OV-GSO-DC / dustem-wrapper_idl

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427f1205 Jean-Michel Glorian version 4.2 merged	1 2 3 4 5 6 7 8	`\Instrument description \Caution: units and flux_conv wrong for MIPS \Caution: units and flux_conv probably wrong for IRAC and bolocam \Caution: PACS wavelengths must be checked \reso_orig in degrees \Wave is in microns \sighit: sigma for one hit (except for some experiments) \sigabs: absolute gain error in percent (%)`
7d3e9c38 Jean-Philippe Bernard modofoed for JWST...	9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 55 56 57 58 59 60 61 62 63 64 65 66 67 68 69 70 71	\|INSTRU \|FILTER \|WAVE \|BUNIT \|FLUX_CONV \|reso_orig \|sighit \|sigabs \|NAME \|Filename \| \|char \|char \|real \|char \|char \|real \|real \|real \|char \|char \| \|NULL \|NULL \|NULL \|NULL \|NULL \|NULL \|NULL \|NULL \|NULL \|NULL \| \JWST NIRCam filters taken from http://svo2.cab.inta-csic.es/svo/theory/fps3 JWST NIRCAM1 0.703912 F070W JWST_NIRCam.F070W.dat JWST NIRCAM2 0.902153 F090W JWST_NIRCam.F090W.dat JWST NIRCAM3 1.154261 F115W JWST_NIRCam.F115W.dat JWST NIRCAM4 1.405323 F140M JWST_NIRCam.F140M.dat JWST NIRCAM5 1.500744 F150W JWST_NIRCam.F150W.dat JWST NIRCAM6 1.627247 F162M JWST_NIRCam.F162M.dat JWST NIRCAM7 1.644536 F164N JWST_NIRCam.F164N.dat JWST NIRCAM8 1.659213 F150W2 JWST_NIRCam.F150W2.dat JWST NIRCAM9 1.845168 F182M JWST_NIRCam.F182M.dat JWST NIRCAM10 1.873899 F187N JWST_NIRCam.F187N.dat JWST NIRCAM11 1.988648 F200W JWST_NIRCam.F200W.dat JWST NIRCAM12 2.095452 F210M JWST_NIRCam.F210M.dat JWST NIRCAM13 2.121318 F212N JWST_NIRCam.F212N.dat JWST NIRCAM14 2.503233 F250M JWST_NIRCam.F250M.dat JWST NIRCAM15 2.761740 F277W JWST_NIRCam.F277W.dat JWST NIRCAM16 2.989121 F300M JWST_NIRCam.F300M.dat JWST NIRCAM17 3.236853 F323N JWST_NIRCam.F323N.dat JWST NIRCAM18 3.231983 F322W2 JWST_NIRCam.F322W2.dat JWST NIRCAM19 3.362067 F335M JWST_NIRCam.F335M.dat JWST NIRCAM20 3.568362 F356W JWST_NIRCam.F356W.dat JWST NIRCAM21 3.624176 F360M JWST_NIRCam.F360M.dat JWST NIRCAM22 4.051653 F405N JWST_NIRCam.F405N.dat JWST NIRCAM23 4.082238 F410M JWST_NIRCam.F410M.dat JWST NIRCAM24 4.281258 F430M JWST_NIRCam.F430M.dat JWST NIRCAM25 4.404314 F444W JWST_NIRCam.F444W.dat JWST NIRCAM26 4.629928 F460M JWST_NIRCam.F460M.dat JWST NIRCAM27 4.654430 F466N JWST_NIRCam.F466N.dat JWST NIRCAM28 4.707791 F470N JWST_NIRCam.F470N.dat JWST NIRCAM29 4.818195 F480M JWST_NIRCam.F480M.dat \JWST MIRI filters taken from http://svo2.cab.inta-csic.es/svo/theory/fps3 