This workshop will focus on active galactic nuclei (AGN) and their study using polarimetry. The workshop will include around forty people, all experts in the field of AGNs and/or polarization.
The goals of the workshop are to:
The idea is to have a short and focused workshop with experts in the fields to drive the forthcoming years of research in extragalactic polarimetry. We also clearly need to constrain the requirements of future polarimetric instrumentation that we could propose to the astronomical community, especially knowing that the next generation of big telescopes and satellites are being designed right now (ELT second wave of instruments, HWO, PRIMA, balloon-borne experiments...). Right now, the future of polarimetry (2030+) is pretty bleak, with the exception of radio band polarimetry.
All attending people are welcomed to present their work and discoveries through oral presentations. It will be possible to bring posters to initiate discussions, but each workshop guest is guaranteed to have an oral presentation. Slots will be allocated for debates and the exchange of ideas in order to best understand the polarimetric needs of the AGN community, keeping in mind their applications to other astronomical sources.
Unlike usual conferences, there are no SOC nor invited presentations, since we are all very knowledgeable in the subject and each of us will have the opportunity to speak. Likewise, there will be no need to go into long introductions to the subject so that we concentrate on the essentials. For this reason, this workshop is truly dedicated to specialists in the field (theoreticians, simulators, observers and instrument designers). Because we want to spark discussion and debate, in the conference room or around a drink, it is an in-person only workshop (although talks will be registered and available to the community later on).
Time | Session | Talk | Speaker |
---|---|---|---|
08h50 - 09h20 | Arrival, badge, coffee and croissants | ||
09h20 - 09h30 | Welcome words | Aims and schedule of the workshop | Frédéric Marin |
09h30 - 09h55 | Observations | From local to high redshift: polarimetry as a tool for studying AGN structure | Marko Stalevski |
09h55 - 10h20 | Observations | Full-Stokes monitoring of AGN jets at mm and cm wavelengths | Ioannis Myserlis |
10h20 - 10h45 | Observations | Results from the last multiwavelength polarization study of the archetypical blazar BL Lacertae | Iván Agudo |
10h45 - 11h10 | Observations | A new perspective on radio-quiet AGN through millimeter polarimetry | Elena Shablovinskaya |
11h10 - 11h35 | Observations | Using (sub)millimeter spectral line polarization to study magnetism and the AGN | Boy Lankhaar |
11h35 - 12h00 | Observations | Infrared polarimetry of galaxies in the local and high-z universe | Enrique Lopez Rodriguez |
12h00 - 14h00 | Lunch break | ||
14h00 - 14h25 | Observations | Pushing the limits of optical polarimetric monitoring of blazars | Yannis Liodakis |
14h25 - 14h50 | Observations | Optical and Radio Polarization Behavior of BL Lacertae during Dramatic Multi-Wavelength Activity in 2020-2023 | Svetlana Jorstad | td>
14h50 - 15h15 | Observations | Probing AGN properties with optical (spectro)polarimetry in lines and continuum | Eugene Malygin |
15h15 - 15h40 | Observations | Quasi-Peridoc Eruptions in GSN 069 as viewed in polarized light | Beatriz Agís González |
15h40 - 16h05 | Coffee break | ||
16h05 - 16h30 | Observations | Scattered synchrotron emission and a giant torus revealed in the polarized light of Centaurus A | Frédéric Marin |
16h30 - 16h55 | Observations | Polarized subcomponents in the optical emission of blazars revealed with multimodal approach | Dmitry Blinov |
16h55 - 17h20 | Observations | Spectropolarimetry of low and high redshift QSO | Alessandro Capetti |
17h20 - 17h45 | Observations | Optical spectropolarimetry of a changing look AGN NGC 3516 | Djordje Savic |
17h45 - 18h10 | Observations | Reducing archival imaging polarimetry from HST/FOC to prepare the future of UV polarimetry | Thibault Barnouin |
18h45 | Social event | A drink in the city center |
Time | Session | Talk | Speaker |
---|---|---|---|
09h00 - 09h30 | Coffee and croissants | ||
9h30 - 9h55 | Observations | The IXPE view of RQ AGN | Giorgio Matt |
9h55 - 10h20 | Observations | A Second Look at the X-ray Polarization of NGC 4151 with IXPE | Vittoria Elvezia Gianolli |
