The $AKARI$ Far-Infrared All-Sky Survey Maps

Abstract

We present a far-infrared all-sky atlas from a sensitive all-sky survey using the Japanese $AKARI$ satellite. The survey covers $>99$% of the sky in four photometric bands centred at 65 $\mu$m, 90 $\mu$m, 140 $\mu$m, and 160 $\mu$m with spatial resolutions ranging from 1 to 1.5 arcmin. These data provide crucial information for the investigation and characterisation of the properties of dusty material in the Interstellar Medium (ISM), since significant portion of its energy is emitted between $\sim$50 and 200 $\mu$m. The large-scale distribution of interstellar clouds, their thermal dust temperatures and column densities, can be investigated with the improved spatial resolution compared to earlier all-sky survey observations. In addition to the point source distribution, the large-scale distribution of ISM cirrus emission, and its filamentary structure, are well traced. We have made the first public release of the full-sky data to provide a legacy data set for use by the astronomical community.

arXiv comment22 pages, 18 figures, accepted to PASJ

References in corpus (41)

• Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds
• Star Formation in Galaxies Along the Hubble Sequence
• Herschel Space Observatory - An ESA facility for far-infrared and submillimetre astronomy
• Interstellar Dust Grains
• The Photodetector Array Camera and Spectrometer (PACS) on the Herschel Space Observatory
• Infrared Emission from Interstellar Dust. IV. The Silicate-Graphite-PAH Model in the Post-Spitzer Era
• Planck 2013 results. I. Overview of products and scientific results
• From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey
• The Infrared Astronomical Mission AKARI
• Planck 2013 results. XI. All-sky model of thermal dust emission
• Characterizing interstellar filaments with Herschel in IC5146
• The COBE Diffuse Infrared Background Experiment Search for the Cosmic Infrared Background: II. Model of the Interplanetary Dust Cloud
• IRIS: A new generation of IRAS maps
• Planck Early Results: All sky temperature and dust optical depth from Planck and IRAS: Constraints on the "dark gas" in our galaxy
• The Infrared Camera (IRC) for AKARI - Design and Imaging Performance
• The global dust SED: Tracing the nature and evolution of dust with DustEM
• The XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST)
• The Far-Infrared Surveyor (FIS) for AKARI
• The Taurus Spitzer Survey: New Candidate Taurus Members Selected Using Sensitive Mid-Infrared Photometry
• The Aquila prestellar core population revealed by Herschel
• Herschel-SPIRE observations of the Polaris flare : structure of the diffuse interstellar medium at the sub-parsec scale
• Infrared Emission from the Radio Supernebula in NGC 5253: A Proto-Globular Cluster?
• VLBA determination of the distance to nearby star-forming regions II. Hubble 4 and HDE 283572 in Taurus
• Formation and evolution of interstellar filaments; Hints from velocity dispersion measurements
• Angular Power Spectra of the COBE DIRBE Maps
• A Herschel study of the properties of starless cores in the Polaris Flare dark cloud region using PACS and SPIRE
• Statistical properties of dust far-infrared emission
• Modeling Thermal Dust Emission with Two Components: Application to the Planck HFI Maps
• Power spectrum of the cosmic infrared background at 60 and 100 microns with IRAS
• Dust in the diffuse emission of the galactic plane - The Herschel/Spitzer SED fitting
• Flight Performance of the AKARI Cryogenic System
• Calibration and Performance of the AKARI Far-Infrared Surveyor (FIS) -- Slow-Scan Observation Mode for Point Sources
• Calibration of the AKARI Far-infrared All Sky Survey Maps
• The AKARI FIS YSO Catalogue
• Cryogenic Capacitive Transimpedance Amplifier for Astronomical Infrared Detectors
• Direct Estimate of Cirrus Noise in Herschel Hi-GAL Images
• Sky Confusion Noise in the Far-Infrared: Cirrus, Galaxies and the Cosmic Far-Infrared Background
• Search for young low-mass stars in a ROSAT selected sample south of the Taurus-Auriga molecular clouds
• Small-scale structure of the galactic cirrus emission
• BLAST05: Power Spectra of Bright Galactic Cirrus at Submillimeter Wavelengths
• A survey of T Tauri stars with AKARI toward the Taurus-Auriga region