JWST MIRI1 5.635257 F560W JWST_MIRI.F560W.dat JWST MIRI2 7.639324 F770W JWST_MIRI.F770W.dat JWST MIRI3 9.953116 F1000W JWST_MIRI.F1000W.dat JWST MIRI4 11.308501 F1130W JWST_MIRI.F1130W.dat JWST MIRI5 12.810137 F1280W JWST_MIRI.F1280W.dat JWST MIRI6 15.063507 F1500W JWST_MIRI.F1500W.dat JWST MIRI7 17.983723 F1800W JWST_MIRI.F1800W.dat JWST MIRI8 20.795006 F2100W JWST_MIRI.F2100W.dat JWST MIRI9 25.364004 F2550W JWST_MIRI.F2550W.dat \JWST NIRISS filters taken from http://svo2.cab.inta-csic.es/svo/theory/fps3 JWST NIRISS1 0.900389 F090W JWST_NIRISS.F090W.dat JWST NIRISS2 1.150102 F115W JWST_NIRISS.F115W.dat JWST NIRISS3 1.405134 F140M JWST_NIRISS.F140M.dat JWST NIRISS4 1.498293 F150W JWST_NIRISS.F150W.dat JWST NIRISS5 1.586646 F158M JWST_NIRISS.F158M.dat JWST NIRISS6 1.983678 F200W JWST_NIRISS.F200W.dat JWST NIRISS7 2.775790 F277W JWST_NIRISS.F277W.dat JWST NIRISS8 3.594819 F356W JWST_NIRISS.F356W.dat JWST NIRISS9 3.828358 F380M JWST_NIRISS.F380M.dat JWST NIRISS10 4.285510 F430M JWST_NIRISS.F430M.dat JWST NIRISS11 4.434596 F444W JWST_NIRISS.F444W.dat JWST NIRISS12 4.816824 F480M JWST_NIRISS.F480M.dat \========= additional filters for PILOT taken from ?? ========== PILOT PILOT1 240 MJy/sr nuInu=cste 0.03666667 NULL NULL PILOT balloon-borne experiment \========= additional filters for Hawc+ taken from Chuss et al 2019 ========== HAWCPLUS HAWCPLUS1 53 MJy/sr nuInu=cste 0.001361111 NULL NULL HAWCPLUS HAWCPLUS2 89 MJy/sr nuInu=cste 0.002166667 NULL NULL HAWCPLUS HAWCPLUS3 154 MJy/sr nuInu=cste 0.003777778 NULL NULL HAWCPLUS HAWCPLUS4 214 MJy/sr nuInu=cste 0.005055556 NULL NULL
e71a7ada Jean-Philippe Bernard modified to work ...	72 73 74 75 76 77 78 79 80 81	\========= additional filters provided by Longji Bing ========== \JPB modified the name of filters to intrument# with # starting from 1, for consistency with the rest. \The resolution of Spitzer IRS, SCUBA2, NIKA2 1.2mm and NIKA2 2.0mm are 3.8", 13.0", 11.7" and 17.0", respectively. IRS IRS1 15.687 MJy/sr NULL 0.001055555 SCUBA2 SCUBA21 863.218 MJy/sr nuInu=cste 0.003611111 NIKA2 NIKA21 1187.537 MJy/sr nuInu=cste 0.003249999 NIKA2 NIKA22 2025.892 MJy/sr nuInu=cste 0.004722222 \=== Non-photometric data (This is not necessary, as spectrometer data don't require information about the instrument) \INSTRU \|FILTER \|WAVE \|BUNIT \|FLUX_CONV \|reso_orig \|sighit \|sigabs \| IRS IRS_spec -32768. MJy/sr NULL
02f2e64b Jean-Philippe Bernard improved	82	`\========= S-PASS ==========`
