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</div> <div class="control"> <button class="button is-small is-link">Go</button> </div> </div> </form> </div> </div> <ol class="breathe-horizontal" start="1"> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2308.10085">arXiv:2308.10085</a> <span> [<a href="https://arxiv.org/pdf/2308.10085">pdf</a>, <a href="https://arxiv.org/ps/2308.10085">ps</a>, <a href="https://arxiv.org/format/2308.10085">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Chemical Physics">physics.chem-ph</span> </div> </div> <p class="title is-5 mathjax"> Analysis of the calculated X-X ro-vibrational transition intensities in molecular hydrogen </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Ushakov%2C+V+G">V. G. Ushakov</a>, <a href="/search/physics?searchtype=author&query=Balashev%2C+S+A">S. A. Balashev</a>, <a href="/search/physics?searchtype=author&query=Medvedev%2C+E+S">E. S. Medvedev</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2308.10085v1-abstract-short" style="display: inline;"> The potential-energy and quadrupole-moment functions of the H$_2$ ground electronic state are well known in literature (Komasa et al., 2019; Wolniewicz et al., 1998), and the line list of the vibrational-rotational transitions was calculated (Roueff et al., 2019). In this paper, we analyze the calculated intensities in order to learn how the intensities will change when analytic quadrupole-moment… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2308.10085v1-abstract-full').style.display = 'inline'; document.getElementById('2308.10085v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2308.10085v1-abstract-full" style="display: none;"> The potential-energy and quadrupole-moment functions of the H$_2$ ground electronic state are well known in literature (Komasa et al., 2019; Wolniewicz et al., 1998), and the line list of the vibrational-rotational transitions was calculated (Roueff et al., 2019). In this paper, we analyze the calculated intensities in order to learn how the intensities will change when analytic quadrupole-moment functions fitted to the ab initio and experimental data are used instead of spline-interpolated functions. We found that the use of splines does not deteriorate the intensities and does not lead to nonphysical saturation, as in heavier molecules, owing to the high precision of the ab initio data and the high density of the grid. The accuracy of the calculated intensities is estimated up to high overtones. Extraction of new spectroscopic information from the observational data that supplements the laboratory measurements is performed. The laboratory and observational data do not help increase the quality of the analytic functions. Numerous anomalies resulting from the destructive interference are identified in the calculated line lists, some of them being situated within the recently observed spectral regions, 1.5-2.5 $渭$m. The intensities of these anomalies can be sensitive to the form of the molecular functions as well as to the proton-to-electron mass ratio. In this connection, the similar Le Roy anomalies (Brown and LeRoy, 1973; Le Roy and Vrscay, 1975) also arising due to the destructive interference in the Lyman and Werner systems are discussed. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2308.10085v1-abstract-full').style.display = 'none'; document.getElementById('2308.10085v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 19 August, 2023; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> August 2023. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2208.01672">arXiv:2208.01672</a> <span> [<a href="https://arxiv.org/pdf/2208.01672">pdf</a>, <a href="https://arxiv.org/format/2208.01672">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Methods for Astrophysics">astro-ph.IM</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> </div> <p class="title is-5 mathjax"> CUBES, the Cassegrain U-Band Efficient Spectrograph </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Cristiani%2C+S">S. Cristiani</a>, <a href="/search/physics?searchtype=author&query=Alcal%C3%A1%2C+J+M">J. M. Alcal谩</a>, <a href="/search/physics?searchtype=author&query=Alencar%2C+S+H+P">S. H. P. Alencar</a>, <a href="/search/physics?searchtype=author&query=Balashev%2C+S+A">S. A. Balashev</a>, <a href="/search/physics?searchtype=author&query=Bastian%2C+N">N. Bastian</a>, <a href="/search/physics?searchtype=author&query=Barbuy%2C+B">B. Barbuy</a>, <a