AKARI/IRC MIR-S slit-less spectroscopic catalogue (Yamagishi+, accepted) ================================================================================ AKARI/IRC MIR-S slit-less spectroscopic catalogue (Ver. 1.0) Yamagishi M., Yamamura I., Mizuki T., Ootsubo T., Baba S., Usui F., Onaka T. ================================================================================ ADC_Keywords: Spectroscopy, infrared ; IR Mission_Name: AKARI Description: A catalogue of mid-infrared slit-less spectra (5.5-12.5 um) extracted from the AKARI/IRC MIR-S spectroscopic observation data. All 886 MIR-S spectroscopic data obtained in Phases 1&2 are analyzed, and 862 spectra of 604 individual sources that are little contaminated by nearby sources are catalogued. We also present a 9 um point source catalogue generated as a by-product. The point source catalogue contains 42,387 sources brighter than 0.3 mJy. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe.txt 80 . This file ReaseNote.txt . . Release note AKARI_MIR-S_slit-less_spec_v1.0.dat 119 862 List of objects [WorkID].dat 26 96 Flux-recalibrated spectrum [WorkID].png . 862 Plot of the spectra [WorkID]_SG1_[long, short].spc 52 58 Toolkit-output SG1 spectrum(1) [WorkID]_SG2_[long, short].spc 52 61 Toolkit-output SG2 spectrum(1) [WorkID]_SG1_[long, short].png . 862 Toolkit-output SG1 image [WorkID]_SG2_[long, short].png . 862 Toolkit-output SG2 image refimage_[WorkID].png . 862 Position of the target on the reference image [ObsID]_S9W_[long, short].fits.gz . 884 Reference image(2) AKARI_MIR-S_slit-less_PSC_v1.0.dat 142 42,837 9 um point source catalogue (AKARI MIR-S slit-less PSC) -------------------------------------------------------------------------------- Note (1): The number of lines depends on the spectrum extraction condition. SG1: 59 or 59 lines, SG2: 61, 62, or 63 lines Note (2): Long- and short-exposure images are available for 884 and 879 observations, respectively, out of 886 observations. -------------------------------------------------------------------------------- Byte-by-byte Description of file: AKARI_MIR-S_slit-less_spec_v1.0.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1-17 A17 --- WorkID WorkID (1) 19-37 A19 --- ObjID Object ID in the AKARI MIR-S slit-less PSC ver. 1.0 39-40 A2 --- Grade Quality flag of the spectrum 42-50 F9.5 deg RAdeg Right Ascension (J2000) 52-60 F9.5 deg DECdeg Declination (J2000) 62-70 E9.3 mJy Flux_phot Photometric flux density at 9 micron (Flux_ape) retrieved from the AKARI MIR-S slit-less PSC ver. 1.0 72-79 E8.2 mJy Flux_phot_err Error of Flux_ape 81-84 F5.3 --- SF_SG1 ?=NaN Absolute flux calibration factor SG1 86-89 F5.3 --- SF_SG1_err ?=NaN Error of SF_SG1 91-94 F5.3 --- SF_SG2 ?=NaN Absolute flux calibration factor SG2 96-99 F5.3 --- SF_SG2_err ?=NaN Error of SF_SG2 101-110 A10 --- ObsDate Observation date 112-119 A8 --- ObsTime Observation time -------------------------------------------------------------------------------- Note (1): WorkID is given in the format of [ObsID]_[SourceID]_[Exposure]. ObsID: Obervation ID, SourceID: source ID defined in each observation, Exposure: source is detected in long (L) or short (S) exposure image. -------------------------------------------------------------------------------- Byte-by-byte Description of file: [WorkID].dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1-6 F6.3 micron Wavelength Observed wavelength 8-16 F9.3 mJy Flux Flux density 18-26 F9.3 mJy Flux_err Error of Flux -------------------------------------------------------------------------------- Byte-by-byte Description of file: [WorkID]_[SG1, SG2]_[long, short].spc -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1-13 F13.4 micron Wavelength Observed wavelength 14-26 F13.4 mJy Flux ?=NaN Flux density 27-39 F13.4 mJy Flux_err_L ?=NaN Lower end of flux error 40-52 F13.4 mJy Flux_err_U ?=NaN Upper end of flux error -------------------------------------------------------------------------------- Byte-by-byte Description of file: AKARI_MIR-S_slit-less_PSC_v1.0.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1-19 A19 --- Name Source name 21-29 F9.5 deg RAdeg Right Ascension (J2000) 31-39 F9.5 deg DEdeg Declination (J2000) 41-49 E9.3 uJy Flux_ape ?=NaN Flux density measured by aperture photometry 51-58 E8.2 uJy Fluxerr_ran_ape ?=NaN Random error of Flux_ape 60-67 E8.2 uJy Fluxerr_sys_ape ?=NaN Systematic calibration error of Flux_ape 69-77 E9.3 uJy Flux_PSF Flux density measured by PSF photometry 79-86 E8.2 uJy Fluxerr_ran_PSF Random error of Flux_PSF 88-95 E8.2 uJy Fluxerr_sys_PSF Systematic calibration error of Flux_PSF 97-98 I2.0 --- Ndet Number of detections 100-100 I1.0 --- Nsource1 Number of nearby objects within a radius of 1 FWHM (3."0) 102-103 I2.0 --- Nsource2 Number of nearby objects within a radius of 20 pixels (23."4) 105-120 A16 --- desig_2MASS ?=---------------- Designation of 2MASS PSC source 122-140 A19 --- desig_WISE ?=J------.---------.- Designation of WISE PSC source 142-142 I1.0 --- Spec_available 1=MIR-S slit-less spectrum is available 0=MIR-S slit-less spectrum is unavailable -------------------------------------------------------------------------------- History: 08-Nov-2018: Documentation prepared at ISAS/JAXA by Mitsuyoshi Yamagishi ================================================================================ (End) Mitsuyoshi Yamagishi [ISAS/JAXA] 08-Nov-2018