IV IPARCOS Congress
Aula Magna M1
Facultad de Ciencias Físicas, UCM
As the institute's cornerstone annual event, the IPARCOS Congress convenes its entire research community—from students just beginning their careers to our senior researchers.
Its purpose is twofold: first, to serve as the main forum for presenting and debating the scientific advancements of the past year; and second, to use this collective review to foster new collaborations and set the scientific priorities for the year to come.
Through a comprehensive program of contributions and talks, the congress aims to showcase the breadth and depth of the institute's scientific output, strengthen internal collaborations and connect researchers across different groups.
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Activity reports: IPARCOS director's report
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09:30
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Short contributions: ---
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09:30
Detecting DM Decay into Gravitons: Theory and Forecasts 13m
Dark matter may not be completely stable, and its decay could lead to new signatures in the form of gravitational waves. In this talk I will present model-independent predictions for the stochastic gravitational wave background produced by dark matter decaying into gravitons. Using this framework, I forecast the sensitivity of current and upcoming gravitational wave detectors to these signals.
Speaker: Álvaro Cendal (Universidad Complutense de Madrid) -
09:43
The CARMENES search for exoplanets around M dwarfs: Discovery of two super-Earth candidates in the inner edge of the habitable zone. 13m
We report evidence of the detection of two super-Earth candidates orbiting nearby M-dwarf stars, identified through CARMENES observations. Both stars show clean periodic signals of a few days and amplitudes consistent with low-mass planets. Thanks to ground-based photometry the stellar activity of the two targets were studied obtaining the stellar rotacional periods. Through Gaussian-process modelling, we efficiently separate stellar variability from true planetary signal. These candidates orbit close to the inner edge of the habitable zone of their host star, providing valuable insight into rocky worlds around cool stars.
Speaker: Javier Banegas Paredes (Universidad Complutense de Madrid) -
09:56
Cosmology and dark sector in TDiff models 13m
General Relativity (GR) is currently the established theory for describing gravity. However, there are certain unresolved theoretical issues (such as the vacuum energy problem) and observational ones (cosmological tensions) that point to the need to consider modifications or extensions of the theory. On the other hand, observations indicate that the universe is undergoing accelerated expansion, which is commonly explained as a consequence of the dominance of a dark energy component whose nature remains unknown. Similarly, it is also known that most of the matter in the universe is present in the form of dark matter, whose nature is likewise unknown. In GR, the fundamental symmetry of the theory is invariance under diffeomorphisms (Diff), which translates into the invariance of physical laws under coordinate transformations. In this talk, we focus on breaking Diff invariance down to the subgroup of transverse diffeomorphisms (TDiff) in the matter sector, specifically studying the cosmological implications that this may have and the possible consequences regarding the description of the dark sector. In particular, we study models with multiple TDiff scalar fields as a possible description of interacting dark matter and dark energy, carrying out an analysis of these models from a phenomenological perspective.
Speaker: Diego Tessainer Bonet (Universidad Complutense de Madrid) -
10:09
Mechanisms that shape star formation: a study on metallicity and HI holes 13m
Understanding the mechanisms that govern star formation in galaxies is essential to uncover their evolution. This work employs Bayesian statistics and data-mining techniques to analyze metallicity gradients, which provide valuable insights into the processing and enrichment of gas in galaxies. A notable trend is the manifestation of the downsizing effect in the resolved properties of galaxies, whereby massive galaxies form stars more rapidly than their lower-mass counterparts.
In addition, Machine Learning techniques will be used to identify HI holes in these galaxies, with the aim of achieving a deeper understanding of how different processes influence galactic evolution. For this, a u-net architecture is employed to quickly identify holes in the atomic gas of a sample of galaxies. Using these, we will further analyze the physics surrounding these structures.
Speaker: Guillermo Valé Arteaga (UCM)
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Coffee break 30m
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Short contributions: ---
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Wormholes: Science or fiction? 13m
Wormholes are objects frequently used in science fiction to traverse great distances on human time scales, taking advantage of these strange geometries to connect regions that appear to be far apart. Surprisingly, these objects are solutions to the field equations of General Relativity if additional fields are included. In particular, the Ellis–Bronnikov solution makes use of a phantom scalar field. But, can they exist in nature?
