Article
Astronomy & Astrophysics
Michail Damoulakis, Rodolfo Barniol Duran, Dimitrios Giannios
Summary: Despite debates on the nature of the compact object at the central engine and the mechanism behind the prompt emission, the striped jet model provides a promising approach to connect various stages of gamma-ray burst (GRB) due to its robust predictions. By using constraints on magnetization and bulk Lorentz factors of the jet flow, the model is tested for GRB flow and its predictions for prompt emission are studied. It is found that the model agrees with observed prompt emission spectra in the majority of bursts, supporting a neutron star central engine over a black hole one.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Raphael Duque, Paz Beniamini, Frederic Daigne, Robert Mochkovitch
Summary: We develop a model that explains the flaring activity in gamma-ray burst X-ray afterglows, suggesting that these flares could be the result of prompt dissipation within the core of the jet and appear to a misaligned observer in the X-ray band. The model takes into account the light travel delays between the core and the observer, as well as the lateral structure of the jet. The study shows that the model can explain flares with typical observing times and luminosities, and can capture different types of morphology.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Evgeny Derishev
Summary: This article establishes relations between the downstream emitting zone parameters and the measurements from a distant observer for an expanding spherical relativistic shock. The relations are formulated using dimensionless effective coefficients and self-evident dimensional estimates. The calculations consider the evolution of the shock's Lorentz factor, geometrical delay due to the shock's front curvature, and the angular dependence of Lorentz boost for frequency and brightness. The relations are primarily intended for gamma-ray burst afterglow studies but may have broader applications.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Jing-Ze Ma, Bing Zhang
Summary: Reverse shock emission is a useful tool for studying the properties of relativistic ejecta in gamma-ray burst afterglows. However, the physical conditions for reverse shock formation and the role of magnetic fields in reverse shock dynamics are still not fully understood. In this study, we use the shock jump conditions to characterize the properties of a magnetized reverse shock. We compare different theories and numerical simulations to reconcile the discrepancies among them. We find that the strict condition for reverse shock formation is sigma < sigma(cr), and propose a characteristic radius for reverse shock formation based on this condition.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
J. F. Graham, P. Schady, A. S. Fruchter
Summary: The distribution of metallicities in long-duration gamma-ray burst (LGRB) host galaxies shows no evolution across different redshifts, in contrast to the mass-metallicity relation of typical galaxies. The lack of evolution in high-metallicity distribution is not due to selection effects. However, using mass-metallicity relationships to estimate host metallicities introduces a substantial systematic bias.
ASTROPHYSICAL JOURNAL
(2023)
Article
Astronomy & Astrophysics
F. Kunzweiler, B. Biltzinger, J. Greiner, J. M. Burgess
Summary: This study presents a new algorithm and automated data analysis pipeline for detecting slowly rising or long-duration transient events in high-energy electromagnetic sky. The algorithm demonstrates high sensitivity and coverage, and during testing on Fermi-GBM data, it successfully detected over 300 untriggered transient signals, one of which was confirmed to originate from a known astrophysical source.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
Haocheng Zhang, Dimitrios Giannios
Summary: Relativistic jets from supermassive black holes may have their polarity changing over time, forming dissipative structures called 'stripes', which accelerate the jet and contribute to large-scale emission. This model can consistently explain jet acceleration, radio emission, and shed light on the nature of blazars.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Tian-Le Zhao, Rajiv Kumar
Summary: This study focuses on the formation and ejection of "blobs" due to magnetic reconnection in the hot flow environment of the accretion disc, and calculates the energy and emission spectrum in different bands near Sagittarius A*. The results show that the observed flares in various bands are a series of magnetic reconnection phenomena, rather than a single event.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
A. E. Camisasca, C. Guidorzi, L. Amati, F. Frontera, X. Y. Song, S. Xiao, S. L. Xiong, S. N. Zhang, R. Margutti, S. Kobayashi, C. G. Mundell, M. Y. Ge, A. Gomboc, S. M. Jia, N. Jordana-Mitjans, C. K. Li, X. B. Li, R. Maccary, M. Shrestha, W. C. Xue, S. Zhang
Summary: Significant progress has been made in the detection, monitoring, and modeling of γ-ray bursts (GRBs) over the past 50 years. However, the process responsible for their prompt emission is still unknown. Recent studies focus on understanding how the GRB jet propagates through the progenitor's stellar envelope and investigating possible energy dissipation processes. The shortest duration of an independent emission episode within a GRB can provide clues about the inner engine activity and help distinguish different effects.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
