instrument_description_DEV_VERSION.xcat
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\------------------------------------------------------------------
\========= instrument_description.xcat
\------------------------------------------------------------------
\instru: instrument name -- must match the non-numerical part of filter name
\filter: filter name used by DustEMWrap
\wave: reference wavelength in microns (see IRAS explanatory supplement for a clear definition of the reference frequency for wide-band instruments).
\NB This is the wavelength used for color correction and absolute calibration. It may not be the same as the wavelength used for the PSF information.
\bunit: typical brightness unit of archival data -- for convenience only
\flux_conv : flux convention -- must be known to dustem_cc.pro, see the User Guide 'Color Corrections' for more information
\reso_orig: typical intrinsic angular resolution in degrees -- for convenience only, this may differ from value used in calibration
\sighit: sigma for one hit -- for convenience only
\sigabs: absolute uncertainty in percent (%) -- for convenience only
\name : filter name used by original instrument team -- for convenience only
\filename : file containing filter transmission information (in subdirectories of Data/FILTERS/) -- instrument-dependent, not fully implemented yet
\ttype : transmission convention (energy/photon) -- for convenience only, not fully implemented yet. Information from SVO.
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
|INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
|char |char |real |char |char |real |real |real |char |char | char |
|NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\========= JWST/NIRCAM throughputs extracted from Pandeia Engine v2.0 (Dec 2022)
\========= according to https://jwst-docs.stsci.edu/jwst-exposure-time-calculator-overview/jwst-etc-pandeia-engine-tutorial/jwst-etc-instrument-throughputs
\========= Contact Scientist: Bryan Hilbert, STScI, hilbert@stsci.edu
\========= Reference wavelength = pivot wavelength, see Gordon et al (2022) AJ, 163, 267G
\========= Transmissions represent total throughput of energy (including the blocking filter if relevant)
\========= DustEMWrap uses averaged module A and B throughputs
\========= RESO_ORIG values are empirical PSF FWHMs, except for F150W2 and F322W2, which use simulated PSF FWHM values
\========= Note that the wavelength for the PSF measurement is not necessarily the pivot wavelength for the flux calibration
\========= see Table 1 https://jwst-docs.stsci.edu/jwst-near-infrared-camera/nircam-performance/nircam-point-spread-functions
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
\char |char |real |char |char |real |real |real |char |char | char |
\NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
NIRCAM NIRCAM1 0.704374 flambda=cste 8.05556e-06 F070W nircam_f070w_totaleff.fits photon
NIRCAM NIRCAM2 0.902676 flambda=cste 9.16667e-06 F090W nircam_f090w_totaleff.fits photon
NIRCAM NIRCAM3 1.154008 flambda=cste 1.11111e-05 F115W nircam_f115w_totaleff.fits photon
NIRCAM NIRCAM4 1.405461 flambda=cste 1.33333e-05 F140M nircam_f140m_totaleff.fits photon
NIRCAM NIRCAM5 1.501331 flambda=cste 1.38889e-05 F150W nircam_f150w_totaleff.fits photon
NIRCAM NIRCAM6 1.627067 flambda=cste 1.52778e-05 F162M nircam_f162m_totaleff.fits photon
NIRCAM NIRCAM7 1.644496 flambda=cste 1.55556e-05 F164N nircam_f164n_totaleff.fits photon
NIRCAM NIRCAM8 1.670903 flambda=cste 1.25000e-05 F150W2 nircam_f150w2_totaleff.fits photon
NIRCAM NIRCAM9 1.845224 flambda=cste 1.72222e-05 F182M nircam_f182m_totaleff.fits photon
NIRCAM NIRCAM10 1.874044 flambda=cste 1.77778e-05 F187N nircam_f187n_totaleff.fits photon
NIRCAM NIRCAM11 1.987502 flambda=cste 1.83333e-05 F200W nircam_f200w_totaleff.fits photon
NIRCAM NIRCAM12 2.095654 flambda=cste 1.97222e-05 F210M nircam_f210m_totaleff.fits photon
NIRCAM NIRCAM13 2.121253 flambda=cste 2.00000e-05 F212N nircam_f212n_totaleff.fits photon
NIRCAM NIRCAM14 2.503264 flambda=cste 2.36111e-05 F250M nircam_f250m_totaleff.fits photon
NIRCAM NIRCAM15 2.776153 flambda=cste 2.55556e-05 F277W nircam_f277w_totaleff.fits photon
NIRCAM NIRCAM16 2.996149 flambda=cste 2.77778e-05 F300M nircam_f300m_totaleff.fits photon
NIRCAM NIRCAM17 3.246888 flambda=cste 2.66667e-05 F322W2 nircam_f322w2_totaleff.fits photon
NIRCAM NIRCAM18 3.236783 flambda=cste 3.00000e-05 F323N nircam_f323n_totaleff.fits photon
NIRCAM NIRCAM19 3.362345 flambda=cste 3.08333e-05 F335M nircam_f335m_totaleff.fits photon
NIRCAM NIRCAM20 3.565652 flambda=cste 3.22222e-05 F356W nircam_f356w_totaleff.fits photon
NIRCAM NIRCAM21 3.623313 flambda=cste 3.33333e-05 F360M nircam_f360m_totaleff.fits photon
NIRCAM NIRCAM22 4.053120 flambda=cste 3.77778e-05 F405N nircam_f405n_totaleff.fits photon
NIRCAM NIRCAM23 4.083447 flambda=cste 3.80556e-05 F410M nircam_f410m_totaleff.fits photon
NIRCAM NIRCAM24 4.281304 flambda=cste 4.00000e-05 F430M nircam_f430m_totaleff.fits photon
NIRCAM NIRCAM25 4.401087 flambda=cste 4.02778e-05 F444W nircam_f444w_totaleff.fits photon
NIRCAM NIRCAM26 4.630002 flambda=cste 4.36111e-05 F460M nircam_f460m_totaleff.fits photon
NIRCAM NIRCAM27 4.654336 flambda=cste 4.38889e-05 F466N nircam_f466n_totaleff.fits photon
NIRCAM NIRCAM28 4.707872 flambda=cste 4.44444e-05 F470N nircam_f470n_totaleff.fits photon
NIRCAM NIRCAM29 4.814268 flambda=cste 4.55556e-05 F480M nircam_f480m_totaleff.fits photon
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\========= JWST/MIRI throughputs extracted from Pandeia Engine v2.0 (Dec 2022)
\========= according to https://jwst-docs.stsci.edu/jwst-exposure-time-calculator-overview/jwst-etc-pandeia-engine-tutorial/jwst-etc-instrument-throughputs
