papers

Publications (25)

astro-ph.HE2021

Simulations of cosmic ray propagation

M. Hanasz, A. Strong, P. Girichidis

We review numerical methods for simulations of cosmic ray (CR) propagation on galactic and larger scales. We present the development of algorithms designed for phenomenological and…

astro-ph.HE2009

Soft gamma-ray sources detected by INTEGRAL

D. Petry, V. Beckmann, H. Halloin +1

We aim to exploit the available INTEGRAL/SPI data to provide time-averaged spectra of the brightest soft gamma-ray sources. Employing a maximum-likelihood fit technique for our SPI…

astro-ph2008

Section on Supernova remnants and cosmic rays of the White Paper on the Status and Future of Ground-based Gamma-ray Astronomy

M. Pohl, A. Abdo, A. Atoyan +19

This is a report on the findings of the SNR/cosmic-ray working group for the white paper on the status and future of ground-based gamma-ray astronomy. The white paper is an APS com…

astro-ph2001

The Crab pulsar in the 0.75-30 MeV range as seen by CGRO COMPTEL

L. Kuiper, W. Hermsen, G. Cusumano +5

We present the time-averaged characteristics of the Crab pulsar in the 0.75-30 MeV energy window using data from the imaging Compton Telescope COMPTEL aboard the Compton Gamma-Ray…

astro-ph2005

SPI/INTEGRAL observation of the Galactic central radian: contribution of discrete sources and implication for the diffuse emission

L. Bouchet, J. P. Roques, P. Mandrou +4

The INTEGRAL observatory has been performing a deep survey of the Galactic central radian since 2003, with the goal of both extracting a catalog of sources and gaining insight into…

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-ph.HE2024

The eROSITA Upper Limits: Description and access to the data

D. Tubín-Arenas, M. Krumpe, G. Lamer +13

The soft X-ray instrument eROSITA on board the Spectrum-Roentgen-Gamma (SRG) observatory has successfully completed four of the eight planned all-sky surveys, detecting almost one…

astro-ph1997

COMPTEL gamma-ray study of the Crab nebula

R. D. van der Meulen, H. Bloemen, K. Bennett +6

We report on a study of the gamma-ray continuum emission from the Crab supernova nebula and on a search for nuclear de-excitation gamma-ray lines. Crab is the brightest continuum s…

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-ph2008

INTEGRAL SPI All-Sky View in Soft Gamma Rays: Study of Point Source and Galactic Diffuse Emissions

L. Bouchet, E. Jourdain, J. P. Roques +4

We have processed the data accumulated with INTEGRAL SPI during 4 years (~ 51 Ms) to study the Galactic ``diffuse'' emission morphology in the 20 keV to 8 MeV energy range. To achi…

astro-ph2004

INTEGRAL observations of the Large Magellanic Cloud region

S. Mereghetti, D. Gotz, A. Paizis +16

We present the preliminary results of the INTEGRAL survey of the Large Magellanic Cloud. The observations have been carried out in January 2003 (about 10^6 s) and January 2004 (abo…

astro-ph.HE2025

The gamma-ray emission from Radio Galaxies and their contribution to the Isotropic Gamma-Ray Background

A. Circiello, A. McDaniel, M. Di Mauro +6

We evaluate the contribution to the Isotropic Gamma-Ray Background (IGRB) coming from Radio Galaxies (RGs), the subclass of radio-loud Active Galactic Nuclei (AGN) with the highest…

astro-ph.HE2010

The 511 keV emission from positron annihilation in the Galaxy

N. Prantzos, C. Boehm, A. M. Bykov +9

The first gamma-ray line originating from outside the solar system that was ever detected is the 511 keV emission from positron annihilation in the Galaxy. Despite 30 years of inte…

astro-ph.HE2022

Abundance and temperature of the outer hot circum-Galactic medium: The SRG/eROSITA view of the soft X-ray background in the eFEDS field

G. Ponti, X. Zheng, N. Locatelli +14

Despite their vital importance to understand galaxy evolution and our own Galactic ecosystem, our knowledge of the physical properties of the hot phase of the Milky Way is still in…

astro-ph1996

COMPTEL detection of the high-energy gamma-ray source 2CG 135+01

R. van Dijk, K. Bennett, H. Bloemen +11

We present an analysis of COMPTEL observations made between November 1991 and May 1994 of 2CG 135+01, a bright gamma-ray source located near the Galactic plane. At energies above 1…

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…

hep-ph2012

Les Houches 2011: Physics at TeV Colliders New Physics Working Group Report

G. Brooijmans, B. Gripaios, F. Moortgat +141

We present the activities of the "New Physics" working group for the "Physics at TeV Colliders" workshop (Les Houches, France, 30 May-17 June, 2011). Our report includes new agreem…

astro-ph2003

Calibration of the Spectrometer aboard the INTEGRAL satellite

Stéphane Schanne, B. Cordier, M. Gros +27

SPI, the Spectrometer on board the ESA INTEGRAL satellite, to be launched in October 2002, will study the gamma-ray sky in the 20 keV to 8 MeV energy band with a spectral resolutio…

astro-ph.SR2024

Compact white-dwarf binaries in the combined SRG/eROSITA/SDSS eFEDS survey

A. Schwope, J. Kurpas, P. Baecke +22

Aims. Compact white-dwarf binaries are selected from spectra obtained in the early SDSS-V plate program. A dedicated set of SDSS plate observations were carried out in the eFEDS fi…

astro-ph2007

The sky distribution of 511 keV positron annihilation line emission as measured with INTEGRAL/SPI

G. Weidenspointner, J. Knoedlseder, P. Jean +10

The imaging spectrometer SPI on board ESA's INTEGRAL observatory provides us with an unprecedented view of positron annihilation in our Galaxy. The first sky maps in the 511 keV an…

astro-ph.GA2022

CHANG-ES XXVI: Insights into cosmic-ray transport from radio halos in edge-on galaxies

M. Stein, V. Heesen, R. -J. Dettmar +13

Galactic winds play a key role in regulating the evolution of galaxies over cosmic time. In recent years, the role of cosmic rays (CR) in the formation of the galactic wind has inc…

astro-ph2003

SPI/INTEGRAL in-flight performance

J. -P. Roques, S. Schanne, A. von Kienlin +23

The SPI instrument has been launched on-board the INTEGRAL observatory on October 17, 2002. SPI is a spectrometer devoted to the sky observation in the 20 keV-8 MeV energy range us…

astro-ph2004

Search for 44Ti gamma-ray line emission from GRO J0852-4642 with INTEGRAL/SPI

A. von Kienlin, D. Attie, S. Schanne +7

The gamma-ray source GRO J0852-4642, discovered by COMPTEL, is a possible counterpart of the supernova remnant RX J0852-4622. Detection of radioactive decay from 44Ti nuclei would…

astro-ph2003

SPI/INTEGRAL observation of the Cygnus region

L. Bouchet, E. Jourdain, J. -P. Roques +22

We present the analysis of the first observations of the Cygnus region by the SPI spectrometer onboard the Integral Gamma Ray Observatory, encompassing 600 ks of data. Thr…

astro-ph2003

INTEGRAL/SPI ground calibration

D. Attié, B. Cordier, M. Gros +30

Three calibration campaigns of the spectrometer SPI have been performed before launch in order to determine the instrument characteristics, such as the effective detection area, th…