3.6k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- National Institute for AstrophysicsIT865 papers
- Centre National de la Recherche ScientifiqueFR635 papers
- Astronomical Observatory of RomeIT475 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR368 papers
- Brera Astronomical ObservatoryIT355 papers
- Goddard Space Flight CenterUS343 papers
- University of PaduaIT336 papers
- Astrophysique, Instrumentation et ModélisationFR332 papers
- California Institute of TechnologyUS323 papers
- Université Paris CitéFR321 papers
- Arcetri Astrophysical ObservatoryIT317 papers
- University College LondonGB308 papers
69 papers · 1 filter
Astrochemistry at work in the L1157-B1 shock: acetaldehyde formation
C. Codella, F. Fontani, C. Ceccarelli +5
The formation of complex organic molecules (COMs) in protostellar environments is a hotly debated topic. In particular, the relative importance of the gas phase processes as compar…
Spatially resolved physical conditions of molecular gas and potential star formation tracers in M83, revealed by the Herschel SPIRE FTS
Ronin Wu, Suzanne Madden, Frédéric Galliano +19
Since the launch of the Herschel Space Observatory, our understanding about the photo-dissociation regions (PDR) has taken a step forward. In the bandwidth of the Fourier Transform…
Reconnection outflow generated turbulence in the solar wind
Z. Vörös, Y. L. Sasunov, V. S. Semenov +3
Petschek-type time-dependent reconnection (TDR) and quasi-stationary reconnection (QSR) models are considered to understand reconnection outflow structures and the features of the…
The 1.4 GHz radio properties of hard X-ray selected AGN
F. Panessa, A. Tarchi, P. Castangia +7
We have analyzed the NVSS and SUMSS data at 1.4 GHz and 843 MHz for a well defined complete sample of hard X-ray AGN observed by INTEGRAL. A large number (70/79) of sources are det…
Radial evolution of intermittency of density fluctuations in the fast solar wind
R. Bruno, D. Telloni, L. Primavera +6
We study the radial evolution of intermittency of density fluctuations in the fast solar wind. The study is performed analyzing the plasma density measurements provided by Helios 2…
Far-infrared line spectra of Seyfert galaxies from the Herschel-PACS Spectrometer
Luigi Spinoglio, Miguel Pereira-Santaella, Kalliopi M. Dasyra +4
We present spectroscopic observations of FIR fine-structure lines of 26 Seyfert galaxies obtained with the Herschel-PACS spectrometer. These observations are complemented by spectr…
Interplay between heartbeat oscillations and wind outflow in microquasar IGR J17091-3624
Agnieszka Janiuk, Mikolaj Grzedzielski, Fiamma Capitanio +1
During the bright outburst in 2011, the black hole candidate IGR J17091-3624 exhibited strong quasi-periodic flare-like events (on timescales of tens of seconds) in some characteri…
The density structure of the L1157 molecular outflow
A. I. Gómez-Ruiz, C. Codella, B. Lefloch +6
We present a multiline CS survey towards the brightest bow-shock B1 in the prototypical chemically active protostellar outflow L1157. We made use of (sub-)mm data obtained in the f…
Deuteration and evolution in the massive star formation process: the role of surface chemistry
F. Fontani, G. Busquet, Aina Palau +5
An ever growing number of observational and theoretical evidence suggests that the deuterated fraction (column density ratio between a species containing D and its hydrogenated cou…
Insights into gas heating and cooling in the disc of NGC 891 from Herschel far-infrared spectroscopy
T. M. Hughes, K. Foyle, M. R. P. Schirm +15
We present Herschel PACS and SPIRE spectroscopy of the most important far-infrared cooling lines in the nearby edge-on spiral galaxy, NGC 891: [CII] 158 m, [NII] 122, 205 m,…
Quantifying the Heating Sources for Mid-infrared Dust Emissions in Galaxies: The Case of M 81
Nanyao Lu, G. J. Bendo, A. Boselli +12
With the newly available SPIRE images at 250 and 500 micron from Herschel Space Observatory, we study quantitative correlations over a sub-kpc scale among three distinct emission c…