\========= Contact Scientist: Karl Gordon, STScI, kgordon@stsci.edu
\========= Reference wavelength = pivot wavelength, see Gordon et al (2022)
\========= Transmissions represent total throughput of energy
\========= RESO_ORIG values are empirical PSF FWHMs for MIRI Wide filters
\========= Note that the wavelength for the PSF measurement is not necessarily the pivot wavelength for the flux calibration
\========= see Table 1 https://jwst-docs.stsci.edu/jwst-mid-infrared-instrument/miri-performance/miri-point-spread-functions
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
\char |char |real |char |char |real |real |real |char |char | char |
\NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
MIRI MIRI1 5.63501415 flambda=cste 5.75000e-05 F0560W miri_f0560w_totaleff.fits photon
MIRI MIRI2 7.63926083 flambda=cste 7.47222e-05 F0770W miri_f0770w_totaleff.fits photon
MIRI MIRI3 9.95294785 flambda=cste 9.11111e-05 F1000W miri_f1000w_totaleff.fits photon
MIRI MIRI4 10.5953262 flambda=cste F1065C miri_f1065c_totaleff.fits photon
MIRI MIRI5 11.3039289 flambda=cste F1140C miri_f1140c_totaleff.fits photon
MIRI MIRI6 11.3086580 flambda=cste 0.000104167 F1130W miri_f1130w_totaleff.fits photon
MIRI MIRI7 12.8100925 flambda=cste 0.000116667 F1280W miri_f1280w_totaleff.fits photon
MIRI MIRI8 15.0635204 flambda=cste 0.000135556 F1500W miri_f1500w_totaleff.fits photon
MIRI MIRI9 15.5129386 flambda=cste F1550C miri_f1550c_totaleff.fits photon
MIRI MIRI10 17.9839002 flambda=cste 0.000164167 F1800W miri_f1800w_totaleff.fits photon
MIRI MIRI11 20.7945621 flambda=cste 0.000187222 F2100W miri_f2100w_totaleff.fits photon
MIRI MIRI12 22.6753973 flambda=cste F2300C miri_f2300c_totaleff.fits photon
MIRI MIRI13 25.3650244 flambda=cste 0.000223056 F2550W miri_f2550w_totaleff.fits photon
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\========= JWST/NIRISS throughputs extracted from Pandeia Engine v2.0 (Dec 2022)
\========= according to https://jwst-docs.stsci.edu/jwst-exposure-time-calculator-overview/jwst-etc-pandeia-engine-tutorial/jwst-etc-instrument-throughputs
\========= Contact Scientist: Steph LaMassa, slamassa@stsci.edu
\========= Reference wavelength = pivot wavelength, see Gordon et al (2022) AJ, 163, 267G
\========= Transmissions represent total throughput of energy (including the blocking filter if relevant)
\========= RESO_ORIG values are empirical PSF FWHMs for NIRISS filters
\========= Note that the wavelength for the PSF measurement is not necessarily the pivot wavelength for the flux calibration
\========= see Table 1 https://jwst-docs.stsci.edu/jwst-near-infrared-imager-and-slitless-spectrograph/niriss-performance/niriss-point-spread-functions
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
\char |char |real |char |char |real |real |real |char |char | char |
\NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
NIRISS NIRISS1 0.900389 flambda=cste 2.44444e-05 F090W niriss_f090w_totaleff.fits photon
NIRISS NIRISS2 1.150102 flambda=cste 2.61111e-05 F115W niriss_f115w_totaleff.fits photon
NIRISS NIRISS3 1.405134 flambda=cste 2.55556e-05 F140M niriss_f140m_totaleff.fits photon
NIRISS NIRISS4 1.498293 flambda=cste 2.55556e-05 F150W niriss_f150w_totaleff.fits photon
NIRISS NIRISS5 1.586646 flambda=cste 2.63889e-05 F158M niriss_f158m_totaleff.fits photon
NIRISS NIRISS6 1.983678 flambda=cste 2.94444e-05 F200W niriss_f200w_totaleff.fits photon
NIRISS NIRISS7 2.775790 flambda=cste 3.16667e-05 F277W niriss_f277w_totaleff.fits photon
NIRISS NIRISS8 3.594819 flambda=cste 3.63889e-05 F356W niriss_f356w_totaleff.fits photon
NIRISS NIRISS9 3.828358 flambda=cste 3.86111e-05 F380M niriss_f380m_totaleff.fits photon
NIRISS NIRISS10 4.285510 flambda=cste 4.16667e-05 F430M niriss_f430m_totaleff.fits photon
NIRISS NIRISS11 4.434596 flambda=cste 4.11111e-05 F444W niriss_f444w_totaleff.fits photon
NIRISS NIRISS12 4.816824 flambda=cste 4.66667e-05 F480M niriss_f480m_totaleff.fits photon
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\========= Information for PILOT taken from Bernard et al (2022)
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
\char |char |real |char |char |real |real |real |char |char | char |
\NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
PILOT PILOT1 240. MJy/sr nuInu=cste 0.03666667
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\========= Filter transmission information for SOFIA/HAWC+ from SVO Filter Service
\========= Reference WAVE, RESO_ORIG and SIGABS from Chuss et al. (2019) ApJ 872 187 --> DEPRECATED this WAVE and FLUX_CONV (6/2/2023)
\========= Note: The filter at 63 microns is not in Chuss et al (2019)
\========= Reference WAVE and FLUX_CONV from https://www.sofia.usra.edu/sites/default/files/Instruments/HAWC_PLUS/Documents/HAWC_ColorCorrecns_OC5.pdf
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
\char |char |real |char |char |real |real |real |char |char | char |
\NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\HAWCPLUS HAWCPLUS1 53. MJy/sr nuInu=cste 0.00141667 15 BAND_A SOFIA_HAWC.A.dat photon
\HAWCPLUS HAWCPLUS2 63. MJy/sr nuInu=cste 0.002916667 BAND_B SOFIA_HAWC.B.dat photon
\HAWCPLUS HAWCPLUS3 89. MJy/sr nuInu=cste 0.00219444 15 BAND_C SOFIA_HAWC.C.dat photon
\HAWCPLUS HAWCPLUS4 155. MJy/sr nuInu=cste 0.0038888890 15 BAND_D SOFIA_HAWC.D.dat photon
\HAWCPLUS HAWCPLUS5 214. MJy/sr nuInu=cste 0.0051944447 20 BAND_E SOFIA_HAWC.E.dat photon
\HAWCPLUS HAWCPLUS1 53.560 MJy/sr flambda=cste 0.00141667 15 BAND_A SOFIA_HAWC.A.dat photon
\HAWCPLUS HAWCPLUS2 63.253 MJy/sr flambda=cste 0.002916667 BAND_B SOFIA_HAWC.B.dat photon