Recent advances in the field of gravitational waves have opened a new observational window to the universe, turning compact objects into ideal laboratories for testing the theory of gravity. The “ringdown” phase is characterized by certain resonance frequencies and characteristic decay times, known as quasinormal modes. This spectrum of modes can be studied using perturbative methods and allows us to analyze stability, where we find that Ellis–Bronnikov wormholes are unstable under radial perturbations. We propose electrically charging these objects to reduce the instabilities and obtain configurations with large lifetimes.
Speaker: Pablo Navarro Moreno (Universidad Complutense de Madrid) -
11:13
From photometry to spectroscopy: Chemical characterisation of M dwarfs 13m
M dwarfs are the most abundant stars in the Galaxy and key targets for stellar population and exoplanet studies, yet their molecularly rich spectra make chemical analysis difficult. This work presents a set of complementary methods to improve metallicity and abundance determinations in M dwarfs using photometry, low- and high-resolution spectroscopy, and data-driven techniques.
Wide FGK+M binary systems serve as empirical calibrators, allowing the well-characterised FGK primaries to anchor the chemical analysis of their M-dwarf companions. We first develop empirical metallicity relations based on Gaia, 2MASS, and CatWISE photometry, using Bayesian regression and neural networks. We then refine the reference abundances of the FGK primaries through high-resolution analysis, including new C and O measurements and updated odd-Z iron-peak abundances. Building on these benchmarks, we introduce a low-resolution spectroscopic method that derives [X/H] for 15 elements in over 770 M dwarfs from CAFOS spectral indices, recovering trends consistent with high-resolution studies. Finally, we analyse new CARMENES high-resolution spectra of M-dwarf secondaries, confirming their metallicity agreement with FGK companions. These approaches provide scalable, reliable tools for characterising M dwarfs in forthcoming large surveys and missions.
Speaker: Christian Duque (UCM) -
11:26
Graviton contribution to the muon anomalous magnetic moment in higher-derivative gravity 13m
Higher-derivative theories of gravity introduce powers of the Ricci scalar and Ricci tensor in the Hilbert-Einstein action in order to improve renormalizability at the cost of adding massive ghost-like particles. The muon anomalous magnetic moment, $a_\mu = \frac{( g_\mu -2 )}{2} $, given its precise measurement, is a perfect observable to test the viability of these theories and impose restrictions on these massive modes. We compute the one-loop graviton contribution to $a_\mu$ in fourth-derivative gravity. We show that said theory improves convergence with respect to General Relativity while also recovering the latter in the limit of large mass ghosts.
Speaker: Diego Voces Porteiro (Universidad Complutense de Madrid (UCM)) -
11:39
A systematic search for spectral hardening in blazar flares with the Fermi-Large Area Telescope 13m
Blazars are among the most powerful gamma-ray emitters, displaying rapid variability and extreme spectral properties. High synchrotron-peaked blazars (HSPs) and extreme high synchrotron-peaked blazars (EHSPs), with synchrotron peaks exceeding $10^{15}$ Hz and $10^{17}$ Hz, respectively, are crucial for understanding the full range of blazar phenomena and testing models of jet physics. Yet, their understanding remains challenging. This work aims to systematically identify and characterize the most extreme γ-ray blazars using data from the Large Area Telescope (LAT) on board the $\textit{Fermi Gamma-ray Space Telescope}$. The focus is on spectral hardening, where the γ-ray spectrum becomes harder at higher energies, particularly during flaring episodes. This phenomenon is characterized by a flux that decreases with energy up to a break in the GeV range, after which the spectrum hardens as the flux begins to rise. While previous studies have reported spectral hardening in a few individual sources, this work presents the first dedicated, systematic analysis of this effect. We examine 138 blazars with high synchrotron peak frequencies from the 4FGL-DR2 catalog, detecting flaring periods using two methods based on Bayesian Block Analysis. We identify two flaring episodes with indications of spectral hardening, in 4FGL J0238.4-3116 and PKS 2155-304, the latter detected independently by both methods but referring to the same period. These events are consistent with expectations from statistical fluctuations, suggesting that spectral hardening is a rare occurrence (< 0.1 %). These results provide the first population-level constraint on the frequency of such events. The scarcity of events reinforces the notion that the dominant blazar emission mechanism is well described by smoothly varying powerlaw spectra across the $\textit{Fermi}$-LAT range, with sharp spectral hardenings representing rare deviations likely tied to exceptional jet conditions or transient physical processes. Although these flares show notable spectral changes, their statistical significance remains modest and motivates future multi-wavelength studies to assess whether these rare flares reflect genuinely distinct physical processes within blazar jets.