S. Dichiara, E. Troja, V Lipunov, R. Ricci, S. R. Oates, N. R. Butler, E. Liuzzo, G. Ryan, B. O'Connor, S. B. Cenko, R. G. Cosentino, A. Y. Lien, E. Gorbovskoy, N. Tyurina, P. Balanutsa, D. Vlasenko, I Gorbunov, R. Podesta, F. Podesta, R. Rebolo, M. Serra, D. A. H. Buckley
Summary: This article presents a multiwavelength analysis of GRB 190829A, which is the fourth closest long GRB ever detected by the Neil Gehrels Swift observatory and the third confirmed case with a very high-energy component. The study reveals two emission components in the event, with a bright reverse shock dominating at early times and a forward shock dominating at later times. The prompt and afterglow properties suggest that GRB 190829A shares similarities with cosmological long GRBs.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
A. Saccardi, S. D. Vergani, A. De Cia, V. D'Elia, K. E. Heintz, L. Izzo, J. T. Palmerio, P. Petitjean, A. Rossi, A. de Ugarte Postigo, L. Christensen, C. Konstantopoulou, A. J. Levan, D. B. Malesani, P. Moller, T. Ramburuth-Hurt, R. Salvaterra, N. R. Tanvir, C. C. Thone, S. Vejlgaard, J. P. U. Fynbo, D. A. Kann, P. Schady, D. J. Watson, K. Wiersema, S. Campana, S. Covino, M. De Pasquale, H. Fausey, D. H. Hartmann, A. J. van der Horst, P. Jakobsson, E. Palazzi, G. Pugliese, S. Savaglio, R. L. C. Starling, G. Stratta, T. Zafar
Summary: The study explores the properties of galaxies in the first billion years after the Big Bang using optical and near-infrared spectroscopy of gamma-ray bursts (GRBs). The analysis detects absorption lines that reveal information about the interstellar medium and chemical abundance of the host galaxy and foreground absorbers. The study demonstrates the potential of GRBs to offer detailed insights into the properties of high-redshift galaxies.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
Kshitij Aggarwal, Sarah Burke-Spolaor, Nicolas Tejos, Giuliano Pignata, J. Xavier Prochaska, Vikram Ravi, Jane F. Kaczmarek, Stefan Oslowski
Summary: In this study, multiwavelength follow-up observations were conducted to search for a host galaxy and persistent radio emission associated with FRB 180309. The localization of the FRB was improved to a region of about 2' x 2', and several candidate host galaxies were identified within this region. Further analysis on the properties of these candidates, including redshift and radio emission, suggests the possibility of isolating a single host for this highly luminous FRB through follow-up spectroscopy.
ASTROPHYSICAL JOURNAL
(2021)
Article
Astronomy & Astrophysics
Rahul Gupta, S. Gupta, T. Chattopadhyay, V Lipunov, A. J. Castro-Tirado, D. Bhattacharya, S. B. Pandey, S. R. Oates, Amit Kumar, Y-D Hu, A. F. Valeev, P. Yu Minaev, H. Kumar, J. Vinko, Dimple Dimple, V Sharma, A. Aryan, A. Castellon, A. Gabovich, A. Moskvitin, A. Ordasi, A. Pal, A. Pozanenko, B-B Zhang, B. Kumar, D. Svinkin, D. Saraogi, D. Vlasenko, E. Fernandez-Garcia, E. Gorbovskoy, G. C. Anupama, K. Misra, K. Sarneczky, L. Kriskovics, M. A. Castro-Tirado, M. D. Caballero-Garcia, N. Tiurina, P. Balanutsa, R. R. Lopez, R. Sanchez-Ramirez, R. Szakats, S. Belkin, S. Guziy, S. Iyyani, S. N. Tiwari, Santosh V. Vadawale, T. Sun, V Bhalerao, V Kornilov, V. V. Sokolov
Summary: This paper presents the timing, spectral, and polarimetric analysis of the prompt emission of GRB 190530A, and provides information about afterglow polarization and characteristic parameters through optical observations and redshift measurements.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Matteo Pais, Tsvi Piran, Ehud Nakar
Summary: Many stripped envelope supernovae exhibit high-velocity material responsible for broad absorption lines in the observed spectrum. Numerical simulations show that when the jet is not deeply choked within the star, the outflow carries a constant amount of energy per logarithmic scale of proper velocity, which depends on the cocoon volume at the breakout time. This phenomenon provides a natural explanation for the fast material seen in stripped envelope SNe not associated with LGRBs and offers insight into the hidden jets.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
B. Schneider, E. Le Floc'h, M. Arabsalmani, S. D. Vergani, J. T. Palmerio
Summary: This study evaluates the impact of size, stellar mass, and star formation rate surface densities on the probability of distant galaxies hosting long GRBs. The results show that there is a bias in stellar density between GRB hosts and the overall population of star-forming sources up to a redshift of approximately 2, suggesting that special environments may be required to enhance the production of GRBs.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Surgery
Dimitrios Kapetanios, Maria Petropoulou, Dimitrios Chatzelas, Georgios Pitoulias, Thomas E. Kalogirou, Afroditi Maria Mitka, Ioakeim T. Giagtzidis, Konstantinos O. Papazoglou, Christos D. Karkos
Summary: This study aimed to investigate the impact of transfusing 2 units of FFP immediately post aneurysm exclusion on perioperative fibrinogen levels and patient outcomes. The results showed that the FFP group had higher 24-hr postoperative fibrinogen levels and lower Delta fib compared to the control group, but there were no significant differences between the two groups in terms of endoleaks, reinterventions, major adverse cardiovascular events, or deaths.