Cited by in corpus (79)

• FOREST Unbiased Galactic plane Imaging survey with the Nobeyama 45-m telescope (FUGIN) I: Project Overview and Initial Results
• An Improved Model of Diffuse Galactic Radio Emission from 10 MHz to 5 THz
• Planck intermediate results. XXIX. All-sky dust modelling with Planck, IRAS, and WISE observations
• A census of dense cores in the Taurus L1495 cloud from the Herschel Gould Belt Survey
• Discovery of Magnetic Fields Along Stacked Cosmic Filaments as Revealed by Radio and X-Ray Emission
• Galactic cold cores VI. Dust opacity spectral index
• Planck's view on the spectrum of the Sunyaev-Zeldovich effect
• The JCMT BISTRO Survey: Magnetic Fields Associated with a Network of Filaments in NGC 1333
• ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP) II. Survey overview: a first look at 1.3 mm continuum maps and molecular outflows
• Predicting dust extinction properties of star-forming galaxies from H-alpha/UV ratio
• Classification of Magnetohydrodynamic Simulations using Wavelet Scattering Transforms
• On the different levels of dust attenuation to nebular and stellar light in star-forming galaxies
• Calibration of the AKARI Far-infrared All Sky Survey Maps
• XMMPZCAT: A catalogue of photometric redshifts for X-ray sources
• The AKARI 2.5-5 Micron Spectra of Luminous Infrared Galaxies in the Local Universe
• The Gaia-ESO Survey: Structural and dynamical properties of the young cluster Chamaeleon I
• Planck far-infrared detection of Hyper Suprime-Cam protoclusters at $\mathbf{z}\sim 4$: hidden AGN and star formation activity
• A star formation study of the ATLAS3D early-type galaxies with the AKARI all-sky survey
• Constraints on AGN feedback from its Sunyaev-Zel'dovich imprint on the cosmic background radiation
• Dust properties in the cold and hot gas phases of the ATLAS3D early-type galaxies as revealed by AKARI
• A new study on a type Iax stellar remnant and its probable association with SN 1181
• A systematic study of Galactic infrared bubbles along the Galactic plane with AKARI and Herschel
• Modeling of the zodiacal emission for the AKARI/IRC mid-infrared all-sky diffuse maps
• Investigation of the Origin of the Anomalous Microwave Emission in Lambda Orionis
• Broadband spectral energy distributions of SDSS-selected quasars and of their host galaxies: intense activity at the onset of AGN feedback
• COMAP Early Science: VI. A First Look at the COMAP Galactic Plane Survey
• The extreme colliding-wind system Apep: resolved imagery of the central binary and dust plume in the infrared
• Mid- and far-infrared properties of Spitzer Galactic bubbles revealed by the AKARI all-sky surveys
• The Lyman Alpha Reference Sample XI: Efficient Turbulence Driven Lyα Escape and the Analysis of IR, CO and [C II]158 μm
• The 1.1 mm Continuum Survey of the Small Magellanic Cloud: Physical Properties and Evolution of the Dust-selected Clouds
• 3D structure of HII region Sh2-235 from tunable-filter optical observations
• Demographics of Protoplanetary Disks: A Simulated Population of Edge-on Systems
• Molecular Cloud Cores with High Deuterium Fractions: Nobeyama Mapping Survey
• Size Dependence of Dust Distribution around the Earth Orbit
• Discovery of a strong ionized-gas outflow in an AKARI-selected Ultra-luminous Infrared Galaxy at z = 0.5
• Environmental impacts on dust temperature of star-forming galaxies in the local Universe
• Low frequency radio continuum imaging and SED modeling of 11 LIRGs: radio-only and FUV to radio bands
• Polycyclic aromatic hydrocarbon emission toward the Galactic bulge
• AKARI far-infrared maps of the zodiacal dust bands
• A Relationship of Polycyclic Aromatic Hydrocarbon Features with Galaxy Merger in Star-forming Galaxies at $z<0.2$
