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GSFC XMM-Newton GOF Status Report #397: XMM-NEWTON NEWS #252


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  • Subject: GSFC XMM-Newton GOF Status Report #397: XMM-NEWTON NEWS #252
  • From: Newsletter for users of the XMM-Newton mission <xmmnews@xxx>
  • Date: Tue, 1 Feb 2022 08:57:16 -0500
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   News #252, 1 February 2022

   CONTENTS

   [1]Anticipated timeline for next XMM-Newton Announcement of
   Opportunity: AO-22
   [2]Let us know about XMM-Newton related Ph.D. and prizes for XMM-Newton
   results
   [3]Workshops announcement:
   Spectral/timing/polarimetry properties of AGN: theory and observations
   of the inner workings in these objects
   SUPERMASSIVE BLACK HOLES AT HIGH REDSHIFT
   [4]Call for a Medium-size and a Fast mission opportunity in ESA's
   Science Programme

   NEWS

Anticipated timeline for next XMM-Newton Announcement of Opportunity: AO-22

   The planned key milestones for the Twenty-second XMM-Newton
   "Announcement of Opportunity" have been established. Within this AO-22
   a new call to submit proposals for observations to be performed with
   the XMM-Newton observatory will be issued.

   To be prepared for this, please find below the anticipated timeline:

   Announcement of Opportunity             17 August 2022
   Due date for Proposals                  7 October 2022 (12:00 UT)
   Final OTAC approved programme           mid December 2022

   For approved proposals only:

   Start of Phase II proposal submission   10 January 2023
   Closure of Phase II proposal submission 3 February 2023
   Start of observations                   May 2023

   The official "Announcement of Opportunity" will be made public in the
   [5]XMM-Newton News and on the [6]XMM-Newton Science Operations Centre
   Home Page.

Let us know about XMM-Newton related Ph.D. and prizes for XMM-Newton results

   As already announced in previous issues of this Newsletter, the
   XMM-Newton team is collecting information about the completion of
   doctorates and Ph.D. theses based on (or making use of) XMM-Newton
   observations.

   We would appreciate if you - being a candidate or a supervisor of a
   doctorate - could let us know details through the page

           [7]https://gcc02.safelinks.protection.outlook.com/?url=http%3A%2F%2Fwww.cosmos.esa.int%2Fweb%2Fxmm-newton%2Fphd-theses&amp;data=04%7C01%7Cxmmnews%40lists.nasa.gov%7C2025e47fc821484ed45608d9e58ac288%7C7005d45845be48ae8140d43da96dd17b%7C0%7C0%7C637793206394599517%7CUnknown%7CTWFpbGZsb3d8eyJWIjoiMC4wLjAwMDAiLCJQIjoiV2luMzIiLCJBTiI6Ik1haWwiLCJXVCI6Mn0%3D%7C3000&amp;sdata=AJM846znStnMlKClnZVmP9papkhuFlE3UEG%2BoWisZZY%3D&amp;reserved=0

   Also, we would be grateful if you could inform us (via a message to
   [8]xmmhelp@sciops.esa.int, with subject "Ph.D. thesis work") in case
   you are aware of theses from, or supervised by, colleagues that make
   use of XMM-Newton data but are not yet included in the above list.

Workshops announcement:
Spectral/Timing/Polarimetry properties of AGN: Theory and observations of the
inner workings in these objects
SUPERMASSIVE BLACK HOLES AT HIGH REDSHIFT

   These two workshops will take place in the framework of the [9]COSPAR
   44th Scientific Assembly, from 16 to 24 July 2022, in Athens (Greece).

