papers

Publications (70)

astro-ph2006

The frontier of darkness: the cases of GRB 040223, GRB 040422, GRB 040624

P. D'Avanzo, P. Filliatre, P. Goldoni +23

Understanding the reasons for the faintness of the optical/near-infrared afterglows of the so-called dark bursts is essential to assess whether they form a subclass of GRBs, and he…

astro-ph2005

Gamma-ray bursts and other sources of giant lightning discharges in protoplanetary systems

B. McBreen, E. Winston, S. McBreen +1

Lightning in the solar nebula is considered to be one of the probable sources for producing the chondrules that are found in meteorites. Gamma-ray bursts (GRBs) provide a large flu…

astro-ph.HE2018

The e-ASTROGAM gamma-ray space observatory for the multimessenger astronomy of the 2030s

V. Tatischeff, A. De Angelis, M. Tavani +74

e-ASTROGAM is a concept for a breakthrough observatory space mission carrying a gamma-ray telescope dedicated to the study of the non-thermal Universe in the photon energy range fr…

astro-ph2005

The weak INTEGRAL bursts GRB040223 and GRB040624: an emerging population of dark afterglows

P. Filliatre, S. Covino, P. D'Avanzo +18

We report here gamma-ray, X-ray and near-infrared observations of GRB040223 along with gamma-ray and optical observations of GRB040624. GRB040223 was detected by INTEGRAL close to…

astro-ph2008

A photometric redshift of for the \agile GRB 080514B

A. Rossi, A. de Ugarte Postigo, P. Ferrero +26

Aims: The AGILE gamma-ray burst GRB 080514B is the first burst with detected emission above 30 MeV and an optical afterglow. However, no spectroscopic redshift for this burst is kn…

astro-ph2007

Polarisation studies of the prompt gamma-ray emission from GRB 041219a using the Spectrometer aboard INTEGRAL

S. McGlynn, D. J. Clark, A. J. Dean +6

The spectrometer aboard INTEGRAL, SPI, has the capability to detect the signature of polarised emission from a bright gamma-ray source. GRB 041219a is the most intense burst locali…

astro-ph1999

Gamma-Ray Bursts and the Origin of Chondrules and Planets

B. McBreen, L. Hanlon

The effect of a nearby -ray burst (GRB) on the preplanetary solar nebula is considered. The intense irradiation by x-rays and -rays would have caused dust balls to become m…

astro-ph2002

Cumulative light curves of gamma-ray bursts and relaxation systems

S. McBreen, B. McBreen, L. Hanlon +1

The cumulative light curves of a large sample of gamma-ray bursts (GRBs) were obtained by summing the BATSE counts. The smoothed profiles are much simpler than the complex and erra…

astro-ph.HE2018

Science with e-ASTROGAM (A space mission for MeV-GeV gamma-ray astrophysics)

A. De Angelis, V. Tatischeff, I. A. Grenier +248

e-ASTROGAM (enhanced ASTROGAM) is a breakthrough Observatory space mission, with a detector composed by a Silicon tracker, a calorimeter, and an anticoincidence system, dedicated t…

astro-ph.SR2026

Stochastic Optical Variability and an rms-flux Relation in the Intermediate Polar EP240309a

S. -Y. Wu, Y. -D. Hu, I. Perez-Garcia +18

Magnetic cataclysmic variables provide a natural laboratory for studying how accretion interacts with compact-object magnetospheres and generates stochastic variability. We present…

astro-ph.HE2019

PHEMTO : Polarimetric High Energy Modular Telescope Observatory

P. Laurent, F. Acero, V. Beckmann +27

With the opening of the X and gamma--ray windows in the sixties, thanks to to sounding rockets and satellite-borne instruments, extremely energetic and violent phenomena were disco…

astro-ph2000

ASCA and other contemporaneous observations of the blazar B2 1308+326

D. Watson, N. Smith, L. Hanlon +8

The high redshift (z=0.997) blazar B2 1308+326 was observed contemporaneously at x-ray, optical and radio wavelengths in June 1996. The x-ray observations were performed with ASCA.…

astro-ph2002

Timing diagrams and correlations in gamma-ray bursts signal jets from accretion into black holes

