AGENDA

Monday afternoon:

• 2pm: Welcome and organisation of the week (Pop/Giorgio)

• 2h15pm: Work with TITANa (Agata)

• 3h15pm: Search for objects without soft X-ray excesses (Riccardo)

Coffee break

• 16:45: Feedback from COSPAR meeting (Francesco)

• 17h15: Preparation working sessions (all)

Summary of the possible actions

• How the soft X-ray excess strength vary with the AGN properties (L/Ledd, BH Mass, Hbeta)

  • start with the P18 sample

Action: Riccardo & Francesco

• Fit AGN spectra with the TITAN tables

  • apply to the P18 sample

Action: Anatoliy & Samuel

• Timing: What about the structure function? Pro and cons? Its application in the litterature? How does it compare to PDS? Action: Barbara + Riccardo

• Constraint on the soft excess from IR nebular lines (see Fernández-Ontiveros & Muñoz-Darias 2021)

Action: Samuel, Pop, Stefano

• X-ray polarimetry from warm corona

Jakub Podgorny has worked on TITAN+STOKES code for XrB. Why not looking at the expected X-ray polarimetry in the soft X-ray band in the case of AGN warm corona?

Action: ?

• Warm corona stability…

Action: Renaud, Pop, Agata,

Tuesday Morning:

• 9am: Constraint on the soft excess from IR nebular lines (see Fernández-Ontiveros & Muñoz-Darias 2021) (Samuel)

• 10am: Modeling of lags in the presence of a warm coronae (Barbara)

• 11am: Timing properties of a accretion flow structure (Julien)

• 12am: Issues with Changing look AGN (Bozena)

Lunch

• 2:30pm: Temperature measurements and variability with NuStar data (Alessandra)

• 3:30pm: UFO in SUBWAYS: a population study (Vittoria)

• 4:30pm-6:00pm: Working session

Summary of the possible actions

• Impact of the presende of a warm corona on the soft and hard lags

Action: Barbara & Julien

Tuesday Morning: Summary of the working sessions

• Fit of the P18 sample with TITAN table (Samuel)

• Search for correlation in the P18 sample from the two coronae fits (Francesco, Riccardo)

• Impact of a warm corona on timing properties (Julien, Barbara)

Potential papers

• on the TITAN fits of the P18 sample (Samuel et al.)

Leader: Samuel

• on the correlation in the P18 sample

No clear correlation... No room for a paper for the moment

Action: Apply to a larger sample. Francesco and Riccardo will check nb of AGN with 1 obs in CAIXA but several OM filters that will be inlcuded in the analysis

• on the impact of the warm corona on timing

Action: work in progress by Julien and Barbara