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6 results for “2422”
Rhamnus sp. from Colombia collected by W. López #2422
<p><strong>File Name</strong>: <span>TOLI-27705-MTV-01-B4-364.jpg</span></p> <p><strong>CÓDIGO FOTO</strong>: <span>TOLI-27705-MTV-01-B4-364</span></p> <p><strong>Nº TOLI</strong>: <span>TOLI-27705</span></p> <p><strong>PARCELA</strong>: <span>MTV-01</span></p> <p><strong>CÓDIGO</strong>: <span>B4-</span></p> <p><strong>Nº COLECTA</strong>: <span>2422</span></p> <p><strong>COLECTORES</strong>: <span>W. López </span></p> <p><strong>Nº MUESTRAS MONTADAS</strong>: <span>1</span></p> <p><strong>Homologación</strong>: <span>Homologado</span></p> <p><strong>Fecha del evento</strong>: <span>04/12/2018.</span></p> <p><strong>Proyecto </strong>: <span>Recursos Botánicos Disponibles en Línea (BRAVO) para la flora colombiana</span></p> <p><strong>Continente</strong>: <span>SA</span></p> <p><strong>Pais</strong>: <span>Colombia</span></p> <p><strong>Estado/Provincia</strong>: <span>Antioquia</span></p> <p><strong>Municipio</strong>: <span>Medellín</span></p> <p><strong>Centro poblado / Cabecera municipal</strong>: <span>Reserva Montevivo</span></p> <p><strong>Elevación minima en metros</strong>: <span>2300</span></p> <p><strong>Elevación maxima en metros</strong>: <span>2600</span></p> <p><strong>Latitud</strong>: <span>6.208312</span></p> <p><strong>Longitud original</strong>: <span>-75.491112</span></p> <p><strong>datum geodésico</strong>: <span>WGS 84</span></p> <p><strong>Latitud decimal</strong>: <span>6.208312</span></p> <p><strong>Longitud decimal</strong>: <span>-75.491112</span></p> <p><strong>Identificado por</strong>: <span>L. Corrales</span></p> <p><strong>Fecha de identificación</strong>: <span>1/10/2019.</span></p> <p><strong>Familia antigua</strong>: <span>Rhamnaceae</span></p> <p><strong>Especie antigua</strong>: <span>Rhamnus goudotiana Triana & Planch.</span></p> <p><strong>Nombre cientifico</strong>: <span>Rhamnus sp.</span></p> <p><strong>Reino</strong>: <span>Plantae</span></p> <p><strong>Filo</strong>: <span>Magnoliophyta</span></p> <p><strong>Clase</strong>: <span>Equisetopsida</span></p> <p><strong>Familia nueva</strong>: <span>Rhamnaceae</span></p> <p><strong>Género nuevo</strong>: <span>Rhamnus</span></p> <p><strong>especie nueva</strong>: <span>sp.</span></p> <p><strong>genero herbario</strong>: <span>Rhamnus</span></p> <p><strong>especie herbario</strong>: <span>sp.</span></p> <p><strong>Especie de herbario para TNRS</strong>: <span>Rhamnus sp.</span></p> <p><strong>Especie corregida herbario y desde TNRS</strong>: <span>Rhamnus indet</span></p> <p><strong>Familia corregida desde TNRS</strong>: <span>Rhamnaceae</span></p> <p><strong></strong>: <span>156</span></p>
Rotational spectroscopy of CH3OD with a re-analysis of CH3OD toward IRAS 16293 - 2422
<p>Supplementary material for the article 'Rotational spectroscopy of CH3OD with a re-analysis of CH3OD toward IRAS 16293 - 2422' by V.V. Ilyushin, H.S.P. Muller, M.N. Drozdovskaya, J.K. Jorgensen, S. Bauerecker, C. Maul, R. Porohovoi, E.A. Alekseev, O. Dorovskaya, O. Zakharenko, F. Lewen, S. Schlemmer, L.-H. Xu, and R.M. Lees accepted for publication by Astronomy and Astrophysics.</p> <p>ADC_Keywords: Interstellar medium; Spectra, millimetric/submm; Spectroscopy</p> <p>Keywords: Molecular data - Methods: laboratory: molecular - Techniques: <br>spectroscopic - ISM: molecules - Astrochemistry - ISM: individual objects: <br>IRAS 16293 - 2422</p> <p>Abstract:</p> <p>We have started a measurement campaign of numerous methanol isotopologs in <br>low-lying torsional states in order to provide extensive line lists for radio <br>astronomical observations from an adequate spectroscopic model and to <br>investigate how the intricate vibration-torsion-rotation interactions manifest <br>themselves in the spectra of different isotopic species. After CD3OH and CD3OD, <br>we turn our focus to CH3OD, which is an important species for studying <br>deuteration in prestellar cores and envelopes that enshroud protostars. <br>Deuteration, in turn, is frequently viewed as a diagnostic tool for star <br>formation. The