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Updates: 24 Mar 2017

WE HAVE MOVED!
(to our own server)
arxiver.moonhats.com

Handy tip: how to pre-select figures

To specify which figures you want to appear alongside your paper, please leave a comment in any .tex file before uploading to arXiv, as in this example:

%@arxiver{fig1.pdf,fig4.png,fig15.eps}

Note: do *not* include the path to the figure (just the name and extension) – the arXiver code will find nested figures automatically. See the FAQ for more details!

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Cosmology and Extragalactic Astrophysics
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Earth and Planetary Astrophysics
Galaxy Astrophysics
High Energy Astrophysical Phenomena
Instrumentation and Methods for Astrophysics
Solar and Stellar Astrophysics
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Applications Astrophysics of Galaxies Atmospheric and Oceanic Physics Atomic and Molecular Clusters Atomic Physics Chaotic Dynamics Chemical Physics Classical Physics Computational Physics Computer Vision and Pattern Recognition Cosmology and Extragalactic Astrophysics Cosmology and Nongalactic Astrophysics Data Analysis, Statistics and Probability Digital Libraries Distributed, Parallel, and Cluster Computing Dynamical Systems Earth and Planetary Astrophysics Fluid Dynamics Galaxy Astrophysics General Relativity and Quantum Cosmology Geophysics High Energy Astrophysical Phenomena High Energy Physics - Experiment High Energy Physics - Lattice High Energy Physics - Phenomenology High Energy Physics - Theory History and Philosophy of Physics Information Theory Instrumentation and Detectors Instrumentation and Methods for Astrophysics Learning Machine Learning Materials Science Mathematical Physics Methodology Nuclear Experiment Nuclear Theory Numerical Analysis Optics Other Condensed Matter Physics and Society Physics Education Plasma Physics Popular Physics Quantum Gases Quantum Physics Solar and Stellar Astrophysics Space Physics Statistical Mechanics Superconductivity

Top Posts & Pages

X-ray Insights into the Nature of PHL 1811 Analogs and Weak Emission-Line Quasars: Unification with a Geometrically Thick Accretion Disk? [GA]
The blazar sequence 2.0 [HEAP]
HST Imaging of Fading AGN Candidates I: Host-Galaxy Properties and Origin of the Extended Gas [GA]
Cosmological constraints on the radiation released during structure formation [CEA]
Kompaneets Model Fitting of the Orion-Eridanus Superbubble II: Thinking Outside of Barnard's Loop [GA]
Software Polarization Spectrometer "PolariS" [IMA]
The Mean Metal-line Absorption Spectrum of Damped Lyman Alpha Systems in BOSS [GA]
James Webb Space Telescope Optical Simulation Testbed II. Design of a Three-Lens Anastigmat Telescope Simulator [IMA]
Discovery of the most metal-poor damped Lyman-alpha system [CEA]
The Origin of Ionized Filaments Within the Orion-Eridanus Superbubble [CL]

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