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Dataset results
6 results for “masers”
Simulation results: Radiative cooling induced coherent maser emission in relativistic plasmas
<p>This repository contains some of the simulation data presented in the recent article titled <em>"Radiative cooling induced coherent maser emission in relativistic plasmas"</em> (<a href="https://arxiv.org/abs/2409.18955" target="_new" rel="noopener">https://arxiv.org/abs/2409.18955</a>). The data available are from 2D particle-in-cell (PIC) simulations, which investigate the effects of radiative cooling in relativistic plasmas and its role in inducing coherent maser emission. The simulations were performed using OSIRIS, a massively parallel and fully-relativistic PIC code.</p> <p>The electric field data in the third direction (E3) included here has been spatially averaged by a factor of 8 in both directions, resulting in a dataset that reflects a resolution 64 times lower than the actual simulation. Additionally, the raw data includes only one two-thousandth of the simulated electron macro-particles. Also included is the phase space data in the x2, p2, and p3 dimensions.</p> <p>These datasets represent key aspects of the simulation results discussed in the paper, where the focus is on understanding the interplay between radiative losses and coherent emission mechanisms.</p> <p>More details on the simulations and the analysis of these results can be found in the corresponding article.</p>
Evolutionary Map of the Universe (EMU): discovering 18-cm OH maser sources in ASKAP continuum images of the SCORPIO field
<p>Data cubes and spectra from the ATCA C3414 project.</p> <p>Data cubes are in fits format.</p> <p>Spectra were extracted from the data cubes following what described in the text. The format is the standard output of the CASA profile tools. Each spectrum contains an header with the column description.</p>
Figures and Data Set of "The Effelsberg survey of FU Orionis and EX Lupi objects II. - H2O maser observations"
<p>This is the full version of the fits files for each source with H2O maser detection for the paper "The Effelsberg survey of FU Orionis and EX Lupi objects II. - H2O maser observations”.<br>We also provide the figures from the paper. </p> <p>The paper is published in Astronomy & Astrophysics, and can be found at: https://doi.org/10.1051/0004-6361/202245032</p> <p>The fits files are given for each source and for each observing date. For the data behind Figure 4, we also provide the multiplied data for V512 Per. The units are in Jy in all cases.</p> <p> </p>
All-metallic magnetic Purcell enhancement in a thermally stable room-temperature maser
<p>This contains the experimental raw data:</p><ul><li>Model_SRRcluster.stl<ul><li>the 3D model of the clustered SRR<br> </li></ul></li><li>01_SRRcluster_ThersholdExperiment_RawData<ul><li>1,300 maser pulses recorded by oscilloscope along with gradually increased laser excitation energy</li><li>corresponding laser excitation energy</li><li>S11 parameter of the resonator measured using vector network analyzer (VNA)<br> </li></ul></li><li>02_SRRcluster_ThermalStabilityExperiment_RawData<ul><li>18,000 maser pulses recorded by oscilloscope:</li><li>corresponding laser excitation energy</li><li>S11 parameters of the resonator before and after the masing experiment, measured using vector network analyzer (VNA)<br> </li></ul></li><li>03_SrTiO3_ThermalStabilityExperiment_RawData<ul><li>12,000 maser pulses recorded by oscilloscope:</li><li>corresponding laser excitation energy</li><li>S11 parameters of the resonator before and after the masing experiment, measured using vector network analyzer (VNA)</li></ul></li></ul><p> </p>
Appendix A: Spectra of nine methanol maser transitions for all observed 408 ATLASGAL sources
<p>This is the full version of Appendix A for the paper: ATLASGAL: 3-mm class I methanol masers in high-mass star formation regions<br> <br> </p>
OH Maser toward IRAS06056+2131: Polarization parameters and evolution status
<p>Data used in the manuscript "OH Maser toward IRAS06056+2131:Polarization parameters and evolution status" submitted to MNRAS</p>
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