present measurements were obtained in two spectroscopic <br>laboratories and cover large fractions of the 34 GHz-1.35 THz range. We <br>employed a torsion-rotation Hamiltonian model for our analysis that is based <br>on the rho-axis method as in previous studies. The resulting model describes <br>the ground and first excited torsional states of CH3OD well up to quantum <br>numbers J </= 51 and Ka </= 18. We derived a line list for radio-astronomical<br>observations from this model that is accurate up to at least 1.35 THz and <br>should be sufficient for all types of radio astronomical searches for this <br>methanol isotopolog in these two lowest torsional states. This line list was <br>applied to a reinvestigation of CH3OD in data from the Protostellar <br>Interferometric Line Survey (PILS) of IRAS 16293-2422 obtained with the Atacama <br>Large Millimeter/submillimeter Array (ALMA). The new accurately determined <br>value for the column density of CH3OD implies that the deuteration in <br>methanol differs in its two functional groups by a factor of ~7.5.</p> <p><br>Description:<br>Table C1 contains assigned microwave transitions of the CH3OD spectrum used<br>in the analysis. Source of data: Khar - Kharkov spectrometer, present work;<br>Koln - Cologne spectrometers, present work; for other source codes (B, C, D, <br>E, L, T, W) see Duan, Y. B., Ozier, I., Tsunekawa, S., & Takagi, K. 2003, <br>J. Mol. Spectrosc., 218, 95</p> <p>Table C2 contains assigned FIR transitions of the CH3OD spectrum used in<br>the analysis. Source of data: Mukhopadhyay, I. 2021, Infrared Phys. Technol., <br>116, 103605.</p> <p>Table C3 contains predicted transitions of the ground and first excited <br>torsional states of CH3OD in the frequency range from 1 GHz up to 2 THz <br>with J up to 55 and |Ka| up to 21. The m values 0/1 and -3/-2 correspond to <br>A/E transitions of the vt = 0 and 1 torsional states, respectively. We limit <br>our calculations to transitions for which uncertainties are less than 0.1 MHz.</p> <p>Table C4 contains torsion-rotation part Qrt(T) of the total internal partition <br>function Q(T)=Qv(T)*Qrt(T), calculated for CH3OD from first principles using <br>the parameter set of Table A.1. In the calculation the states up to J=65 and <br>vt=11 were included. The vibrational part Qv(T) (omitting the torsional <br>vibration since it is taken into account in Qrt) may be estimated in <br>the harmonic approximation using the vibrational frequencies reported <br>by T. Schimanouchi, Tables of Molecular Vibrational Frequencies, Vol. I: <br>consolidated (National Bureau of Standards, Washington, DC, 1972), pp. 1-160. </p> <p> </p> <p>File Summary:<br>-----------------------------------------------------------------------------------------------------------------------<br> FileName Lrecl Records Explanations<br>-----------------------------------------------------------------------------------------------------------------------<br>readme.txt 80 <br>tablec1.dat 75 11118 Assigned microwave transitions of the CH3OD <br> spectrum used in the analysis. <br>tablec2.dat 71 5465 Assigned FIR transitions of the CH3OD spectrum <br> used in the analysis. <br>tablec3.dat 87 25111 Predicted transition frequencies of the ground and <br> first excited torsional states of CH3OD in the <br> frequency range from 1 GHz up to 2 THz.<br>tablec4.dat 16 30 Torsion-rotation part Qrt(T) of the total internal <br> partition function Q(T)=Qv(T)*Qrt(T), calculated <br> for CH3OD from first principles.<br>------------------------------------------------------------------------------------------------------------------------</p>
Trento 1936 - Building 2422
