{"id":1095,"date":"2021-10-26T14:53:24","date_gmt":"2021-10-26T11:53:24","guid":{"rendered":"https:\/\/users.utu.fi\/jurpou\/?page_id=1095"},"modified":"2024-12-14T22:08:21","modified_gmt":"2024-12-14T20:08:21","slug":"presentations","status":"publish","type":"page","link":"https:\/\/users.utu.fi\/jurpou\/presentations\/","title":{"rendered":"Presentations"},"content":{"rendered":"

Recent selected talks<\/h1>\n
\n
\n

X-ray and optical polarimetry<\/h2>\n
\n

 <\/p>\n

X-ray polarization from Comptonizing inflows and outflows [pdf]<\/a>
\ntalk at the conference From The Dolomites To The Event Horizon: Sledging Down The Black Hole Potential Well<\/a>
\nSesto, Italy, July 9, 2024<\/p>\n

X-ray polarimetric view of accreting neutron stars [pdf]<\/a>
\ninvited talk at the workshop Accretion Disks: The First 50 Years<\/a>
\nISSI, Bern, June 19, 2024<\/p>\n

\u041f\u043e\u043b\u044f\u0440\u0438\u043c\u0435\u0442\u0440\u0438\u0447\u0435\u0441\u043a\u0438\u0435 \u043d\u0430\u0431\u043b\u044e\u0434\u0435\u043d\u0438\u044f \u0430\u043a\u043a\u0440\u0435\u0446\u0438\u0440\u0443\u044e\u0449\u0438\u0445 \u0447\u0435\u0440\u043d\u044b\u0445 \u0434\u044b\u0440 \u0437\u0432\u0435\u0437\u0434\u043d\u044b\u0445 \u043c\u0430\u0441\u0441 \u0441\u043f\u0443\u0442\u043d\u0438\u043a\u043e\u043c IXPE (Polarimetric observations of accreting black holes with IXPE) \u00a0[pdf] <\/a>
\ninvited talk at High Energy Astrophysics 2023<\/a>
\nMoscow, Russia, December 21, 2023<\/p>\n

\u0420\u0435\u043d\u0442\u0433\u0435\u043d\u043e\u0432\u0441\u043a\u0430\u044f \u043f\u043e\u043b\u044f\u0440\u0438\u043c\u0435\u0442\u0440\u0438\u044f \u0441 IXPE (X-ray polarimetry with IXPE)\u00a0\u00a0[pdf] <\/a>
\ninvited talk at High Energy Astrophysics 2022<\/a>
\nMoscow, Russia, December 20, 2022<\/p>\n

X-ray polarimetry of accreting neutron stars:\u00a0First results from the\u00a0Imaging X-ray Polarimetry Explorer [pdf]<\/a>
\ninvited talk at international conference From holography to machine learning<\/a>, Helsinki, Finland, October 25, 2022<\/p>\n

Black hole spin- orbit misalignment in the black hole X-ray binary MAXI J1820+070 [pdf]<\/a>
\ntalk at the Astronomer’s Days, Jyv\u00e4skyl\u00e4, May 24, 2022<\/p>\n

High-precision optical polarimetry as a\u00a0tool to learn about orbital orientation\u00a0and nature of optical emission of black\u00a0hole X-ray binaries [pdf]<\/a>
\ninvited seminar at Univ. of Southampton, UK, April 29, 2022<\/p>\n

Polarization by electron scattering [pdf]<\/a>
\nHEA group meeting, Turku, March 31, 2021<\/p>\n

IXPE and perspectives to measure polarization in the X-rays [pdf] <\/a>
\ninvited talk at High Energy Astrophysics 2020<\/a>
\nMoscow, Russia, December 23, 2020<\/p>\n

High precision optical and X-ray polarimetry of accreting black holes [pdf] <\/a>
\nseminar at the AstroSpace Center, Lebedev Physical Institute,
\nMoscow, Russia, May 23, 2019<\/p>\n

Polarization as a tool to study compact objects [pdf] <\/a>
\ntalk at Time for Accretion <\/a>
\nSigtuna, Sweden, August 8, 2018<\/p>\n

X-ray polarimetry: at last? [pdf] <\/a>
\ntalk at High Energy Astrophysics 2017 <\/a>
\nMoscow, Russia, December 21, 2017<\/p>\n

Polarization in X-ray millisecond pulsars [pdf] <\/a>
\ninvited talk at The coming of age of X-ray polarimetry
\nRome, Italy, April 27-30, 2009
\nsee book
\nX-ray Polarimetry: A New Window in Astrophysics <\/a><\/p>\n