\HAWCPLUS HAWCPLUS3 89.305 MJy/sr flambda=cste 0.00219444 15 BAND_C SOFIA_HAWC.C.dat photon
\HAWCPLUS HAWCPLUS4 156.480 MJy/sr flambda=cste 0.0038888890 15 BAND_D SOFIA_HAWC.D.dat photon
\HAWCPLUS HAWCPLUS5 216.969 MJy/sr flambda=cste 0.0051944447 20 BAND_E SOFIA_HAWC.E.dat photon
HAWCPLUS HAWCPLUS1 53.560 MJy/sr fnu=cste 0.00141667 15 BAND_A SOFIA_HAWC.A.dat photon
HAWCPLUS HAWCPLUS2 63.253 MJy/sr fnu=cste 0.002916667 BAND_B SOFIA_HAWC.B.dat photon
HAWCPLUS HAWCPLUS3 89.305 MJy/sr fnu=cste 0.00219444 15 BAND_C SOFIA_HAWC.C.dat photon
HAWCPLUS HAWCPLUS4 156.480 MJy/sr fnu=cste 0.0038888890 15 BAND_D SOFIA_HAWC.D.dat photon
HAWCPLUS HAWCPLUS5 216.969 MJy/sr fnu=cste 0.0051944447 20 BAND_E SOFIA_HAWC.E.dat photon
\HAWCPLUS HAWCPLUS1 53.560 MJy/sr nuInu=cste 0.00141667 15 BAND_A SOFIA_HAWC.A.dat photon
\HAWCPLUS HAWCPLUS2 63.253 MJy/sr nuInu=cste 0.002916667 BAND_B SOFIA_HAWC.B.dat photon
\HAWCPLUS HAWCPLUS3 89.305 MJy/sr nuInu=cste 0.00219444 15 BAND_C SOFIA_HAWC.C.dat photon
\HAWCPLUS HAWCPLUS4 156.480 MJy/sr nuInu=cste 0.0038888890 15 BAND_D SOFIA_HAWC.D.dat photon
\HAWCPLUS HAWCPLUS5 216.969 MJy/sr nuInu=cste 0.0051944447 20 BAND_E SOFIA_HAWC.E.dat photon
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\========= Information for JCMT/SCUBA2 from SVO Filter Service
\========= http://svo2.cab.inta-csic.es/theory/fps3/index.php
\========= Note misnomer of SVO filenames. 450GHz is actually 450um, 850GHz is actually 850um
\========= RESO_ORIG values are typical values from SCUBA2 public legacy surveys
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
\char |char |real |char |char |real |real |real |char |char | char |
\NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
SCUBA2 SCUBA21 449. MJy/sr nuInu=cste 0.00222222 SC450um JCMT_SCUBA2.450GHz.dat energy
SCUBA2 SCUBA22 861. MJy/sr nuInu=cste 0.00375000 SC850um JCMT_SCUBA2.850GHz.dat energy
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\========= Information for NIKA2 from SVO Filter Service and IRAM NIKA2 wiki
\========= Contact Scientist: Carsten Kramer, kramer@iram.fr
\========= http://svo2.cab.inta-csic.es/theory/fps3/index.php
\========= https://publicwiki.iram.es/Continuum/NIKA2/Main
\========= WAVE (150.0, 260.0GHz), FLUX_CONV and RESO_ORIG (12".5, 18".5) from Perotto et al (2020)
\========= Previous release RESO_ORIG =[11".2,17".7] from NIKA2 wiki
\========= The transmission curve at 1mm used by DustEMWrap is the average of A1 and A3
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
\char |char |real |char |char |real |real |real |char |char | char |
\NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
NIKA2 NIKA21 1153.04789 MJy/sr NIKA2 0.0034722222 NIKA1mm NIKA2_1mm_avg.xcat energy
NIKA2 NIKA22 1998.61648 MJy/sr NIKA2 0.0051388890 NIKA2mm NIKA2_2mm.xcat energy
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\========= Information for Spitzer IRS PU imaging filters from SVO Filter Service
\========= http://svo2.cab.inta-csic.es/theory/fps3/index.php
\========= WAVE (sec 4.2.4) and RESO_ORIG (4.2.3) values are from the Spitzer IRS Handbook
\========= https://irsa.ipac.caltech.edu/data/SPITZER/docs/irs/irsinstrumenthandbook/8/
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
\char |char |real |char |char |real |real |real |char |char | char |
\NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
IRS IRS1 15.80 MJy/sr nuInu=cste 0.0010555555 IRS_PU_BLUE Spitzer_IRS.Blue.dat photon
IRS IRS2 22.30 MJy/sr nuInu=cste 0.0014722223 IRS_PU_RED Spitzer_IRS.Red.dat photon
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\========= Information for S-PASS taken from Carretti et al (2019)
\========= Flux convention does not really matter (narrow band of 8 MHz for 2.3 GHz). Resolution is 8.9' (0.148333 deg)
\========= Reference frequency is 2.303 GHz (130174.74 micron)
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
\char |char |real |char |char |real |real |real |char |char | char |
\NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
SPASS SPASS1 130174.74 MJy/sr NULL 0.14833333 5.0
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\========= Information for ZOA-FF (Zone of Avoidance Free-Free) taken from Alves, M. I. R., et al, 2015, MNRAS, 450, 2025
\========= Flux convention does not really matter (narrow band of ? MHz for 1.4 GHz)
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
\char |char |real |char |char |real |real |real |char |char | char |
\NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\CHIPASS ZOA_FF1 214286. MJy/sr NULL 0.24 5.0
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\========= Information for CHIPASS taken from Calabretta, M. et al. 2014, PASA, 31, 7
\========= Flux convention does not really matter (narrow band of 64 MHz for 1.4 GHz)
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
\char |char |real |char |char |real |real |real |char |char | char |
\NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
CHIPASS CHIPASS1 214286. MJy/sr NULL 0.24 5.0
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\========= Information for IRAC taken from SVO filter service and Spitzer IRAC handbook at IRSA
\========= https://irsa.ipac.caltech.edu/data/SPITZER/docs/irac/iracinstrumenthandbook/15/
\========= https://irsa.ipac.caltech.edu/data/SPITZER/docs/irac/iracinstrumenthandbook/IRAC_Instrument_Handbook.pdf
\========= RESO_ORIG are typical values taken from public legacy data (1.7", 1.7", 1.9", 2.0", e.g. Meixner et al 2006)
\========= FLUX_CONV: "The conventions used by IRAC are the same as those used by IRAS (Beichman et al. 1988), COBE/DIRBE (Hauser et al. 1998), and ISO (Blommaert et al. 2003)" (IRAC instrument hand book).
