1<?xml version="1.0" encoding="utf-8"?> 2<!-- Produced with astropy.io.votable version 0.2.dev2731 3 http://www.astropy.org/ --> 4<VOTABLE version="1.1" xmlns="http://www.ivoa.net/xml/VOTable/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:noNamespaceSchemaLocation="http://www.ivoa.net/xml/VOTable/v1.1"> 5 <DESCRIPTION> 6 VOTable generated from the original AAS Journal Machine Readable 7 Table 8 </DESCRIPTION> 9 <COOSYS ID="J2000" epoch="J2000." equinox="J2000." system="eq_FK5"/> 10 <RESOURCE ID="aj285677t2_votable" type="results"> 11 <DESCRIPTION> 12 Intrinsically Red Sources observed by Spitzer in the Galactic Mid- 13 Plane (Robitaille T.P. et al.) 14 </DESCRIPTION> 15 <LINK href="https://doi.org/10.1088/0004-6256/136/6/2413"/> 16 <TABLE nrows="18949"> 17 <DESCRIPTION> 18 Final red source catalog 19 </DESCRIPTION> 20 <FIELD ID="col1" arraysize="25" datatype="char" name="Name" ucd="meta.id;meta.main" unit="---"> 21 <DESCRIPTION> 22 GLIMPSE source name 23 </DESCRIPTION> 24 </FIELD> 25 <FIELD ID="col2" datatype="float" name="GLON" precision="4" ucd="pos.galactic.lon" unit="deg" width="8"> 26 <DESCRIPTION> 27 Galactic longtitude (1) These coordinates are set to the average 28 position of the source at 4.5 and at 8.0 microns. This 29 position may differ slightly from the `official' 30 GLIMPSE position in cases where PSF fitting was used to 31 determine the flux of the source if the position of the source 32 was adjusted to obtain a better residual. 33 </DESCRIPTION> 34 </FIELD> 35 <FIELD ID="col3" datatype="float" name="GLAT" precision="4" ucd="pos.galactic.lat" unit="deg" width="7"> 36 <DESCRIPTION> 37 Galactic latitude (1) These coordinates are set to the average 38 position of the source at 4.5 and at 8.0 microns. This 39 position may differ slightly from the `official' 40 GLIMPSE position in cases where PSF fitting was used to 41 determine the flux of the source if the position of the source 42 was adjusted to obtain a better residual. 43 </DESCRIPTION> 44 </FIELD> 45 <FIELD ID="col4" datatype="float" name="RAdeg" precision="4" ucd="pos.eq.ra" unit="deg" width="8"> 46 <DESCRIPTION> 47 Right Ascension in decimal degrees (J2000) (1) These coordinates 48 are set to the average position of the source at 4.5 49 and at 8.0 microns. This position may differ slightly from the 50 `official' GLIMPSE position in cases where PSF fitting was used 51 to determine the flux of the source if the position of 52 the source was adjusted to obtain a better residual. 53 </DESCRIPTION> 54 </FIELD> 55 <FIELD ID="col5" datatype="float" name="DEdeg" precision="4" ucd="pos.eq.dec" unit="deg" width="8"> 56 <DESCRIPTION> 57 Declination in decimal degrees (J2000) (1) These coordinates are 58 set to the average position of the source at 4.5 and 59 at 8.0 microns. This position may differ slightly from the 60 `official' GLIMPSE position in cases where PSF fitting was used 61 to determine the flux of the source if the position of 62 the source was adjusted to obtain a better residual. 63 </DESCRIPTION> 64 </FIELD> 65 <FIELD ID="col6" datatype="float" name="Jmag" precision="2" ucd="phot.mag;em.IR.J" unit="mag" width="5"> 66 <DESCRIPTION> 67 ? 