 <\/p>\n

\n
\n

Stellar-mass black holes<\/h2>\n
\n

\u041f\u043e\u043b\u044f\u0440\u0438\u043c\u0435\u0442\u0440\u0438\u0447\u0435\u0441\u043a\u0438\u0435 \u043d\u0430\u0431\u043b\u044e\u0434\u0435\u043d\u0438\u044f \u0430\u043a\u043a\u0440\u0435\u0446\u0438\u0440\u0443\u044e\u0449\u0438\u0445 \u0447\u0435\u0440\u043d\u044b\u0445 \u0434\u044b\u0440 \u0437\u0432\u0435\u0437\u0434\u043d\u044b\u0445 \u043c\u0430\u0441\u0441 \u0441\u043f\u0443\u0442\u043d\u0438\u043a\u043e\u043c IXPE (Polarimetric observations of accreting black holes with IXPE) \u00a0[pdf] <\/a>
\ninvited talk at High Energy Astrophysics 2023<\/a>
\nMoscow, Russia, December 21, 2023<\/p>\n

Black hole spin- orbit misalignment in the black hole X-ray binary MAXI J1820+070 [pdf]<\/a>
\ntalk at the Astronomer’s Days, Jyv\u00e4skyl\u00e4, May 24, 2022<\/p>\n

High-precision optical polarimetry as a\u00a0tool to learn about orbital orientation\u00a0and nature of optical emission of black\u00a0hole X-ray binaries [pdf]<\/a>
\ninvited seminar at Univ. of Southampton, UK, April 29, 2022<\/p>\n

High precision optical and X-ray polarimetry of accreting black holes [pdf] <\/a>
\nseminar at the AstroSpace Center, Lebedev Physical Institute,
\nMoscow, Russia, May 23, 2019<\/p>\n

Polarization as a tool to study compact objects [pdf] <\/a>
\ntalk at Time for Accretion <\/a>
\nSigtuna, Sweden, August 8, 2018<\/p>\n

What can we learn about accretion in AGN from stellar-mass black holes? [pdf] <\/a>
\ntalk at The radio and X-ray connection in accreting objects<\/a>
\nMonopoli, Italy, May 24, 2018<\/p>\n

Hybrid hot flow as the source of optical-to-X-ray emission of black hole binaries [pdf] <\/a>
\ntalk at The X-ray Universe 2017<\/a>
\nRome, Italy, June 6, 2017<\/p>\n

On the origin of optical\/infrared flares in accreting black holes [pdf] <\/a>
\ntalk at Shining from the Heart of Darkness: black hole accretion and jets<\/a>
\nKathmandu, Nepal, October 18, 2016<\/p>\n

On the origin of optical\/infrared flares in the low hard state of black hole binaries [pdf] <\/a>
\ntalk at Joint Space-Science Institute workshop Putting Accretion Theory to the Test <\/a>
\nAnnapolis, USA, November 5, 2013<\/p>\n

\n
\n

Neutron stars, accreting ms pulsars, X-ray bursts, and equation of state<\/h2>\n
\n

X-ray polarimetric view of accreting neutron stars [pdf]<\/a>
\ninvited talk at the workshop Accretion Disks: The First 50 Years<\/a>
\nISSI, Bern, June 19, 2024<\/p>\n

X-ray bursts and atmospheres [pdf]<\/a>
\ninvited talk at the conference Weather and Climate on Neutron Stars, Princeton\/Columbia Univ., USA, April 4, 2022<\/p>\n

\u041c\u0438\u043b\u043b\u0438\u0441\u0435\u043a\u0443\u043d\u0434\u043d\u044b\u0435 \u043f\u0443\u043b\u044c\u0441\u0430\u0440\u044b \u043a\u0430\u043a \u043b\u0430\u0431\u043e\u0440\u0430\u0442\u043e\u0440\u0438\u0438 \u0441\u0432\u0435\u0440\u0445\u043f\u043b\u043e\u0442\u043d\u043e\u0439 \u043c\u0430\u0442\u0435\u0440\u0438\u0438 (Millisecond pulsars as laboratories of ultradense matter) [pdf] <\/a>
\ntalk at High Energy Astrophysics 2019<\/a>
\nMoscow, Russia, December 19, 2019<\/p>\n

Neutron star atmosphere models to study dense matter [pdf] <\/a>
\ntalk at The Future of X-ray Timing<\/a>
\nAmsterdam, the Netherlands, October 23, 2019<\/p>\n

X-ray millisecond pulsars, constraints on the EOS and X-ray polarimetry
\n [pdf] <\/a>
\ntalk at X-ray topics in Astronomy: from history to the future (R\u00fcdiger Staubert’s 80th birthday)<\/a>
\nT\u00fcbingen, Germany, April 17, 2019<\/p>\n

Constraining equation of state of neutron stars using astrophysical measurements [pdf] <\/a>
\ntalk at XXXIV International Conference on Interaction of Intense Energy Fluxes with Matter <\/a>
\nElbrus, Russia, March 2, 2019<\/p>\n

Neutron star mass and radius constraints from millisecond X-ray pulsars and X-ray bursters [pdf] <\/a>
\ntalk at Fire and ice: Hot QCD meets cold and dense matter<\/a>
\nSaariselk\u00e4, Finland, April 3, 2018<\/p>\n

X-ray bursts and the equation of state [pdf] <\/a>
\ntalk at ECT* workshop Neutron-rich matter and neutron stars<\/a>
\nTrento, Italy, September 30, 2013<\/p>\n

