BEGIN:VCALENDAR PRODID:-//Microsoft Corporation//Outlook 16.0 MIMEDIR//EN VERSION:2.0 METHOD:REQUEST X-MS-OLK-FORCEINSPECTOROPEN:TRUE BEGIN:VTIMEZONE TZID:W. Europe Standard Time BEGIN:STANDARD DTSTART:16011028T030000 RRULE:FREQ=YEARLY;BYDAY=-1SU;BYMONTH=10 TZOFFSETFROM:+0200 TZOFFSETTO:+0100 END:STANDARD BEGIN:DAYLIGHT DTSTART:16010325T020000 RRULE:FREQ=YEARLY;BYDAY=-1SU;BYMONTH=3 TZOFFSETFROM:+0100 TZOFFSETTO:+0200 END:DAYLIGHT END:VTIMEZONE BEGIN:VEVENT ATTENDEE;CN="Juan Pablo Vega Gonzalez";RSVP=TRUE:mailto:Juan.Pablo.Vega.Gon zalez@ext.esa.int CLASS:PUBLIC CREATED:20241011T121350Z DESCRIPTION:Monday\, October 21\n \nSession 1: INTEGRAL and its legacy\n \n Convenor: Pietro Ubertini\n \n14:30 Matthias Ehle & Jan-Uwe Ness ……… ……………………………………………………………… ……………………………….. Opening\, announcements\, and missi on status updates\nESA/ESAC\, Madrid\n \n14:45 Olga Dubrovina ………… ……………………………………………………………… ……………………………………………………………… ….. The INTEGRAL Project: Historical Overview\nUniversity of Padua\n \n1 5:15 Guillaume Belanger…………………………………………… ……………………………………………………………… …………………….Unveiling the INTEGRAL Science Legacy Archive\nES A/ESAC\, Madrid\n \n15:30 Carlo Ferrigno…………………………… ……………………………………………………………… …………………………………………….MMODA: Multi-Messenger Online Data Analysis\nUniversity of Geneva\n \n15:45 Oliver Pedros …… ……………………………………………………………… ……………………………………. 22 years of Cd-Te detector in space\, the challenges of ISGRI calibration\n \nThroughout 22 years of ope ration in space\, the ISGRI Cd/Te detector has been exposed to continuous bombardment of high energy particles\, inevitably leading to significant e volution of its properties. This introduces new challenges for the calibra tion of the instrument\, the precision of which is fundamental for scienti fic analysis of the data. We present key characteristics of the detector e volution from mission launch until today and explain the calibration pipel ine allowing us to continuously provide reliable\, well calibrated data to the community.\n \nSession 2: Multi-messenger and time domain astronomy\n \nConvenor: Carlo Ferrigno (University of Geneva)\n \n16:30 Volodymyr Sav chenko………………………………………………………… …………………………………INTEGRAL contributions to establish ment of multi-messenger Astronomy\nUniversity of Geneva\n \nI will review unique and fundamental contributions made by INTEGRAL to emergence and est ablishment of multi-messenger astronomy in the last decade\, focusing on o bservations of transient counterparts of gravitational wave and neutrino e vents.\n \n17:00 Alicia M Sintes…………………………………… ……………………………………………………..Multi-messen ger astronomy with current and future gravitational-wave facilities\nUnive rsitat Illes Balears\n \nGW170817 brought the beginning of the era of mult i-messenger astrophysics with gravitational waves. As the breadth and dept h of gravitational wave detection capabilities grows\, so do the opportuni ties for multi-messenger observations. This talk will survey the near- and medium-term future for ground[1]and space-based gravitational wave observ atories\, the astrophysical sources with the potential to also be observed electromagnetically\, and the promise of how joint observations will answ er longstanding questions in astrophysics\, cosmology\, and fundamental ph ysics.\n \n17:30 Eric Burns ……………………………………… ………………………………………………………… Fast Lo calization of Gamma-Ray Bursts: Implications of a Technical Challenge\nDep artment of Physics and Astronomy\, Louisiana State University (Presented r emotely)\n \nGamma-ray bursts are the most luminous events from the big ba ng\, and are foundational sources for time-domain\, multiwavelength\, and multi-messenger astrophysics. We will discuss the revolution brought about by rapid localization of these events\, and the global follow-up communit y it created. We will discuss the technical difficulties missions face in achieving this capability\, discuss what INTEGRAL has or could enable\, an d what future missions lie ahead. We will also emphasize why this capabili ty is needed for the future.\n \n \n-~-~-~-~-~-~-~-~-~-~-~-~-~-~-~-~-~-~-~ -~-~-~-\n-- Do not delete or change any of the following text. -- \n \nWhe n it's time\, join your Webex meeting here. \n \n \nMeeting number (access code): 2373 940 6614\nMeeting password: KkPwUyK8k44 \n \n \nJoin meeting \n \nTap to join from a mobile device (attendees only) \n+44-20-3478- 5289\,\,23739406614## United Kingdom Toll \n\nJoin by phone \n+44-20-3478-5289 United King dom Toll \nGlobal call-in numbers \n \nJoin from a video s ystem or application\nDial 23739406614@esait.webex.com \nYou can also dial 62.109.219.4 and enter your meeting n umber. \n \n \nIf you are a host\, click here and logi n site to view host information. \n \n \nNeed help? Go to http://help.webe x.com \n \n \n DTEND;TZID="W. Europe Standard Time":20241021T180000 DTSTAMP:20241011T121350Z DTSTART;TZID="W. Europe Standard Time":20241021T143000 LAST-MODIFIED:20241011T121350Z LOCATION:Rooms D1/D2 ORGANIZER;CN="Juan Pablo Vega Gonzalez":mailto:Juan.Pablo.Vega.Gonzalez@ext .esa.int PRIORITY:5 SEQUENCE:0 SUMMARY;LANGUAGE=en-gb:INTEGRAL Workshop 2024 – Day 1 – Mon Oct 21 PM – Sessions 1-2 TRANSP:OPAQUE UID:040000008200E00074C5B7101A82E0080000000040378A84DB1BDB01000000000000000 010000000A968FC5928C1144081B68D8ABF540CDE X-ALT-DESC;FMTTYPE=text/html:

