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 <[email protected]>
Co-authored-by: P. L. Lim <[email protected]>

.gitignore

@@ -53,6 +53,7 @@ distribute-*.tar.gz
 .tox
 .*.sw[op]
 *~
+._*
 .project
 .pydevproject
 .settings

CHANGES.rst

@@ -59,6 +59,8 @@ Specviz
 Other Changes and Additions
 ---------------------------
 
+- Added a UV Galactic linelist. [#1522]
+
 2.8 (2022-07-21)
 ================
 

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

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"
   }
 }