The Living Swift-XRT Point Source Catalogue (LSXPS) is a unique facility: it is updated in near real-time, enabling a sensitive, “live” search for new high-energy transients. This opens up a new area of transient phase-space for exploration, as evidenced by the LSXPS discovery of the enigmatic event Swift J0230. However, the majority of transient candidates detected are faint, classified as...
High-energy neutrinos could be produced in the interaction of charged cosmic rays with matter or radiation surrounding astrophysical sources. To look for transient sources associated with neutrino emission, a follow-up program of neutrino alerts has been operating within the ANTARES Collaboration since 2009. For the highest energy neutrinos. this program has triggered the Neil Gehrels Swift...
Before the launch of the Neil Gehrels Swift observatory, little was known about the origin of short Gamma-ray Burst. While the short duration of the high-energy emission pointed out to a merger of compact objects, proof was lacking, and nothing was known about the afterglow emission.
At this conference, I will briefly discuss how Swift, thanks to the the unique capability of autonomous...
I will present 3D relativistic magnetohydrodynamic simulations of incipient Gamma-Ray Burst (GRB) jets piercing through realistic binary neutron star merger environments.
Applying the methods we developed to extend the 3D jet evolution up to tens of seconds without loss of resolution, we are able to reach a nearly ballistic expansion regime, with most of the jet energy converted into kinetic...
X-ray pulsars offer a unique laboratory for the study of radiation processes in extreme accretion are X-ray pulsars. These are found typically in high-mass X-ray binaries (HMXBs), while the brightest and most variable ones are those where the donor is a Be star (i.e. BeXRBs). Their environment combines some of the strongest magnetic fields (> 10^12 G) and effects of strong gravity, while also...
We present X-ray to radio frequency observations of the bright long gamma-ray burst GRB 210702A. Our ALMA observations show a significant rebrightening by a factor of approximately 2 beginning at 8.2 days post-burst and rising to peak brightness at 18.1 days before declining again. This is the first such rebrightening seen in a millimeter afterglow light curve. A standard forward shock model...
We have developed a density estimator for 1-D point processes. It is based on the continuous smooth function approximation, while information in the global density distribution is also applied. Using MC simulations we have determined the optimal parameters for low count distributions like the GRBs' redshift data. The results detailing the GRBs' redshift distribution also discussed briefly.
In August 2017, the groundbreaking observation of GW170817 marked the first-ever identification of a binary neutron star merger, accompanied by the detection of a Gravitational Wave (GW) and a gamma-ray burst (GRB). The GRB exhibited prompt gamma-ray emission and an afterglow across radio, optical, and X-ray bands, originating from a relativistic jet formed post-merger at an angle of 20-30...
Observations of transient phenomena, such as GRBs, FRBs, novae/supernovae explosions, coupled with the detection of cosmic messengers like high-energy neutrinos and gravitational waves, have transformed astrophysics. Maximizing the discovery potential necessitates tools for swiftly acquiring an overview of the most relevant information for each new detection. Introducing Astro-COLIBRI, a...
The Palomar 60-inch (1.5 metre) telescope, P60, conducted an automated optical GRB follow-up programme from 2005 to 2017. P60 was able to respond automatically, in less than three minutes, to well-localised Swift GRB alerts, and it was one of the largest optical telescopes with such a programme. The automatic response to the alerts built an unbiased GRB afterglow sample, making it a valuable...
GRB 221009A is the brightest gamma-ray burst ever detected by the Swift Observatory, with the highest peak gamma-ray flux for a GRB. It was detected once by the Burst Alert Telescope (BAT) during the prompt emission and again during the high-energy afterglow phase–a feat matched by no other GRB. Early data (t < 60 d) has shown a complicated picture with several projects finding a wide range...
Gamma-Ray Bursts (GRBs) are among the most energetic phenomena in the universe, acting as excellent astrophysical laboratories in which to study extreme processes. For the last twenty years, not only has the SWIFT telescope immensely contributed to the field of GRB detection but it has also allowed for follow-up observations thanks to its rapid and precise localization. During this period, the...
The physical origin of Fast Radio Bursts (FRBs) is still unknown. Many models consider magnetars as possible FRB sources, supported by the observational association of FRBs with the galactic magnetar SGR 1935+2154. Magnetars are also thought to be the source of the power of a fraction of Gamma Ray Bursts (GRBs), opening the possibility that the two extreme phenomena have a common...