Outflow of hot and cold molecular gas from the obscured secondary nucleus of NGC3256: closing in on feedback physics
Bjorn Emonts, Javier Piqueras-Lopez, Luis Colina +5
The nuclei of merging galaxies are often deeply buried in dense layers of gas and dust. In these regions, gas outflows driven by starburst and AGN activity are believed to play a c…
High-resolution, 3D radiative transfer modeling : I. The grand-design spiral galaxy M51
Ilse De Looze, Jacopo Fritz, Maarten Baes +20
Context: Dust reprocesses about half of the stellar radiation in galaxies. The thermal re-emission by dust of absorbed energy is considered driven merely by young stars and, conseq…
Optical and X-ray behaviour of the high mass X-ray transient A0535+26/HDE245770 in February-March 2014
F. Giovannelli, G. S. Bisnovatyi-Kogan, I. Bruni +3
The optical behaviour of the Be star in the high-mass X-ray transient A0535+26/HDE245770 shows that at periastron the luminosity is typically enhanced by 0.02 to a few tenths magni…
The major upgrade of the MAGIC telescopes, Part I: The hardware improvements and the commissioning of the system
MAGIC Collaboration, J. Aleksic, S. Ansoldi +162
The MAGIC telescopes are two Imaging Atmospheric Cherenkov Telescopes (IACTs) located on the Canary island of La Palma. The telescopes are designed to measure Cherenkov light from…
The major upgrade of the MAGIC telescopes, Part II: A performance study using observations of the Crab Nebula
MAGIC Collaboration, J. Aleksic, S. Ansoldi +163
MAGIC is a system of two Imaging Atmospheric Cherenkov Telescopes located in the Canary island of La Palma, Spain. During summer 2011 and 2012 it underwent a series of upgrades, in…
The Large Observatory For x-ray Timing
M. Feroci, J. W. den Herder, E. Bozzo +341
The Large Observatory For x-ray Timing (LOFT) was studied within ESA M3 Cosmic Vision framework and participated in the final down-selection for a launch slot in 2022-2024. Thanks…
Radiation tests of the Silicon Drift Detectors for LOFT
E. Del Monte, P. Azzarello, E. Bozzo +13
During the three years long assessment phase of the LOFT mission, candidate to the M3 launch opportunity of the ESA Cosmic Vision programme, we estimated and measured the radiation…
Baseline design of the filters for the LAD detector on board LOFT
M. Barbera, B. Winter, J. Coker +4
The Large Observatory for X-ray Timing (LOFT) was one of the M3 missions selected for the phase A study in the ESA's Cosmic Vision program. LOFT is designed to perform high-time-re…
The LOFT Ground Segment
E. Bozzo, A. Antonelli, A. Argan +27
LOFT, the Large Observatory For X-ray Timing, was one of the ESA M3 mission candidates that completed their assessment phase at the end of 2013. LOFT is equipped with two instrumen…
The design of the wide field monitor for LOFT
S. Brandt, M. Hernanz, L. Alvarez +41
LOFT (Large Observatory For x-ray Timing) is one of the ESA M3 missions selected within the Cosmic Vision program in 2011 to carry out an assessment phase study and compete for a l…
The Large Area Detector of LOFT: the Large Observatory for X-ray Timing
S. Zane, D. Walton, T. Kennedy +56
LOFT (Large Observatory for X-ray Timing) is one of the five candidates that were considered by ESA as an M3 mission (with launch in 2022-2024) and has been studied during an exten…
Optimisation of the design for the LOFT Large Area Detector Module
D. Walton, B. Winter, S. Zane +25
LOFT (Large Observatory for X-ray Timing) is an X-ray timing observatory that, with four other candidates, was considered by ESA as an M3 mission (with launch in 2022-2024) and has…
Hyper-velocity impact test and simulation of a double-wall shield concept for the Wide Field Monitor aboard LOFT
E. Perinati, M. Rott, A. Santangelo +10
The space mission LOFT (Large Observatory For X-ray Timing) was selected in 2011 by ESA as one of the candidates for the M3 launch opportunity. LOFT is equipped with two instrument…