e71a7ada Jean-Philippe Bernard modified to work ...	83	`\information taken from Carretti et al. 2019`
02f2e64b Jean-Philippe Bernard improved	84 85	`\flux convention does not really matter (narrow band of 8 MHz for 2.3 GHz) SPASS SPASS1 130435 MJy/sr NULL 0.14833333 5.0`
427f1205 Jean-Michel Glorian version 4.2 merged	86 87 88 89 90 91 92 93 94 95 96 97 98 99 100 101 102 103 104 105 106 107 108 109 110 111 112 113 114 115 116 117 118 119 120 121 122 123 124 125 126 127 128 129 130 131 132 133 134 135 136 137 138 139 140 141 142 143 144 145 146 147 148 149 150 151 152 153 154 155 156 157 158 159 160 161 162 163 164 165 166 167 168 169 170 171 172 173 174 175 176 177 178 179 180 181 182 183 184 185 186 187 188 189 190 191 192 193 194 195 196 197 198 199 200 201 202 203 204 205 206 207 208 209 210 211 212 213 214 215 216 217 218 219 220 221 222 223 224 225 226 227 228 229 230 231 232 233 234 235 236 237 238 239 240 241 242 243 244 245 246 247 248 249 250 251 252 253 254 255 256 257 258 259 260 261 262 263 264 265 266 267 268 269 270 271 272 273 274 275 276 277 278 279 280 281 282 283 284 285 286 287 288 289 290 291 292 293 294 295 296 297 298 299 300 301 302 303 304 305 306 307 308 309 310 311 312 313 314 315 316 317	\========= IRAC ========== \resolution taken to be 1.7, 1.7, 1.9, 2" (eg Meixner et al) IRAC IRAC1 3.55000 MJy/sr IRAC 0.000472222 IRAC IRAC2 4.49300 MJy/sr IRAC 0.000472222 IRAC IRAC3 5.73100 MJy/sr IRAC 0.000527778 IRAC IRAC4 7.87200 MJy/sr IRAC 0.000555556 \========= IRAS ========== \ang resolution from IRIS web site: 3.8,3.8,4.0,4.3' \ang resolution error: +-0.2 in all bands \sig_hit=[0.04,0.05,0.03,0.06] ;errors in MJy/sr (according to MAMD, this is for "average" coverage, not 1 hit) \iris_abs_error=[5.1,15.1,10.4,13.5] ; in % from www.cita.utoronto.ca/~mamd/IRIS/IrisTechnical.html IRAS IRAS1 12.0000 MJy/sr nuInu=cste 0.0633333 0.04 5.1 IRAS IRAS2 25.0000 MJy/sr nuInu=cste 0.0633333 0.05 15.1 IRAS IRAS3 60.0000 MJy/sr nuInu=cste 0.0666667 0.03 10.4 IRAS IRAS4 100.000 MJy/sr nuInu=cste 0.0716667 0.06 13.5 \========= AKARI ========== \Akari filters are S9w, L18w, N60, WS, N160, WL (Ryou) \Akari filters are N60, WS, N160, WL \wavelength provided by M. Juvela & Ryou Ohsawa AKARI AKARI1 9.000 MJy/sr nuInu=cste AKARI AKARI2 18.000 MJy/sr nuInu=cste AKARI AKARI3 65.000 MJy/sr nuInu=cste AKARI AKARI4 90.000 MJy/sr nuInu=cste AKARI AKARI5 140.000 MJy/sr nuInu=cste AKARI AKARI6 160.000 MJy/sr nuInu=cste \========= MIPS ========== \resolution taken