From 3ae8e0683c5a996ea56f9da6dfb9aa619f535ff6 Mon Sep 17 00:00:00 2001 From: Nimisha Kumari <69207026+nimishak-cosmos@users.noreply.github.com> Date: Tue, 2 Aug 2022 16:06:23 -0400 Subject: [PATCH] Added the file UV_linelist_vacuum.csv (#1522) * Added the file UV_linelist_vacuum.csv after a chat with Richard O steen as there were discrepancies in wavelengths of existing linelists. * Deleted the ._UV_linelist_vacuum.list. The UV_linelist_vacuum.csv is the file to be added. The information about this file is in the previous commit. * Add line metadata and changelog, remove Microsoft BOM character * Ignore generated file Co-authored-by: Ricky O'Steen Co-authored-by: P. L. Lim <2090236+pllim@users.noreply.github.com> --- .gitignore | 1 + CHANGES.rst | 2 + jdaviz/data/linelists/UV_linelist_vacuum.csv | 132 +++++++++++++++++++ jdaviz/data/linelists/linelist_metadata.json | 6 + 4 files changed, 141 insertions(+) create mode 100644 jdaviz/data/linelists/UV_linelist_vacuum.csv diff --git a/.gitignore b/.gitignore index 9d59eb7029..e804983ce8 100644 --- a/.gitignore +++ b/.gitignore @@ -53,6 +53,7 @@ distribute-*.tar.gz .tox .*.sw[op] *~ +._* .project .pydevproject .settings diff --git a/CHANGES.rst b/CHANGES.rst index a377ad1fba..8775e9a18d 100644 --- a/CHANGES.rst +++ b/CHANGES.rst @@ -59,6 +59,8 @@ Specviz Other Changes and Additions --------------------------- +- Added a UV Galactic linelist. [#1522] + 2.8 (2022-07-21) ================ diff --git a/jdaviz/data/linelists/UV_linelist_vacuum.csv b/jdaviz/data/linelists/UV_linelist_vacuum.csv new file mode 100644 index 0000000000..0c2e2b79a1 --- /dev/null +++ b/jdaviz/data/linelists/UV_linelist_vacuum.csv @@ -0,0 +1,132 @@ +Line Name,Rest Value +C I,1157.19 +N IV,1168.6 +C IV,1168.87 +C IV,1168.99 +N IV,1169.06 +N IV,1169.48 +C III,1175.53 +N III,1183.03 +N III,1184.54 +Mn II,1199.39 +N I,1199.55 +N I,1200.22 +N I,1200.71 +Si III,1206.5 +H I,1215.67 +N V,1238.82 +N V,1242.8 +C III,1247.38 +S II,1250.58 +S II,1253.81 +Si II,1260.42 +C I,1277.24 +Si III,1294.54 +C III,1296.33 +Si III,1296.74 +Si III,1298.93 +O I,1302.17 +Si II,1304.37 +Ni II,1317.22 +C II,1323.93 +N III,1324.35 +C I,1328.83 +C II,1334.53 +C II*,1335.71 +O IV,1341.64 +Fe V,1345.61 +Fe V,1362.86 +Fe V,1363.08 +Fe V,1364.82 +O V,1371.3 +Si IV,1393.76 +Si IV,1402.77 +Si III,1417.24 +C III,1426.45 +Fe V,1427.27 +C III,1427.85 +Fe V,1430.44 +Ni II,1454.84 +Co II,1466.21 +Ni II,1467.26 +Ni II,1467.76 +C III,1478 +N IV],1486.5 +S V,1501.76 +Si II,1526.71 +Fe IV,1530.04 +Si II*,1533.43 +C IV,1548.19 +C IV,1550.77 +C I,1560.31 +C I*,1560.68 +Fe II,1608.45 +Fe II,1611.2 +C III,1620.4 +He II,1640.42 +C I,1656.93 +C I*,1657.38 +C I*,1657.91 +O III],1660.81 +Fe V,1662.32 +O III],1666.15 +Al II,1670.79 +Ni II,1709.6 +Fe IV,1717.9 +N IV,1718.55 +Ni II,1741.55 +Ni II,1751.91 +Si II,1808.01 +Si I,1845.52 +Al III,1854.72 +Al III,1862.79 +Si III],1883 +Si III],1892.03 +Fe II,1901.77 +C III],1906.68 +C III],1908.73 +Fe III,1922.79 +Fe III,1923.01 +Fe III,1923.88 +Fe III,1924.53 +Fe III,1926.04 +Fe III,1926.3 +Fe III,1930.39 +Fe III,1931.51 +Fe III,1932.82 +Fe III,1949.67 +Fe III,1950.33 +Fe III,1951.01 +Fe III,1952.65 +Fe III,1953.33 +Fe III,1954.61 +Fe III,1958.59 +Fe III,1960.32 +Fe III,1962.72 +Fe III,1964.15 +Fe III,1966.41 +Zn II,2026.14 +Cr II,2026.27 +Mg I,2026.48 +Cr II,2056.25 +N II],2140 +C III,2163.61 +Fe II,2249.88 +Fe II,2260.78 +C III,2297.58 +[O III],2321.66 +C II],2326 +[O III],2331 +Fe II,2344.21 +Fe II,2374.46 +Fe II,2382.76 +[O II],2470.97 +[O II],2471.09 +Mn II,2576.88 +Fe II,2586.65 +Mn II,2594.5 +Fe II,2600.17 +Mn II,2606.46 +Mg II,2796.35 +Mg II,2803.53 +Mg I,2852.96 diff --git a/jdaviz/data/linelists/linelist_metadata.json b/jdaviz/data/linelists/linelist_metadata.json index ecdca14e99..15fee9369e 100644 --- a/jdaviz/data/linelists/linelist_metadata.json +++ b/jdaviz/data/linelists/linelist_metadata.json @@ -73,5 +73,11 @@ "units": "micron", "filename_base": "PAH", "Citations/Notes": " PAH features (Galaxies)\n\"ISO-SWS spectra of galaxies: Continuum and features\"\nSturm, E. et al. 2000, A&A, 358, 481\nTable 2 (features at < 4 microns from ISO)\nand\n\"The Mid-Infrared Spectrum of Star-Forming Galaxies:\nGlobal Properties of Polycyclic Aromatic Hydrocarbon Emission\"\nSmith, J. D. T. et al. 2007, ApJ, 656, 770\nTable 3 (features at > 5 microns from Spitzer" + }, + "UV Galactic": { + "units": "Angstrom", + "filename_base": "UV_linelist_vacuum", + "Citations/Notes": "Taken from Lietherer+2011: https://ui.adsabs.harvard.edu/abs/2011AJ....141...37L/abstract", + "medium": "vacuum" } }