A Full-Sky H-alpha Template for Microwave Foreground Prediction
arXiv:astro-ph/0301558 · doi:10.1086/374411
Abstract
A full-sky H-alpha map with 6 arcmin (FWHM) resolution is presented. This map is a composite of the Virginia Tech Spectral line Survey (VTSS) in the north and the Southern H-Alpha Sky Survey Atlas (SHASSA) in the south. The Wisconsin H-Alpha Mapper (WHAM) survey provides a stable zero-point over 3/4 of the sky on a 1 degree scale. This composite map can be used to provide limits on thermal bremsstrahlung (free-free emission) from ionized gas known to contaminate microwave-background data. The map is available on the WWW for public use.
20 pages, 7 figures, ApJS in press, get data at http://skymaps.info
Cited by in corpus (371)
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
- Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results
- Three Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Polarization Analysis
- A New Electron Density Model for Estimation of Pulsar and FRB Distances
- Giant Gamma-ray Bubbles from Fermi-LAT: AGN Activity or Bipolar Galactic Wind?
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Foreground Emission
- Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Temperature Analysis
- Fast Radio Burst Discovered in the Arecibo Pulsar ALFA Survey
- The Galactic O-Star Spectroscopic Survey (GOSSS). II. Bright Southern Stars
- Detection of non-Gaussianity in the WMAP 1-year data using spherical wavelets
- Planck 2018 results. IV. Diffuse component separation
- Radio observational constraints on Galactic 3D-emission models
- The warm ionized medium in spiral galaxies
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Angular Power Spectra
- The Aao/Ukst Supercosmos H-alpha Survey (SHS)
- Correlation of CMB with large-scale structure: I. ISW Tomography and Cosmological Implications
- Microwave ISM Emission Observed by WMAP
- The Vertical Structure of Warm Ionised Gas in the Milky Way
- Joint Bayesian component separation and CMB power spectrum estimation
- A full sky, low foreground, high resolution CMB map from WMAP
- Planck 2013 results. XII. Component separation
- Hemispherical power asymmetry in the three-year Wilkinson Microwave Anisotropy Probe sky maps
- Planck 2015 results. IX. Diffuse component separation: CMB maps
- The pre-launch Planck Sky Model: a model of sky emission at submillimetre to centimetre wavelengths
- The outer scale of turbulence in the magneto-ionized Galactic interstellar medium
- Extended Anomalous Foreground Emission in the WMAP 3-Year Data
- Correlation of CMB with large-scale structure: II. Weak lensing
- Separation of anomalous and synchrotron emissions using WMAP polarization data
- High sensitivity measurements of the CMB power spectrum with the extended Very Small Array
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Galactic Foreground Emission
- Planck early results. XX. New light on anomalous microwave emission from spinning dust grains
- An Improved Model of Diffuse Galactic Radio Emission from 10 MHz to 5 THz
- Evidence Of Dark Matter Annihilations In The WMAP Haze
- Non-Gaussian Signatures in the Temperature Fluctuation Observed by the Wilkinson Microwave Anisotropy Probe
- The non-Gaussian Cold Spot in WMAP: significance, morphology and foreground contribution
- A determination of the Spectra of Galactic components observed by WMAP
- A Survey of Extragalactic Faraday Rotation at High Galactic Latitude: The Vertical Magnetic Field of the Milky Way towards the Galactic Poles
- MILCA, a Modified Internal Linear Combination Algorithm to extract astrophysical emissions from multi-frequency sky maps
- A new, large-scale map of interstellar reddening derived from HI emission
- The Kinematics of the Scorpius-Centaurus OB Association from Gaia DR1
- Observations of the Large Magellanic Cloud with Fermi
- M Dwarfs in SDSS Stripe 82: Photometric Light Curves and Flare Rate Analysis