   Spectral/Timing/Polarimetry properties of AGN: Theory and observations
   of the inner workings in these objects

   The main aim of this event is to bring together both theorists and
   observers, and to review the latest advances in the field of physics of
   AGN, including:
     * X-ray spectral/timing properties of AGN
     * X-ray polarimetric observations of AGN
     * X-ray corona properties and modelling
     * the disc/corona interplay and recent multi-wavelength campaigns
     * X-ray reflection and disc thermal reverberation
     * the nature of the 'soft excess'
     * the nature of the inner accretion flow in AGN

   Supermassive Black Holes at High Redshifts

   Optical and near-IR surveys are exploring very efficiently supermassive
   black holes (SMBH) at high redshifts, and follow-up mm-observations,
   e.g. with ALMA, are offering an unprecedented view of the physical
   properties of their host galaxies. Optically selected AGN, however, may
   only form the tip of the iceberg as they are prone to obscuration.
   X-ray surveys represent the perfect tool to peer through obscuration
   and discover these hidden SMBH. The situation is rapidly changing with
   the serendipitous XMM and Chandra catalogues and certainly with the
   eROSITA all-sky survey.

   This meeting will bring together the results coming from current
   optical and X-ray surveys, and from observations with state-of-the art
   mm and radio interferometers, trying to define solid paths for the
   future JWST, ATHENA, Lynx and AXIS surveys.
   Further details are given in the events Web pages:

   [10]https://gcc02.safelinks.protection.outlook.com/?url=https%3A%2F%2Fwww.cospar-assembly.org%2Fadmin%2Fsession_cospar.php%3Fsession%3D10&amp;data=04%7C01%7Cxmmnews%40lists.nasa.gov%7C2025e47fc821484ed45608d9e58ac288%7C7005d45845be48ae8140d43da96dd17b%7C0%7C0%7C637793206394599517%7CUnknown%7CTWFpbGZsb3d8eyJWIjoiMC4wLjAwMDAiLCJQIjoiV2luMzIiLCJBTiI6Ik1haWwiLCJXVCI6Mn0%3D%7C3000&amp;sdata=0CWG0oV2g9sSafJKHYdioO10eTzaWror4wDqIAwg%2Byo%3D&amp;reserved=0
                                     65

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                                     70

Call for a Medium-size and a Fast mission opportunity in ESA's Science Programme

   The ESA Director of Science solicits the scientific community in ESA's
   Member States for proposals for both a "Fast" mission opportunity (to
   be launched in the 2030-2031 timeframe) and for a Medium mission
   opportunity (to be launched around 2037).

   The new long-term scientific plan Voyage 2050, for the Science
   Programme of the European Space Agency, has been issued in June 2021.
   The plan includes three Large (L) missions in selected science themes
   (Moons of the Giant Planets, From Temperate Exoplanets to the Milky
   Way, and New Physical Probes of the Early Universe) and a set of Medium
   (M) and Fast (F) missions.

   The definition of the F and M space missions is based on a competitive,
   peer-reviewed selection process. Even though the Voyage 2050 plan
   identifies a set of possible themes for the Medium missions, proposals
   in all fields of space science will be considered, with no prejudice.

   The deadline for receipt of Phase-1 proposals is

                    12:00 (noon) CET on 14 February 2022

   Full information can be found at

          [12]https://gcc02.safelinks.protection.outlook.com/?url=https%3A%2F%2Fwww.cosmos.esa.int%2Fweb%2Fcall-for-missions-2021&amp;data=04%7C01%7Cxmmnews%40lists.nasa.gov%7C2025e47fc821484ed45608d9e58ac288%7C7005d45845be48ae8140d43da96dd17b%7C0%7C0%7C637793206394599517%7CUnknown%7CTWFpbGZsb3d8eyJWIjoiMC4wLjAwMDAiLCJQIjoiV2luMzIiLCJBTiI6Ik1haWwiLCJXVCI6Mn0%3D%7C3000&amp;sdata=yDMUczhSJ1a5NhshlEijlrHXMHcBAMqRvmZTBXr5UsI%3D&amp;reserved=0

   XMM-Newton Science Operations Centre at
   ESA’s European Space Astronomy Centre,
   Villanueva de la Cañada, Madrid, Spain

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