Speaker: Adithiya Dinesh -
11:52
Ghosts in Higher Derivative Quantum Field Theories 13m
When treated as a Quantum Field Theory, General Relativity cannot describe gravity at all energy scales due to the non-renormalizability of the Hilbert-Einstein action. As a consequence, ongoing efforts aim to construct modified actions that improve renormalizability. This way, it might be possible to develop a Quantum Gravity Theory that can make reliable predictions at arbitrarily high energies. One of such modifications involves adding higher derivative terms to the Hilbert-Einstein action. However, these higher-derivative terms also introduce ghost states — which are degrees of freedom with negative energy — that need to be "cured". In this presentation, we will discuss the main problems of a higher derivative theory with a toy model: the Pais-Uhlenbeck oscillator, a scalar higher derivative field theory. We will show how this higher derivative field can be consistently decomposed in two canonical Klein-Gordon fields —standard and ghost— and how the Green's function construction remains consistent from a path integral perspective.
Speaker: Eric García Hemon (Departamento de Física Teórica, Facultad de Ciencias Físicas, Universidad Complutense de Madrid) -
12:05
"The MEGARA/GTC Optical Perspective on the X-ray Ultra-Fast Outflow (UFO) in IRAS17020+4544" 13m
Outflows are crucial to AGN feedback, transporting mass and energy from the nucleus to the host galaxy across various scales. Theoretical models suggest that sub-relativistic Ultra Fast Outflows (UFOs), which interact with the ISM, decelerate and lose ionization, potentially driving large-scale, multi-phase outflows observable in optical and molecular gas.
The Narrow Line Seyfert 1 galaxy IRAS 17020+4544 offers a rare local laboratory to study AGN-driven outflows in action. It hosts a complex X-ray Ultra Fast Outflow (UFO), a powerful cold molecular outflow spatially resolved in CO with NOEMA millimeter observations, and a low-power radio jet that may be driving shocks into the interstellar medium (ISM).
In this work, we present MEGARA/GTC optical IFU observations of the ionized gas component over an area of ~140 kpc^2, within the region covered by the molecular outflow. We perform a detailed kinematic and energetic analysis of the ionized outflow (i.e., measuring its velocities, mass, momentum, and kinetic power) and compare it across the different (i.e., from X-ray to mm bands) gas phases to test whether the outflow retains its energy on galactic scales (i.e., following the "energy-conserving" regime).
Intriguingly, we find evidence for positive feedback in the central regions, suggesting that the outflow may not only be expelling some of the gas but also compressing it and triggering star formation. These results provide new insights into the role of AGN winds in shaping the evolution of NLSy1 galaxies.Speaker: Enrica Bellocchi (Universidad Complutense de Madrid - IPARCOS) -
12:18
The trans-Planckian problem in cosmology 13m
This talk presents an overview of the research I am carrying out in my PhD thesis.
Cosmological inflation is the leading framework for describing the physics of the early universe, originally introduced to solve the flatness, horizon, and monopole problems of the standard Big Bang model. It also provides a natural mechanism for generating primordial curvature perturbations: quantum fluctuations of the inflaton field are stretched beyond the Hubble radius during inflation and later re-enter as classical seeds for cosmic structure. The resulting nearly scale-invariant spectrum has been confirmed with high precision by Cosmic Microwave Background observations.Despite these successes, inflation faces a conceptual challenge when extrapolating observable modes back to the onset of the inflationary era. If inflation lasts significantly longer than the minimal number of e-folds, the comoving modes corresponding to current CMB scales would originate at sub-Planckian wavelengths, where the standard description of spacetime and quantum fields becomes unreliable. This “trans-Planckian problem’’ raises the possibility that unknown ultraviolet physics could imprint corrections on inflationary predictions, potentially modifying the primordial power spectrum.
