Title: The WISE Catalog of Galactic H II Regions Authors: Anderson L.D., Bania T.M., Balser D.S., Cunningham V., Wenger T.V., Johnstone B.M., Armentrout W.P. Table: Distances for WISE Sources ================================================================================ Byte-by-byte Description of file: datafile6.txt -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 15 A15 --- WISE WISE indentifier 17- 19 F3.1 kpc Near ? Near kinematic distance 21- 24 F4.1 kpc Far ? Far kinematic distance 26- 28 F3.1 kpc Tan ? Tangent point distance 30- 33 F4.1 kpc RGal ? Distance from Galactic center 35- 40 F6.1 km/s VT ? Tangent point velocity 42 A1 --- KDAR Kinematic Distance Ambiguity Resolution 44- 47 F4.1 kpc Dis ? Distance from the Sun 49- 51 F3.1 kpc e_Dis ? The 1{sigma} error in Dis 53- 55 A3 deg Azi ? Galactic Azimuthal angle 57- 60 I4 pc z ? Height about the Galactic plane 62- 80 A19 --- Method Method used to derive distance (1) 82- 83 A2 --- Ref Reference code (2) -------------------------------------------------------------------------------- Note (1): "Parallax" for maser parallax distances, "OG/Kin" for outer Galaxy kinematic distances, "TP/Kin" for tangent point kinematic distances, "HIEA+HISA/Kin" for HIE/A and HISA kinematic distances from Anderson et al. (2009), "HIEA/Kin" for HIE/A kinematic distances, "H2CO/Kin." for H2CO absorption kinematic distances, "IRDC+HISA (Mol)/Kin" for kinematic distances from Dunham et al. (2011), "Visible/Kin" for inner Galaxy Sharpless HII region kinematic distances (near distances assumed). Kinematic distances derived from molecular line observations use the above designations, but include "(Mol)", i.e., "OG (Mol)/Kin". Note (2): 1 = Anderson & Bania (2009a); 2 = Anderson et al. (2012); 3 = Ando et al. (2011); 4 = Araya et al. (2002); 5 = Bania, Anderson, & Balser (2012); 6 = Bartkiewicz et al. (2008); 7 = Brunthaler et al. (2009); 8 = Caswell & Haynes (1987); 9 = Dunham et al. (2011); 10 = Hachisuka et al. (2009); 11 = Hirota et al. (2008a); 12 = Hirota et al. (2008b); 13 = Honma et al. (2007); 14 = Honma et al. (2011); 15 = Immer et al. (2013); 16 = Jones & Dickey (2012); 17 = Kurayama et al. (2011); 18 = Menten et al. (2007); 19 = Moellenbrock et al. (2009); 20 = Moscadelli et al. (2009); 21 = Niinuma et al. (2011); 22 = Oh et al. (2010); 23 = Reid et al. (2009a); 24 = Reid et al. (2009c); 25 = Rygl et al. (2010); 26 = Rygl et al. (2012); 27 = Sanna et al. (2009); 28 = Sanna et al. (2012); 29 = Sato et al. (2008); 30 = Sato et al. (2010a); 31 = Sato et al. (2010b); 32 = Sewilo et al. (2004b); 33 = Shiozaki et al. (2011); 34 = Urquhart et al. (2012); 35 = Urquhart et al. (2012)/Roman-Duval et al. (2009); 36 = Watson et al. (2003); 37 = Wu et al. (2012); 38 = Xu et al. (2006); 39 = Xu et al. (2009); 40 = Xu et al. (2011); 41 = Xu et al. (2013); 42 = Zhang et al. (2009). -------------------------------------------------------------------------------- G000.003+00.127 G000.008+00.036 G000.025-00.232 G000.029-00.090 G000.041+00.021 G000.043+00.013 G000.052-00.205 G000.079-00.211 G000.079-00.626 G000.082-00.097 G000.099-00.168 G000.114-00.092 G000.120-00.556 G000.120-00.633 G000.121-00.304 G000.125-00.086 G000.129-00.674 G000.132+00.039 G000.138-00.115 G000.158-00.065 G000.170+00.153 G000.176-00.062 G000.197-00.007 G000.199-00.512 G000.208-00.002 G000.227-00.502 G000.279-00.059 G000.279-00.482 G000.298-01.051 G000.314-00.194 G000.314-00.205 G000.316-00.149 G000.319-00.119 G000.328-00.804 G000.331-00.065 G000.335-00.016 G000.346-00.028 G000.352-00.020 G000.360-00.141 G000.382+00.017 G000.394-00.132 G000.397-00.091 G000.401+00.408 G000.408-00.881 G000.410-00.778 G000.411-00.060 G000.414-00.021 G000.418-00.081 G000.421-00.555 G000.436-00.084 G000.452-00.904 G000.455-00.476 G000.456-00.808 G000.460-00.048 G000.471-00.055 G000.475-00.675 G000.477-00.130 G000.479+00.072 G000.484-00.900 G000.486+00.201 G000.490-00.074 G000.492+00.191 G000.496-00.828 G000.497+00.159 G000.498-00.678 G000.501+00.190 G000.504-00.789 G000.519+00.177 G000.519-00.051 G000.520+00.195 G000.522-00.011 G000.523+00.168 G000.525+00.190 G000.528+00.180 G000.529-00.107 G000.530+00.131 G000.530-00.156 G000.533-00.082 G000.534+00.168 G000.541-00.046 G000.544-00.227 G000.547-00.060 G000.548-00.852 G000.548-00.836 G000.551+00.060 G000.557-00.079 G000.563-00.852 G000.563-00.037 G000.563-00.824 G000.567-00.097 G000.574+00.128 G000.579-00.045 G000.583-00.871 G000.586-00.127 G000.587-00.086 G000.591+00.050 G000.593-00.047 G000.595-00.618 G000.596-00.171 G000.599-00.049 G000.600-00.121 G000.601-00.069 G000.602-00.051 G000.602+00.333 G000.605-00.202 G000.616-00.052 G000.624-00.046 G000.630-00.027 G000.638-00.115 G000.649-00.080 0.7 7.8 0.9 6 -10 Parallax 24 G000.657-00.041 G000.660-00.052 G000.666-00.036 G000.666-00.051 G000.668+00.641 G000.670-00.043 G000.670-00.035 G000.674+00.083 G000.676-00.043 G000.681-00.064 G000.681-00.035 G000.692-00.047 G000.697-00.053 G000.711-00.039 G000.719+00.029 G000.729-00.103 0.1 8.5 89 -15 Nuclear Disk G000.755-00.027 G000.775-00.087 G000.800+00.010 G000.801+00.205 G000.820-00.254 G000.829+00.198 G000.834-00.457 G000.843-00.106 G000.929-00.520 G000.930-00.235 G000.957-00.234 G001.005-00.236 G001.011-00.217 G001.050+00.007 G001.055-00.154 G001.061-00.235 G001.099-00.090 G001.114-00.114 G001.119-00.266 G001.125-00.106 G001.138+00.807 G001.157+00.064 G001.218-00.034 G001.321+00.101 G001.330+00.088 G001.330+00.145 G001.362+00.118 G001.488-00.199