Results 81 to 90 of about 657,244 (303)

Compliant Robotics in Space: A Prospective Review of Soft and Deformable Systems for Space Missions

Advanced Intelligent Systems, EarlyView.
Compliant robots are increasingly becoming integral to space exploration due to their adaptability, flexibility, and lightweight design. This article reviews categories such as soft, reconfigurable, and hyper‐redundant robots and their evolving role in enhancing space missions.
Hamed Rahimi Nohooji, Holger Voos
wiley   +1 more source

Towards understanding the Planck thermal dust models

, 2017
Understanding the properties of dust emission in the microwave domain is an important premise for the next generation of cosmic microwave background (CMB) experiments, devoted to the measurement of the primordial $B$-modes of polarization. In this paper,
Liu, Hao, Naselsky, Pavel, von Hausegger, Sebastian   +2 more
core   +1 more source

Is Phenylnitrene a Missing Link in the Formation of Polycyclic Aromatic Nitrogen Heterocycles?

Angewandte Chemie International Edition, Accepted Article.
The incorporation of heteroatoms into the framework of polycyclic aromatic hydrocarbons (PAHs), in particular of nitrogen to yield polycyclic aromatic nitrogen heterocycles (PANHs), has been proposed for both astronomical and combustion environments, but no suitable precursors and pathways have been found.
Rahel Arns, Rory McClish, Patrick Hemberger, Andras Bodi, Jordy Bouwman, Tina Kasper, Domenik Schleier   +6 more
wiley   +1 more source

Laboratory Study of Dust Mobilization on Airless Planetary Bodies in the Solar Wind Plasma

The Planetary Science Journal
Dust charging, and the subsequent mobilization and transport, have been suggested to explain a number of unresolved and unusual features observed on airless planetary surfaces.
A. Cabra, X. Wang, M. Horányi
doaj   +1 more source

First Constraints on Dense Molecular Gas at z = 7.5149 from the Quasar Pōniuā‘ena

The Astrophysical Journal Letters, 2023
We report the detection of CO(6–5) and CO(7–6) and their underlying continua from the host galaxy of quasar J100758.264+211529.207 (Pōniuā‘ena) at z = 7.5149, obtained with the NOrthern Extended Millimeter Array.
Chiara Feruglio, Umberto Maio, Roberta Tripodi, Jan Martin Winters, Luca Zappacosta, Manuela Bischetti, Francesca Civano, Stefano Carniani, Valentina D’Odorico, Fabrizio Fiore, Simona Gallerani, Michele Ginolfi, Roberto Maiolino, Enrico Piconcelli, Rosa Valiante, Maria Vittoria Zanchettin   +15 more
doaj   +1 more source

The Distortion of the Cosmic Microwave Background Spectrum Due to Intergalactic Dust [PDF]

, 2016
Infrared emission from intergalactic dust might compromise the ability of future experiments to detect subtle spectral distortions in the Cosmic Microwave Background (CMB) from the early Universe. We provide the first estimate of foreground contamination of the CMB signal due to diffuse dust emission in the intergalactic medium.
arxiv   +1 more source

Galaxy And Mass Assembly (GAMA): the 0.013 < z < 0.1 cosmic spectral energy distribution from 0.1 m to 1 mm [PDF]

, 2012
We use the Galaxy And Mass Assembly survey (GAMA) I data set combined with GALEX, Sloan Digital Sky Survey (SDSS) and UKIRT Infrared Deep Sky Survey (UKIDSS) imaging to construct the low-redshift (z < 0.1) galaxy luminosity functions in FUV, NUV, ugriz ...
A. M. Hopkins, A. S. G. Robotham, A. W. Graham, B. Madore, C. C. Popescu, C. J. Conselice, C. S. Frenk, D. H. Jones, D. T. Hill, D. Thomas, D. Wijesinghe, E. Andrae, E. Cameron, E. N. Taylor, E. van Kampen, H. R. Parkinson, I. K. Baldry, J. A. Peacock, J. Bland-Hawthorn, J. Liske, J. Loveday, K. A. Pimbblet, K. Kuijken, Kroupa, L. Dunne, L. Kelvin, M. Alpaslan, M. Brown, M. Colless, M. Gunawardhana, M. Prescott, M. Seibert, N. Bourne, P. Norberg, R. C. Nichol, R. G. Sharp, R. J. Tuffs, S. Brough, S. M. Croom, S. P. Bamford, S. P. Driver, S. Phillipps, S. Wilkins, W. J. Sutherland   +43 more
core   +3 more sources

Redshift‐Agnostic Machine Learning Classification: Unveiling Peak Performance in Galaxy, Star, and Quasar Classification (Using SDSS DR17)

Astronomische Nachrichten, EarlyView.
ABSTRACT Classification of galaxies, stars, and quasars using spectral data is fundamental to astronomy, but often relies heavily on redshift. This study evaluates the performance of 10 machine learning algorithms on SDSS data to classify these objects, with a particular focus on scenarios where redshift information is unavailable.
Debashis Chatterjee, Prithwish Ghosh
wiley   +1 more source

Illuminating the Dark Side of Cosmic Star Formation. II. A Second Date with RS-NIRdark Galaxies in COSMOS

The Astrophysical Journal, 2023
About 12 billion years ago, the Universe was first experiencing light again after the dark ages, and galaxies filled the environment with stars, metals, and dust. How efficient was this process? How fast did these primordial galaxies form stars and dust?
Meriem Behiri, Margherita Talia, Andrea Cimatti, Andrea Lapi, Marcella Massardi, Andrea Enia, Cristian Vignali, Matthieu Bethermin, Andreas Faisst, Fabrizio Gentile, Marika Giulietti, Carlotta Gruppioni, Francesca Pozzi, Vernesa Smolçić, Gianni Zamorani   +14 more
doaj   +1 more source

GAMA/G10-COSMOS/3D-HST: the 0 < z < 5 cosmic star formation history, stellar-mass, and dust-mass densities [PDF]

, 2017
We use the energy-balance code MAGPHYS to determine stellar and dust masses, and dust corrected star-formation rates for over 200,000 GAMA galaxies, 170,000 G10-COSMOS galaxies and 200,000 3D-HST galaxies.
S. Driver, S. Andrews, E. D. Cunha, L. Davies, C. Lagos, A. Robotham, K. Vinsen, A. Wright, M. Alpaslan, J. Bland-Hawthorn, N. Bourne, S. Brough, M. Bremer, M. Cluver, M. Colless, C. Conselice, L. Dunne, S. Eales, H. Gomez, B. Holwerda, A. Hopkins, P. Kafle, L. Kelvin, J. Loveday, J. Liske, S. Maddox, S. Phillipps, K. Pimbblet, K. Rowlands, A. Sansom, E. Taylor, Lingyu Wang, S. Wilkins   +32 more
semanticscholar   +1 more source