\========= FLUX_CONV: This is nu*Inu=cste.
\========= FLUX_CONV: "Note that our definition of the color correction (Eq4.8) looks slightly different from that of IRAS, because we used the system spectral response R in electrons/photon, instead of ergs/photon"
\========= FLUX_CONV: This color correction is called "IRAC" in DustemWrap
\========= WAVE: is taken as lambda_0 of Tab 4.3 of the IRAC instrument hand book. Verified JPB 17/01/2023
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
\char |char |real |char |char |real |real |real |char |char | char |
\NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
IRAC IRAC1 3.544 MJy/sr IRAC 0.000472222 IRAC3p6 irac1.dat energy
IRAC IRAC2 4.487 MJy/sr IRAC 0.000472222 IRAC4p5 irac2.dat energy
IRAC IRAC3 5.710 MJy/sr IRAC 0.000527778 IRAC5p8 irac3.dat energy
IRAC IRAC4 7.841 MJy/sr IRAC 0.000555556 IRAC8 irac4.dat energy
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\========= Information for IRAS taken from SVO filter service and IRAS handbook at IRSA
\========= https://irsa.ipac.caltech.edu/IRASdocs/exp.sup/toc.html
\========= RESO_ORIG are typical values for the IRIS reprocessing of the IRAS data
\========= https://www.cita.utoronto.ca/~mamd/IRIS/IrisTechnical.html
\========= ang resolution [arcmin]: [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] expressed as %
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
\char |char |real |char |char |real |real |real |char |char | char |
\NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
IRAS IRAS1 12.0000 MJy/sr nuInu=cste 0.0633333 0.04 5.1 IRAS1 IRAS12.txt energy
IRAS IRAS2 25.0000 MJy/sr nuInu=cste 0.0633333 0.05 15.1 IRAS2 IRAS25.txt energy
IRAS IRAS3 60.0000 MJy/sr nuInu=cste 0.0666667 0.03 10.4 IRAS3 IRAS60.txt energy
IRAS IRAS4 100.000 MJy/sr nuInu=cste 0.0716667 0.06 13.5 IRAS4 IRAS100.txt energy
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\========= Information for AKARI taken from SVO filter service and AKARI handbook at JAXA
\========= https://www.ir.isas.jaxa.jp/AKARI/about/
\========= WAVE for AKARI/IRC: see Table 4.6.6 https://www.ir.isas.jaxa.jp/AKARI/Observation/support/IRC/IDUM/IRC_DUM.pdf
\========= WAVE for AKARI/FIS: see Table 4.6 https://www.ir.isas.jaxa.jp/AKARI/Observation/support/FIS/IDUM/FIS_IDUM_1.3.pdf
\========= RESO_ORIG for AKARI/FIS: see Section 3.1.1 PSFs https://www.ir.isas.jaxa.jp/AKARI/Observation/support/FIS/IDUM/FIS_IDUM_1.3.pdf
\========= RESO_ORIG for AKARI/IRC: see Wada et al (2008) Table 5
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
\char |char |real |char |char |real |real |real |char |char | char |
\NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\========= AKARI ====================================================================================================
AKARI AKARI1 2.40 MJy/sr nuInu=cste 0.0012222222 N2 AKARI_IRC.N2.dat energy
AKARI AKARI2 3.20 MJy/sr nuInu=cste 0.0012222222 N3 AKARI_IRC.N3.dat energy
AKARI AKARI3 4.10 MJy/sr nuInu=cste 0.0012222222 N4 AKARI_IRC.N4.dat energy
AKARI AKARI4 7.00 MJy/sr nuInu=cste 0.0014166667 S7 AKARI_IRC.S7.dat energy
AKARI AKARI5 9.00 MJy/sr nuInu=cste 0.0014166667 S9W AKARI_IRC.S9W.dat energy
AKARI AKARI6 11.00 MJy/sr nuInu=cste 0.0014166667 S11 AKARI_IRC.S11.dat energy
AKARI AKARI7 15.00 MJy/sr nuInu=cste 0.0015000000 L15 AKARI_IRC.L15.dat energy
AKARI AKARI8 18.00 MJy/sr nuInu=cste 0.0015000000 L18W AKARI_IRC.L18W.dat energy
AKARI AKARI9 24.00 MJy/sr nuInu=cste 0.0015000000 L24 AKARI_IRC.L24.dat energy
AKARI AKARI10 65.00 MJy/sr nuInu=cste 0.010277778 N60 AKARI_FIS.N60.dat energy
AKARI AKARI11 90.00 MJy/sr nuInu=cste 0.010833333 WIDE-S AKARI_FIS.WIDE-S.dat energy
AKARI AKARI12 140.00 MJy/sr nuInu=cste 0.016111111 WIDE-L AKARI_FIS.WIDE-L.dat energy
AKARI AKARI13 160.00 MJy/sr nuInu=cste 0.016944444 N160 AKARI_FIS.N160.dat energy
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\========= Information for MIPS taken from SVO filter service and Spitzer MIPS handbook at IRSA
\========= https://irsa.ipac.caltech.edu/data/SPITZER/docs/mips/mipsinstrumenthandbook/
\========= https://irsa.ipac.caltech.edu/data/SPITZER/docs/mips/mipsinstrumenthandbook/MIPS_Instrument_Handbook.pdf
\========= RESO_ORIG are typical values taken from public legacy data (6, 18, 40", e.g. Meixner et al 2006)
\========= WAVE taken from mips instrument handbook, p99 of PDF
\========= Caution, the flux convention is not nuInu=cste, see Eq 4.2 of MIPS instrument handbook, p99. verified JPB 17/01/2023
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
\char |char |real |char |char |real |real |real |char |char | char |
\NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
MIPS MIPS1 23.675 MJy/sr MIPS 0.00166667 MIPS24 MIPSfiltsumm_24.txt energy
MIPS MIPS2 71.440 MJy/sr MIPS 0.00500000 MIPS70 MIPSfiltsumm_70.txt energy
MIPS MIPS3 155.899 MJy/sr MIPS 0.0111111 MIPS160 MIPSfiltsumm_160.txt energy
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\========= Information for SPIRE taken from SVO filter service and SPIRE handbook at IRSA
\========= https://irsa.ipac.caltech.edu/data/Herschel/docs/nhsc/spire/spire_om.pdf
\========= By default, DustEMWrap uses the transmission curves for extended sources (_E.dat)
\========= Point-sources transmission curves are provided (but commented here by default)
\========= RESO_ORIG [18.1,25.2,36.9"] are typical values taken from Matt Griffin SDP2009 slides
\=========