- CMB component separation by parameter estimation
- Properties of the dense core population in Orion B as seen by the Herschel Gould Belt survey
- Fermi Large Area Telescope observations of Local Group galaxies: Detection of M31 and search for M33
- The Dark Universe
- Correlating the CMB with Luminous Red Galaxies : The Integrated Sachs-Wolfe Effect
- The State-of-Play of Anomalous Microwave Emission (AME) Research
- Spinning dust emission: the effect of rotation around a non-principal axis
- Magnetic Fields in Large Diameter HII Regions Revealed by the Faraday Rotation of Compact Extragalactic Radio Sources
- A needlet ILC analysis of WMAP 7-year data: estimation of CMB temperature map and power spectrum
- Low-order multipole maps of CMB anisotropy derived from WMAP
- Planck 2015 results. XXV. Diffuse low-frequency Galactic foregrounds
- The Spectrum of the Diffuse Galactic Light I: The Milky Way in Scattered Light
- Modelling the Galactic distribution of free electrons
- OB associations and their origins
- Warm-Hot Gas in and around the Milky Way: Detection and Implications of OVII Absorption toward LMC X-3
- Microwave ISM Emission in the Green Bank Galactic Plane Survey: Evidence for Spinning Dust
- The HIPASS survey of the Galactic plane in Radio Recombination Lines
- Multipole vector anomalies in the first-year WMAP data: a cut-sky analysis
- Assessing the effects of foregrounds and sky removal in WMAP
- Linear polarization structures in LOFAR observations of the interstellar medium in the 3C196 field
- A Sino-German lambda6 cm polarization survey of the Galactic plane I. Survey strategy and results for the first survey region
- Detection of the Small Magellanic Cloud in gamma-rays with Fermi/LAT
- A Sino-German 6cm polarization survey of the Galactic plane VII. Small supernova remnants
- A catalogue of integrated H-alpha fluxes for 1,258 Galactic planetary nebulae
- Exact likelihood evaluations and foreground marginalization in low resolution WMAP data
- Bianchi Type VII_h Models and the WMAP 3-year Data
- Structure in the Rotation Measure Sky
- ARCADE 2 Observations of Galactic Radio Emission
- Cross-correlation of CMB with large-scale structure: weak gravitational lensing
- Optically thick HI dominant in the local interstellar medium; an alternative interpretation to "dark gas"
- DESI 2024 II: Sample Definitions, Characteristics, and Two-point Clustering Statistics
- Planck intermediate results. XIV. Dust emission at millimetre wavelengths in the Galactic plane
- The Coherent Magnetic Field of the Milky Way
- Fast and Efficient Template Fitting of Deterministic Anisotropic Cosmological Models Applied to WMAP Data
- A re-analysis of the three-year WMAP temperature power spectrum and likelihood
- Properties of Galactic cirrus clouds observed by BOOMERanG
- Anomalous parity asymmetry of WMAP power spectrum data at low multpoles: is it cosmological or systematics?
- Probing accretion of ambient cloud material into the Taurus B211/B213 filament
- A Sino-German 6 cm polarization survey of the Galactic plane II. The region from 129 degree to 230 degree longitude
- Triggered Star Formation in the Orion Bright-Rimmed Clouds
- A simulation pipeline for the Planck mission
- The Spitzer survey of interstellar clouds in the Gould Belt. II. The Cepheus Flare observed with IRAC and MIPS
- Diffuse gamma-ray emission in the vicinity of young star cluster Westerlund 2
- SKAO HI Intensity Mapping: Blind Foreground Subtraction Challenge
- New Constraints on the Galactic Halo Magnetic Field using Rotation Measures of Extragalactic Sources Towards the Outer Galaxy
- Spectroscopy of Very Low Mass Stars and Brown Dwarfs in the Lambda Orionis Star Forming Region
- Cosmic rays, gas and dust in nearby anticentre clouds : I -- CO-to-H2 conversion factors and dust opacities
- Electron Density Structure of the Local Galactic Disk
- Planck Intermediate Results. IX. Detection of the Galactic haze with Planck