X-ray bursts and the equation of state [pdf] <\/a>
\ntalk at The European Week of Astronomy and Space Science 2013 Symposium “Extreme physics of neutron stars” <\/a>
\nTurku, Finland, June 10, 2013<\/p>\n

Time-dependent simulations of the spreading layers and the origin of quasi-period oscillations in accreting weakly-magnetized neutron stars [pdf] <\/a>
\ntalk at Physics of Neutron Stars<\/a>
\nSt. Petersburg, Russia, June 24-27, 2008<\/p>\n

\n
\n

Ultra-luminous X-ray sources, ULX pulsars, X-ray pulsars<\/h2>\n
\n

X-ray polarimetry of accreting neutron stars:\u00a0First results from the\u00a0Imaging X-ray Polarimetry Explorer [pdf]<\/a>
\ninvited talk at international conference From holography to machine learning<\/a>, Helsinki, Finland, October 25, 2022<\/p>\n

Ultraluminous X-ray pulsars [pdf] <\/a>
\nseminar at the High Energy Division of the Space Research Institute (IKI), Moscow, Russia, March 19, 2019<\/p>\n

Ultraluminous X-ray pulsars: the high-B interpretation [pdf] <\/a>
\ntalk at ESA ULX pulsar workshop<\/a>
\nESAC, Madrid, Spain, June 8, 2018<\/p>\n

Ultraluminous X-ray pulsars
\n [pdf] <\/a>
\ntalk at Physics of neutron stars 2017, 50 years after <\/a>
\nSt. Petersburg, Russia, July 14, 2017<\/p>\n

A reflection model for the cyclotron lines in the spectra of X-ray pulsars [pdf] <\/a>
\ntalk at Explosive Transients: Lighthouses of the Universe <\/a>
\nSantorini, Greece, September 18, 2013<\/p>\n

On the association of the ultraluminous X-ray sources in the Antennae galaxies with young stellar clusters [pdf] <\/a>
\ntalk at Oulu high-energy astrophysics workshop in honour of Dmitri I. Nagirner’s 75th birthday, Oulu, Finland, April 17, 2013<\/p>\n

\n
\n

Blazars<\/h2>\n
\n

Gamma-ray breaks and absorption within broad-line region [pdf] <\/a>
\ntalk at Future directions of relativistic jets <\/a>
\nSkokloster, Sweden, September 1, 2013<\/p>\n

Spectral features in blazars: implications for gamma-ray production [pdf] <\/a>
\ntalk at MAGIC collaboration meeting, Turku, Finland, June 12, 2013<\/p>\n","protected":false},"excerpt":{"rendered":"

Recent selected talks X-ray and optical polarimetry   X-ray polarization from Comptonizing inflows and outflows [pdf] talk at the conference From The Dolomites To The Event Horizon: Sledging Down The Black Hole Potential Well Sesto, Italy, July 9, 2024 X-ray polarimetric view of accreting neutron stars [pdf] invited talk at the workshop Accretion Disks: The […]<\/p>\n","protected":false},"author":1500,"featured_media":0,"parent":0,"menu_order":2,"comment_status":"closed","ping_status":"closed","template":"","meta":{"site-sidebar-layout":"default","site-content-layout":"","ast-site-content-layout":"default","site-content-style":"default","site-sidebar-style":"default","ast-global-header-display":"","ast-banner-title-visibility":"","ast-main-header-display":"","ast-hfb-above-header-display":"","ast-hfb-below-header-display":"","ast-hfb-mobile-header-display":"","site-post-title":"","ast-breadcrumbs-content":"","ast-featured-img":"","footer-sml-layout":"","ast-disable-related-posts":"","theme-transparent-header-meta":"","adv-header-id-meta":"","stick-header-meta":"","header-above-stick-meta":"","header-main-stick-meta":"","header-below-stick-meta":"","astra-migrate-meta-layouts":"default","ast-page-background-enabled":"default","ast-page-background-meta":{"desktop":{"background-color":"var(--ast-global-color-4)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"tablet":{"background-color":"","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"mobile":{"background-color":"","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""}},"ast-content-background-meta":{"desktop":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"tablet":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"mobile":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""}},"footnotes":""},"class_list":["post-1095","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/users.utu.fi\/jurpou\/wp-json\/wp\/v2\/pages\/1095","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/users.utu.fi\/jurpou\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/users.utu.fi\/jurpou\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/users.utu.fi\/jurpou\/wp-json\/wp\/v2\/users\/1500"}],"replies":[{"embeddable":true,"href":"https:\/\/users.utu.fi\/jurpou\/wp-json\/wp\/v2\/comments?post=1095"}],"version-history":[{"count":15,"href":"https:\/\/users.utu.fi\/jurpou\/wp-json\/wp\/v2\/pages\/1095\/revisions"}],"predecessor-version":[{"id":2178,"href":"https:\/\/users.utu.fi\/jurpou\/wp-json\/wp\/v2\/pages\/1095\/revisions\/2178"}],"wp:attachment":[{"href":"https:\/\/users.utu.fi\/jurpou\/wp-json\/wp\/v2\/media?parent=1095"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}