<u>Coordinates</u>: N/A <br><u>Length</u>: 12.62 m<br><u>Width</u>: 6.66 m<br><u>Height</u>: 9.35 m<br><u>Points</u>: 8 <br><u>Vertices</u>: 36 <br><u>Primitives</u>: 12 <br><br><u>Main Files:</u><br><table><tbody><tr><th>Filename</th><th>.glb</th><th>.xml</th><th>.obj</th></tr><tr><td><a href="https://zenodo.org/api/records/12693063/files/building_2422.obj/content">building_2422.obj</a></td><td></td><td></td><td><a href="https://zenodo.org/api/records/12693063/files/building_2422.obj/content">Link</a></td></tr><tr><td><a href="https://zenodo.org/api/records/12693063/files/building_2422.glb/content">building_2422.glb</a></td><td><a href="https://zenodo.org/api/records/12693063/files/building_2422.glb/content">Link</a></td><td></td><td></td></tr><tr><td><a href="https://zenodo.org/api/records/12693063/files/11575736_metsmods.xml/content">11575736_metsmods.xml</a></td><td></td><td><a href="https://zenodo.org/api/records/12693063/files/11575736_metsmods.xml/content">Link</a></td><td></td></tr><tr><td><a href="https://zenodo.org/api/records/12693063/files/11575736_edm.xml/content">11575736_edm.xml</a></td><td></td><td><a href="https://zenodo.org/api/records/12693063/files/11575736_edm.xml/content">Link</a></td><td></td></tr></tbody></table><br><br><u>Thumbnails:</u><br><table><tbody><tr><th>Perspective</th><th>1000x1000</th><th>512x512</th><th>256x256</th><th>128x128</th></tr><tr><td>Perspective 1</td><td><a href="https://zenodo.org/api/records/12693063/files/building_2422_perspective_1.png/content">Link</a></td><td><a href="https://zenodo.org/api/records/12693063/files/building_2422_perspective_1_512x512.png/content">Link</a></td><td><a href="https://zenodo.org/api/records/12693063/files/building_2422_perspective_1_256x256.png/content">Link</a></td><td><a href="https://zenodo.org/api/records/12693063/files/building_2422_perspective_1_128x128.png/content">Link</a></td></tr><tr><td>Perspective 2</td><td><a href="https://zenodo.org/api/records/12693063/files/building_2422_perspective_2.png/content">Link</a></td><td><a href="https://zenodo.org/api/records/12693063/files/building_2422_perspective_2_512x512.png/content">Link</a></td><td><a href="https://zenodo.org/api/records/12693063/files/building_2422_perspective_2_256x256.png/content">Link</a></td><td><a href="https://zenodo.org/api/records/12693063/files/building_2422_perspective_2_128x128.png/content">Link</a></td></tr><tr><td>Perspective 3</td><td><a href="https://zenodo.org/api/records/12693063/files/building_2422_perspective_3.png/content">Link</a></td><td><a href="https://zenodo.org/api/records/12693063/files/building_2422_perspective_3_512x512.png/content">Link</a></td><td><a href="https://zenodo.org/api/records/12693063/files/building_2422_perspective_3_256x256.png/content">Link</a></td><td><a href="https://zenodo.org/api/records/12693063/files/building_2422_perspective_3_128x128.png/content">Link</a></td></tr><tr><td>Perspective 4</td><td><a href="https://zenodo.org/api/records/12693063/files/building_2422_perspective_4.png/content">Link</a></td><td><a href="https://zenodo.org/api/records/12693063/files/building_2422_perspective_4_512x512.png/content">Link</a></td><td><a href="https://zenodo.org/api/records/12693063/files/building_2422_perspective_4_256x256.png/content">Link</a></td><td><a href="https://zenodo.org/api/records/12693063/files/building_2422_perspective_4_128x128.png/content">Link</a></td></tr><tr><td>Perspective Top</td><td><a href="https://zenodo.org/api/records/12693063/files/building_2422_perspective_top.png/content">Link</a></td><td><a href="https://zenodo.org/api/records/12693063/files/building_2422_perspective_top_512x512.png/content">Link</a></td><td><a href="https://zenodo.org/api/records/12693063/files/building_2422_perspective_top_256x256.png/content">Link</a></td><td><a href="https://zenodo.org/api/records/12693063/files/building_2422_perspective_top_128x128.png/content">Link</a></td></tr></tbody></table><br><br><br><u>Changelog</u>: <br> - v<a href="https://doi.org/10.5281/zenodo.12545183">0.0.2</a>: Thumbnails added, Description updated with Link Tables.<br> - v<a href="https://doi.org/10.5281/zenodo.12693063">0.0.3</a>: Added XMLs for Europeana Data Model (EDM) and MetsMods.<br>
IO Islamic 2422. Ḥabîb-alsiyar, General History, First Volume
<p>IO Islamic 2422. Ḥabîb-alsiyar, General History, First Volume</p>
Binary black-hole simulation SXS:BBH:2422
Simulation of a black-hole binary system evolved by the <a href="https://www.black-holes.org/code/SpEC.html">SpEC code</a>.
doi_dedup___::173015928a0eb610e4445cb9b02c2565
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