- The large-scale anomalous microwave emission revisited by WMAP
- Triggered Star Formation by Massive Stars
- The light variability of the helium strong star HD 37776 as a result of its inhomogeneous elemental surface distribution
- Optical-NIR dust extinction towards Galactic O stars
- Results from the Wilkinson Microwave Anisotropy Probe
- Broadband Radio Polarimetry and Faraday Rotation of 563 Extragalactic Radio Sources
- The star formation history of Upper Scorpius and Ophiuchus
- Milky Way scattering properties and intrinsic sizes of active galactic nuclei cores probed by very long baseline interferometry surveys of compact extragalactic radio sources
- The Temperature of the CMB at 10 GHz
- Nested shells reveal the rejuvenation of the Orion-Eridanus superbubble
- 3D dynamics of the Orion cloud complex -- Discovery of coherent radial gas motions at the 100-pc scale
- The Case for a Low Extragalactic Gamma-ray Background
- A needlet ILC analysis of WMAP 9-year polarisation data: CMB polarisation power spectra
- The Spectroscopy of Plasma Evolution from Astrophysical Radiation Mission
- The cosmic-ray and gas content of the Cygnus region as measured in gamma rays by the Fermi Large Area Telescope
- Antisymmetry in the Faraday Rotation Sky Caused by a Nearby Magnetized Bubble
- A radio-polarisation and rotation measure study of the Gum Nebula and its environment
- The C-Band All-Sky Survey (C-BASS): Design and capabilities
- The Per-Tau Shell: A Giant Star-Forming Spherical Shell Revealed by 3D Dust Observations
- Hierarchical progressive surveys. Multi-resolution HEALPix data structures for astronomical images, catalogues, and 3-dimensional data cubes
- Ultraviolet Extinction at High Galactic Latitudes
- Observation of the Far-ultraviolet Continuum Background with SPEAR/FIMS
- GALEX Diffuse Observations of the Sky: The Data
- The impact of Solar wind variability on pulsar timing
- A CGPS Look at the Spiral Structure of the Outer Milky Way I: Distances and Velocities to Star Forming Regions
- Faraday Tomography of the North Polar Spur: Constraints on the distance to the Spur and on the Magnetic Field of the Galaxy
- A comprehensive overview of the Cold Spot
- Faraday screens associated with local molecular clouds
- The impact of Galactic synchrotron emission on CMB anisotropy measurements. I. Angular power spectrum analysis of total intensity all-sky surveys
- Galactic foreground contributions to the WMAP5 maps
- VSA Observations of the Anomalous Microwave Emission in the Perseus Region
- MAGMO: Coherent magnetic fields in the star forming regions of the Carina-Sagittarius spiral arm tangent
- On the Origins of the High-Latitude H-alpha Background
- Estimating the spectral indices of correlated astrophysical foregrounds by a second-order statistical approach
- CMB and foregrounds in WMAP first year data
- Galactic interstellar turbulence in the southern sky seen through spatial gradients of the polarization vector
- Densities and filling factors of the DIG in the Solar neighbourhood
- Ultraviolet to optical diffuse sky emission as seen by the Hubble Space Telescope Faint Object Spectrograph
- Detection of diffuse gamma-ray emission near the young massive cluster NGC 3603
- Measurement of a Magnetic Field in a Leading Arm High Velocity Cloud
- Radio spectral properties and the magnetic field of the SNR S147
- The magnetic environment of the Orion-Eridanus superbubble as revealed by Planck
- Estimating the Porosity of the Interstellar Medium from Three-Dimensional Photoionization Modeling of H II Regions
- Constraining Spinning Dust Parameters with the WMAP Five-Year Data
- A Last Look at the Microwave Haze/Bubbles with WMAP
- The Positron Puzzle
- Synchrotron Radiation from the Galactic Center in Decaying Dark Matter Scenario
- PFP 1: A Large Annular Planetary Nebula Caught in the First Stages of ISM Interaction
- On the origins of the diffuse H-alpha emission: Ionized gas or dust-scattered H-alpha halos?