Metallicity plays a key role in the evolution of stars, and obtaining accurate gas-phase metallicity measurements are therefore also important when studying the progenitors of stellar explosions, such as supernovae and gamma ray bursts (GRBs). However, there are well known limitations in how well the metallicity of galaxies can be measured, predominantly related to the quality of the generally...
In recent years Swift/UVOT has taken on a key role in identifying and following up transients. While automated source detection and difference imaging can help in finding transients, these tools cannot distinguish between real transients and star-like image artefacts caused by stray light. Image artefacts such as readout streaks or various ring structures are easy to identify by eye, and we...
Time profiles of GRB prompt emission are still far from being understood, despite intensive efforts to characterise them in terms of duration, hardness ratio, minimum variability timescale, averaged and individual power density spectra. Surprisingly, the number of peaks that one could observe in a GRB light curve has mostly been overlooked.
For the first time, we studied and modelled the...
A successful description of the inner engine activity of long gamma-ray bursts (LGRBs) holds the key to deciphering the variety and complexity exhibited by their light curves (LCs). Although the knowledge of GRB spectral properties has made huge strides thanks to technological advancement, temporal properties remain mostly unintelligible. In particular, an open question is whether they...
INAF will play a key role in the newborn multi-messenger astronomy field allowing us to study and identify the likely faint and rapidly fading electromagnetic counterparts of the hundreds gravitational wave (GW) events expected by the 2nd generation GW detectors network at full sensitivity together with upcoming electromagnetic facilities like Rubin telescope.
In this talk, I will present all...
The Magellanic Clouds (MCs) provide an unparalleled laboratory for studying high-mass X-ray binaries (HMXBs) due to their moderate, well-constrained distances and relative isolation from the Galactic plane. Among these systems, Be X-ray binaries (BeXRBs) – featuring Be-type stars as donor companions – stand out for their remarkable variability, including prominent outbursts in both X-ray and...
GRB 221009A stood out as the brightest GRB detected to date, offering a remarkable opportunity to delve into the intricacies of GRB physics. In this work, we investigated the prompt emission and afterglow characteristics of this unique burst utilizing observations from several missions like Swift, Fermi, and INTEGRAL including our early photometric (prior prompt emission) and spectroscopic...
The detection and follow-up observations of high-redshift (z > 6) gamma-ray bursts (GRBs) provide a unique opportunity to explore the properties of the distant Universe. GRB\,240218A, discovered by Swift/BAT, is one of the few identified so far, and with a redshift of $z=6.782$ is the burst with the second highest spectroscopic $z$ measured to date. Following the detection by high-energy...
Due to the large number of Swift GRB detections, it has been possible to select sub-samples of long GRBs that are reasonably complete in redshift and with observed prompt and afterglow emission. We perform Bayesian inference to constrain the distributions of burst parameters of the population, in accordance with the observed physical properties of the BAT6 sample. We use the structured jet...
Recently we searched for large scale structures in the Universe using 542 GRBs with known redshifts. In our published paper we checked for over densities on different scales. In our new work, we extend our search to larger scales. We found several deviations, among them a group of four GRBs and an extended volume of the so called Hercules–Corona Borealis Great Wall (HCBGW). The estimated 2 Gpc...
Gamma-Ray Bursts (GRBs) rank among the most energetic phenomena in the Universe. Thanks to the Swift and Fermi observatories, significant progress has been made in GRB science over the past decades, but one area of research that now requires exploration are the still elusive GRB orphan afterglows. We define orphan afterglows as GRB afterglows viewed off-axis, which have hence a negligible...
We are now in the era of rapid-response observations of gamma-ray bursts (GRBs). Multiwavelength observations are essential in GRB and other transient phenomena studies. A rapid follow-up is crucial as the analysis of the GRB afterglow properties may be impacted by its rapid fade. Early-time observations taken with the onboard Neil Gehrels Swift Observatory ($\textit{Swift}$) instruments...
The prompt phase X- and γ-ray light curves of gamma-ray bursts (GRBs) exhibit erratic and complex behaviour, often with multiple pulses. The temporal shape of individual pulses is often modelled as ‘fast rise exponential decay’ (FRED). Here, we introduce a novel fitting function to quantify pulse asymmetry. We conduct a light curve and a time-resolved spectral analysis on 61 pulses from 22...
The detection of GRB 170817A, coincident with the gravitational wave signal GW170817 from a binary neutron star (BNS) merger, confirmed the link between short gamma-ray bursts (sGRBs) and compact object mergers. I will present a study focused on the identification of potential sGRBs associated with BNS mergers by analyzing the Fermi GBM Burst Catalog using an unsupervised machine learning...