S. McBreen, B. McBreen, F. Quilligan +1

The temporal properties of a sample of 498 bright gamma-ray bursts (GRBs) with durations between 0.05 s and 674 s were analysed. The large range in duration (T90) is accompanied by…

astro-ph.CO2013

Light from the Cosmic Frontier: Gamma-Ray Bursts

L. Amati, J. -L. Atteia, L. Balazs +41

Gamma-Ray Bursts (GRBs) are the most powerful cosmic explosions since the Big Bang, and thus act as signposts throughout the distant Universe. Over the last 2 decades, these ultra-…

astro-ph.SR2022

Photometric and spectroscopic evolution of the interacting transient AT 2016jbu (Gaia16cfr)

S. J. Brennan, M. Fraser, J. Johansson +68

We present the results from a high cadence, multi-wavelength observation campaign of AT 2016jbu (aka Gaia16cfr), an interacting transient. This dataset complements the current lite…

astro-ph.HE2022

Progenitor, environment, and modelling of the interacting transient, AT 2016jbu (Gaia16cfr)

S. J. Brennan, M. Fraser, J. Johansson +67

We present the bolometric lightcurve, identification and analysis of the progenitor candidate, and preliminary modelling of AT2016jbu (Gaia16cfr). We find a progenitor consistent w…

astro-ph2000

ISO detection of a 60micron source near GRB970508

L. Hanlon, R. J. Laureijs, L. Metcalfe +18

The Infrared Space Observatory observed the field of the --ray burst GRB 970508 with the CAM and PHT instruments on May 21 and 24, 1997 and with PHT in three filters in Novembe…

astro-ph.CO2009

High energy emission and polarisation limits for the INTEGRAL burst GRB 061122

S. McGlynn, S. Foley, B. McBreen +6

(Abridged) GRB 061122 is one of the brightest GRBs detected within INTEGRAL's field of view to date. The two gamma-ray detectors on INTEGRAL were used to investigate the spectral c…

astro-ph2001

Temporal properties of the short gamma-ray bursts

S. McBreen, F. Quilligan, B. McBreen +2

A temporal analysis has been performed on a sample of 100 bright gamma-ray bursts (GRBs) with T90<2s from the BATSE current catalog. The GRBs were denoised using a median filter an…

astro-ph2002

Kerr black holes and time profiles of gamma-ray bursts

S. McBreen, B. McBreen, L. Hanlon +1

The cumulative light curves of gamma-ray bursts (GRBs) smooth the spiky nature of the running light curve. The cumulative count increases in an approximately linear way with time t…

astro-ph2003

INTEGRAL Spectrometer SPI's GRB detection capabilities. GRBs detected inside SPI's FoV and with the anticoincidence system ACS

A. von Kienlin, V. Beckmann, A. Rau +15

The spectrometer SPI, one of the two main instruments of the INTEGRAL spacecraft, offers significant gamma-ray burst detection capabilities. In its 35 deg (full width) field of vie…

astro-ph2008

GRB 070707: the first short gamma-ray burst observed by INTEGRAL

S. McGlynn, S. Foley, S. McBreen +4

INTEGRAL has observed 47 long-duration GRBs (T_90 > 2s) and 1 short-duration GRB (T_90 < 2s) in five years of observation since October 2002. This work presents the properties of t…

astro-ph2000

ISO observations of the Wolf-Rayet galaxy NGC 7714 and its companion object NGC 7715

B. O'Halloran, L. Metcalfe, M. Delaney +5

The interacting system Arp 284 consisting of the Wolf-Rayet galaxy NGC 7714 and its irregular companion NGC 7715 was observed using the Infrared Space Observatory. Deconvolved ISOC…

astro-ph2003

Similarities in the temporal properties of gamma-ray bursts and soft gamma-ray repeaters