- Magnetic fields in the Milky Way from pulsar observations: effect of the correlation between thermal electrons and magnetic fields
- 3D magnetic field morphology of the Perseus molecular cloud
- Optically thick HI does not dominate dark gas in the local ISM
- A Sino-German 6cm polarization survey of the Galactic plane IV. The region from 60deg to 129deg longitude
- Diffuse polarized emission in the LOFAR Two-meter Sky Survey
- The COMPLETE Nature of the Warm Dust Ring in Perseus
- Separating the EoR Signal with a Convolutional Denoising Autoencoder: A Deep-learning-based Method
- Bayesian component separation and CMB estimation for the 5-year WMAP temperature data
- HI, CO, and Dust in the Perseus Cloud
- SDSS IV MaNGA: Deep observations of extra-planar, diffuse ionized gas around late-type galaxies from stacked IFU spectra
- Detecting Sunyaev-Zel'dovich clusters with PLANCK: II. Foreground components and optimised filtering schemes
- 3D Dust Mapping Reveals that Orion Forms Part of a Large Ring of Dust
- HI filaments are cold and associated with dark molecular gas. HI4PI based estimates of the local diffuse CO-dark H2 distribution
- The isotropic radio background revisited
- Triggered Star Formation on the Border of the Orion-Eridanus Superbubble
- COSMOSOMAS Observations of the CMB and Galactic Foregrounds at 11 GHz: Evidence for anomalous microwave emission at high Galactic Latitude
- The White Dwarf Population in NGC 1039 (M34) and the White Dwarf Initial-Final Mass Relation
- Gas shells and magnetic fields in the Orion-Eridanus superbubble
- Scintillation timescale measurement of the highly active FRB20201124A
- Diffuse gamma-ray emission toward the massive star-forming region, W40
- Searching for Time-Dependent Axion Dark Matter Signals in Pulsars
- The Diffuse Galactic Far-Ultraviolet Sky
- The POlarised GLEAM Survey (POGS) II: Results from an All-Sky Rotation Measure Synthesis Survey at Long Wavelengths
- Comparing Planck and WMAP: Maps, Spectra, and Parameters
- S-PASS/ATCA: a window on the magnetic universe in the southern hemisphere
- C-Band All-Sky Survey: A First Look at the Galaxy
- Multi-scale analysis of the Monoceros OB 1 star-forming region: II. Colliding filaments in the Monoceros OB1 molecular cloud
- Through thick or thin: Multiple components of the magneto-ionic medium towards the nearby region Sharpless 2-27 revealed by Faraday tomography
- A Sino-German 6\ cm polarization survey of the Galactic plane. V. Large supernova remnants
- Orion A's complete 3D magnetic field morphology
- WARPFIELD Population Synthesis: The physics of (extra-)Galactic star formation and feedback driven cloud structure and emission from sub-to-kpc scales
- The Herschel Virgo Cluster Survey. XX. Dust and gas in the foreground Galactic cirrus
- Discovery of an Apparent High Latitude Galactic Supernova Remnant
- Identification of Spinning Dust in Halpha-Correlated Microwave Emission
- Foreground Analysis Using Cross-Correlations of External Templates on the 7-year WMAP data
- Absolutely calibrated radio polarimetry of the inner Galaxy at 2.3 GHz and 4.8 GHz
- A Broadband Study of Galactic Dust Emission
- Far UV and Optical Emissions from Three Very Large Supernova Remnants Located at Unusually High Galactic Latitudes
- A polarization census of bright pulsars using the Ultra-Wideband Receiver on the Parkes radio telescope
- The Global Magneto-Ionic Medium Survey: A Faraday Depth Survey of the Northern Sky Covering 1280-1750 MHz
- Polarization observations of SNR G156.2+5.7 at lambda 6cm
- K 1-6: an asymmetric planetary nebula with a binary central star
- Determination of the Cosmic Infrared Background from COBE/FIRAS and Planck HFI Observations
- Far-ultraviolet fluorescent molecular hydrogen emission map of the Milky Way Galaxy
- Mapping young stellar populations towards Orion with Gaia DR1
- Exploring the Cosmic Reionization Epoch in Frequency Space: An Improved Approach to Remove the Foreground in 21 cm Tomography
- Flux calibration of the AAO/UKST SuperCOSMOS H-alpha Survey
- Detecting Sunyaev-Zel'dovich clusters with PLANCK: III. Properties of the expected SZ-cluster sample
- Planck intermediate results. XII: Diffuse Galactic components in the Gould Belt System
- Measuring the redshift dependence of the CMB monopole temperature with PLANCK data
- Comparison of the Diffuse Halpha and FUV Continuum Backgrounds: On the Origins of the Diffuse Halpha Background
- 21 new long-term variables in the GX 339-4 field: two years of MeerKAT monitoring
- Faraday Rotation as a Diagnostic of Galactic Foreground Contamination of CMB Maps
- Far-UV Observations of a Thermal Interface in the Orion-Eridanus Superbubble
- Six Faint Gamma-ray Pulsars Seen with the Fermi Large Area Telescope -- Towards a Sample Blending into the Background
- Far-ultraviolet Observations of the Taurus-Perseus-Auriga Complex
- Preliminary evidence for a virial shock around the Coma galaxy cluster
- A Millimeter-Wave Galactic Plane Survey With The BICEP Polarimeter
- An Old Supernova Remnant within an HII Complex at l {\approx} 173{\circ}: FVW 172.8+1.5
- Kompaneets Model Fitting of the Orion-Eridanus Superbubble II: Thinking Outside of Barnard's Loop
- Radio properties of the low surface brightness SNR G65.2+5.7
- BeyondPlanck XIII. Intensity foreground sampling, degeneracies, and priors
- G107.0+9.0: A New Large Optically Bright, Radio and X-Ray Faint Galactic Supernova Remnant in Cepheus
- Discovery of Extensive Optical Emission Associated with the X-ray Bright, Radio Faint Galactic SNR G156.2+5.7
- Redshifted intergalactic 3He+ 8.7 GHz hyperfine absorption
- The Complex Large-scale Magnetic Fields in the First Galactic Quadrant as Revealed by the Faraday Depth Profile Disparity
- Polarization shadows of extragalactic sources by the local magneto-ionic ISM
- Excited-state hydroxyl maser polarimetry: Who ate all the πs?