2MASS J band magnitude (2) The zero-magnitude fluxes assumed 68 throughout this paper are: F_{nu}_(J) = 1594 Jy, 69 F_{nu}_(H) = 1024 Jy, F_{nu}_(K_s_) = 666.7 Jy, 70 F_{nu}_(3.6 microns) = 280.9 Jy, F_{nu}_(4.5 microns) = 179.7 Jy, 71 F_{nu}_(5.8 microns) = 115.0 Jy, F_{nu}_(8.0 microns) = 64.13 Jy, 72 F_{nu}_(MSX E) = 8.75 Jy, F_{nu}_(24.0 micron) = 7.14 Jy. 73 </DESCRIPTION> 74 </FIELD> 75 <FIELD ID="col7" datatype="float" name="Hmag" precision="2" ucd="phot.mag;em.IR.H" unit="mag" width="5"> 76 <DESCRIPTION> 77 ? 2MASS H band magnitude (2) The zero-magnitude fluxes assumed 78 throughout this paper are: F_{nu}_(J) = 1594 Jy, 79 F_{nu}_(H) = 1024 Jy, F_{nu}_(K_s_) = 666.7 Jy, 80 F_{nu}_(3.6 microns) = 280.9 Jy, F_{nu}_(4.5 microns) = 179.7 Jy, 81 F_{nu}_(5.8 microns) = 115.0 Jy, F_{nu}_(8.0 microns) = 64.13 Jy, 82 F_{nu}_(MSX E) = 8.75 Jy, F_{nu}_(24.0 micron) = 7.14 Jy. 83 </DESCRIPTION> 84 </FIELD> 85 <FIELD ID="col8" datatype="float" name="Kmag" precision="2" ucd="phot.mag;em.IR.K" unit="mag" width="5"> 86 <DESCRIPTION> 87 ? 2MASS K_s_ band magnitude (2) The zero-magnitude fluxes assumed 88 throughout this paper are: F_{nu}_(J) = 1594 Jy, 89 F_{nu}_(H) = 1024 Jy, F_{nu}_(K_s_) = 666.7 Jy, 90 F_{nu}_(3.6 microns) = 280.9 Jy, F_{nu}_(4.5 microns) = 179.7 Jy, 91 F_{nu}_(5.8 microns) = 115.0 Jy, F_{nu}_(8.0 microns) = 64.13 Jy, 92 F_{nu}_(MSX E) = 8.75 Jy, F_{nu}_(24.0 micron) = 7.14 Jy. 93 </DESCRIPTION> 94 </FIELD> 95 <FIELD ID="col9" datatype="float" name="G3.6mag" precision="2" ucd="phot.mag;em.IR.3-4um" unit="mag" width="5"> 96 <DESCRIPTION> 97 ? GLIMPSE catalog 3.6 micron band magnitude (2) The zero- 98 magnitude fluxes assumed throughout this paper are: 99 F_{nu}_(J) = 1594 Jy, F_{nu}_(H) = 1024 Jy, F_{nu}_(K_s_) = 666.7 100 Jy, F_{nu}_(3.6 microns) = 280.9 Jy, F_{nu}_(4.5 101 microns) = 179.7 Jy, F_{nu}_(5.8 microns) = 115.0 Jy, 102 F_{nu}_(8.0 microns) = 64.13 Jy, F_{nu}_(MSX E) = 8.75 103 Jy, F_{nu}_(24.0 micron) = 7.14 Jy. 104 </DESCRIPTION> 105 </FIELD> 106 <FIELD ID="col10" datatype="float" name="G4.5mag" precision="2" ucd="phot.mag;em.IR.4-8um" unit="mag" width="5"> 107 <DESCRIPTION> 108 GLIMPSE catalog 4.5 micron band magnitude (2) The zero-magnitude 109 fluxes assumed throughout this paper are: F_{nu}_(J) = 110 1594 Jy, F_{nu}_(H) = 1024 Jy, F_{nu}_(K_s_) = 666.7 Jy, 111 F_{nu}_(3.6 microns) = 280.9 Jy, F_{nu}_(4.5 microns) = 179.7 Jy, 112 F_{nu}_(5.8 microns) = 115.0 Jy, F_{nu}_(8.0 microns) = 64.13 Jy, 113 F_{nu}_(MSX E) = 8.75 Jy, F_{nu}_(24.0 micron) = 7.14 Jy. 114 </DESCRIPTION> 115 </FIELD> 116 <FIELD ID="col11" datatype="float" name="G5.8mag" precision="2" ucd="phot.mag;em.IR.4-8um" unit="mag" width="5"> 117 <DESCRIPTION> 118 ? GLIMPSE catalog 5.8 micron band magnitude (2) The zero- 119 magnitude fluxes assumed throughout this paper are: 120 F_{nu}_(J) = 1594 Jy, F_{nu}_(H) = 1024 Jy, F_{nu}_(K_s_) = 666.7 121 Jy, F_{nu}_(3.6 microns) = 280.9 Jy, F_{nu}_(4.5 122 microns) = 179.7 Jy, F_{nu}_(5.8 microns) = 115.0 Jy, 123 F_{nu}_(8.0 microns) = 64.13 Jy, F_{nu}_(MSX E) = 8.75 124 Jy, F_{nu}_(24.0 micron) = 7.14 Jy. 125 </DESCRIPTION> 126 </FIELD> 127 <FIELD ID="col12" datatype="float" name="G8.0mag" precision="2" ucd="phot.mag;em.IR.4-8um" unit="mag" width="4"> 128 <DESCRIPTION> 129 GLIMPSE catalog 8.0 micron band magnitude (2) The zero-magnitude 130 fluxes assumed throughout this paper are: F_{nu}_(J) = 131 1594 Jy, F_{nu}_(H) = 1024 Jy, F_{nu}_(K_s_) = 666.7 Jy, 132 F_{nu}_(3.6 microns) = 280.9 