III IPARCOS Congress

Session

PhD students

11 Dec 2024, 09:00

Aula Magna M1 (Facultad de Ciencias Físicas, UCM)

16. Satellite quenching in zoom-in simulations of a Milky Way-mass halo: a new project within the AGORA Collaboration

Ramón Rodríguez Cardoso (UCM)

11/12/2024, 09:00

Satellite galaxies experience multiple physical processes when interacting with their host halos, often leading to the quenching of star formation. In the Local Group, satellite quenching has been shown to be highly efficient, affecting most satellites except the most massive ones. While recent surveys are studying Milky Way analogs to assess how representative our Local Group is, the dominant...

2. Description of femtoscopic correlations with realistic pion-kaon interactions: the kappa/K0*(700) case

Alejandro Canoa Monsalve (Universidad Complutense de Madrid)

11/12/2024, 09:10

The ALICE collaboration has recently reported pi+-K_S femtoscopic correlations in pp collisions[1]. Here we show [2] how they can be well described using existing realistic pi-K interactions obtained from a dispersive analysis of scattering data [3], containing an accurate description of the kappa/K0*(700) resonance pole. [1] . Acharya et al. (ALICE), Phys. Lett. B 856, 138915 (2024),...

10. Developments for the camera trigger system of the Cherenkov Telescope Array

Alejandro Pérez Aguilera

11/12/2024, 09:20

15. Preliminary results of the study of low-mass dwarf galaxies from the ITP Dwarfs4MOSAIC

Mrs María Chillarón Víctor

11/12/2024, 09:30

The study of the first galaxies which contributed to the ionization of the universe will become possible with an integral field and multi-object spectrograph like MOSAIC (significant contribution from GUAIX), set to be installed on the 39m Extremely Large Telescope (ELT), currently under construction. As a pilot study for that, a detailed two-dimensional study of the physical properties of a...

12. Gamma-ray astronomy activities in CIEMAT

Mr Juan Bernete Medrano

11/12/2024, 09:40

The CIEMAT Gamma-Ray Astronomy group works within the MAGIC and CTA-LST collaborations, covering a wide range of activities from hardware development and testing to data analysis and scientific research. This talk will summarize our main contributions and their role in advancing gamma-ray astrophysics.

13. Mapping the diffuse magnetised gas in the Shapley Supercluster

David Alonso López (UCM)

11/12/2024, 09:50

Most of the ‘missing’ baryons in the local Universe are expected to reside in some diffuse gas phase of the intergalactic medium. In fact, recent results from X-ray absorption studies and Fast Radio Bursts indicate that all the baryons are essentially accounted for, but it remains to be determined exactly where they lie. Studies that cross-correlate galaxies with the thermal Sunyaev-Zel’dovich...

27. Pairwise learning framefork for timing characterization in TOF-PET

José Andrés Avellaneda González (Universidad Complutense de Madrid)

11/12/2024, 10:00

28. Exoplanetary systems around M dwarfs with radial velocities: use of multidimensional Gaussian process to quantify the stellar noise

Javier Benegas Paredes (IPARCOS-UCM)

11/12/2024, 10:10

In order to find Earth-like planets in the habitable zone of M dwarfs, it becomes essential to quantify the stellar noise in the radial velocity (RV) data in order to measure planetary signals. This is why the use of multidimensional Gaussian processes can be a clear evolution towards the study and characterisation of exoplanets and their host stars, this will be done using the pyaneti...

30. DUNE’S SENSITIVITY TO SOLAR NEUTRINOS

Sergio Manthey Corchado (CIEMAT)

11/12/2024, 10:20