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 CLASS:PUBLIC CREATED:20241011T121724Z DESCRIPTION:Thursday\, October 24\n \nSession 13: From INTEGRAL to the next generation high-energy facilities\n \nConvenors: P. Ubertini (INAF\, IAPS \, Roma) / E. Bozzo (University of Geneva)\n \n14:30 Julien Malzac …… ……………………………………………………………… ……………………………………………………………… …………………The Compton Spectrometer and Imager\nIRAP (CNRS\, UPS \, OMP\, CNES)\, France\n \nThe Compton Spectrometer and Imager (COSI) is a NASA Astrophysics Small Explorer (SMEX) satellite mission in development with a planned launch to low-Earth orbit in 2027. COSI is a wide-field ga mma-ray telescope designed to survey the entire sky at 0.2-5 MeV. It provi des imaging\, spectroscopy\, and polarimetry of astrophysical sources\, an d its germanium detectors provide excellent energy resolution for emission line measurements\, including the positron annihilation line at 0.511 MeV and nuclear lines. Polarimetry measurements focus on studies of accreting black holes\, including Active Galactic Nuclei. The instantaneous field o f view for the germanium detectors is >25% of the sky\, and they are surro unded on the sides and bottom by active shields\, providing background rej ection as well as allowing for detection of gamma-ray bursts and other gam ma-ray transients over most of the sky. This presentation will include an overview of the COSI mission and science and the project status.\n \n14:50 Carlotta Pittori………………………………………………… ……………………………………………………………… ……………………………………………………………… ….The AGILE Legacy\nINAF-OAR and ASI-SSDC\, Rome\n \nAGILE has been a un ique and successful space mission of the Italian Space Agency (ASI)\, with the programmatic and technical contribution of INAF and INFN. During almo st 17 years of observations\, since the launch on April 23\, 2007 to the s atellite re-entry on February 14\, 2024\, AGILE contributed to high-energy astrophysics and terrestrial physics with many discoveries and detections . Thanks to its sky monitoring capability and fast ground segment alert sy stem\, AGILE produced several important scientific results\, among which t he unexpected discovery of strong and rapid gamma-ray flares from the Crab Nebula over daily timescales (Bruno Rossi Prize 2012). I will give an ove rview of the main AGILE scientific results\, including some recent updates on the science of Gamma-Ray Bursts (GRBs)\, Fast Radio Bursts (FRBs) and the hunt for electromagnetic counterparts to Gravitational Waves (GW) and cosmic neutrinos. With the satellite re-entry the in-orbit phase ends\, bu t a new phase of scientific work on the AGILE legacy data archive opens: A GILE may still hold future surprises.\n \n15:10 Matteo Guainazzi ……… ……………………………………………………………… ……………………………………………………………… ………………………………………………. NewAthena\nESA\, E STEC\, Noordwijk\n \nNewAthena is a powerful\, open observatory\, enabling unprecedented studies of a wide range of astronomical phenomena. These in clude distant gamma-ray bursts\, the hot gas found in the space around clu sters of galaxies\, accreting compact objects such as black holes over the ir whole mass range and neutron stars\, supernova explosion and remnants\, stars\, white dwarfs\, exoplanets and their parent stars\, Jupiter’s au roras and comets in our own Solar System\, and the interstellar medium (ga s and dust). The scientific payload comprises: the X-ray Integral Field Un it a cryogenic imaging spectrometer covering the 0.2 to 12 keV energy rang e with energy resolution of less than 4 eV at 7 keV over ∼1500 pixels co vering an effective diameter of 4’\, and\; the Wide Field Imager (WFI) c overing the 0.1 to 12 keV energy range\, with 40’x40’ field of view (F oV)\, excellent spatial and energy resolution and count rate capabilities up to the Crab regime and beyond. During each sky observation one of the t wo instruments will be placed in the focal plane of a single X-ray telesco pe with a large collecting area exceeding 1 square-meter at 1 keV\, and an angular resolution of 9” (HalfEnergy Width\, 1 keV on-axis)\, averaging to 10” over the WFI FoV.\n \n15:30 Enrico Bozzo\nUniversity of Geneva\n \nIn this talk\, I will provide a brief summary of the different probe mi ssion concepts that have been sub[1]mitted in response to the NASA PROBE M ISSION call at the end of 2023. The probe mission concepts known so far ar e: LEM\, STROBE-X\, HEX-P\, ARCUS\, and AXIS.\n \n15:30 Concluding Remarks \n \n16:10 End of conference\n \n-~-~-~-~-~-~-~-~-~-~-~-~-~-~-~-~-~-~-~-~- ~-~-\n-- Do not delete or change any of the following text. -- \n \nWhen i t's time\, join your Webex meeting here. \n \n \nMeeting number (access co de): 2373 940 6614\nMeeting password: KkPwUyK8k44 \n \n \nJoin meeting \n \nTap to join from a mobile device (attendees only) \n+44-20-3478-528 9\,\,23739406614## United Kingdom Toll \n\nJoin by phone \n+44-20-3478-5289 United Kingdom Toll \nGlobal call-in numbers \n \nJoin from a video syst em or application\nDial 23739406614@esait.webex.com \nYou can also dial 62.109.219.4 and enter your meeting numb er. \n \n \nIf you are a host\, click here and login s ite to view host information. \n \n \nNeed help? Go to http://help.webex.c om \n \n \n \n \n \n \n DTEND;TZID="W. Europe Standard Time":20241024T161500 DTSTAMP:20241011T121724Z DTSTART;TZID="W. Europe Standard Time":20241024T143000 LAST-MODIFIED:20241011T121724Z 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 4 – Thu Oct 24 PM – Session 13 TRANSP:OPAQUE UID:040000008200E00074C5B7101A82E00800000000C0EEEA6ADF1BDB01000000000000000 010000000A6D6BAB27627EB4F98FAEC1A04AA9977 X-ALT-DESC;FMTTYPE=text/html:

