\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 (%) |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 \========= 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 \========= S-PASS ========== \information taken from Carretti et al. 2019 \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 \========= 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