to be 6,18,40" (eg Meixner et al) MIPS MIPS1 23.6800 MJy/sr MIPS 0.00166667 MIPS MIPS2 71.4200 MJy/sr MIPS 0.00500000 MIPS MIPS3 155.900 MJy/sr MIPS 0.0111111 \========= SPIRE ========== \Spire resolution below correspond to 18.1,25.2,36.9" (Matt Griffin SDP2009 slides) SPIRE SPIRE1 250.000 MJy/sr nuInu=cste 0.00502778 SPIRE SPIRE2 350.000 MJy/sr nuInu=cste 0.00700000 SPIRE SPIRE3 500.000 MJy/sr nuInu=cste 0.0102500 \========= PACS ========== \PACS resolution taken to be 5,8,13" (P. Andre .pdf). Must confirm \PACS PACS1 75.000 MJy/sr nuInu=cste 0.00138889 \PACS PACS2 110.000 MJy/sr nuInu=cste 0.00222222 \PACS PACS3 170.000 MJy/sr nuInu=cste 0.00361111 \Wavelengths and flux conventions from Marc Sauvage email on Oct 16 2009 \resolution 9.01, 9.84, 13.645" from ScanReleaseNote \Caution, this is cross-scan + in-scan average in // mode (dirty) PACS PACS1 70.000 MJy/sr nuInu=cste 0.00250278 PACS PACS2 100.000 MJy/sr nuInu=cste 0.00273333 PACS PACS3 160.000 MJy/sr nuInu=cste 0.00379028 \========= WMAP ========== \K must be checked. \resolution from lambda: 0.88 0.66 0.51 0.35 0.22 \sigabs 1% Dixit GL but ... \sigabs 0.1% Dixit Bennett et al 2003 \sig-hit as computed in psd_wmap_data.pro in MJy/sr from Tab 1 of Bennett 2003 : \W: 1.7616037 \V: 0.35912723 \Q: 0.11226172 \Ka: 0.049682426 \K: 0.022302618 \INSTRU \|FILTER \|WAVE \|BUNIT \|FLUX_CONV \|reso_orig \|sighit \|sigabs \| WMAP WMAP1 3200. MJy/sr CMB 0.22 1.762 0.1 WMAP WMAP2 4900. MJy/sr CMB 0.35 0.359 0.1 WMAP WMAP3 7300. MJy/sr CMB 0.51 0.112 0.1 WMAP WMAP4 9100. MJy/sr CMB 0.66 0.049 0.1 WMAP WMAP5 13000. MJy/sr CMB 0.88 0.022 0.1 \Fake WMAP at 10' WMAP10 WMAP101 3200. MJy/sr CMB 0.166667 1.762 0.1 WMAP10 WMAP102 4900. MJy/sr CMB 0.166667 0.359 0.1 WMAP10 WMAP103 7300. MJy/sr CMB 0.166667 0.112 0.1 WMAP10 WMAP104 9100. MJy/sr CMB 0.166667 0.049 0.1 WMAP10 WMAP105 13000. KMJy/sr CMB 0.166667 0.022 0.1 \========= MSX ========== \wfilt=[8.28,12.13,14.65,21.34] \Everything should be checked. MSX MSX1 8.28 MJy/sr nuInu=cste 0.005083 MSX MSX2 12.13 MJy/sr nuInu=cste 0.005083 MSX MSX3 14.65 MJy/sr nuInu=cste 0.005083 MSX MSX4 21.34 MJy/sr nuInu=cste 0.005083 \========= BOLOCAM ========== \wfilt=[1105.4] \Everything should be checked. BOLOCAM BOLOCAM1 1105.4 MJy/sr nuInu=cste 0 \========= DIRBE ========== \wfilt_dirbe=[1.25,2.2,3.5,4.9,12,25.,60.,100.,140,240] \dirbe_abs_errs=[3.1,3.1,3.1,3.0,5.1,15.1,10.4,13.5,10.6,11.6] ;in %, from Hauser et al 98 ApJ 508, 25 tab 2 \nuInu=[2.4,1.6,0.9,0.8,0.9,0.9,0.9,0.5,32.8,10.7] ;1-sig nuInu in nW/m2/sr from Hauser et al 98 ApJ 508, 25 tab 2 \above are in 0.7�*0.7� \gives in MJy/sr in 1� beam: \0.0007, 0.089, 0.00046, 0.00065, 0.001, 0.0025, 0.0052, 0.007, 0.766, 0.35 (see dustem_dirbe_errors.pro) \INSTRU \|FILTER \|WAVE \|BUNIT \|FLUX_CONV \|reso_orig \|sighit \|sigabs \| DIRBE DIRBE1 1.25 MJy/sr nuInu=cste 1. 