2k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- A. Zezas3 profiles106 · h 46
- P. Reig2 profiles88 · h 30
- I. Papadakis2 profiles84 · h 43
- V. Charmandaris2 profiles76 · h 70
- V. Pavlidou2 profiles58 · h 50
- C. Soukoulis54 · h 111
- K. Tassis2 profiles52 · h 26
- E. Stratakis47 · h 63
- N. Kylafis2 profiles43 · h 34
- C. Galiotis39 · h 57
- D. Blinov3 profiles33 · h 41
- M. Kafesaki33 · h 54
- University of CreteGR1.1k papers
- California Institute of TechnologyUS231 papers
- Centre National de la Recherche ScientifiqueFR216 papers
- Center for Astrophysics Harvard & SmithsonianUS175 papers
- FORTH Institute of Electronic Structure and LaserGR151 papers
- Max Planck Institute for Radio AstronomyDE139 papers
- Observatoire de ParisFR102 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR94 papers
- Goddard Space Flight CenterUS93 papers
- Max Planck Institute for Extraterrestrial PhysicsDE89 papers
- Aalto UniversityFI84 papers
- Leiden UniversityNL82 papers
19 papers · 2 filters
Localizing the -ray emitting region in the blazar TXS 2013+370
E. Traianou, T. P. Krichbaum, B. Boccardi +9
The -ray production mechanism and its localization in blazars are still a matter of debate. The main goal of this paper is to constrain the location of the high-energy emission…
Stabilizing effect of magnetic helicity on magnetic cavities in the intergalactic medium
Simon Candelaresi, Fabio Del Sordo
We investigate the effect of magnetic helicity on the stability of buoyant magnetic cavities as found in the intergalactic medium. In these cavities, we insert helical magnetic fie…
Star-forming Clumps in Local Luminous Infrared Galaxies
K. L. Larson, T. Díaz-Santos, L. Armus +15
We present narrow-band near-infrared imaging of Pa and Pa emission of 48 local Luminous Infrared Galaxies (LIRGs) from the Great Observatories All-Sky LIRG Survey (GOAL…
Probing fragmentation and velocity sub-structure in the massive NGC 6334 filament with ALMA
Y. Shimajiri, Ph. Andre, E. Ntormousi +3
Herschel surveys of Galactic clouds support a paradigm for low-mass star formation in which dense filaments play a crucial role. The detailed fragmentation properties of star-formi…
Modeling the magnetized Local Bubble from dust data
V. Pelgrims, K. Ferrière, F. Boulanger +2
The Sun is embedded in the so-called Local Bubble (LB) -- a cavity of hot plasma created by supernova explosions and surrounded by a shell of cold, dusty gas. Knowing the local dis…
The inner view of NGC 1052 using multiple X-ray observations
Natalia Osorio-Clavijo, Omaira González-Martín, Iossif Papadakis +2
In this paper, we make a multi-epoch analysis of NGC 1052, one of the prototypical LLAGN, using XMM-Newton, Suzaku and NuSTAR observations, taken from 2001 to 2017. This is the fir…
Discrete star formation events in the central Bar of the Small Magellanic Cloud
A. Strantzalis, D. Hatzidimitriou, A. Zezas +3
We present the results of the photometric analysis of a large part of the main body of the Small Magellanic Cloud. Using the 6.5m Magellan Telescope at the Las Campanas Observatory…
A diagnostic tool for the identification of Supernova Remnants
M. Kopsacheili, A. Zezas, I. Leonidaki
We present new diagnostic tools for distinguishing supernova remnants (SNRs) from HII regions. Up to now, sources with flux ratio [S II]/H higher than 0.4 have been considere…
Multi-wavelength structure analysis of local cluster galaxies. The WINGS project
A. Psychogyios, M. Vika, V. Charmandaris +6
We present a multi-wavelength analysis of the galaxies in nine clusters selected from the WINGS dataset, examining how galaxy structure varies as a function of wavelength and envir…
The presence of interstellar scintillation in the 15 GHz interday variability of 1158 OVRO-monitored blazars
J. Y. Koay, D. L. Jauncey, T. Hovatta +8
We have conducted the first systematic search for interday variability in a large sample of extragalactic radio sources at 15 GHz. From the sample of 1158 radio-selected blazars mo…
Local Bubble contribution to the 353-GHz dust polarized emission
R. Skalidis, V. Pelgrims
It has not been shown so far whether the diffuse Galactic polarized emission at frequencies relevant for cosmic microwave background (CMB) studies originates from nearby or more di…
SOFIA/HAWC+ traces the magnetic fields in NGC 1068
E. Lopez-Rodriguez, C. D. Dowell, T. J. Jones +21
We report the first detection of galactic spiral structure by means of thermal emission from magnetically aligned dust grains. Our 89 m polarimetric imaging of NGC 1068 with the…
A Very Large Array Survey of Luminous Extranuclear Star-forming Regions in Luminous Infrared Galaxies in GOALS
S. T. Linden, Y. Song, A. S. Evans +13
We present the first results of a high-resolution Karl G. Jansky Very Large Array (VLA) imaging survey of luminous and ultra-luminous infrared galaxies (U/LIRGs) in the Great Obser…
Robust Identification of Active Galactic Nuclei through HST Optical Variability in GOODS-S: Comparison with the X-ray and mid-IR Selected Samples
E. Pouliasis, I. Georgantopoulos, A. Z. Bonanos +9
Identifying Active Galactic Nuclei (AGNs) through their X-ray emission is efficient, but necessarily biased against X-ray-faint objects. We aim to characterize this bias by compari…
X-ray Binary Luminosity Function Scaling Relations for Local Galaxies Based on Subgalactic Modeling
Bret D. Lehmer, Rafael T. Eufrasio, Panayiotis Tzanavaris +7
We present new Chandra constraints on the X-ray luminosity functions (XLFs) of X-ray binary (XRB) populations, and their scaling relations, for a sample of 38 nearby galaxies (D =…
Hot Dust-Obscured Galaxies with Excess Blue Light
R. J. Assef, M. Brightman, D. J. Walton +10
Hot Dust-Obscured Galaxies (Hot DOGs) are among the most luminous galaxies in the Universe. Powered by highly obscured, possibly Compton-thick, active galactic nuclei (AGNs), Hot D…
The far-infrared polarization spectrum of Rho Ophiuchi A from HAWC+/SOFIA observations
Fabio P. Santos, David T. Chuss, C. Darren Dowell +23
We report on polarimetric maps made with HAWC+/SOFIA toward Rho Oph A, the densest portion of the Rho Ophiuchi molecular complex. We employed HAWC+ bands C (89 m) and D (154 …
Extreme Starlight Polarization in a Region with Highly Polarized Dust Emission
G. V. Panopoulou, B. S. Hensley, R. Skalidis +2
Galactic dust emission is polarized at unexpectedly high levels, as revealed by Planck. The origin of the observed polarization fractions can be identified by charact…
The core and stellar mass functions in massive collapsing filaments
Evangelia Ntormousi, Patrick Hennebelle
The connection between the pre-stellar core mass function (CMF) and the stellar initial mass function (IMF) lies at the heart of all star formation theories. In this paper, we stud…