Tools for advanced High-Energy Astrophysics data analysis
One of the activities carried out in the AHEAD2020 programme includes the study and development of Advanced Data Analysis tools for High Energy (WP14). The main objectives of this work-package are:
- to maximize the scientific output from next generation X-ray observatories such as Athena, XRISM, eROSITA, Einstein Probe, defining and developing appropriate tools for the new capabilities offered by those missions;
- support the community for best data exploitation.
XRISM/Resolve and Athena/X-IFU
micro-calorimeters will provide in the next decades spectra
with unprecedented energy resolution in the X-ray band.
Furthermore, X-IFU will be the first X-ray integral field
instrument with a number of pixels similar to current
optical/NIR IFU.
eROSITA
first and Athena/WFI later will revolutionize the field of
X-ray surveys, opening new large discovery spaces on this
field.
SVOM,
Einstein Probe, HERMES, eXTP will provide monitoring for HE
transients, alerts and transients light curves with
unprecedented timing.
First meeting: Monday 21 February 2022
The meeting will assess the progresses
made within the the
framework of the AHEAD2020 WP14 project during the first 2 years of the programme,
and will design the work of the next two
years by collecting additional inputs from community experts in the general fields of
instrumentation, spectroscopy, imaging, timing,
data-analysis, statistics and background-modelling.
Meeting's Agenda:
| MORNING SESSION |
* |
||
| Report + Introduction |
F. Fiore |
WPL |
10:30-10:42 |
| TRIGGERING |
|||
|
|
P. O'Brien |
TL |
10:42-10:54 |
|
|
G. Di Lillo |
I |
10:54-11:11 |
| SOURCE DETECTION and SURVEYS |
|||
|
|
A. Georgakakis |
TL |
11:11-11:23 |
|
|
G. Lanzuisi |
I |
11:23-11:40 |
| MACHINE LEARNING 1 |
|||
|
|
F. Carrera |
TL |
11:40-11:52 |
| EXTENDED SOURCES 1 |
|||
Blind source separation/reconstruction in extended sources |
F. Acero- G. Pratt |
TL |
11:52-12:04 |
|
|
P. Mazzotta |
TL |
12:04-12:14 |
|
|
S. Ettori |
TL |
12:14-12:24 |
| AFTERNOON
SESSION |
* |
||
| EXTENDED SOURCES 2 |
|||
|
|
D. Eckert |
I |
14:30-14:47 |
Tools for analysis of X-ray extended sources |
J. Sanders |
I |
14:47-15:04 |
Tools for analysis of cluster of galaxies in the eROSITA survey |
V. Ghirardini |
I |
15:04-15:21 |
| MACHINE LEARNING
2 |
|||
Machine Learning approach to Background Estimation in Fermi/GBT lightcurves |
R. Crupi |
I |
15:50-16:07 |
Machine learning techniques for micro-calorimeter data-reduction |
M. Ceballos |
TL |
15:38-15:50 |
| HIGH RESOLUTION
TIME-RESOLVED SPECTROSCOPY |
|||
High resolution spectroscopy |
E. Behar |
I |
15:50-16:07 |
Tool for high resolution spectral-timing |
E. Costantini |
TL |
16:07-16:19 |
Blind Line Search and Time-Evolving Photoionization |
F. Nicastro |
TL |
16:19-16:31 |
| BACKGROUND AND
CALIBRATION |
|||
Advanced Background Modeling |
S. Lotti |
TL |
16:31-16:43 |
Cross calibrations Analysis |
J. Nevalainen |
TL |
16:43-16:55 |
* I = Invited; TL = Task-Leader; WPL=Work-Package Leader
Links