Jy, F_{nu}_(4.5 microns) = 179.7 Jy, 133 F_{nu}_(5.8 microns) = 115.0 Jy, F_{nu}_(8.0 microns) = 64.13 Jy, 134 F_{nu}_(MSX E) = 8.75 Jy, F_{nu}_(24.0 micron) = 7.14 Jy. 135 </DESCRIPTION> 136 </FIELD> 137 <FIELD ID="col13" datatype="float" name="4.5mag" precision="2" ucd="phot.mag;em.IR.4-8um" unit="mag" width="5"> 138 <DESCRIPTION> 139 This paper's 4.5 micron band magnitude (2) The zero-magnitude 140 fluxes assumed throughout this paper are: F_{nu}_(J) = 141 1594 Jy, F_{nu}_(H) = 1024 Jy, F_{nu}_(K_s_) = 666.7 Jy, 142 F_{nu}_(3.6 microns) = 280.9 Jy, F_{nu}_(4.5 microns) = 179.7 Jy, 143 F_{nu}_(5.8 microns) = 115.0 Jy, F_{nu}_(8.0 microns) = 64.13 Jy, 144 F_{nu}_(MSX E) = 8.75 Jy, F_{nu}_(24.0 micron) = 7.14 Jy. 145 </DESCRIPTION> 146 </FIELD> 147 <FIELD ID="col14" datatype="float" name="8.0mag" precision="2" ucd="phot.mag;em.IR.4-8um" unit="mag" width="4"> 148 <DESCRIPTION> 149 This paper's 8.0 micron band magnitude (2) The zero-magnitude 150 fluxes assumed throughout this paper are: F_{nu}_(J) = 151 1594 Jy, F_{nu}_(H) = 1024 Jy, F_{nu}_(K_s_) = 666.7 Jy, 152 F_{nu}_(3.6 microns) = 280.9 Jy, F_{nu}_(4.5 microns) = 179.7 Jy, 153 F_{nu}_(5.8 microns) = 115.0 Jy, F_{nu}_(8.0 microns) = 64.13 Jy, 154 F_{nu}_(MSX E) = 8.75 Jy, F_{nu}_(24.0 micron) = 7.14 Jy. 155 </DESCRIPTION> 156 </FIELD> 157 <FIELD ID="col15" datatype="float" name="Emag" precision="2" ucd="phot.mag;em.IR.8-15um" unit="mag" width="5"> 158 <DESCRIPTION> 159 ? This paper's MSX E band magnitude (2) The zero-magnitude fluxes 160 assumed throughout this paper are: F_{nu}_(J) = 1594 161 Jy, F_{nu}_(H) = 1024 Jy, F_{nu}_(K_s_) = 666.7 Jy, 162 F_{nu}_(3.6 microns) = 280.9 Jy, F_{nu}_(4.5 microns) = 179.7 Jy, 163 F_{nu}_(5.8 microns) = 115.0 Jy, F_{nu}_(8.0 microns) = 64.13 Jy, 164 F_{nu}_(MSX E) = 8.75 Jy, F_{nu}_(24.0 micron) = 7.14 Jy. 165 </DESCRIPTION> 166 </FIELD> 167 <FIELD ID="col16" datatype="float" name="24mag" precision="2" ucd="phot.mag;em.IR.15-30um" unit="mag" width="4"> 168 <DESCRIPTION> 169 ? This paper's 24 micron band magnitude (2) The zero-magnitude 170 fluxes assumed throughout this paper are: F_{nu}_(J) = 171 1594 Jy, F_{nu}_(H) = 1024 Jy, F_{nu}_(K_s_) = 666.7 Jy, 172 F_{nu}_(3.6 microns) = 280.9 Jy, F_{nu}_(4.5 microns) = 179.7 Jy, 173 F_{nu}_(5.8 microns) = 115.0 Jy, F_{nu}_(8.0 microns) = 64.13 Jy, 174 F_{nu}_(MSX E) = 8.75 Jy, F_{nu}_(24.0 micron) = 7.14 Jy. 175 </DESCRIPTION> 176 </FIELD> 177 <FIELD ID="col17" arraysize="2" datatype="char" name="f_Name" ucd="meta.code" unit="---"> 178 <DESCRIPTION> 179 Flag on Name (3) This column lists two characters, which are 180 flags for 4.5 and 8.0 microns respectively. A = 181 GLIMPSE Catalog magnitudes are in agreement with the independent 182 magnitudes calculated in this paper; I = the independent 183 magnitudes calculated in this paper should be trusted 184 over the GLIMPSE Catalog magnitudes. 185 </DESCRIPTION> 186 </FIELD> 187 <DATA> 188 <TABLEDATA> 189 <TR> 190 <TD>SSTGLMC G000.0000+00.1611</TD> 191 <TD> 0.0000</TD> 192 <TD> 0.1611</TD> 193 <TD>266.2480</TD> 194 <TD>-28.8521</TD> 195 <TD/> 196 <TD/> 197 <TD/> 198 <TD> 9.78</TD> 199 <TD> 9.19</TD> 200 <TD> 8.64</TD> 201 <TD>8.05</TD> 202 <TD> 9.13</TD> 203 <TD>8.17</TD> 204 <TD/> 205 <TD/> 206 <TD>AA</TD> 207 </TR> 208 </TABLEDATA> 209 </DATA> 210 </TABLE> 211 </RESOURCE> 212</VOTABLE> 213