- Foreground separation using a flexible maximum-entropy algorithm: an application to COBE data
- Determination of the Far-Infrared Cosmic Background Using COBE/DIRBE and WHAM Data
- Two Radio Supernova Remnants Discovered in the Outer Galaxy
- Identifying the Radio Bubble Nature of the Microwave Haze
- Low-frequency pulse profile variation in PSR B2217+47: evidence for echoes from the interstellar medium
- The bispectrum and 21cm foregrounds during the Epoch of Reionization
- Molecular Hydrogen Fluorescence in the Eridanus Superbubble
- Observations of the Cosmic Microwave Background and Galactic Foregrounds at 12-17 GHz with the COSMOSOMAS Experiment
- Disentangling the Faraday rotation sky
- Diffuse gamma-ray emission from the vicinity of young massive star cluster RSGC 1
- How to Identify and Separate Bright Galaxy Clusters from the Low-frequency Radio Sky?
- A 3D View of Orion: I. Barnard's Loop
- Tracing Milky Way scattering by compact extragalactic radio sources
- Determination of the cosmic far-infrared background level with the ISOPHOT instrument
- A Unified Model for the Fan Region and the North Polar Spur: A bundle of filaments in the Local Galaxy
- Discovery and timing of three millisecond pulsars in radio and gamma-rays with the GMRT and Fermi-LAT
- Investigation of the Origin of the Anomalous Microwave Emission in Lambda Orionis
- The One-dimensional Fourier Representation and Large Angular Scale Foreground Contamination in the 3-year Wilkinson Microwave Anisotropy Probe data
- Non-Gaussianity due to Possible Residual Foreground Signals in WMAP 1st-year Data Using Spherical Wavelet Approaches
- Cosmic-rays, gas, and dust in nearby anti-centre clouds : III -- Dust extinction, emission, and grain properties
- The warm Gaseous Disk and the Anisotropic Circumgalactic Medium of the Milky Way
- Pseudo-Dipole Signal Removal from WMAP Data
- The interface between the stellar wind and interstellar medium around R Cassiopeiae revealed by far-infrared imaging
- Optical Discovery of an Apparent Galactic Supernova Remnant G159.6+7.3
- Multi-frequency scatter broadening evolution of pulsars - II. Scatter broadening of nearby pulsars
- Symmetry and anti-symmetry of the CMB anisotropy pattern
- The C-Band All-Sky Survey (C-BASS): Template Fitting of Diffuse Galactic Microwave Emission in the Northern Sky
- The coherent magnetic field of the Milky Way halo, Local Bubble and Fan Region
- C2H N=1-0 and N2H+ J=1-0 observations of Planck Galactic cold clumps
- The C-Band All-Sky Survey (C-BASS): Constraining diffuse Galactic radio emission in the North Celestial Pole region
- A "Missing" Supernova Remnant revealed by the 21-cm Line of Atomic Hydrogen
- Template fitting of WMAP 7-year data: anomalous dust or flattening synchrotron emission?