The two high-energy instruments onboard the SVOM satellite, ECLAIRs and GRM, are expected to bring significant contributions in answering fundamental questions on Gamma-Ray Bursts (GRBs) and other high-energy transients. In particular, their joint analysis represents a clear asset compared to other missions for GRB prompt emission spectroscopy (Bernardini et al. 2017). This leads to stringent...
Gamma-ray bursts (GRBs) exhibit a rich variety of X-ray lightcurve behaviors, including flares and plateau/shallow decay phases, whose origins remain debated. Existing studies often rely on diverse analysis techniques applied to limited GRB samples, leading to results that may be difficult to generalize. In this study, we introduce a new data-driven, model-independent method for automatically...
Time lags between the arrival time of different photon energies provide valuable insight into the emission mechanisms of Gamma-Ray Bursts (GRBs). Using data from the Fermi Gamma-ray Burst Monitor (GBM, between 10 - 500 keV) and the Large Area Telescope (LAT), particularly those obtained with the Low Energy (LLE) technique (30 - 100 MeV), we analyze a sample of 70 GRBs to investigate the...
We present time-averaged and time-resolved (where possible) spectral analysis of prompt emission of a dozen GRBs (including GRB 990123) simultaneously detected by Konus-Wind and BeppoSAX/WFC instruments. Modelling the prompt emission spectra recorded in a wide energy range with the empirical functions is discussed in the context of thermal and non-thermal origin of emission.
Recent associations of high-energy neutrinos with active galactic nuclei (AGN) have rekindled interest in leptohadronic models of radiation from astrophysical sources. The rapid growth in multi-messenger data acquisition highlights an emerging need for fast numerical models capable of application to large source samples. In this contribution, we introduce [LeHaMoC][1], an open-source,...
A large and growing sample of Swift XRT observations allows us to draw conclusions about the population properties of GRBs. I will present two examples of this. One builds on the scale-free nature of GRB afterglow dynamics and synchrotron spectra, deploying scale-invariance to interpret the spread of observed fluxes when binned by light-curve slope at the time of observation. This spread is...
GRS 1915+105 is one of the brightest black hole X-ray binaries (BHXBs) since it was first detected by GRANAT/WATCH in 1992 until it faded into a quiescent state in recent years. We studied its long-term activity using MAXI/GSC and Swift/BAT data for the duration of 2009 – 2019, the last ten years of its active state. We found that the 10 years’ activity of GRS 1915+105 can be classified into...
A new method (PSF method) for measuring photometries of moderately saturated UVOT sources has been proposed, which increases the dynamic range of UVOT. The brightest UV/optical flash was discovered in GRB 2201101A with the PSF method. Considering the very rapid brightening stage, the scenario of a refresh shock is adopted to explain the optical flash. In addition, we proposed a method (clean...
Long gamma-ray bursts are produced by the collapse of a massive star at the end of its life. Typically, LGRB spectra are found to be absorbed by a significant amount of gas within their host galaxy. We can estimate the amount of this gas through broadband spectroscopy. X-ray spectra provide the most complete estimate as they probe the total amount of material along the line of sight compared...
We present a detailed study of the multi-wavelength properties of a sample of short GRBs with extended emission (EE) observed by Swift. The sample consists of 11 events, selected from the SBAT4 catalog by D’Avanzo et al., (2014), which was subsequently expanded to include events up to 2021. This sample exclusively contains only short GRBs with favorable observational conditions for the...
The Swift UVOT plays a crucial role in time-domain astronomy, but light curves, especially in the UV, are plagued with "dropouts," outliers with photometric fluxes that are up to 30% lower than surrounding points. These dropouts are caused by localized sensitivity variations in the detector. We have developed algorithms that map out the detector plane and flag these points, producing more...
We review the contributions of Swift/UVOT to our understanding of interstellar dust and hot stars and young stellar populations in both the Milky Way and other galaxies. These two research areas are closely intertwined: UV-bright objects can only be fully understood when the effects of foreground dust are accounted for, yet those same effects can only be studied by observing the properties of...
Nova explosions are thermonuclear events on top of an accreting white dwarf. The nova event results in the increase of the optical luminosity by 7-8 orders of magnitude that makes the nova outburst detectable at any distance in the Galaxy. However, due to the resulting distance distribution of novae in the Galaxy, the host system remains unknown for most cases. Accretion powers X-rays in the...