Thursda y\, October 24

 \;

Ses sion 13: From INTEGRAL to the next generation high-energy facilities< /o:p>

 \;

Conven ors: P. Ubertini (INAF\, IAPS\, Roma) / E. Bozzo (University of Geneva)

 \;

14:30< /span> Julien Mal zac ……………………………………………………… ……………………………………………………………… ………………………………The Compton Spectrometer and Imager

IRAP (CNRS\, UPS\, OMP\, CNES)\, France< /o:p>

< o:p> \;

The Compton Spectrometer and Imager (COSI) is a NASA Astrophysi cs Small Explorer (SMEX) satellite mission in development with a planned l aunch to low-Earth orbit in 2027. COSI is a wide-field gamma-ray telescope designed to survey the entire sky at 0.2-5 MeV. It provides imaging\, spe ctroscopy\, and polarimetry of astrophysical sources\, and its germanium d etectors provide excellent energy resolution for emission line measurement s\, including the positron annihilation line at 0.511 MeV and nuclear line s. Polarimetry measurements focus on studies of accreting black holes\, in cluding Active Galactic Nuclei. The instantaneous field of view for the ge rmanium detectors is >\;25% of the sky\, and they are surrounded on the sides and bottom by active shields\, providing background rejection as wel l as allowing for detection of gamma-ray bursts and other gamma-ray transi ents over most of the sky. This presentation will include an overview of t he COSI mission and science and the project status.

< p class=MsoNormal style='text-indent:36.0pt'> \;

14:50 Carlotta Pittori…… ……………………………………………………………… ……………………………………………………………… ……………………………………………….The AGILE Legacy

INAF-OAR and ASI-SSDC\, Rome

 \;

AGILE has been a unique and successful space mi ssion of the Italian Space Agency (ASI)\, with the programmatic and techni cal contribution of INAF and INFN. During almost 17 years of observations\ , since the launch on April 23\, 2007 to the sate llite re-entry on February 14\, 2024\, AGILE contributed to high-energy as trophysics and terrestrial physics with many discoveries and detections. T hanks to its sky monitoring capability and fast ground segment alert syste m\, AGILE produced several important scientific results\, among which the unexpected discovery of strong and rapid gamma-ray flares from the Crab Ne bula over daily timescales (Bruno Rossi Prize 2012). I will give an overvi ew of the main AGILE scientific results\, including some recent updates on the science of Gamma-Ray Bursts (GRBs)\, Fast Radio Bursts (FRBs) and the hunt for electromagnetic counterparts to Gravitational Waves (GW) and cos mic neutrinos. With the satellite re-entry the in-orbit phase ends\, but a new phase of scientific work on the AGILE legacy data archive opens: AGIL E may still hold future surprises.