S. McBreen, L. Moran, B. McBreen +3

Magnetars are modelled as sources that derive their output from magnetic energy that substantially exceeds their rotational energy. An implication of the recent polarization measur…

astro-ph.HE2018

INTEGRAL results on the electromagnetic counterparts of gravitational waves

S. Mereghetti, V. Savchenko, C. Ferrigno +18

Thanks to its high orbit and a set of complementary detectors providing continuous coverage of the whole sky, the INTEGRAL satellite has unique capabilities for the identification…

astro-ph2004

Gamma-ray bursts and X-ray melting of material as a potential source of chondrules and planets

P. Duggan, B. McBreen, A. J. Carr +4

The intense radiation from a gamma-ray burst (GRB) is shown to be capable of melting stony material at distances up to 300 light years which subsequently cool to form chondrules. T…

astro-ph2004

Gamma-ray bursts and X-ray melting of material to form chondrules and planets

P. Duggan, B. McBreen, A. J. Carr +7

Chondrules are millimeter sized objects of spherical to irregular shape that constitute the major component of chondritic meteorites that originate in the region between Mars and J…

astro-ph2004

Preliminary INTEGRAL Analysis of GRB040106

L. Moran, L. Hanlon, A. von Kienlin +9

On January 6th 2004, the IBAS burst alert system triggered the 8th gamma-ray burst (GRB) to be detected by the INTEGRAL satellite. The position was determined and publicly distribu…

astro-ph.HE2014

GRB 120711A: an intense INTEGRAL burst with long-lasting soft gamma-ray emission and a powerful optical flash

A. Martin-Carrillo, L. Hanlon, M. Topinka +20

A long and intense gamma-ray burst (GRB) was detected by INTEGRAL on July 11 2012 with a duration of ~115s and fluence of 2.8x10^-4 erg cm^-2 in the 20 keV-8 MeV energy range. GRB…

astro-ph2010

Photometry and spectroscopy of GRB 060526: A detailed study of the afterglow and host galaxy of a z=3.2 gamma-ray burst

C. C. Thöne, D. A. Kann, G. Jóhannesson +58

Aims: With this paper we want to investigate the highly variable afterglow light curve and environment of gamma-ray burst (GRB) 060526 at . Methods: We present one of the…

astro-ph2001

Temporal properties of gamma-ray bursts as signatures of jets from the central engine

F. Quilligan, B. McBreen, L. Hanlon +3

A comprehensive temporal analysis has been performed on the 319 brightest GRBs with T90>2s from the BATSE current catalog. The rise times, fall times, full-widths at half maximum (…

astro-ph.HE2021

INTEGRAL Results on Gamma-Ray Bursts and Polarization of Hard X-ray Sources

D Gotz, C. Gouiffes, J. Rodriguez +9

In this paper we first review the results obtained by the INTEGRAL mission in the domain of Gamma-Ray Bursts (GRBs), thanks to the INTEGRAL Burst Alert System, which is able to del…

astro-ph.HE2013

X-ray behaviour of GRBs detected by INTEGRAL/JEM-X

A. Martin-Carrillo, L. Hanlon

INTEGRAL's JEM-X instrument offers a very rare opportunity to observe the full prompt X-ray emission from GRBs and the transition to the afterglow phase. A study of prompt X-ray fl…

astro-ph.HE2018

X-shooter and ALMA spectroscopy of GRB 161023A - A study of metals and molecules in the line of sight towards a luminous GRB

A. de Ugarte Postigo, C. C. Thöne, J. Bolmer +45

Long gamma-ray bursts are produced during the dramatic deaths of massive stars with very short lifetimes, meaning that they explode close to the birth place of their progenitors. D…

astro-ph.HE2017

INTEGRAL Detection of the First Prompt Gamma-Ray Signal Coincident with the Gravitational Wave Event GW170817

V. Savchenko, C. Ferrigno, E. Kuulkers +20

We report the e INTernational Gamma-ray Astrophysics Laboratory (INTEGRAL) detection of the short gamma-ray burst GRB 170817A (discovered by Fermi-GBM) with a signal-to-noise ratio…

astro-ph.HE2016

Supplement: Localization and broadband follow-up of the gravitational-wave transient GW150914