0.0007 3.1 DIRBE DIRBE2 2.2 MJy/sr nuInu=cste 1. 0.089 3.1 DIRBE DIRBE3 3.5 MJy/sr nuInu=cste 1. 0.00046 3.1 DIRBE DIRBE4 4.9 MJy/sr nuInu=cste 1. 0.00065 3.0 DIRBE DIRBE5 12. MJy/sr nuInu=cste 1. 0.001 5.1 DIRBE DIRBE6 25. MJy/sr nuInu=cste 1. 0.0025 15.1 DIRBE DIRBE7 60. MJy/sr nuInu=cste 1. 0.0052 10.4 DIRBE DIRBE8 100. MJy/sr nuInu=cste 1. 0.007 13.5 DIRBE DIRBE9 140. MJy/sr nuInu=cste 1. 0.766 10.6 DIRBE DIRBE10 240. MJy/sr nuInu=cste 1. 0.35 11.6 \========= DIRBE ========== \nu_archeops=[143.,217.,353.,545.] ;GHz \resolution must be checked ARCHEOPS ARCHEOPS1 550.07791 K CMB 0. ARCHEOPS ARCHEOPS2 849.27042 K CMB 0. ARCHEOPS ARCHEOPS3 1381.5321 K CMB 0. ARCHEOPS ARCHEOPS4 2096.4508 K CMB 0. \========= HFI ========== \nu_hfi=[100.,143.,217.,353.,545.,857.] ;GHz \ 3000.00 2097.90 1382.49 849.858 550.459 350.058 \Must check if freq is the reference \resolution res=[4.25,4.7,4.8,4.7,7.0,9.6] ;median value Taken from Ma et al. \ 0.0708333 0.0783333 0.0800000 0.0783333 0.116667 0.160000 \From F. Bouchet email for DR2 release \ Freq: 100 143 217 353 545 857 GHz \ FWHM: 9.94 7.04 4.66 4.41 4.47 4.23 arcmin \leads to: 0.165667 0.117333 0.0776667 0.0735000 0.0745000 0.0705000 \ FWHM from latest table by FRB (email Oct 18 2010) \ FWHM: 9.53 7.08 4.71 4.5 4.68 4.41 arcmin \leads to: \ 0.158833 0.118000 0.0785000 0.0750000 0.0780000 0.0735000 \sig-hit in practice taken from internal noise in PSD \values below from FRB table: \in muK for 1 sq deg: 1.8 0.9 1.3 4.7 70 4.E3 \lead to:0.121905 0.0523205 0.0180480 0.00796892 0.00281441 0.00274250 (see dustem_hfi_errors) \INSTRU \|FILTER \|WAVE \|BUNIT \|FLUX_CONV \|reso_orig \|sighit \|sigabs \| \HFI HFI1 349.81617 MJy/sr nuInu=cste 0.0735000 0.1219 7. \HFI HFI2 550.07791 MJy/sr nuInu=cste 0.0780000 0.118 7. \HFI HFI3 849.27042 MJy/sr nuInu=cste 0.0750000 0.0785 2. \HFI HFI4 1381.5321 MJy/sr nuInu=cste 0.0785000 0.075 2. \HFI HFI5 2096.4508 MJy/sr nuInu=cste 0.118000 0.075 2. \HFI HFI6 2997.9246 MJy/sr nuInu=cste 0.158833 0.0735 2. \The foloowing flux conventions are used to compute cc using official routine. \INSTRU \|FILTER \|WAVE \|BUNIT \|FLUX_CONV \|reso_orig \|sighit \|sigabs \| HFI HFI1 349.81617 MJy/sr HFI 0.0735000 0.1219 7. HFI HFI2 550.07791 MJy/sr HFI 0.0780000 0.118 7. HFI HFI3 849.27042 MJy/sr HFI 0.0750000 0.0785 2. HFI HFI4 1381.5321 MJy/sr HFI 0.0785000 0.075 2. HFI HFI5 2096.4508 MJy/sr HFI 0.118000 0.075 2. HFI HFI6 2997.9246 MJy/sr HFI 0.158833 0.0735 2. \Fake HFI at 10' HFI10 HFI101 349.81617 MJy/sr nuInu=cste 0.166667 0.1219 7. HFI10 HFI102 550.07791 MJy/sr nuInu=cste 0.166667 0.118 7. HFI10 HFI103 849.27042 MJy/sr nuInu=cste 0.166667 0.0785 2. HFI10 HFI104 1381.5321 MJy/sr nuInu=cste 0.166667 0.075 2. HFI10 HFI105 2096.4508 MJy/sr nuInu=cste 0.166667 0.075 2. HFI10 HFI106 2997.9246 MJy/sr nuInu=cste 0.166667 0.0735 2. \========= LFI ========== \nu_lfi=[30.,44.,70.] ;GHz \fwhm from Clive's email of Oct 18 2010: 13.01, 27.92, 32.65 \leading to: 0.216833 0.465333 0.544167 \Units TBC LFI LFI1 4285.71 MJy/sr nuInu=cste 0.216833 5. LFI LFI2 6818.18 MJy/sr nuInu=cste 0.465333 5. LFI LFI3 10000.0 MJy/sr nuInu=cste 0.544167 5. \Fake LFI at 10' LFI10 LFI101 4285.71 MJy/sr nuInu=cste 0.166667 5. LFI10 LFI102 6818.18 MJy/sr nuInu=cste 0.166667 5. LFI10 LFI103 10000.0 MJy/sr nuInu=cste 0.166667 5. \========= SPM ========== \wfilt_spm=[200,260,360.,580] \resolutions: 2,2,2.5,3.5' \Everything should be checked. SPM SPM1 200.00 MJy/sr nuInu=cste 0.0333333 SPM SPM2 260.00 MJy/sr nuInu=cste 0.0333333 SPM SPM3 360.00 MJy/sr nuInu=cste 0.0416667 SPM SPM4 580.00 MJy/sr nuInu=cste 0.0583333 \========= ISOPHOT ========== \reso_orig values arbitrary \sighit values arbitrary \sigabs values arbitrary \INSTRU \|FILTER \|WAVE \|BUNIT \|FLUX_CONV \|reso_orig \|sighit \|sigabs \| ISOPHOT ISOPHOTP1 3.30000 MJy/sr nuInu=cste 0.0633333 0.04 5.1 ISOPHOT ISOPHOTP2 3.60000 MJy/sr nuInu=cste 0.0633333 0.04 5.1 ISOPHOT ISOPHOTP3 4.80000 MJy/sr nuInu=cste 0.0633333 0.04 5.1 ISOPHOT ISOPHOTP4 7.30000 MJy/sr nuInu=cste 0.0633333 0.04 5.1 ISOPHOT ISOPHOTP5 7.70000 MJy/sr nuInu=cste 0.0633333 0.04 5.1 ISOPHOT ISOPHOTP6 10.0000 MJy/sr nuInu=cste 0.0633333 0.04 5.1 ISOPHOT ISOPHOTP7 11.3000 MJy/sr nuInu=cste 0.0633333 0.04 5.1 ISOPHOT ISOPHOTP8 12.0000 MJy/sr nuInu=cste 0.0633333 0.04 5.1 ISOPHOT ISOPHOTP9 12.8000 MJy/sr nuInu=cste 0.0633333 0.04 5.1 ISOPHOT ISOPHOTP10 15.0000 MJy/sr nuInu=cste 0.0633333 0.04 5.1 ISOPHOT ISOPHOTP11 20.0000 MJy/sr nuInu=cste 0.0633333 0.04 5.1 ISOPHOT ISOPHOTP12 25.0000 MJy/sr nuInu=cste 0.0633333 0.04 5.1 ISOPHOT ISOPHOTP13 60.0000 MJy/sr nuInu=cste 0.0633333 0.04 5.1 ISOPHOT