Speaker: Christian Durán Romero (Univ. Complutense de Madrid)
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12:45
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Group picture
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Lunch break 1h 30m
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Short contributions: ---
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Pruning for Deep Neural Network compression for low-latency event characterisation in imaging atmospheric Cherenkov telescopes 13m
Arrays of imaging atmospheric Cherenkov telescopes (IACTs) are superb instruments to probe the very-high-energy gamma-ray sky. Cosmic rays entering the atmosphere create air showers comprised of particles which produce Cherenkov light. It is detected by IACTs and contains spatial, temporal and calorimetric information of the event. Upon detection, IACT trigger systems determine, on real time, whether data is to be recorded. When trigger levels are surpassed, the signals from all pixels in the camera are digitised. Events can be classified as hadronic or electromagnetic, according to the particle that generated the shower. However, hadronic showers are tens of thousands of times more common than gamma-rays. Thus, computational resource needs could be reduced by performing a rough selection at trigger-level. We study the viability of deep neural network implementation in specialised hardware (FPGAs) at trigger level. The Deep Learning (DL) based Python package CTLearn performs full-event reconstruction: direction and energy estimation, as well as classification of the particle type which originated the shower. We implement non-structural pruning, a compression strategy, on a ResNet model using CTLearn and evaluate its performance and how it differs when varying the hyperparameters. This is part of the long-term goal of implementing DL models in the camera trigger for the CTAO telescopes.
Speaker: Dafne Martín Domínguez (UCM-GAE) -
14:43
Toward a better understanding of the nucleon’s 3D structure through kinematic power corrections 13m
In recent years, significant progress has been made in understanding the 3D structure of the nucleon, driven by the development of TMD factorization. Although this framework has demonstrated strong predictive power, it still exhibits certain limitations that may be addressed by incorporating power corrections. By including kinematic power corrections (KPCs), we have successfully described the angular distributions of the Drell-Yan process, and we have found that these corrections play an even more prominent role in semi-inclusive deep inelastic scattering. Altogether, these findings suggest that current TMD distributions need to be updated: a new fit including KPCs is required to improve TMD extractions and, consequently, the tomographic picture of the nucleon.
Speaker: Sara Piloñeta Álvarez -
14:56
Deep-learning techniques in ground-based imaging gamma-ray observatories and the CTLearn package 13m
Gamma rays are key when it comes to studying topics such as dark matter from an indirect perspective or the Lorentz invariance, as well as probing a wide range of astrophysical phenomena that provide a deeper understanding of the most energetic events in the universe. They can be detected through Imaging Atmospheric Cherenkov Telescopes (IACTs), which capture images of extensive air showers generated by gamma rays and cosmic rays (high-energy particles of astrophysical origin) when they interact with the atmosphere. One of the main challenges about these images is the reconstruction of the event’s properties, i.e., obtaining the direction of arrival, energy and type (gamma ray, proton, electron, etc.) of the particles that triggered the shower. AI techniques, such as deep learning methods, have been demonstrated to be suitable for the reconstruction of these events since they are used to analyze and exploit loads of data for carrying out classification and characterization tasks. This presentation provides a brief introduction to gamma-ray astronomy and IACTs, followed by a focus on enhancing IACT event reconstruction using deep learning through the CTLearn package with the application of Transfer Learning and Attention techniques, within the framework of the Cherenkov Telescope Array Observatory (CTAO).
Speaker: Alexander Cerviño -
15:09
On femtoscopic correlations of light hadrons 13m
The ALICE collaboration has recently carried out measurements of femtoscopic correlations with light-hadron particle pairs, such as $\pi^+ K_S$ and $K^+ K_S$. Here we discuss how the $\pi^+ K_S$ data can be well reproduced using realistic interactions while accounting for the so-called finite-range potential (FRP) correction. Furthermore, we present predictions for other light-hadron channels that accurately describe the resonances involved.
Speaker: Alejandro Canoa Monsalve (Universidad Complutense de Madrid) -
15:22
The complete trigger chain simulations of the new LST camera 13m
CTAO North will consist of four Large Size Telescopes (LSTs), designed to detect very low-energy gamma rays. Given the limited lifespan of current cameras, new prototypes are being developed for the next generation of LSTs. The LST AdvCam, based on silicon photomultipliers, digitises signals from its nearly 8,000 pixels at 1 GHz, generating a volume of data that requires highly efficient trigger systems, since the vast majority of images correspond simply to Night Sky Background, not interesting for astrophysical analysis. Unlike the previous camera, AdvCam performs digitisation before triggering, allowing advanced algorithms to be applied to improve sensitivity at lower energies. In this presentation, we analyse different types of algorithms, from the simplest, such as ORs, to Convolutional Neural Networks, and their final implications for the telescope response.