- Far-Ultraviolet Observations of the Spica Nebula and the Interaction Zone
- Thermal and non-thermal emission in the Cygnus X region
- New insights into foreground analysis of the WMAP five-year data using FASTICA
- Blazar jet evolution revealed by multi-epoch broadband radio polarimetry
- Trade-off between angular resolution and straylight contamination in CMB anisotropy experiments. II. Straylight evaluation
- Detecting the HI Power Spectrum in the Post-Reionization Universe with SKA-Low
- Analysis of Spatial Structure of the SPica H II Region
- The QUaD Galactic Plane Survey 1: Maps And Analysis of Diffuse Emission
- New Galactic Planetary Nebulae selected by radio and multi-wavelength characteristics
- Warm Ionized Medium Throughout the Sagittarius-Carina Arm
- WMAP 9-year CMB estimation using sparsity
- Non-Gaussian Foreground Residuals of the WMAP First Year Maps
- Optical Emission Associated with the Galactic Supernova Remnant G179.0+2.6
- Analysis of WMAP 7-year Temperature Data: Astrophysics of the Galactic Haze
- Impact of early dark energy on the Planck SZ cluster sample
- Galactic foreground contribution to the BEAST CMB Anisotropy Maps
- Gas and Dust Properties in the Chamaeleon Molecular Cloud Complex based on the Optically Thick HI
- A High-Velocity Cloud Impact Forming a Supershell in the Milky Way
- High resolution H-alpha imaging of the Northern Galactic Plane, and the IGAPS images database
- Dark matter implications of the WMAP-Planck Haze
- GSH 006-15+7: A local Galactic supershell featuring transition from HI emission to absorption
- QUIJOTE Scientific results. III. Microwave spectrum of intensity and polarization in the Taurus molecular cloud Complex and L1527
- A Sino-German 6cm polarisation survey of the Galactic plane IX. HII regions
- A new perspective on turbulent Galactic magnetic fields through comparison of linear polarisation decomposition techniques
- Bursts from Space: MeerKAT - The first citizen science project dedicated to commensal radio transients
- QUIJOTE scientific results -- X. Spatial variations of Anomalous Microwave Emission along the Galactic plane
- BeyondPlanck XVI. Limits on Large-Scale Polarized Anomalous Microwave Emission from Planck LFI and WMAP
- Magnetic fields of the W4 superbubble
- Properties of dust and detection of Halpha emission in LDN 1780
- A broadband radio view of transient jet ejecta in the black hole candidate X-ray binary MAXI J1535-571
- Foreground removal from CMB temperature maps using an MLP neural network
- Far-Ultraviolet Cooling Features of the Antlia Supernova Remnant
- Evidence for Inverted Spectrum 20 GHz Emission in the Galactic Plane
- Contribution of Radio Halos to the Foreground for SKA EoR Experiments
- Towards a complete picture of the Sco-Cen outflow
- First optical identification of the SRG/eROSITA-detected supernova remnant G 116.6-26.1 I. Preliminary results
- A census of compact sources at 162MHz: first data release from the MWA Phase II IPS Survey
- Spectroscopy of diffuse light in dust clouds. Scattered light and the solar neighbourhood radiation field
- Bayesian analysis of white noise levels in the 5-year WMAP data
- A FAST Survey of HINSA in PGCCs Guided by HC3N
- Scattered H-alpha emission from a large translucent cloud G294-24
- Diffuse Far-ultraviolet Observation of the Lupus Loop Region
- Noise power spectrum estimation and fast map making for CMB experiments
- The cosmic-ray content of the Orion-Eridanus superbubble
- Puzzling large-scale polarization in the galaxy cluster Abell 523
- Analysis of Polarized Dust Emission Using Data from the First Flight of SPIDER
- NE2025: An Updated Electron Density Model for the Galactic Interstellar Medium
- The GALANTE photometric survey of the northern Galactic plane: Project description and pipeline
- Galactic Structure Toward the Carina Tangent
- Cross-Correlation analysis of WMAP and EGRET in Wavelet Space
- Early phases in the stellar and substellar formation and evolution: Infrared and submillimeter data in the Barnard 30 dark cloud
- Diffuse -ray emission around the massive star forming region of Carina Nebula Complex