ISOPHOTP14 100.000 MJy/sr nuInu=cste 0.0633333 0.04 5.1 \ ISOPHOT ISOPHOTC1 65.000 MJy/sr nuInu=cste 0.0633333 0.04 5.1 ISOPHOT ISOPHOTC2 60.000 MJy/sr nuInu=cste 0.0633333 0.04 5.1 ISOPHOT ISOPHOTC3 80.000 MJy/sr nuInu=cste 0.0633333 0.04 5.1 ISOPHOT ISOPHOTC4 90.000 MJy/sr nuInu=cste 0.0633333 0.04 5.1 ISOPHOT ISOPHOTC5 100.000 MJy/sr nuInu=cste 0.0633333 0.04 5.1 ISOPHOT ISOPHOTC6 105.000 MJy/sr nuInu=cste 0.0633333 0.04 5.1 ISOPHOT ISOPHOTC7 120.000 MJy/sr nuInu=cste 0.0633333 0.04 5.1 ISOPHOT ISOPHOTC8 150.000 MJy/sr nuInu=cste 0.0633333 0.04 5.1 ISOPHOT ISOPHOTC9 170.000 MJy/sr nuInu=cste 0.0633333 0.04 5.1 ISOPHOT ISOPHOTC10 180.000 MJy/sr nuInu=cste 0.0633333 0.04 5.1 ISOPHOT ISOPHOTC11 200.000 MJy/sr nuInu=cste 0.0633333 0.04 5.1 \=== Non-photometric data \INSTRU \|FILTER \|WAVE \|BUNIT \|FLUX_CONV \|reso_orig \|sighit \|sigabs \| PARKES PARKES1 -32768. Kkm/s NULL 0.0166667 AVDO AVDO1 0.55 mag NULL 0.0433333 XMM XMM1 -32768. cts/s NULL 0.000555 \HI LAB data: 1.7 Kkm/s taken from Bernard Planck early paper. absolute accuracy 10% assumed. HI_CENT_II HI_II -32768. Kkm/s NULL 0.6 1.7 10. LABII LABII1 -32768. Kkm/s NULL 0.6 1.7 10. \CO data \NANTEN sig-hit of 1.2 Kkm/s has tio be checked. Maybe 3-sig. Varies on sky. 10% absolute assumed \DHT2001: 1.2 Kkm/s assumed. 24% is from intercalib with NANTEN NANTEN NANTEN1 -32768. Kkm/s NULL 0.0433333 1.2 10. DHT DHT1 -32768. Kkm/s NULL 0.146667 1.2 24. CO12_COMB NANTEN1 -32768. Kkm/s NULL 0.0666667 1.2 10. CO12_COMBNVNANTEN1 -32768. Kkm/s NULL 0.0666667 1.2 10. \resolution 6': http://astrometry.fas.harvard.edu/skymaps/halpha/processing.html WHAM HALPHA -32768. R NULL 0.1 1. 10. \8.6 GHz sighit corresponds to 0.5 Jy/beam for Nside=4096 ATCAPRAD ATCAPRAD1 34859.587 MJy/sr ? 0.00972222 16.56 2. \4.8 GHz sighit corresponds to 0.5 Jy/beam for Nside=4096 ATCAPRAD ATCAPRAD2 62456.760 MJy/sr ? 0.00611111 10.4 2. \========= WISE ========== \wfilt=[3.4,4.6,12.,22.] \ filters from http://wise2.ipac.caltech.edu/docs/release/prelim/expsup/sec4_3g.html#WISEZMA WISE WISE1 3.40000 MJy/sr nuInu=cste 0.0169444 WISE WISE2 4.60000 MJy/sr nuInu=cste 0.0017778 WISE WISE3 12.0000 MJy/sr nuInu=cste 0.0018055 WISE WISE4 22.0000 MJy/sr nuInu=cste 0.0033333 \========= LABOCA ========== LABOCA LABOCA1 869.570 MJy/sr LABOCA 0.0053333 \========= GISMO ========== GISMO GISMO1 2000.00 MJy/sr nuInu=cste 0.0046389 \========= BOLOCAM ========== \wfilt=[1105.4] \Everything should be checked. BOLOCAM BOLOCAM1 1105.4 MJy/sr nuInu=cste 0