ANNALS OF VASCULAR SURGERY
(2021)
Review
Multidisciplinary Sciences
Maria Petropoulou, Orestis Efthimiou, Gerta Ruecker, Guido Schwarzer, Toshi A. Furukawa, Alessandro Pompoli, Huiberdina L. Koek, Cinzia Del Giovane, Nicolas Rodondi, Dimitris Mavridis
Summary: The article provides an overview of methods for evaluating the effects of complex interventions with meta-analytical models, highlighting methodology, new developments, benefits, drawbacks, and potential challenges of each method. With the development of easy-to-use software tools, meta-analytical methods focusing on components of multicomponent interventions are expected to become more popular. Different meta-analytical methods are illustrated through examples comparing psychotherapies for panic disorder.
Article
Astronomy & Astrophysics
Manuel Meyer, Maria Petropoulou, Ian M. Christie
Summary: The study discusses the mechanism of fast gamma-ray variability in blazars focusing on magnetic reconnection events. By using advanced simulations, they generate realistic gamma-ray light curves and compare them with observed gamma-ray flares from FSRQs, finding similar flux levels and variability patterns when the reconnection layer is slightly misaligned with the line of sight. They suggest that emission from fast plasmoids moving close to the line of sight could explain the fast variability observed in FSRQs and call for further research on fast variability as evidence for magnetic reconnection events.
ASTROPHYSICAL JOURNAL
(2021)
Article
Astronomy & Astrophysics
Hayk Hakobyan, Maria Petropoulou, Anatoly Spitkovsky, Lorenzo Sironi
Summary: In this study, the important role of plasmoids in shaping particle energy spectra in relativistic reconnection is demonstrated. Through simulations in pair plasmas with different magnetizations, a secondary particle energization process inside compressing plasmoids is studied, revealing a linear increase in magnetic field with time leading to particle energization as a result of magnetic moment conservation. The shape of the injected power law distribution of particles is conserved with the emergence of an additional nonthermal tail at higher energies, followed by an exponential cutoff whose energy increases over time.
ASTROPHYSICAL JOURNAL
(2021)
Article
Astronomy & Astrophysics
Agniva Roychowdhury, Eileen T. Meyer, Markos Georganopoulos, Peter Breiding, Maria Petropoulou
Summary: The broad high-energy spectral component in blazars is often explained by various inverse Compton scattering processes. However, it has not been clearly identified in most cases due to limitations in physical models. AP Librae, a low-synchrotron-peaking BL Lac object, has an extremely broad high-energy spectrum covering a wide range of energy levels. Standard synchrotron self-Compton models have failed to reproduce the high-energy emission in AP Librae. It is suggested that the emission may arise from inverse Compton scattering of cosmic microwave background photons by a relativistic jet in kiloparsec scales. The newly obtained observational data from Hubble Space Telescope and Atacama Large Millimeter/submillimeter Array have confirmed this suggestion.