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
\char |char |real |char |char |real |real |real |char |char | char |
\NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\Following three lines for point source transmission curves
SPIRE SPIRE1 250.000 MJy/sr nuInu=cste 0.00502778 PSW Herschel_SPIRE.PSW.dat energy
SPIRE SPIRE2 350.000 MJy/sr nuInu=cste 0.00700000 PMW Herschel_SPIRE.PMW.dat energy
SPIRE SPIRE3 500.000 MJy/sr nuInu=cste 0.0102500 PLW Herschel_SPIRE.PLW.dat energy
\Following three lines for extended source transmission curves
\SPIRE SPIRE1 250.000 MJy/sr nuInu=cste 0.00502778 PSW Herschel_SPIRE.PSW_E.dat energy
\SPIRE SPIRE2 350.000 MJy/sr nuInu=cste 0.00700000 PMW Herschel_SPIRE.PMW_E.dat energy
\SPIRE SPIRE3 500.000 MJy/sr nuInu=cste 0.0102500 PLW Herschel_SPIRE.PLW_E.dat energy
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\========= Information for PACS taken from SVO filter service and PACS handbook at ESA
\========= https://www.cosmos.esa.int/documents/12133/996891/PACS+Explanatory+Supplement/
\========= RESO_ORIG [5.6, 6.8, 10.7] are from Table 4.3 of the handbook. Likely to be a lower limit for fast scanning mode obs (see Table 7.3)
\========= WAVE is from the reference wavelength quoted in PACS Explanatory Supplement, p142,143, Table 7.5. Verified JPB 17/01/2023
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
\char |char |real |char |char |real |real |real |char |char | char |
\NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
PACS PACS1 70.0 Jy/pixel nuInu=cste 0.001555556 PACS_BLUE Herschel_Pacs.blue.dat energy
PACS PACS2 100.0 Jy/pixel nuInu=cste 0.001888889 PACS_GREEN Herschel_Pacs.green.dat energy
PACS PACS3 160.0 Jy/pixel nuInu=cste 0.002972222 PACS_RED Herschel_Pacs.red.dat energy
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\========= RESO_ORIG from Lambda: [0.88 0.66 0.51 0.35 0.22]
\========= sigabs 1% from Guilaine Lagache (paper ?) but ...
\========= sigabs 0.1% from 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
\========= WAVE (computed from 23,33,41,61,94 GHz) taken from Bennett et al ApJSup 148:97–1172003, Tab1, frequency.
\========= Apparently the same as used in Miville Deschenes et al 2008, A&A 490, 1093–1102
\========= no confirmation in WMAP explanatory supplement ...
\========= IDL> print,cmic/([23,33,41,61,94.]*1.e9) = 13034.454 9084.6201 7312.0109 4914.6305 3189.2816
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
\char |char |real |char |char |real |real |real |char |char | char |
\NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
WMAP WMAP1 3189.2816 MJy/sr CMB 0.22 1.762 0.1 WMAP_W wmap_bandpass_W_v3.xcat energy
WMAP WMAP2 4914.6305 MJy/sr CMB 0.35 0.359 0.1 WMAP_V wmap_bandpass_V_v3.xcat energy
WMAP WMAP3 7312.0109 MJy/sr CMB 0.51 0.112 0.1 WMAP_Q wmap_bandpass_W_v3.xcat energy
WMAP WMAP4 9084.6201 MJy/sr CMB 0.66 0.049 0.1 WMAP_Ka wmap_bandpass_Ka_v3.xcat energy
WMAP WMAP5 13034.454 MJy/sr CMB 0.88 0.022 0.1 WMAP_K wmap_bandpass_K_v3.xcat energy
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\========= Information for MSX from SVO filter service and MSX handbooks at IRSA
\========= Transmission curves are in the PSC explanatory guide V1.2 (but not v2.3)
\========= https://irsa.ipac.caltech.edu/data/MSX/docs/MSX_psc_es.pdf
\========= https://irsa.ipac.caltech.edu/data/MSX/docs/msxpsc2.3_explguide.pdf
\========= https://irsa.ipac.caltech.edu/applications/MSX/MSX/imageDescriptions.htm
\========= https://heasarc.gsfc.nasa.gov/W3Browse/all/msxpsc.html
\========= RESO_ORIG values [18.3"] from Price et al (2001) corresponds to full res MSX Galactic Plane survey
\========= WAVE : MSX_psc_es.pdf clearly states how color correction should be done. I did not check that this is nuInu=cste (signed JPB)
\========= WAVE : MSX_psc_es.pdf uses ``isophotal'' wavelengths listed in Table 1 of the Explanatory Guide, which are the ones listed below
\========= NAME : Also consistent with msxpsc2.3_explguide.pdf
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
\char |char |real |char |char |real |real |real |char |char | char |
\NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
MSX MSX1 4.29 MJy/sr nuInu=cste 0.005083 MSXB1 MSX_MSX.B1.dat energy
MSX MSX2 4.35 MJy/sr nuInu=cste 0.005083 MSXB2 MSX_MSX.B2.dat energy
MSX MSX3 8.28 MJy/sr nuInu=cste 0.005083 MSXA MSX_MSX.A.dat energy
MSX MSX4 12.13 MJy/sr nuInu=cste 0.005083 MSXC MSX_MSX.C.dat energy
MSX MSX5 14.65 MJy/sr nuInu=cste 0.005083 MSXD MSX_MSX.D.dat energy
MSX MSX6 21.34 MJy/sr nuInu=cste 0.005083 MSXE MSX_MSX.E.dat energy
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\========= Information for BOLOCAM is from Bolocam website at CSO and Aguirre et al (2010)
\========= http://www.cso.caltech.edu/bolocam/ProposerInfo.html
\========= Origin of transmission file unknown
\========= RESO_ORIG [33"] is typical value for BGPS from Aguirre et al (2010)
\========= WAVE from Aguirre et al (2011) -- 271.1GHz = 0.0011058371650761754 m
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
\char |char |real |char |char |real |real |real |char |char | char |
\NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
BOLOCAM BOLOCAM1 1105.837165 MJy/sr nuInu=cste 0.0091666663 BOLOCAM_1p1mm bolocam_1p1.txt energy
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\========= Information for WISE from SVO filter service and WISE website
\========= Filters from http://wise2.ipac.caltech.edu/docs/release/prelim/expsup/sec4_3g.html#WISEZMA