10h25 - 10h45 | Observations | Photo-polarimetric monitoring program TOP-MAPCAT in the era of multi-wavelength polarization | Jorge Otero-Santos |
10h45 - 11h10 | Community discussion | Next targets and scientific questions that observations could sove | |
11h10 - 11h35 | Simulations | Spectro-polarimetric AGN torus models with SKIRT | Bert Vander Meulen |
11h35 - 12h00 | Simulations | Fully relativistic Monte-Carlo radiative transfer code for spectra and polarization from disk-corona system | Sudeb Ranjan Datta |
12h00 - 14h00 | Lunch break | ||
14h00 - 14h25 | Simulations | Warm coronas in accreting black holes: from dynamo processes up to radiated spectra (outsider's view) | Jiri Horak |
14h25 - 14h50 | Simulations | X-ray Polarization by Reflection from Accretion Discs | Michal Dovciak |
14h50 - 15h15 | Simulations | X-ray polarization models: reprocessing in distant components of radio-quiet AGNs | Jakub Podgorny |
15h15 - 15h40 | Simulations | The Origin of the X-Ray Polarization in the Circinus Galaxy | Atsushi Tanimoto |
15h40 - 16h05 | Coffee break | ||
16h05 - 16h30 | Simulations | Effect of gravitational microlensing on the polarisation of multiply imaged quasars | Dominique Sluse |
16h30 - 16h55 | Simulations | Decoding Blazar Polarimetry | Lente Dreyer |
16h55 - 17h20 | Simulations | Polarization from Turbulence and Shocks in Blazars | Alan Marscher |
17h20 - 17h45 | Simulations | Probing Particle Acceleration in Blazars with Multi-Wavelength Polarimetr | Haocheng Zhang |
17h45 - 18h10 | Community discussion | What are the needs of the community in terms of simulations? | |
19h30 | Social event | Conference diner |
Time | Session | Talk | Speaker |
---|---|---|---|
9h00 - 9h30 | Coffee and croissants | ||
9h30 - 9h55 | Current and future instruments | ALMA polarization observations | Rosita Paladino |
9h55 - 10h20 | Current and future instruments | Dust Polarimetry and the PRIMA Far-infrared Probe | Brandon Hensley |
10h20 - 10h45 | Current and future instruments | High resolution AGN observations with VLTI/MATISSE | Violeta Gámez Rosas |
10h45 - 11h10 | Current and future instruments | The Habitable Worlds Observatory | Chris Packham |
11h10 - 11h35 | Current and future instruments | IFU spectro-polarimetry with the FiberPol-6D | Sabyasachi Chattopadhyay |
11h35 - 12h00 | Current and future instruments | X-ray polarimetry: IXPE and future | Romana Mikusincova |
12h00 - 14h00 | Lunch break | ||
14h00 - 14h25 | Current and future instruments | StokeSat - A Small Satellite for Soft X-ray Polarimetry | Yannis Liodakis |
14h25 - 14h50 | Current and future instruments | Gamma-Ray Polarimetry with Conversions to e+e- Pairs | Denis Bernard |
14h50 - 15h15 | Current and future instruments | Gamma-Ray Polarimetry for AGNs: Possibilities and Requirements | Merlin Kole |
15h15 - 16h20 | Community discussion | What should be the next polarimeters? | |
16h20 - 16h30 | Closing words | Acknowledgments and summary of the workshop | Frédéric Marin |
Last update (September, 28)
Name | Institute | Country |
---|---|---|
Beatriz Agís González | Institute of Astrophysics, Foundation for Research and Technology-Hellas | Greece |
Ivan Agudo | Instituto de Astrofisica de Andalucia-CSIC | Spain |
Thibault Barnouin (LOC) | Astronomical observatory of Strasbourg | France |
Denis Bernard | LLR, Ecole Polytechnique, CNRS/IN2P3 and IPP | France |
Julie Bierdermann (LOC) | Astronomical observatory of Strasbourg | France |
Alessandro Capetti | Istituto Nazionale di Astrofisica - Torino | Italy |
Sabyasachi Chattopadhyay | South African Astronomical Observatory (SAAO) | South Africa |
Michal Dovciak | Astronomical Institute of the CAS | Czech Republic |
Lente Dreyer | Centre for Space Research, North-West University | South Africa |
Violeta Gamez Rosas | Leiden University | Netherland |
Vittoria Elvezia Gianolli | Université Grenoble Alpes and Università Roma Tre | France |
Brandon S. Hensley | JPL/Caltech | USA | Jiri Horak | Astronomical Institute of the CAS | Czech Republic |
Svetlana Jorstad | IAR, Boston University | USA |
Merlin Kole | University of New Hampshire | USA |
Boy Lankhaar | Chalmers University of Technology | Sweden |
Yannis Liodakis | NASA Marshall Space Flight Center | USA |
Enrique Lopez-Rodriguez | University of South Carolina | USA |