Monday\, October 21

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Session 1: INTEGRAL and its legacy

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Convenor: Pietro Ubertini

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14:30 Matthias Ehle &\; Jan-Uwe Ness …\;…\; 230\;…\;…\;…\;…\;…\;…\;…\;…\;̷ 0\;…\;…\;…\;…\;…\;…\;…\;…\;…\ ;…\;…\;…\;…\;…\;…\;…\;…\;…\;& #8230\;…\;…\;…\;…\;…\;…\;…\;…\;.. Opening\, announcements\, and mission status updates

ESA/ESAC\, Madrid

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14:45 Olga Dubrovina  230\;…\;…\;…\;…\;…\;…\;…\;…\;̷ 0\;…\;…\;…\;…\;…\;…\;…\;…\;…\ ;…\;…\;…\;…\;…\;…\;…\;…\;…\;& #8230\;…\;…\;…\;…\;…\;…\;…\;…\; 230\;…\;…\;…\;…\;…\;…\;…\;…\;̷ 0\;…\;…\;…\;…\;…\;…\;.. The INTEGRAL Project : Historical Overview

University of Padua

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15:15 Guillaume Belanger…\;…\;…\;…\;…\;…\;…\ ;…\;…\;…\;…\;…\;…\;…\;…\;…\;& #8230\;…\;…\;…\;…\;…\;…\;…\;…\; 230\;…\;…\;…\;…\;…\;…\;…\;…\;̷ 0\;…\;…\;…\;…\;…\;…\;…\;…\;…\ ;…\;…\;…\;…\;…\;.Unveiling the INTEGRAL Science L egacy Archive

