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The Hi-GAL compact source catalogue – I. The physical properties of the clumps in the inner Galaxy (−71$_{.}^{\circ}$0 < ℓ < 67$_{.}^{\circ}$0) / Elia, Davide (INAF, Rome) ; Molinari, S. (INAF, Rome) ; Schisano, E. (INAF, Rome) ; Pestalozzi, M. (INAF, Rome) ; Pezzuto, S. (INAF, Rome) ; Merello, M. (INAF, Rome) ; Noriega-Crespo, A. (Baltimore, Space Telescope Sci.) ; Moore, T.J. T. (Liverpool John Moores U., ARI) ; Russeil, D. (Marseille, Lab. Astrophys.) ; Mottram, J.C. (Heidelberg, Max Planck Inst. Astron.) et al.
Hi-GAL is a large-scale survey of the Galactic plane, performed with Herschel in five infrared continuum bands between 70 and 500 $\mu$m. We present a band-merged catalogue of spatially matched sources and their properties derived from fits to the spectral energy distributions (SEDs) and heliocentric distances, based on the photometric catalogs presented in Molinari et al. [...]
arXiv:1706.01046.- 2017 - 44 p. - Published in : Mon. Not. R. Astron. Soc. 471 (2017) 100-143 Fulltext: PDF;

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(91)

Spatial distribution of star formation related to ionized regions throughout the inner Galactic plane / Palmeirim, P. (Marseille, Lab. Astrophys. ; Porto U., Astron. Dept.) ; Zavagno, A. (Marseille, Lab. Astrophys.) ; Elia, D. (INAF, Rome) ; Moore, T.J. T. (Liverpool John Moores U., ARI) ; Whitworth, A. (Cardiff U.) ; Tremblin, P. (MdlS, Saclay) ; Traficante, A. (INAF, Rome) ; Merello, M. (INAF, Rome) ; Russeil, D. (Marseille, Lab. Astrophys.) ; Pezzuto, S. (INAF, Rome) et al.
We present a comprehensive statistical analysis of star-forming objects located in the vicinities of 1 360 bubble structures throughout the Galactic Plane and their local environments. The compilation of ~70 000 star-forming sources, found in the proximity of the ionized (Hii) regions and detected in both Hi-GAL and GLIMPSE surveys, provided a broad overview of the different evolutionary stages of star-formation in bubbles, from prestellar objects to more evolved young stellar objects (YSOs). [...]
arXiv:1705.09877.- 2017-09-05 - 14 p. - Published in : Astron. Astrophys. 605 (2017) A35 Fulltext: PDF;

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(41)

First detection of the Crab Nebula at TeV energies with a Cherenkov telescope in dual-mirror Schwarzschild-Couder configuration: the ASTRI-Horn telescope / Lombardi, S. (Rome Observ. ; ASDC, Frascati) ; Catalano, O. (IASF, Palermo) ; Scuderi, S. (IASF, Milan) ; Antonelli, L.A. (Rome Observ. ; ASDC, Frascati) ; Pareschi, G. (Brera Observ.) ; Antolini, E. (Bologna Observ.) ; Arrabito, L. (U. Montpellier 2, LUPM) ; Bellassai, G. (Catania Astrophys. Observ.) ; Bernlöhr, K. (Heidelberg, Max Planck Inst.) ; Bigongiari, C. (Rome Observ.) et al.
We report on the first detection of very high-energy (VHE) gamma-ray emission from the Crab Nebula by a Cherenkov telescope in dual-mirror Schwarzschild-Couder (SC) configuration. The result has been achieved by means of the 4 m size ASTRI-Horn telescope, operated on Mt. [...]
arXiv:1909.12149.- 2020-02-01 - 6 p. - Published in : Astron. Astrophys. 634 (2020) A22 Fulltext: PDF;

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(30)

Euclid preparation. Sensitivity to non-standard particle dark matter model / Euclid Collaboration
The Euclid mission of the European Space Agency will provide weak gravitational lensing and galaxy clustering surveys that can be used to constrain the standard cosmological model and its extensions, with an opportunity to test the properties of dark matter beyond the minimal cold dark matter paradigm. [...]
arXiv:2406.18274 ; TTK-24-26. - 31.
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(29)

An accurate solar axions ray-tracing response of BabyIAXO / IAXO collaboration
BabyIAXO is the intermediate stage of the International Axion Observatory (IAXO) to be hosted at DESY. [...]
arXiv:2411.13915. - 39.
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(29)

First joint observation by the underground gravitational-wave detector KAGRA with GEO 600 / KAGRA Collaboration
We report the results of the first joint observation of the KAGRA detector with GEO600. KAGRA is a cryogenic and underground gravitational-wave detector consisting of a laser interferometer with three-kilometer arms, and located in Kamioka, Gifu, Japan. [...]
arXiv:2203.01270; LIGO-P2100286.- 2022-06-14 - 37 p. - Published in : PTEP 2022 (2022) 063F01 Fulltext: 2203.01270 - PDF; document - PDF;

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(26)

Search for Subsolar-Mass Binaries in the First Half of Advanced LIGO’s and Advanced Virgo’s Third Observing Run / LIGO Scientific Collaboration
We report on a search for compact binary coalescences where at least one binary component has a mass between 0.2 $M_\odot$ and 1.0 $M_\odot$ in Advanced LIGO and Advanced Virgo data collected between 1 April 2019 1500 UTC and 1 October 2019 1500 UTC. We extend previous analyses in two main ways: we include data from the Virgo detector and we allow for more unequal mass systems, with mass ratio $q \geq 0.1$. [...]
arXiv:2109.12197; LIGO-P2100163-v8.- 2022-08-05 - 16 p. - Published in : Phys. Rev. Lett. 129 (2022) 061104 Fulltext: PDF;

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(24)

Euclid. IV. The NISP Calibration Unit / Euclid Collaboration
The near-infrared calibration unit (NI-CU) on board Euclid's Near-Infrared Spectrometer and Photometer (NISP) is the first astronomical calibration lamp based on light-emitting diodes (LEDs) to be operated in space. [...]
arXiv:2405.13494. - 21.
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(23)

Dark Matter searches using gravitational wave bar detectors: quark nuggets and newtorites / ROG collaboration
Many experiments have searched for supersymmetric WIMP dark matter, with null results. This may suggest to look for more exotic possibilities, for example compact ultra-dense quark nuggets, widely discussed in literature with several different names. [...]
arXiv:1512.06249.- 2016 - Published in : Astropart. Phys. 78 (2016) 52-64 External link: Preprint

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(22)

Euclid. I. Overview of the Euclid mission / Euclid Collaboration
The current standard model of cosmology successfully describes a variety of measurements, but the nature of its main ingredients, dark matter and dark energy, remains unknown. [...]
arXiv:2405.13491. - 94.
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