B. P. Abbott, R. Abbott, T. D. Abbott +1538

This Supplement provides supporting material for arXiv:1602.08492 . We briefly summarize past electromagnetic (EM) follow-up efforts as well as the organization and policy of the c…

astro-ph.HE2017

INTEGRAL IBIS, SPI, and JEM-X observations of LVT151012

V. Savchenko, A. Bazzano, E. Bozzo +18

During the first observing run of LIGO, two gravitational wave events and one lower-significance trigger (LVT151012) were reported by the LIGO/Virgo collaboration. At the time of L…

astro-ph.HE2011

GRIPS - Gamma-Ray Imaging, Polarimetry and Spectroscopy

J. Greiner, K. Mannheim, F. Aharonian +65

We propose to perform a continuously scanning all-sky survey from 200 keV to 80 MeV achieving a sensitivity which is better by a factor of 40 or more compared to the previous missi…

astro-ph2005

ISO observations of the interacting galaxy Markarian 297: with the powerful supernova remnant 1982aa

L. Metcalfe, B. O'Halloran, B. McBreen +10

Markarian (Mkn) 297 is a complex system with two interacting galaxies. Observations were made with ISO using ISOCAM, ISOPHOT and LWS. We present ISOCAM maps at 6.7, 7.7, 12 and 14.…

astro-ph2008

The Spectral Lag of GRB060505: A Likely Member of the Long Duration Class

S. McBreen, S. Foley, D. Watson +7

Two long gamma-ray bursts, GRB 060505 and GRB 060614, occurred in nearby galaxies at redshifts of 0.089 and 0.125 respectively. Due to their proximity and durations, deep follow-up…

astro-ph.HE2019

All-Sky-ASTROGAM: The MeV Gamma-Ray Companion to Multimessenger Astronomy

V. Tatischeff, A. De Angelis, M. Tavani +33

All-Sky-ASTROGAM is a gamma-ray observatory operating in a broad energy range, 100 keV to a few hundred MeV, recently proposed as the "Fast" (F) mission of the European Space Agenc…

astro-ph.HE2024

Fires in the deep: The luminosity distribution of early-time gamma-ray-burst afterglows in light of the Gamow Explorer sensitivity requirements

D. A. Kann, N. E. White, G. Ghirlanda +58

Gamma-ray bursts (GRBs) are ideal probes of the Universe at high redshift (z > 5), pinpointing the locations of the earliest star-forming galaxies and providing bright backlights t…

astro-ph.IM2017

The e-ASTROGAM gamma-ray space mission

V. Tatischeff, M. Tavani, P. von Ballmoos +48

The e-ASTROGAM is a gamma-ray space mission to be proposed as the M5 Medium-size mission of the European Space Agency. It is dedicated to the observation of the Universe with unpre…

astro-ph.HE2010

Gamma-Ray Bursts Overview

B. McBreen, S. Foley, L. Hanlon

It is now more than 40 years since the discovery of gamma-ray bursts (GRBs) and in the last two decades there has been major progress in the observations of bursts, the afterglows…

astro-ph.IM2019

Web application for galaxy-targeted follow-up of electromagnetic counterparts to gravitational wave sources

L. Salmon, L. Hanlon, R. M. Jeffrey +1

The Laser Interferometer Gravitational Wave Observatory (LIGO) and Virgo Collaboration's Observing Run 3 has demanded the development of widely-applicable tools for gravitational w…

astro-ph.HE2017

INTEGRAL observations of GW170104

V. Savchenko, C. Ferrigno, E. Bozzo +16

We used data from the INTErnational Gamma-Ray Astrophysics Laboratory (INTEGRAL) to set upper-limits on the -ray and hard X-ray prompt emission associated with the gravitationa…

astro-ph.HE2017

A kilonova as the electromagnetic counterpart to a gravitational-wave source

S. J. Smartt, T. -W. Chen, A. Jerkstrand +118

Gravitational waves were discovered with the detection of binary black hole mergers and they should also be detectable from lower mass neutron star mergers. These are predicted to…

astro-ph.SR2026

Ellipsoidal modulation and multi-wavelength activity in the pre-cataclysmic binary RX J1553.0+4457