To date, radio studies of GRB afterglows have been triggered because of their multiwavelength properties i.e. high energetics or optical brightness. This has left us with a biased image of the radio properties of GRB afterglows and very little information on their earlier time behaviour. In this talk, I will provide an update on the PanRadio GRB program that has been we have been running on...
MAXI J1631-479 is a bright black hole X-ray transient discovered in 2018. MAXI-GSC and Swift-XRT data does not show a typical q-shape but an inverse Y-shape in the hardness and intensity diagram (HID) during the course of the outburst. Using MAXI and Swift data, we demonstrate such an inverse Y-shape and observed various states, low/hard, hard and soft intermediate, and high/soft states, are...
Non-jetted AGN exhibit hard X-ray emission with a power law spectrum above $\sim$2 keV, which is thought to be produced through Comptonization of soft photons by electrons and positrons (pairs) in the vicinity of the black hole. The origin and composition of this plasma source, known as the corona, is a matter open for debate.
Our study focuses on the role of relativistic protons accelerated...
The Exploring the X-ray Transient and variable Sky (EXTraS) project represents the most thorough living search for new X-ray pulsators in the XMM-Newton archive, having led to the discovery of about 60 new pulsators and still counting. In 2022, we discovered an X-ray pulsator on the outskirts of the Large Magellanic Cloud (LMC). The source (J0456 from now on) shows a coherent signal with a...
A subclass of hybrid Gamma-ray bursts (GRBs) with long duration and peculiar spectral and timing properties was discovered to be related with compact binary mergers. Their main prompt gamma-ray phase is preceded by a fainter and spectrally softer pulse that we interpret as a precursor, possibly produced by a different physical mechanism.
I present the results from the analysis of the...
Be X-ray binaries (BeXRBs) are highly variable systems that host the majority of X-ray pulsars (XRPs). In these systems, accreting material is transferred via the magnetic field lines of the Neutron Star (NS) and concentrated into an accretion column (AC) near its magnetic poles. The AC dynamics suggest a presence of sub-critical and super-critical regimes in which the luminosity and the...
SRGA J144459.2-604207 is a newly discovered X-ray binary transient. First detected by the SRG/ Mikhail Pavlinsky ART-XC telescope on February 21, 2024, the X-ray detection was then confirmed by the MAXI instrument on-board of the ISS. NICER data taken on February 21 evidenced the presence of an X-ray pulsation at approximately 447.8 Hz and of type-I X-ray bursts, establishing that SRGA...
The dynamic environment which exists in black hole accretion discs has traditionally been probed in stellar-mass Galactic black holes where the timescale for changes is short. In principle, if the quantity of material in a disc around a super-massive black hole is small and is not replenished, then the disc will drain on a timescale of a few hundred days and the system can pass through several...
The hysteresis behavior of X-ray binaries during their outbursts remains a mystery. In this work, we developed a paradigm where the disk material accretes in two possible, mutually exclusive, ways (Ferreira et al. 2006). In the usual alpha-disk mode (SAD, Shakura & Sunayev 73), the dominant local torque is due to a radial transport of the disk angular momentum. In the jet-emitting disk mode...
Ultraluminous X-ray sources (ULXs) are extragalactic, non-nuclear X-ray point sources with luminosities exceeding the Eddington limit for a 10 solar-mass black hole. These sources are widely believed to be X-ray binaries containing black holes or neutron stars that accrete matter at super-Eddington rates. However, the exact mechanisms and geometry of this accretion process remain poorly...
Supernovae exhibiting circumstellar matter (CSM) interactions and dynamic signatures provide critical insights into the mass-loss histories of massive stars. SN2022ffg, a Type II supernova observed shortly after the explosion, displayed flash-ionized emission lines of H, He, N, and C lasting for over a week, indicating interaction with a dense nearby CSM. The supernova’s Swift-UV light curve...
WZ Sge-type stars are an extreme subgroup of the dwarf nova class of cataclysmic variables. In contrast to ordinary SU UMa-type dwarf novae, the WZ Sge-type stars exhibit only very rare (approximately once a decade) and long superoutbursts (a few weeks) with amplitudes exceeding 6 mag, and no normal outbursts. A unique property of superoutbursts is the appearance of superhumps, low-amplitude...