\========= RESO_ORIG are typical values from https://wise2.ipac.caltech.edu/docs/release/allsky/
\========= WAVE values are isophotal wavelenghts given by Wright et al (2010)
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
\char |char |real |char |char |real |real |real |char |char | char |
\NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
WISE WISE1 3.35260 MJy/sr flambda=cste 0.0016944 W1 RSR-W1.EE.txt energy
WISE WISE2 4.60280 MJy/sr flambda=cste 0.0017778 W2 RSR-W2.EE.txt energy
WISE WISE3 11.5608 MJy/sr flambda=cste 0.0018055 W3 RSR-W3.EE.txt energy
WISE WISE4 22.0883 MJy/sr flambda=cste 0.0033333 W4 RSR-W4.EE.txt energy
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\========= Information for LABOCA from SVO filter service and APEX website
\========= http://www.apex-telescope.org/bolometer/laboca/technical/
\========= RESO_ORIG [18".6] is from http://www.apex-telescope.org/bolometer/laboca/technical/
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
\char |char |real |char |char |real |real |real |char |char | char |
\NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
LABOCA LABOCA1 876.000 MJy/sr LABOCA 0.005166667 LABOCA_345GHz laboca_passband_normalized.txt energy
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\========= Information for SABOCA from SVO filter service and APEX website
\========= http://www.apex-telescope.org/bolometer/saboca/technical/
\========= RESO_ORIG [7".8] is typical value from Ragan et al (2013)
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
\char |char |real |char |char |real |real |real |char |char | char |
\NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
SABOCA SABOCA1 357.000 MJy/sr SABOCA 0.0021666668 SABOCA_852GHz saboca_passband_normalized.txt energy
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\========= Information for GISMO is from IRAM wiki https://publicwiki.iram.es/Continuum/GISMO/Main
\========= RESO_ORIG [16".7] is from IRAM GISMO wiki
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
\char |char |real |char |char |real |real |real |char |char | char |
\NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
GISMO GISMO1 2000.00 MJy/sr nuInu=cste 0.0046389 GISMO_2mm GISMO_TRANSMISSION.txt
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\========= Information for DIRBE is from SVO filter service and LAMBDA
\========= https://lambda.gsfc.nasa.gov/product/cobe/c_spectral_res.html
\========= https://lambda.gsfc.nasa.gov/product/cobe/dirbe_exsup.html
\========= 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 0.7deg*0.7deg
\========= gives in MJy/sr in 1deg 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)
\========= WAVE taken from https://lambda.gsfc.nasa.gov/product/cobe/dirbe_exsup.html, chapt 2, tab 2.2-2. Verified JPB 17/01/2023
\========= NAME are not the names from the official documentation
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
\char |char |real |char |char |real |real |real |char |char | char |
\NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
DIRBE DIRBE1 1.25 MJy/sr nuInu=cste 1. 0.0007 3.1 DIRBE_1p25m COBE_DIRBE.1p25m.dat photon
DIRBE DIRBE2 2.2 MJy/sr nuInu=cste 1. 0.089 3.1 DIRBE_2p2m COBE_DIRBE.2p2m.dat photon
DIRBE DIRBE3 3.5 MJy/sr nuInu=cste 1. 0.00046 3.1 DIRBE_3p5m COBE_DIRBE.3p5m.dat photon
DIRBE DIRBE4 4.9 MJy/sr nuInu=cste 1. 0.00065 3.0 DIRBE_4p9m COBE_DIRBE.4p9m.dat photon
DIRBE DIRBE5 12.0 MJy/sr nuInu=cste 1. 0.001 5.1 DIRBE_12m COBE_DIRBE.12m.dat photon
DIRBE DIRBE6 25.0 MJy/sr nuInu=cste 1. 0.0025 15.1 DIRBE_25m COBE_DIRBE.25m.dat photon
DIRBE DIRBE7 60.0 MJy/sr nuInu=cste 1. 0.0052 10.4 DIRBE_60m COBE_DIRBE.60m.dat photon
DIRBE DIRBE8 100.0 MJy/sr nuInu=cste 1. 0.007 13.5 DIRBE_100m COBE_DIRBE.100m.dat photon
DIRBE DIRBE9 140.0 MJy/sr nuInu=cste 1. 0.766 10.6 DIRBE_140m COBE_DIRBE.140m.dat photon
DIRBE DIRBE10 240.0 MJy/sr nuInu=cste 1. 0.35 11.6 DIRBE_240m COBE_DIRBE.240m.dat photon
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\========= Information for ARCHEOPS from SVO filter service and Macias-Perez et al 2007 A&A 467, 1313–1344
\========= WAVE assumed to correspond to reference frequencies [545.,353.,217.,143.] GHz ==> [550.07791,849.27043,1381.5321,2096.4509] microns
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
\char |char |real |char |char |real |real |real |char |char | char |
\NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
ARCHEOPS ARCHEOPS1 550.07791 K CMB KS3.545GHz ARCHEOPS_KS3.545GHz.dat energy
ARCHEOPS ARCHEOPS2 849.27043 K CMB KS3.353GHz ARCHEOPS_KS3.353GHz.dat energy
ARCHEOPS ARCHEOPS3 1381.5321 K CMB KS3.217GHz ARCHEOPS_KS3.217GHz.dat energy
ARCHEOPS ARCHEOPS4 2096.4509 K CMB KS3.143GHz ARCHEOPS_KS3.143GHz.dat energy
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\========= Information for PLANCK HFI from SVO filter service and Planck-HFI DR3 products at IRSA
\========= https://irsa.ipac.caltech.edu/data/Planck/release_3/ancillary-data/HFI_Products.html
\========= The HFI flux convention forces compute cc using the official Planck routine
\========= RESO_ORIG from Planck wiki https://wiki.cosmos.esa.int/planck-legacy-archive/index.php/Beams
\========= in arcmin: [9.60,7.18,4.87,4.78,4.71,4.51]
\========= Origin of following uncertainty information unknown...
\========= sig-hit 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)
\========= WAVE from Planck collaboration, 2014, A&A 571, A9.