S. -Y. Wu, M. Gritsevich, Q. -H. Lao +39

RX J1553.0+4457 (TMTS J15530469+4457458) is a detached post-common-envelope binary containing a cool white dwarf and an active late-type companion. We present a multi-wavelength st…

astro-ph2005

Out of the darkness: the infrared afterglow of the INTEGRAL burst GRB 040422 observed with the VLT

P. Filliatre, P. D'Avanzo, S. Covino +15

GRB 040422 was detected by the INTEGRAL satellite at an angle of only 3 degrees from the Galactic plane. Analysis of the prompt emission observed with the SPI and IBIS instruments…

astro-ph.HE2016

INTEGRAL upper limits on gamma-ray emission associated with the gravitational wave event GW150914

V. Savchenko, C. Ferrigno, S. Mereghetti +14

Using observations of the INTErnational Gamma-Ray Astrophysics Laboratory (INTEGRAL), we put upper limits on the gamma-ray and hard X-ray prompt emission associated with the gravit…

astro-ph2004

INTEGRAL Spectrometer Analysis of GRB030227 & GRB030131

L. Moran, L. Hanlon, B. McBreen +9

The spectrometer SPI on board INTEGRAL is capable of high-resolution spectroscopic studies in the energy range 20keV to 8MeV for GRBs which occur within the fully coded field of vi…

astro-ph.HE2017

Colour variations in the GRB 120327A afterglow

A. Melandri, S. Covino, E. Zaninoni +42

We present a comprehensive temporal and spectral analysis of the long Swift GRB 120327A afterglow data to investigate the possible causes of the observed early time colour variatio…

astro-ph2000

ISO observations of a sample of 60 micron peaker galaxies

R. J. Laureijs, D. Watson, L. Metcalfe +9

The sample of IRAS galaxies with spectral energy distributions that peak near 60 microns are called Sixty Micron Peakers (SMPs or 60PKs). Their generally peculiar and amorphous mor…

astro-ph.HE2016

Localization and broadband follow-up of the gravitational-wave transient GW150914

B. P. Abbott, R. Abbott, T. D. Abbott +1538

A gravitational-wave (GW) transient was identified in data recorded by the Advanced Laser Interferometer Gravitational-wave Observatory (LIGO) detectors on 2015 September 14. The e…

astro-ph2005

INTEGRAL and XMM-Newton observations of the low-luminosity and X-ray rich burst GRB 040223

S. McGlynn, S. McBreen, L. Hanlon +6

GRB 040223 was observed by INTEGRAL and XMM-Newton. GRB 040223 has a peak flux of (1.6+/-0.13) x10^-8 ergs cm^-2 s^-1, a fluence of (4.4+/-0.4)x10^-7 ergs cm^-2 and a steep photon…

astro-ph2008

Global characteristics of GRBs observed with INTEGRAL and the inferred large population of low-luminosity GRBs

S. Foley, S. McGlynn, L. Hanlon +2

INTEGRAL has two sensitive gamma-ray instruments that have detected 46 gamma-ray bursts (GRBs) up to July 2007. We present the spectral, spatial, and temporal properties of the bur…

astro-ph2004

XMM-Newton observations of the BL Lac MS0205.7+3509: a dense, low-metallicity absorber

D. Watson, B. McBreen, L. Hanlon +5

The high-frequency-peaked BL Lac, MS0205.7+3509 was observed twice with XMM-Newton. Both X-ray spectra are synchrotron-dominated, with mean 0.2--10keV fluxes of 2.80+/-0.01 and 3.3…

astro-ph2006

Observations of the intense and ultra-long burst GRB041219a with the Germanium Spectrometer on INTEGRAL