Speaker: Jorge Buces Sáez (UCM-GAE) -
15:35
Understanding large local CP violation in B± → K±π+π− using dispersive methods 13m
We utilize the universality of pion–pion (ππ) final-state interactions at small invariant masses to understand the enhanced local CP violation in B± → K±π+π−, using a dispersive approach. From a fit to the integrated CP-asymmetry data, we successfully predict the Dalitz-plot kinematic distribution of the asymmetry in the low-energy ππ region, including the large local CP violation recently observed by LHCb. An essential role is played by the contributions of isospin 2. This formalism, whose parameters have a physical meaning, can be adapted straightforwardly to other systems with CP violation enhanced by final-state interactions.
Speaker: Alba Reyes Torrecilla (Universidad Complutense de Madrid and IPARCOS) -
15:48
Quantum computing fragmentation functions 13m
One of the most anticipated applications of quantum information science is the simulation of complex systems. Those involving quarks and gluons are particularly compelling, as their real-time phenomenology remains elusive to computational techniques such as traditional Monte Carlo methods. Overcoming these challenges could provide unprecedented insights into the dynamics of partons.
In this context, we discuss the calculation of fragmentation functions, key to describe how quarks and gluons transform into observable hadrons. As we move along we introduce a series of strategies to face the problem using quantum computers, all grounded in a codification paradigm where particles and their internal degrees of freedom are the central objects.
Speaker: Juan José Gálvez Viruet (Univ. Complutense de Madrid)
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Coffee break 30m
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Short contributions: ---
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The Central Trigger Processor Board (CTPB) for the CTAO LST Advanced Camera 13m
The Cherenkov Telescope Array Observatory (CTAO) is the next-generation ground-based gamma-ray instrument. Its Large-Sized Telescopes (LSTs) are specifically designed to observe the low-energy range and capture fast transient events. To enhance their capabilities, an Advanced SiPM-based Camera is currently under development and requires a robust digital trigger system. This contribution presents the status of the Central Trigger Processor Board (CTPB), the subsystem responsible for managing Level 2 and stereo triggers.
We report on the ongoing definition of the CTPB architecture and the evaluation of several technological approaches through dedicated test benches. Specifically, we explore the potential implementation of Machine Learning algorithms on FPGAs, such as Convolutional Neural Networks and clustering techniques, for efficient event discrimination. We also present preliminary tests on high-speed data transmission and discuss the assessment of different communication protocols. These studies guide the design choices for the CTPB to meet the demanding requirements of the LST Advanced Camera.
Speaker: María Molina Delicado (UCM-GAE) -
16:58
Relevance of on and off transitions in quantum pair production experiments 13m
Analog gravity experiments, such as those realized in Bose-Einstein condensates, often aim at simulating cosmological pair production due to the dynamical expansion of the Universe. However, these experiments have a start and an end, which introduces unavoidable transitions out of and into static regimes that alter the intended expansion profile. We show that the resulting particle spectra can be overwhelmingly dominated by these transition periods, which calls for a careful interpretation of experimental outcomes. In prospective Schwinger effect experiments, by contrast, transition effects do not dominate particle production, and such a reinterpretation may not be necessary.
Speaker: Álvaro Álvarez-Domínguez (Universidad Complutense de Madrid e IPARCOS) -
17:11
Probing Extreme Particle Acceleration in Blazars: A New Population of EHSP Candidates and Their TeV Prospects 13m
Extreme high-synchrotron-peaked blazars (EHSPs), defined by synchrotron peaks above 10^17 Hz, represent an uncommon subclass of blazars that challenge conventional blazar emission models and probe the limits of particle acceleration in relativistic jets. Yet, the number of identified EHSPs remains small, limiting comprehensive studies of their population and physical characteristics. In this contribution, we present a systematic study aimed at identifying and characterizing new EHSP candidates using a sample of 124 gamma-ray blazars selected from a wider catalogue based on their high synchrotron peak frequencies, low variability, and good broadband data coverage. The spectral energy distributions (SEDs) of the sample blazars are built using archival data complemented by Swift and Fermi-LAT observations, and modelled within a one zone synchrotron/synchrotron-self-Compton (SSC) framework. We identify 66 new EHSP candidates, significantly expanding the known population. A clear correlation emerges between synchrotron peak frequency and the magnetic-to-kinetic energy density ratio, with the most extreme sources approaching equipartition. This indicates that as the synchrotron peak shifts to higher frequencies, the energy stored in the magnetic field becomes comparable to that of the relativistic electrons, suggesting a more balanced and energetically efficient jet environment in the most extreme blazars. Our results suggest that 9 high-synchrotron peaked/EHSPs could be detected by the Cherenkov Telescope Array Observatory (CTAO) above 5σ significance (and 20 above 3σ) in 20-hour observations, implying that while the overall detection rate remains modest, a subset of these sources is within reach of next-generation very-high-energy gamma-ray instruments.