\========= It is assumed that the filter frequencies (857, 545,353,217, 143 100 GHz are the reference frequencies used for color correction. This is TBC)
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
\char |char |real |char |char |real |real |real |char |char | char |
\NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
HFI HFI1 349.81618 MJy/sr HFI 0.0735000 0.1219 7. HFI857GHz PLANCK_HFI.857GHz.dat energy
HFI HFI2 550.07791 MJy/sr HFI 0.0780000 0.118 7. HFI545GHz PLANCK_HFI.545GHz.dat energy
HFI HFI3 849.27043 MJy/sr HFI 0.0750000 0.0785 2. HFI353GHz PLANCK_HFI.353GHz.dat energy
HFI HFI4 1381.5321 MJy/sr HFI 0.0785000 0.075 2. HFI217GHz PLANCK_HFI.217GHz.dat energy
HFI HFI5 2096.4509 MJy/sr HFI 0.118000 0.075 2. HFI143GHz PLANCK_HFI.143GHz.dat energy
HFI HFI6 2997.9246 MJy/sr HFI 0.158833 0.0735 2. HFI100GHz PLANCK_HFI.100GHz.dat energy
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\========= Information for Planck LFI from SVO filter service and Planck-HFI DR3 products at IRSA
\========= https://irsa.ipac.caltech.edu/data/Planck/release_3/ancillary-data/LFI_Products.html
\========= RESO_ORIG from Planck wiki https://wiki.cosmos.esa.int/planckpla2015/index.php/Beams_LFI
\========= in deg: [0.53899997,0.45200002,0.22183333]
\========= WAVE same assumption as for HFI leads to: 4282.7494 6813.4647 9993.0817. This is also TBC
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
\char |char |real |char |char |real |real |real |char |char | char |
\NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
LFI LFI1 4282.7494 MJy/sr nuInu=cste 0.22183333 LFI70GHz PLANCK_LFI.070GHz.dat energy
LFI LFI2 6813.4647 MJy/sr nuInu=cste 0.45200000 LFI44GHz PLANCK_LFI.044GHz.dat energy
LFI LFI3 9993.0817 MJy/sr nuInu=cste 0.53900000 LFI30GHz PLANCK_LFI.030GHz.dat energy
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\========= Information for PRONAOS SPM
\====== There is no such document as a expalanory supplement for PRONAOS-SPM.
\====== The values below reflect the knowledge of JPB and what was done in the PRONAOS papers, in particular Pajot et al. 2006, A&A 447, 769–781
\====== WAVE from Pajot 2006. Verified JPB 17/01/2023
\====== RESO_ORIG from Pajot 2006, geometrical beam FWHM in tab 4 (2.0,2.0,2.5,3.5'). Verified JPB 17/01/2023
\====== FLUX_CONV assumed nuInu=cste, like in Pajot et al. 2006. Verified JPB 17/01/2023
\====== SIGABS taken to be 8%, as quoted in Pajot et al. 2006. Verified JPB 17/01/2023
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
\char |char |real |char |char |real |real |real |char |char | char |
\NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
SPM SPM1 200.00 MJy/sr nuInu=cste 0.0333333 8.0
SPM SPM2 260.00 MJy/sr nuInu=cste 0.0333333 8.0
SPM SPM3 360.00 MJy/sr nuInu=cste 0.0416667 8.0
SPM SPM4 580.00 MJy/sr nuInu=cste 0.0583333 8.0
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\========= Information for ISOCAM
\========= reso_orig values arbitrary
\========= sighit values arbitrary
\========= sigabs values arbitrary
\========= WAVE taken from ISOCAM Handbook : http://general-tools.cosmos.esa.int/iso/manuals/HANDBOOK/cam_hb/ p97 (color correction) and Tab. 2.3 (SW filters) and 2.4 (LW filters). Verified JPB 17/01/2023
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
\char |char |real |char |char |real |real |real |char |char | char |
\NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
ISOCAM ISOCAM1 2.80 MJy/sr nuInu=cste 0.0633333 0.04 5.1 SW4 ISOCAM_SW4_transmission.xcat photon
ISOCAM ISOCAM2 3.00 MJy/sr nuInu=cste 0.0633333 0.04 5.1 SW7 ISOCAM_SW7_transmission.xcat photon
ISOCAM ISOCAM3 3.30 MJy/sr nuInu=cste 0.0633333 0.04 5.1 SW2 ISOCAM_SW2_transmission.xcat photon
ISOCAM ISOCAM4 3.60 MJy/sr nuInu=cste 0.0633333 0.04 5.1 SW1 ISOCAM_SW1_transmission.xcat photon
ISOCAM ISOCAM5 3.70 MJy/sr nuInu=cste 0.0633333 0.04 5.1 SW6 ISOCAM_SW6_transmission.xcat photon
ISOCAM ISOCAM6 3.90 MJy/sr nuInu=cste 0.0633333 0.04 5.1 SW9 ISOCAM_SW9_transmission.xcat photon
ISOCAM ISOCAM7 4.05 MJy/sr nuInu=cste 0.0633333 0.04 5.1 SW8 ISOCAM_SW8_transmission.xcat photon
ISOCAM ISOCAM8 4.00 MJy/sr nuInu=cste 0.0633333 0.04 5.1 SW5 ISOCAM_SW5_transmission.xcat photon
ISOCAM ISOCAM9 4.26 MJy/sr nuInu=cste 0.0633333 0.04 5.1 SW11 ISOCAM_SW11_transmission.xcat photon
ISOCAM ISOCAM10 4.50 MJy/sr nuInu=cste 0.0633333 0.04 5.1 SW3 ISOCAM_SW3_transmission.xcat photon
ISOCAM ISOCAM11 4.50 MJy/sr nuInu=cste 0.0633333 0.04 5.1 LW1 ISOCAM_LW1_transmission.xcat photon
ISOCAM ISOCAM12 4.60 MJy/sr nuInu=cste 0.0633333 0.04 5.1 SW10 ISOCAM_SW10_transmission.xcat photon
ISOCAM ISOCAM13 6.00 MJy/sr nuInu=cste 0.0633333 0.04 5.1 LW4 ISOCAM_LW4_transmission.xcat photon
ISOCAM ISOCAM14 6.80 MJy/sr nuInu=cste 0.0633333 0.04 5.1 LW5 ISOCAM_LW5_transmission.xcat photon
ISOCAM ISOCAM15 6.70 MJy/sr nuInu=cste 0.0633333 0.04 5.1 LW2 ISOCAM_LW2_transmission.xcat photon
ISOCAM ISOCAM16 7.70 MJy/sr nuInu=cste 0.0633333 0.04 5.1 LW6 ISOCAM_LW6_transmission.xcat photon
ISOCAM ISOCAM17 9.60 MJy/sr nuInu=cste 0.0633333 0.04 5.1 LW7 ISOCAM_LW7_transmission.xcat photon
ISOCAM ISOCAM18 11.30 MJy/sr nuInu=cste 0.0633333 0.04 5.1 LW8 ISOCAM_LW8_transmission.xcat photon