The French-Chinese SVOM satellite (Space Variable Objects Monitor) was launched on June 22, 2024, from the Xichang launch site in China. The mission's objectives focus on detecting and studying astrophysical transient events, with a primary emphasis on Gamma-Ray Bursts (GRBs). The GRB Trigger of the ECLAIRs instrument onboard SVOM has already detected several notable bursts and initiated...
Launched on June 22, 2024, the SVOM satellite extends its mission beyond gamma-ray burst (GRB) science, exploring a wide range of high-energy phenomena and transient astrophysical sources. This presentation highlights SVOM's activities on the Observatory Science related to non-GRB sources. We will showcase the architecture and functionality of the quick-look analysis pipeline for ECLAIRs...
The beginning of the 21st Century saw the advent of two satellites that revolutionised the high-energy astrophysics. The AGILE satellite, for the first time, used a Silicon pair conversion detector for gamma-ray detection, allowing for a leap forward with respect to previous spark chamber technology. The Swift satellite combined optical, UV and X-ray telescopes with an unprecedented repointing...
Despite decades of research, predicting outbursts of X-ray transients, and witnessing their beginning stages, remains very challenging. The cause of these X-ray brightenings is thought to be the sudden increase of accretion of matter onto a black hole or neutron star, initiated by the ionization of hydrogen in the accretion disc. I present recent observational advances in our understanding of...
The MAGIC telescopes, designed to observe gamma rays at energies exceeding 50 GeV, have significantly advanced their scientific capabilities through multi-wavelength (MWL) campaigns involving the Neil Gehrels Swift Observatory. Beginning operations just two years after Swift, the young MAGIC collaboration rapidly embraced MWL campaigns, integrating Swift's X-ray and UV observations with TeV...
Classical and Recurrent novae occur on the white dwarf component of a close, or not so close, binary system. They participate in the cycle of Galactic chemical evolution in which grains and metal enriched gas in their ejecta are a source of heavy elements for the ISM. Once in the diffuse gas, this material is ultimately incorporated into new regions of star formation. We have continued our...
Recent years have seen a growing sample of TeV emission detections in gamma-ray burst afterglows, as well as an increasing role for structured jets in afterglow modelling. Using a kinetic approach, with adiabatic expansion and fully self-consistent IC scattering, we show that the structure of an afterglow jet impacts its TeV emission, with jets where the energy falls off more sharply with...
The ASTRI Mini–Array is currently being installed in Tenerife at the Observatorio del Teide to explore the gamma-ray sky in the 1-100 TeV energy range with unmatched angular resolution (a few arcminutes) across a wide field of view (10.5 deg). The array consists of nine IACTs (Imaging Atmospheric Cherenkov Telescopes), each equipped with a 4-meter diameter dual-mirror system featuring a...
The SVOM (Space-based multi-band astronomical Variable Objects Monitor) observatory is dedicated to the exploration and progress of Gamma-Ray Burst (GRB) science. The two wide field of view instruments on board the satellite – ECLAIRs and GRM – are currently monitoring the transient sky and detecting GRBs in both X- and gamma-ray energy bands (from 4 keV to 5 MeV, jointly). In addition to GRB...
I will present the results of our ongoing Swift monitoring of Be/X-ray transients that we started almost ten years ago. We have followed up more than ten galactic systems (i.e., GRO J1008-57, SAX J2103.5+4545, GX 304-1, GRO J1750-27, KS 1947+300) during and after their outbursts. The aim of our monitoring campaigns was to study the process of low-level accretion onto magnetized (10^12-10^13 G)...
The last 20 years have been studded with a wealth of unexpected results in high-energy astrophysics, as typified by discoveries made by Swift, INTEGRAL, and other high-energy observatories. Here we would like to highlight the major role played by Swift/XRT in supporting the INTEGRAL mission in consolidating new findings, allowing a better classification/characterisation of unknown sources,...
Over the past decade, the Swift satellite carried out a dedicated observational campaign targeting unassociated gamma-ray sources (UGSs), which constitute ~30% of the gamma-ray detections reported by the Fermi satellite. UGSs are of significant interest in high-energy astrophysics, potentially hiding new unidentified blazars, the most numerous class of extragalactic gamma-ray sources and...
The tidal forces from SMBHs can disrupt stars in their vicinity. These tidal disruption events (TDEs) manifest themselves as a luminous, short-lived, flares coming from the nuclei of otherwise quiescent galaxies and represent an important tool to study the properties of dormant SMBHs. They are exquisite multi-wavelength sources, as they produce very bright flares in different bands of the...