ESA/ESAC\, Madrid< /span>

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15:30 Carlo Fer rigno…\;…\;…\;…\;…\;…\;…\;…\;̷ 0\;…\;…\;…\;…\;…\;…\;…\;…\;…\ ;…\;…\;…\;…\;…\;…\;…\;…\;…\;& #8230\;…\;…\;…\;…\;…\;…\;…\;…\; 230\;…\;…\;…\;…\;…\;…\;…\;…\;̷ 0\;…\;…\;…\;…\;…\;…\;.MMODA: Multi-Messenger Online Data Analysis

University of Geneva< o:p>

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15:4 5 Oliver Pedros …\;…\;…\;…\; …\;…\;…\;…\;…\;…\;…\;…\;…\;&# 8230\;…\;…\;…\;…\;…\;…\;…\;…\;R 30\;…\;…\;…\;…\;…\;…\;…\;…\;… \;…\;…\;…\;…\;…\;…\;…\;…\;. 22 yea rs of Cd-Te detector in space\, the challenges of ISGRI calibration

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Throughout 22 years of operation in spac e\, the ISGRI Cd/Te detector has been exposed to continuous bombardment of high energy particles\, inevitably leading to s ignificant evolution of its properties. This introduces new challenges for the calibration of the instrument\, the precision of which is fundamental for scientific analysis of the data. We present key characteristics of th e detector evolution from mission launch until today and explain the calib ration pipeline allowing us to continuously provide reliable\, well calibr ated data to the community.

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Session 2: Multi-messenger and tim e domain astronomy

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Con venor: Carlo Ferrigno (University of Geneva)

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16:30 Volodymyr Savchenko… \;…\;…\;…\;…\;…\;…\;…\;…\;…\; …\;…\;…\;…\;…\;…\;…\;…\;…\;&# 8230\;…\;…\;…\;…\;…\;…\;…\;…\;R 30\;…\;…\;…\;…\;…\;…\;INTEGRAL contributions to establishment of multi-messenger Astronomy

University of Geneva

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I will review unique and fundamental contributions made by INTEGRAL to emergence and establish ment of multi-messenger astronomy in the last decade\, focusing on observa tions of transient counterparts of gravitational wave and neutrino events.

& nbsp\;

17:00 Alicia M Sintes…\;…\;…\;…\ ;…\;…\;…\;…\;…\;…\;…\;…\;…\;& #8230\;…\;…\;…\;…\;…\;…\;…\;…\; 230\;…\;…\;…\;…\;…\;…\;…\;…\;̷ 0\;…\;…\;..Multi-messenger astronomy wi th current and future gravitational-wave facilities< /p>

Universitat Illes Balears

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GW170817 brought the beginning of the era of multi-messenger astrophysics with gravitational waves. As the breadth and depth of gravita tional wave detection capabilities grows\, so do the opportunities for mul ti-messenger observations. This talk will survey the near- and medium-term future for ground[1] and space-based gravitational wave observatories\, the astrophysical sourc es with the potential to also be observed electromagnetically\, and the pr omise of how joint observations will answer longstanding questions in astr ophysics\, cosmology\, and fundamental physics.

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17:30 Eric Burns …\;…\;…\;…\;…\; …\;…\;…\;…\;…\;…\;…\;…\;…\;&# 8230\;…\;…\;…\;…\;…\;…\;…\;…\;R 30\;…\;…\;…\;…\;…\;…\;…\;…\;… \;…\;…\;…\;…\; Fast Localization of Gamma-Ray Bursts: Implications of a Technical Challenge

Depar tment of Physics and Astronomy\, Louisiana State University (Presented rem otely)

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Gamma-ray bursts are the most luminous events from the big bang\, and are foundational sources for time-domain\, multiw avelength\, and multi-messenger astrophysics. We will discuss the revoluti on brought about by rapid localization of these events\, and the global fo llow-up community it created. We will discuss the technical difficulties m issions face in achieving this capability\, discuss what INTEGRAL has or c ould enable\, and what future missions lie ahead. We will also emphasize w hy this capability is needed for the future.

 \;

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