Speaker: María Láinez (UCM) -
17:24
HEFT, SMEFT, and ALPs in Multi-Boson Production 13m
Recently, the ATLAS and CMS collaborations have accumulated growing statistics on processes involving the production of two or more electroweak (EW) bosons, such as HH and WWZ. These multi-boson final states play a crucial role in probing the structure of the EW symmetry-breaking sector and exploring its possible extensions within the framework of Effective Field Theories (EFTs), both in the linear (SMEFT) and non-linear (HEFT) realizations. It is well known that SMEFT constitutes a specific limit of HEFT, where correlations among Wilson coefficients arise. These correlations can be experimentally tested through the study of multi-boson production channels.
Furthermore, if the Standard Model (SM) is embedded in a larger symmetry group that undergoes spontaneous breaking, the resulting (pseudo)-Goldstone bosons can produce observable effects in SM processes. Such effects can be systematically investigated within the framework of the ALP EFT, taking into account both linear and non-linear realizations of EW symmetry breaking.
This presentation will provide an overview of comprehensive results on multi-boson production within both SMEFT and HEFT, together with the corresponding constraints derived from current experimental data. It will also include a discussion of a global fit of ALP parameters in the linear scenario using ATLAS and CMS multi-boson measurements, as well as an analysis of the non-linear case.
Speaker: Dr Alexandre Salas-Bernárdez (Universidad Complutense de Madrid) -
17:37
Probing Particle Acceleration in Low-Luminosity AGN: The Case of NGC 4278 13m
Low-luminosity active galactic nuclei (LLAGN) occupy the low-accretion, low-luminosity end of the AGN population, where jet activity and particle acceleration can be modest. A significant subset of them are LINERs, nearby galactic nuclei characterized by weakly ionized emission lines. The recent TeV detection of the LINER/LLAGN NGC 4278 therefore offers a rare opportunity to probe high-energy processes in this faint regime. Using MEGARA optical spectroscopy together with the LHAASO TeV results, we find that the large-scale ionized outflows in NGC 4278 cannot supply the energy needed to produce the TeV emission. Instead, contemporaneous Fermi-LAT and Swift data point to a compact nuclear accelerator, consistent with the observed variability and hard GeV spectrum. This indicates that the TeV photons originate in the innermost jet region, while the optical outflows trace larger-scale jet gas interactions that coexist but do not power the gamma rays. NGC 4278 thus becomes a benchmark for understanding high-energy activity in LINERs and a compelling nearby target for the Cherenkov Telescope Array Observatory, the next-generation facility for very high energy gamma-ray astronomy.
Speaker: Alberto Dominguez (Universidad Complutense de Madrid & IPARCOS)
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Activity reports: ...
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The experience of IPARCOS Camp 2025 15m
In this brief presentation, We would like to share some thoughts about the IPARCOS Camp activity that was organized for the predoctoral researchers of the Institute on this previous May at El Escorial. Besides the purely scientific activities (research dissemination, sharing expertises, synergies), the workshop paid particular attention to team building. Likewise, there were especial sessions devoted to the identification of issues, requests and proposals by the community of junior researchers at IPARCOS. The general conclusion was that it would be beneficial that these activities were periodically repeated in the following years.
Speakers: Jose Luis Contreras Gonzalez (GAE/EMFTEL Universidad Complutense de Madrid), Prof. Juan J. Sanz Cillero (Universidad Complutense de Madrid & IPARCOS) -
18:05
EDIW Plan @ IPARCOS 15m
This talk would like to publicly present and discuss the recently approved Equity, Diversity, Inclusion and Welfare (EDIW) Plan at IPARCOS.
Speaker: Mercedes Martín Benito (IPARCOS) -
18:20
Discussion 15m
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Cocktail 1h 25m
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