Transitional millisecond pulsars (tMSPs) bridge the evolutionary gap between accreting neutron stars in low-mass X-ray binaries and millisecond radio pulsars, offering a unique laboratory to study the interplay between accretion and pulsar activity. These systems exhibit a distinctive subluminous X-ray state characterized by alternating high, low and flaring emission modes.
Swift/XRT has...
The majority of discovered rocky exoplanets in the habitable zone (HZ) orbits around old M-dwarfs, but it is unclear if the high-energy emission of these stars provides a suitable environment for the origin of life. According to Spinelli el al. 2023, the current Near Ultraviolet (NUV) luminosity of M-dwarfs hosting HZ exoplanets is too low to trigger RNA precursors formation on them. By...
Synchrotron radiation has been for decades the main candidate to explain prompt emission in gamma-ray bursts (GRBs), while shocks have been widely employed as dissipation mechanisms. Although most GRB detectors, such as BAT, are sensitive to energies starting from ~10 keV, the emission in soft X-rays, such as detected by Swift's XRT, and optical wavelengths is also crucial to understand and...
The $E_{\rm p,i}$--$L_{\rm iso}$ correlation of long gamma-ray bursts (LGRBs) has been regarded for a long time as a fundamental correlation for standardizing LGRBs to probe the cosmology and constrain LGRB physics. However, the authenticity of this correlation may be affected by potential selection effects, which are likely overlooked in the current small sample of LGRBs with measured...
ECLAIRs, the leading instrument onboard the SVOM mission, is tasked to autonomously search for Gamma-Ray Bursts (GRBs) and other high-energy transients within its wide field of view ( ~2 sr) in the 4-150 keV energy range. To complement the onboard detection capabilities and to take advantage of a better understanding of the instrumental context and huge computing resources, an offline trigger...
The detection of faint optical transients is a critical component of gravitational wave (GW) follow-up efforts. Compact object mergers (e.g., binary neutron stars) produce kilonovae -- thermal transients powered by the radioactive decay of r-process elements. Unlike GRB jets, kilonovae are comparatively isotropic and thus may offer a higher likelihood of detection. However, their faintness...
The timing analysis of transient events (TEs) offers a powerful tool for exploring numerous open questions in modern astrophysics. We have developed the mathematical and physical methods required to estimate delays between two lists of Time of Arrival (ToA) measurements. The HERMES mission, scheduled to launch in March 2025, will deploy a constellation of six nano-satellites in Low Earth Orbit...
In recent decades, distinct subtypes of Type Ia supernovae (SNe Ia) have been discovered that deviate from the canonical luminosity-width relationship. These non-standardizable objects risk contaminating high redshift (z > 0.5) cosmological samples, including those anticipated from the Roman Space Telescope and LSST. While SN Ia subtypes are traditionally determined using peak-light optical...
Ultraluminous X-ray sources (ULXs) are an intriguing class of X-ray binaries, most of them observed in nearby galaxies, with luminosity > 10^39 erg/s. Observational evidences favor their interpretation as super-Eddington accretors. Swift/XRT has played a fundamental role in the characterization of ULXs long-term evolution, being the only active X-ray telescope, which allows regular and...
The plateau phase observed in the early X-ray light curve of GRBs (lasting up to thousands of seconds) has been a subject of debate since its discovery by the Neil Gehrels Swift Observatory in 2005. First, I will show that the plateau phase can be explained within the classical GRB model by considering a jet Lorentz factor of tens expanding in a wind-type environment. In this model, the end...
The search for periodicity in the multi-wavelength high variable emission of blazars is a key feature to understand dynamical processes
at work in this class of active galactic nuclei. The blazar PG 1553+113 is an attractive target due to the evidence of periodic oscillations
observed at different wavelengths, with a solid proof of a 2.2-year modulation detected in the γ-ray, UV and optical...
Over the past decade, the proliferation of sky surveys has enabled the discovery of many Type Ia Supernovae (SNe Ia) promptly after they explode, unveiling new, peculiar phenomena in their first days. In this talk, I will highlight recent discoveries relating to early-time flux excesses, which Swift showed are especially prominent in the UV, discovered for a growing number of SNe Ia. First,...
We present a study aiming at measuring the correlation between X-ray absorption and absorption due to the presence of molecular gas from larger scales in the host galaxies of nearby AGN. The study will be carried out through the hard X-ray selected AGN in the IBIS AGN CO survey (IBISCO), focussing in particular on those AGN identified as “ideal targets”, i.e. those where there are indications...