• Radio-Infrared Correlation for Local Dusty Galaxies and Dusty AGNs from the AKARI All Sky Survey
• The SCUBA-2 Ambitious Sky Survey: a catalogue of beam-sized sources in the Galactic longitude range 120 to 140
• A Low Frequency Pilot Survey of Southern HII Regions in the Vela Constellation
• MaLeFiSenta: Machine Learning for FilamentS Identification and orientation in the ISM
• Asteroseismic age constraints on the open cluster NGC 2477 using oscillating stars identified with TESS FFI
• Infrared Colours and Spectral Energy Distributions of Hard X-ray Selected Obscured and Compton-thick AGN
• The Nearby Evolved Stars Survey: I. JCMT/SCUBA-2 Sub-millimetre detection of the detached shell of U Antliae
• CMB Shadows: The Effect of Interstellar Extinction on Cosmic Microwave Background Polarization and Temperature Anisotropy
• The young stellar population of Lynds 1340. An infrared view
• Heliocentric Distance Dependence of Zodiacal Light Observed by Hayabusa2#
• Surface Brightness Correction for Compact Extended Sources Observed by the AKARI Far-Infrared Surveyor (FIS) in the Slow-Scan Mode
• Bayesian decomposition of the Galactic multi-frequency sky using probabilistic autoencoders
• The effects of stellar feedback on molecular clumps in the Lagoon Nebula (M8)
• Star and Cluster Formation in the Sh2-112 Filamentary Cloud Complex
• Herschel-PACS photometry of faint stars
• How long can LBVs sleep? A long-term photometric vaiability and spectral study of the Galactic candidate luminous blue variable MN112
• Dust Mass Associated with the Supernova Remnant IC 443 when Emission Meets Extinction
• Sharpening up Galactic all-sky maps with complementary data - A machine learning approach
• Searching for giant planets in the outer Solar System with far-infrared all-sky surveys
• AKARI Mission Program: Excavating Mass Loss History in Extended Dust Shells of Evolved Stars (MLHES) I. Far-IR Photometry
• A source of gamma rays coincident with the shell of the supernova remnant CTB 80
• On Surface Brightness and Flux Calibration for Point and Compact Extended Sources in the AKARI Far-IR All-Sky Survey (AFASS) Maps
• Modelling the diffuse dust emission around Orion
• Nearly Full-Sky Low-Multipole Cosmic Microwave Temperature Anisotropy: I. Foreground Cleaned Maps
• AMI-CL J0300+2613: a Galactic anomalous-microwave-emission ring masquerading as a galaxy cluster
• Near-Ultraviolet Radiation toward Molecular Cloud N4 in W 50/SS 433: Evidence for Direct Interaction of the Jet with Molecular Cloud
• Mid-infrared spectroscopy of zodiacal emission with AKARI/IRC
• Relation of internal attenuation, dust emission, and the size of spiral galaxies. Calibration at low-z and how to use it as a cosmological test at high-z
• Infrared observations of the flaring maser source G358.93-0.03 -- SOFIA confirms an accretion burst from a massive young stellar object
• Fermi-bubble bulk and edge analysis reveals dust, cooling breaks, and cosmic-ray diffusion, facilitating a self-consistent model
• Space Missions for Astronomy and Astrophysics in Korea: Past, Present, and Future
• Image Stacking Analysis of SDSS Galaxies with AKARI Far-Infrared Surveyor Maps at 65μm, 90μm, and 140μm
• Millimeter-wave CO and SiO Observations toward the Broad-velocity-width Molecular Feature CO 16.134-0.553: a Smith cloud scenario?
• A Gaia view on the star formation in the Monoceros OB1 and R1 associations
• Gamma-ray emission toward supergiant shells in the Large Magellanic Cloud
• The peculiar nebula Simeis 57: II. Distance, nature and excitation
• Detection of polarized Fermi-bubble synchrotron and dust emission
• A likely detection of a local interplanetary dust cloud passing near the Earth in the AKARI mid-infrared all-sky map
• The dusty envelopes of asymptotic giant branch stars with ultraviolet excesses