposed investigation will allow to study di erent emission models for the two extreme cases of microquasars with INTEGRAL and simultaneous optical IR and radio observations. This proposal is a continuation of our earlier accepted observations that started in AO1. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-45rroez
title: 8860069

description: Crab spring 2005 IBIS 10 deg arc
DOI: 10.57780/esa-46a9p4l
title: 0720006

description: This proposal aims at studying the keV to GeV spectrum and hard X-ray variability of the brightest quasar 3C 273 at obtaining the deepest hard X-ray extragalactic survey and at measuring annihilation and hard X-ray emission from the central region of the Virgo cluster.   SPI is the only available instrument for the next decades to be able to detect the presence of anti-matter in the jet of 3C 273. This detection would have profound implications on models explaining jet creation acceleration and collimation as well as the high-energy emission of AGN.   The three other instruments of INTEGRAL have enough sensitivity to follow the complex spectral variations of 3C 273 from the optical to the hard X-rays for the first time in coordination with GeV measurements by GLAST. This is a unique opportunity to study the correlations between the various emission components of 3C 273 from the eV to the GeV range and compare them with model predictions. Such observations are possible for the first time during AO6  are easy and have far reaching implications.  Key observations will finally be obtained on the hard X-ray emission of M87 probably generated by interaction of its radio bubble and the cooling flow of the Virgo cluster as well as on the expected cluster annihilation emission.  Current INTEGRAL observations of the 3C 273 field already provide the deepest hard X-ray extragalactic survey ever made. With the additional exposure we aim at reaching a flux limit of 0.1 mCrab. This will allow to detect sources with typical luminosity up to a redshift of 0.1 probing the evolution of AGN in the hard X-rays over the last billion years. It will also allow to study the implication of absorption for the cosmic X-ray background the absorption/luminosity relationship and the local AGN luminosity function. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-46s6a24
title: 1820009

description: We propose to continue the INTEGRAL/multi-wavelengh monitoring of GRS 1915+105 with the goal to understand the tight connections that exist between the different emitting media and placed in a broader context understand accreting-ejecting sources in general. We will still take advantage of other facilities we included in the past AOs (the Sardinia and Medicina radio telescopes Insight-HXMT in the X-rays and possibly NICER). We will also include infrared/optical (ESO) through  dedicated proposals.  We require 45 ks pointings taken every second revolution in order to 1) probe the physics of accretion by studying the 0.5-500 keV emission of the source 2) study the origin of the high variability of GRS 1915+105 3) understand the connections between accretion and ejection processes and 4) constrain physical models of emission processes through broad-band spectral and temporal analysis. Points 1) and 2) can be done by looking into the interplay between the soft and hard X-ray emitters (JEM-X and IBIS + HXMT and/or NICER) point 3) and 4) need contemporaneous broad-band coverages and timing studies (with NICER and HXMT). Besides these specific points this monitoring will allow us to accumulate more data and thus have a better view of the (rather unknown) behaviour of this source beyond 200 keV.  It should be noted that GRS 1915+105 lies in a quite crowded field with many variable sources such as X-ray binaries of all types the enigmatic microquasar SS 433 and a couple of highly absorbed IGR sources. This survey will also  permit all these sources to be studied in a regular manner. Such a monitoring will greatly participate to the INTEGRAL legacy by bringing new data for a dozen of exciting Galactic sources. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-49b9xxt
title: 0120187

description: We propose  short (90ksec) INTEGRAL observations of five bright Seyfert galaxies to be performed simultaneously with XMM-Newton. The principle goals of the INTEGRAL study are to measure with very high precision the spectral properties of the Compton reflection bump and the high energy cutoff. We have selected a range of Seyfert types in order to search for any systematic effects of the reflection due to the inclinations of these systems to the line of sight.The XMM-Newton simultaneous observations are essential to the achieve the goals of this proposal especially in measuring the reflection bump. A good knowledge of the complex 2-15keV spectrum is needed to model the gamma-ray spectrum with the precision required. In most cases JEM-X would only give four or five independent spectral points but the use of EPIC would nail down the X-ray tail with extremely high accuracy and in particular determine the ionisation state of the reflecting material.We will apply for XMM-Newton time in their AO2. The execution of this proposal would be conditional on the success of the XMM-Newton proposal. [truncated! Please see actual data for full text]