Eugene Malygin | Special astrophysical observatory of RAS | Russia |
Frédéric Marin (organizer) | Astronomical observatory of Strasbourg | France |
Alan Marscher | Boston University | USA |
Giorgio Matt | University Roma III | Italy |
Max Millar-Blanchaer | University of California, Santa Barbara | USA |
Romana Mikusincova | INAF-IAPS, Rome | Italy |
Ioannis Myserlis | Institut de Radioastronomie Millimétrique (IRAM) | Granada, Spain |
Thomas Oliveira (LOC) | Astronomical observatory of Strasbourg | France |
Jorge Otero-Santos | Instituto de Astrofísica de Andalucía | Spain |
Chris Packham | University of Texas at San Antonio | USA |
Rosita Paladino | University of Bologna | Italy |
Jakub Podgorny | Astronomical Institute of the Czech Academy of Sciences | Czech Republic |
Sudeb Ranjan Datta | Astronomical Institute of the Czech Academy of Sciences | Czech Republic |
Mattéo Sautron (LOC) | Astronomical observatory of Strasbourg | France |
Elena Shablovinskaya | Universidad Diego Portales | Chile |
Dominique Sluse | University of Liege | Belgium |
Marzena Sniegowska | Nicolaus Copernicus Astronomical Center | Poland |
Marko Stalevski | University of Belgrade | Serbia |
Atsushi Tanimoto | Kagoshima University | Japan |
Bert Vander Meulen | Astronomical Observatory, Ghent University. | Belgium |
Haocheng Zhang | University of Maryland Baltimore County | USA |
Traveling to Strasbourg
By plane. Strasbourg Airport is located in Entzheim, 10 km from the city center. A shuttle train service runs between the airport and Strasbourg station four times an hour (9 minute journey). Taxis are also available all day. Strasbourg is also easily accessible from the Bâle-Mulhouse, Frankfort and Paris international airports (trains connections).
By train. There are a number of direct trains from Paris and the biggest cities in France and Europe every day. When you arrive at Strasbourg railway station (Gare Centrale) by train, the entire city is at your feet and the cathedral is never very far away.
By car. If you are driving to Strasbourg we recommend you go to the Relay-Tram (P+R) car parks located alongside the tram lines. After parking here, both you and your passengers, up to seven people, can easily get to the city center by tram using the same ticket you got when parkking your car.
Hotels
There are many hotels within a 15-minute walk of the conference venue. We recommend staying on the central island of Strasbourg, not far from the cathedral. From there you can easily walk or take the tram C, E or F to the astronomical observatory.
The conference venue
The conference will take place in the amphitheater of the astronomical observatory of Strasbourg (Observatoire Astronomique de Strasbourg, 11 Rue de l'Université, 67000 Strasbourg). The observatory is accessible from 9:00 a.m. to 6:00 p.m. There will be the possibility of storing suitcases on site.
Two social events, not obligatory, will be offered free of charge to those participating in this workshop.
On Monday 14th in the evening, each participant will receive two tokens to go have a drink at the “Les Berthom” bar in the city center. It is a French beer bar, warm but not too noisy where you can enjoy a good beer while discussing science or something else. Each token represents a drink (a beer or a soft drink). Other or excess drinks will be at your expense.
On Tuesday 15th in the evening, you will be invited to the main hall of the astronomical observatory for a cocktail dinner prepared by Strasbourg chefs (the cocktail includes vegetarian options, please let us know if you have any allergies). To accompany the food, an Alsatian winemaker will come and introduce you to his wines. Possibility of buying bottles of wine at a reduced price from the winegrower the same evening (be careful if you are traveling by plane).
The workshop is only upon invitation, but if you cannot attend, do not hesitate to let us know about experts in similar fields as yours. Our goal is to have lively discussions on AGN and polarimetry, and any keen eye is welcomed.
The workshop do not have conference fees and the social events are also free of charge.
Each participant is strongly encouraged to orally present their latest discoveries in the field of AGNs, polarimetry or any other associated field (modeling, instrumentation, etc.). The deadline to submit an abstract is Friday the 13th, September.