 \;

15:10 Matteo Guainazzi ……………………………………… ……………………………………………………………… ……………………………………………………………… ………………. NewAthena< /b>

ESA\, ESTEC\, Noordwijk

 \;

NewAthena is a powerful\, open observatory\, enabling unprecedented studies of a wide range of astronomical phenomena. These include distant gamma-ray bursts\, the hot gas found in the space ar ound clusters of galaxies\, accreting compact objects such as black holes over their whole mass range and neutron stars\, supernova explosion and re mnants\, stars\, white dwarfs\, exoplanets and their parent stars\, Jupite r’s auroras and comets in our own Solar System\ , and the interstellar medium (gas and dust). The scientific payload compr ises: the X-ray Integral Field Unit a cryogenic imaging spectrometer cover ing the 0.2 to 12 keV energy range with energy resolution of less than 4 e V at 7 keV over ∼1500 pixels covering an effective diameter of 4< span style='font-size:12.0pt\;mso-bidi-font-family:Aptos'>’\, and\; the Wide Field Imager (WFI) covering the 0.1 to 12 keV energy range\, with 40’x40< /span>’ field of view (FoV)\, excellent spatial and energy resolution and count rate capabilities up to the Crab regime and beyond. During each sky observation one of the two instruments will be placed in the focal plane of a single X-ray telesc ope with a large collecting area exceeding 1 square-meter at 1 keV\, and a n angular resolution of 9” (HalfEnergy Width\, 1 keV on-axis)\, averaging to 10” over the WFI FoV.

 \;

1 5:30 Enrico Bozzo< /span>

University of Geneva

 \;

In this talk\, I will provide a brief summary< /span> of the different probe mission concepts that have been sub[1]mitted in r esponse to the NASA PROBE MISSION call at the end of 2023. The probe missi on concepts known so far are: LEM\, STROBE-X\, HE X-P\, ARCUS\, and AXIS.

 \;

15:30 Concluding Remarks

&nb sp\;

16:10 End of conference

 \;

-~-~-~-~-~-~-~-~-~-~-~-~-~-~-~-~-~-~-~-~ -~-~-

-- Do not delete or change any of the following text. --

 \;

When it's time\, join your Webex meeting here. < /o:p>

 \;< /o:p>

 \;

Mee ting number (access code): 2373 940 6614

Meeting pa ssword: KkPwUyK8k44

 \;

 \;

Join meeting

 \;

Tap to join from a mobile device (attendees only)  \;
+44-20-3478-5289\,\,23739406614## Unite d Kingdom Toll \;

Join by phone  \;
+44-20-3 478-5289 United Kingdom Toll  \;
< /span>Global call-in numbers

 \;

Join from a video system or application
Dial 23739406614@esait.webex.com  \;
You can also dial 62.109.219.4 and enter your meet ing number.

 \;

 \;

If you are a host\, click here and login site to view host information.

 \;< /o:p>

 \;

Need help? Go to http://help.web ex.com

 \;< /o:p>

< /span>

 \;

 \;

 \;< /p>

 \;

 \ ;

X-MICROSOFT-CDO-BUSYSTATUS:BUSY X-MICROSOFT-CDO-IMPORTANCE:1 X-MICROSOFT-DISALLOW-COUNTER:FALSE X-MS-OLK-AUTOFILLLOCATION:FALSE X-MS-OLK-CONFTYPE:0 BEGIN:VALARM TRIGGER:-PT15M ACTION:DISPLAY DESCRIPTION:Reminder END:VALARM END:VEVENT END:VCALENDAR