instrument_description.xcat
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\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 |
|char |char |real |char |char |real |real |real |
|NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |
\========= 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