S. McBreen, L. Hanlon, S. McGlynn +5

GRB041219a is the brightest burst localised by INTEGRAL. The intense burst occurred about ~250s after the precursor and the long delay enabled optical and near infrared telescopes…

astro-ph2002

ISO observations of Hickson Compact Group 31 with the central Wolf-Rayet galaxy NGC 1741

B. O'Halloran, L. Metcalfe, B. McBreen +5

Hickson Compact Group (HCG) 31, consisting of the Wolf-Rayet galaxy NGC 1741 and its irregular dwarf companions, was observed using the Infrared Space Observatory. The deconvolved…

astro-ph.SR2019

Full orbital solution for the binary system in the northern Galactic disc microlensing event Gaia16aye

Łukasz Wyrzykowski, P. Mróz, K. A. Rybicki +182

Gaia16aye was a binary microlensing event discovered in the direction towards the northern Galactic disc and was one of the first microlensing events detected and alerted to by the…

astro-ph2004

INTEGRAL and XMM-Newton Observations of GRB040106

L. Moran, S. Mereghetti, D. Gotz +10

On January 6th 2004, the IBAS burst alert system triggered the 8th gamma-ray burst (GRB) to be located by the INTEGRAL satellite. The position was determined and publicly distribut…

astro-ph.HE2020

INTEGRAL discovery of a burst with associated radio emission from the magnetar SGR 1935+2154

S. Mereghetti, V. Savchenko, C. Ferrigno +23

We report on INTEGRAL observations of the soft -ray repeater SGR 1935+2154 performed between 2020 April 28 and May 3. Several short bursts with fluence of

astro-ph.HE2013

GRB 130606A within a sub-DLA at redshift 5.91

A. J. Castro-Tirado, R. Sánchez-Ramírez, S. L. Ellison +38

Events such as GRB130606A at z=5.91, offer an exciting new window into pre-galactic metal enrichment in these very high redshift host galaxies. We study the environment and host ga…

astro-ph.IM2018

The THESEUS space mission concept: science case, design and expected performances

L. Amati, P. O'Brien, D. Goetz +208

THESEUS is a space mission concept aimed at exploiting Gamma-Ray Bursts for investigating the early Universe and at providing a substantial advancement of multi-messenger and time-…

astro-ph1999

Simultaneous Multifrequency Observations of the BL Lac MS 0205.7+3509

D. Watson, L. Hanlon, B. McBreen +7

Radio and optical observations of the possible microlensed BL Lac source MS 0205.7+3509 were obtained simultaneously with ASCA x-ray measurements in February 1997. A single power l…

astro-ph2002

Temporal properties of short and long gamma-ray bursts

S. McBreen, F. Quilligan, B. McBreen +2

A temporal analysis was performed on a sample of 100 bright short GRBs with T90 < 2s from the BATSE Current Catalog along with a similar analysis on 319 long bright GRBs with T90 >…

astro-ph.IM2021

Time Domain Astronomy with the THESEUS Satellite

S. Mereghetti, S. Balman, M. Caballero-Garcia +74

THESEUS is a medium size space mission of the European Space Agency, currently under evaluation for a possible launch in 2032. Its main objectives are to investigate the early Univ…

astro-ph2008

Optical and infrared flares from a transient Galactic soft gamma-ray repeater

A. J. Castro-Tirado, A. de Ugarte Postigo, J. Gorosabel +33

Soft gamma-ray repeaters (SGRs) are a rare type of gamma-ray transient sources that are ocasionally detected as bursts in the high-energy sky. They are thought to be produced by ma…

astro-ph1998

ISO Mid-Infrared Observations of Abell 370

L. Metcalfe, B. Altieri, H. Aussel +11

We report on the mid-IR imaging at 7 and 10 microns of the galaxy cluster Abell 370, obtained with the ISOCAM instrument onboard ESA's Infrared Space Observatory (ISO), as part of…

astro-ph.IM2021

The THESEUS space mission: science goals, requirements and mission concept

L. Amati, P. T. O'Brien, D. Götz +31

THESEUS, one of the two space mission concepts being studied by ESA as candidates for next M5 mission within its Comsic Vision programme, aims at fully exploiting Gamma-Ray Bursts…