ASTROPHYSICAL JOURNAL
(2022)
Article
Astronomy & Astrophysics
S. Stathopoulos, M. Petropoulou, P. Giommi, G. Vasilopoulos, P. Padovani, A. Mastichiadis
Summary: Blazar flares have the potential to produce enhanced neutrino signals, including those from X-ray flares. By analyzing the X-ray data of 66 blazars observed by the X-ray Telescope, we find that the majority of neutrino events originate from flares with durations of 1-10 days. We calculate the average yearly neutrino rate for each source, with Mkn 421 having the highest predicted rate.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Margaritis Chatzis, Maria Petropoulou, Georgios Vasilopoulos
Summary: A toy model for radio emission in high-mass X-ray binaries was proposed, predicting the relation between GHz luminosity and accretion X-ray luminosity, with different characteristics for various X-ray luminosity scenarios. Bayesian modeling of radio observations of SwiftJ0243.6+6124 supported shock origin for radio detections at sub-Eddington X-ray luminosities.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
P. Padovani, P. Giommi, R. Falomo, F. Oikonomou, M. Petropoulou, T. Glauch, E. Resconi, A. Treves, S. Paiano
Summary: Eight years after the first detection of high-energy astrophysical neutrinos by IceCube, we still have limited understanding of their origin. However, evidence is accumulating to support the idea that blazars may be sources of neutrinos. A recent study focused on 47 blazars and found that some of them are associated with neutrino track events detected by IceCube. Additionally, the study discussed the frequency of masquerading BL Lacs and presented two theoretical scenarios for neutrino emission. Future observations will help test these theories.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
A. Mastichiadis, M. Petropoulou, N. D. Kylafis
Summary: This study investigates whether the radiative coupling between the hot Comptonizing corona and the cold accretion disk can generate QPOs in BHXRBs. The results show that under certain conditions, the dynamic corona-disk system exhibits oscillations with frequencies similar to those observed in the power spectra of BHXRBs. Therefore, this picture may have implications for other systems that contain similar components.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Medicine, General & Internal
Nils Brockelmann, Sara Balduzzi, Louisa Harms, Jessica Beyerbach, Maria Petropoulou, Charlotte Kubiak, Martin Wolkewitz, Joerg J. Meerpohl, Lukas Schwingshackl
Summary: This study aimed to evaluate the agreement of effect estimates between randomized controlled trials (RCTs) and cohort studies and identify factors associated with disagreement. The results showed that, on average, there was no significant difference in effect estimates between RCTs and cohort studies, but there was some inconsistency in certain situations.
Article
Astronomy & Astrophysics
I Liodakis, T. Hovatta, V Pavlidou, A. C. S. Readhead, R. D. Blandford, S. Kiehlmann, E. Lindfors, W. Max-Moerbeck, T. J. Pearson, M. Petropoulou
Summary: The origin of Petaelectronvolt (PeV) astrophysical neutrinos is fundamental to our understanding of the high-energy Universe. Neutrino astronomy represents the greatest challenge faced by the astronomy and physics communities. Efforts have been made to prove or disprove that jets are neutrino emitters, but so far, no conclusive result has been obtained. Larger programs in the future will be able to detect a significant correlation between neutrinos and jetted active galactic nuclei if the brightest radio sources are considered as neutrino emitters.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Medicine, General & Internal
Julia Stadelmaier, Isabelle Roux, Maria Petropoulou, Lukas Schwingshackl
Summary: This study aimed to evaluate the bias associated with certain methodological characteristics in nutrition research. The findings suggest that most characteristics may not exaggerate intervention effect estimates, except for trials with subjective outcomes.
Article
Astronomy & Astrophysics
A. S. Karaferias, G. Vasilopoulos, M. Petropoulou, P. A. Jenke, C. A. Wilson-Hodge, C. Malacaria
Summary: This study presents a method to estimate posterior distributions for parameters in the standard accretion torque model and binary orbital parameters for X-ray binaries using a nested sampling algorithm. The spin evolution of two Be X-ray binary systems in the Magellanic Clouds during major outbursts and a newly discovered Galactic ultra-luminous X-ray source are investigated. The method identified the more favorable torque model for each system and yielded meaningful ranges for the neutron star and orbital parameters. Contrary to standard predictions, the analysis showed that certain parameters are not proportional to each other when surpassing the Eddington limit.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Proceedings Paper
Astronomy & Astrophysics
M. Petropoulou, M. Meyer, I. Christie
Summary: Magnetic reconnection is a potential mechanism for the fast gamma-ray variability in blazars, with simulations and calculations producing results consistent with observational data. The characteristics of light curve variability and fast gamma-ray flares from reconnection events can be observed with the Fermi Large Area Telescope, providing important insights into the origin of gamma-ray radiation in blazars.
37TH INTERNATIONAL COSMIC RAY CONFERENCE, ICRC2021
(2022)
Article
Astronomy & Astrophysics
Ze-Rui Wang, Ruo-Yu Liu, Maria Petropoulou, Foteini Oikonomou, Rui Xue, Xiang-Yu Wang
Summary: Blazars are a class of active galactic nuclei that exhibit complex variability properties, including multiwavelength and orphan flares. This paper presents a unified model to explain these flares, proposing that they are the result of a combination of a quasistable background emission and a transient enhancement caused by a strong energy dissipation event.