ISOCAM ISOCAM19 12.00 MJy/sr nuInu=cste 0.0633333 0.04 5.1 LW10 ISOCAM_LW10_transmission.xcat photon
ISOCAM ISOCAM20 14.30 MJy/sr nuInu=cste 0.0633333 0.04 5.1 LW3 ISOCAM_LW3_transmission.xcat photon
ISOCAM ISOCAM21 14.90 MJy/sr nuInu=cste 0.0633333 0.04 5.1 LW9 ISOCAM_LW9_transmission.xcat photon
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\========= Information for ISOPHOTP
\========= reso_orig values arbitrary
\========= sighit values arbitrary
\========= sigabs values arbitrary
\========= WAVE, NAME from http://general-tools.cosmos.esa.int/iso/manuals/HANDBOOK/pht_hb/ p233 for color correction, Tab 2.2 for lambda_ref
\========= WAVE, NAME Verified JPB 17/01/2023
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
\char |char |real |char |char |real |real |real |char |char | char |
\NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
ISOPHOTP ISOPHOTP1 3.30 MJy/sr nuInu=cste 0.0633333 0.04 5.1 P3.29
ISOPHOTP ISOPHOTP2 3.60 MJy/sr nuInu=cste 0.0633333 0.04 5.1 P3.6
ISOPHOTP ISOPHOTP3 4.80 MJy/sr nuInu=cste 0.0633333 0.04 5.1 P4.85
ISOPHOTP ISOPHOTP4 7.30 MJy/sr nuInu=cste 0.0633333 0.04 5.1 P7.3
ISOPHOTP ISOPHOTP5 7.70 MJy/sr nuInu=cste 0.0633333 0.04 5.1 P7.7
ISOPHOTP ISOPHOTP6 10.0 MJy/sr nuInu=cste 0.0633333 0.04 5.1 P10
ISOPHOTP ISOPHOTP7 11.30 MJy/sr nuInu=cste 0.0633333 0.04 5.1 P11.3
ISOPHOTP ISOPHOTP8 12.00 MJy/sr nuInu=cste 0.0633333 0.04 5.1 P11.5
ISOPHOTP ISOPHOTP9 12.80 MJy/sr nuInu=cste 0.0633333 0.04 5.1 P12.8
ISOPHOTP ISOPHOTP10 15.00 MJy/sr nuInu=cste 0.0633333 0.04 5.1 P16
ISOPHOTP ISOPHOTP11 20.00 MJy/sr nuInu=cste 0.0633333 0.04 5.1 P20
ISOPHOTP ISOPHOTP12 25.00 MJy/sr nuInu=cste 0.0633333 0.04 5.1 P25
ISOPHOTP ISOPHOTP13 60.00 MJy/sr nuInu=cste 0.0633333 0.04 5.1 P60
ISOPHOTP ISOPHOTP14 100.0 MJy/sr nuInu=cste 0.0633333 0.04 5.1 P100
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\========= Information for ISOPHOT C
\========= reso_orig values arbitrary
\========= sighit values arbitrary
\========= sigabs values arbitrary
\========= WAVE, NAME from http://general-tools.cosmos.esa.int/iso/manuals/HANDBOOK/pht_hb/ p233 for color correction, Tab 2.2 for lambda_ref
\========= WAVE, NAME Verified JPB 17/01/2023
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
\char |char |real |char |char |real |real |real |char |char | char |
\NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
ISOPHOTC ISOPHOTC1 65.00 MJy/sr nuInu=cste 0.0633333 0.04 5.1 C50 ISO_PHT-C.50mu.dat energy
ISOPHOTC ISOPHOTC2 60.00 MJy/sr nuInu=cste 0.0633333 0.04 5.1 C60 ISO_PHT-C.60mu.dat energy
ISOPHOTC ISOPHOTC3 80.00 MJy/sr nuInu=cste 0.0633333 0.04 5.1 C70 ISO_PHT-C.70mu.dat energy
ISOPHOTC ISOPHOTC4 90.00 MJy/sr nuInu=cste 0.0633333 0.04 5.1 C90 ISO_PHT-C.90mu.dat energy
ISOPHOTC ISOPHOTC5 100.00 MJy/sr nuInu=cste 0.0633333 0.04 5.1 C100 ISO_PHT-C.100mu.dat energy
ISOPHOTC ISOPHOTC6 105.00 MJy/sr nuInu=cste 0.0633333 0.04 5.1 C105 ISO_PHT-C.105mu.dat energy
ISOPHOTC ISOPHOTC7 120.00 MJy/sr nuInu=cste 0.0633333 0.04 5.1 C120 ISO_PHT-C.120mu.dat energy
ISOPHOTC ISOPHOTC8 150.00 MJy/sr nuInu=cste 0.0633333 0.04 5.1 C135 ISO_PHT-C.135mu.dat energy
ISOPHOTC ISOPHOTC9 170.00 MJy/sr nuInu=cste 0.0633333 0.04 5.1 C160 ISO_PHT-C.160mu.dat energy
ISOPHOTC ISOPHOTC10 180.00 MJy/sr nuInu=cste 0.0633333 0.04 5.1 C180 ISO_PHT-C.180mu.dat energy
ISOPHOTC ISOPHOTC11 200.00 MJy/sr nuInu=cste 0.0633333 0.04 5.1 C200 ISO_PHT-C.200mu.dat energy
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\================ DUMMY FILTER, DO NOT DELETE!
\================ This last dummy filter needs to be included so that DustEMWrap copes with spectral data
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\INSTRU |FILTER |WAVE |BUNIT |FLUX_CONV |RESO_ORIG |SIGHIT |SIGABS |NAME |FILENAME | TTYPE |
\char |char |real |char |char |real |real |real |char |char | char |
\NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL |NULL | NULL |
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
UNKNOWN SPECTRUM -32768. MJy/sr NONE 0
\-------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
\===============FILTERS AND MODIFS PLANNED FOR FUTURE RELEASES===================================
\============== http://svo2.cab.inta-csic.es/theory/fps3/index.php================================
\==== Priority A
\ 2MASS - J,H, Ks
\ BLAST - 250, 350, 500
\ IRSF - J H Ks
\ WMAP -- cross check SVO
\ ISO -- cross check SVO
\ SPT
\ JCMT
\ UKIRT
\ APEX -- cross check SVO, add current instruments
\ SOFIA instruments
\ IRAM -- MAMBO2
\==== Priority B
\ PANSTARRS IR
\ BOOMERANG
\ TOPHAT
\ MAXIMA
\ OLIMPO
\ QUIJOTE
\ SPIDER
\ BICEP
\ Subaru IR instruments
\ LMT
\ HST NIR instruments
\ Gemini IR instruments
\ CFHT IR instruments
\ Keck IR instruments
\ Euclid IR instruments
\ Roman (WFIRST) IR instruments
\ LaSilla IR instruments
\ Paranal IR instruments
\==== Priority C
\ NIRT/IRTF
\ NOAO/NEWFIRM
\ CAHA IR instruments
\ NIRT/IRTF
\ LCO IR
\ AAO IR
\ CTIO IR
\ LICK IR
\ GTC IR
\ OVRO / Polatron
\ WHT IR instruments
\ Paranal UV/VIS instruments
\ HST UV/VIS
\ DENIS J Ks
\==== Priority D
\ Liverpool IR
\ MKO IR
\=============== END FILE instrument_description_DEV_VERSION.xcat ===================================