href="/search/physics?searchtype=author&query=Battino%2C+U">U. Battino</a>, <a href="/search/physics?searchtype=author&query=Calcines%2C+A">A. Calcines</a>, <a href="/search/physics?searchtype=author&query=Calderone%2C+G">G. Calderone</a>, <a href="/search/physics?searchtype=author&query=Cambianica%2C+P">P. Cambianica</a>, <a href="/search/physics?searchtype=author&query=Carini%2C+R">R. Carini</a>, <a href="/search/physics?searchtype=author&query=Carter%2C+B">B. Carter</a>, <a href="/search/physics?searchtype=author&query=Cassisi%2C+S">S. Cassisi</a>, <a href="/search/physics?searchtype=author&query=Castilho%2C+B+V">B. V. Castilho</a>, <a href="/search/physics?searchtype=author&query=Cescutti%2C+G">G. Cescutti</a>, <a href="/search/physics?searchtype=author&query=Christlieb%2C+N">N. Christlieb</a>, <a href="/search/physics?searchtype=author&query=Cirami%2C+R">R. Cirami</a>, <a href="/search/physics?searchtype=author&query=Coretti%2C+I">I. Coretti</a>, <a href="/search/physics?searchtype=author&query=Cooke%2C+R">R. Cooke</a>, <a href="/search/physics?searchtype=author&query=Covino%2C+S">S. Covino</a>, <a href="/search/physics?searchtype=author&query=Cremonese%2C+G">G. Cremonese</a>, <a href="/search/physics?searchtype=author&query=Cunha%2C+K">K. Cunha</a>, <a href="/search/physics?searchtype=author&query=Cupani%2C+G">G. Cupani</a>, <a href="/search/physics?searchtype=author&query=da+Silva%2C+A+R">A. R. da Silva</a>, <a href="/search/physics?searchtype=author&query=De+Caprio%2C+V">V. De Caprio</a> , et al. (52 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2208.01672v1-abstract-short" style="display: inline;"> In the era of Extremely Large Telescopes, the current generation of 8-10m facilities are likely to remain competitive at ground-UV wavelengths for the foreseeable future. The Cassegrain U-Band Efficient Spectrograph (CUBES) has been designed to provide high-efficiency (>40%) observations in the near UV (305-400 nm requirement, 300-420 nm goal) at a spectral resolving power of R>20,000 (with a lowe… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2208.01672v1-abstract-full').style.display = 'inline'; document.getElementById('2208.01672v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2208.01672v1-abstract-full" style="display: none;"> In the era of Extremely Large Telescopes, the current generation of 8-10m facilities are likely to remain competitive at ground-UV wavelengths for the foreseeable future. The Cassegrain U-Band Efficient Spectrograph (CUBES) has been designed to provide high-efficiency (>40%) observations in the near UV (305-400 nm requirement, 300-420 nm goal) at a spectral resolving power of R>20,000 (with a lower-resolution, sky-limited mode of R ~ 7,000). With the design focusing on maximizing the instrument throughput (ensuring a Signal to Noise Ratio (SNR) ~20 per high-resolution element at 313 nm for U ~18.5 mag objects in 1h of observations), it will offer new possibilities in many fields of astrophysics, providing access to key lines of stellar spectra: a tremendous diversity of iron-peak and heavy elements, lighter elements (in particular Beryllium) and light-element molecules (CO, CN, OH), as well as Balmer lines and the Balmer jump (particularly important for young stellar objects). The UV range is also critical in extragalactic studies: the circumgalactic medium of distant galaxies, the contribution of different types of sources to the cosmic UV background, the measurement of H2 and primordial Deuterium in a regime of relatively transparent intergalactic medium, and follow-up of explosive transients. The CUBES project completed a Phase A conceptual design in June 2021 and has now entered the detailed design and construction phase. First science operations are planned for 2028. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2208.01672v1-abstract-full').style.display = 'none'; document.getElementById('2208.01672v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 2 August, 2022; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> August 2022. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">SPIE proceedings, SPIE Astronomical Telescopes + Instrumentation 2022, Montr茅al, Canada; 20 pages, 13 figures, 2 tables</span> </p> </li> </ol> <div class="is-hidden-tablet">  <span class="help" style="display: inline-block;"><a href="https://github.com/arXiv/arxiv-search/releases">Search v0.5.6 released 2020-02-24</a>  </span> </div> </div> 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