- New continuum and polarization observations of the Cygnus Loop with FAST II. Images and analyses
- A Comparison of Multi-Phase Magnetic Field Tracers in a High-Galactic Latitude Region of the Filamentary Interstellar Medium
- Astronomy with Small Telescopes
- Detection of Extensive Optical Emission from the Extremely Radio Faint Galactic Supernova Remnant G182.4+4.3
- QUIJOTE Scientific Results -- XVII. Studying the Anomalous Microwave Emission in the Andromeda Galaxy with QUIJOTE-MFI
- Turbulent magnetic field in the HII region Sh 2-27
- A hard spectrum diffuse gamma-ray component associated with HII gas in the Galactic plane
- Probing the filamentary nature of star formation in the California giant molecular cloud
- Cross-correlation analysis of CMB with foregrounds for residuals
- A Low Frequency Pilot Survey of Southern HII Regions in the Vela Constellation
- Contribution of Galactic free-free emission to the foreground for EoR signal in SKA experiments
- Massive Stellar Content of the Galactic Supershell GSH 305+01-24
- Bayesian foreground analysis with CMB data
- X-ray counterpart detection and gamma-ray analysis of the SNR G279.0+01.1 with eROSITA and Fermi-LAT
- Cosmic ray backgrounds for dark matter indirect detection
- Ghost of a Shell: Magnetic Fields of Galactic Supershell GSH 006157
- Tomography of X-ray Nova Muscae 1991: Evidence for ongoing mass transfer and stream-disc overflow
- Bidimensional Exploration of the warm-Temperature Ionised gaS (BETIS) II. Revisiting the ionisation mechanism of the extraplanar diffuse ionised gas
- GSH 90-28-17: a Possible Old Supernova Remnant
- Calibrating Column Density Tracers with Gamma-ray Observations of the Ophiuchi Molecular Cloud
- The C-Band All-Sky Survey (C-BASS): Simulated parametric fitting in single pixels in total intensity and polarization
- QUIJOTE scientific results -- VI. The Haze as seen by QUIJOTE
- Study of X-ray emission from the S147 nebula with SRG/eROSITA: X-ray imaging, spectral characterization, and a multiwavelength picture
- Constraints on the SZ Power Spectrum on Degree Angular Scales in WMAP Data
- A new method of reconstructing Galactic three-dimensional structures using ultralong-wavelength radio observations
- Signatures of Recent Cosmic-Ray Acceleration in the High-Latitude -Ray Sky
- A Comparative Analysis To Deal With Missing Spectral Information Caused By RFI In Cosmological HI 21CM Observations
- Towards Optimal Foreground Mitigation Strategies for Interferometric HI Intensity Mapping in the Low-Redshift Universe
- Significant foreground unrelated non-acoustic anisotropy on the one degree scale in WMAP 5-year observations
- Revealing a new region of gamma-ray emission in the vicinity of HESS J1825-137
- Gas physical conditions and kinematics of the giant outflow Ou4
- Power Spectrum Analysis of Polarized Emission from the Canadian Galactic Plane Survey
- MIRIS Paα Galactic Plane Survey. I. Comparison with IPHAS Hα in l = 96°-116°
- Bidimensional Exploration of the warm-Temperature Ionised gaS (BETIS) I. Showcase sample and first results
- Bayesian decomposition of the Galactic multi-frequency sky using probabilistic autoencoders
- Diffuse gamma-ray emission around the Rosette Nebula
- The Orion-Taurus ridge: a synchrotron radio loop at the edge of the Orion-Eridanus superbubble
- Sharpening up Galactic all-sky maps with complementary data - A machine learning approach
- Foreground removal from WMAP 7yr polarization maps using an MLP neural network
- Associations Between Scattering Screens and Interstellar Medium Filaments
- Distant probes of RM structure -- Where is the Faraday Rotation towards the Magellanic Leading Arm?
- A new understanding of the Gemini-Monoceros X-ray enhancement from discoveries with eROSITA
- Model Independent Foreground Power Spectrum Estimation using WMAP 5-year Data
- The Galactic Faraday rotation sky 2020
- Candidates of Halpha emitting regions in Magellanic Stream IV cloud
- The bandmerged Planck Early Release Compact Source Catalogue: Probing sub-structure in the molecular gas at high Galactic latitude
- Magnetic field strength in an intermediate-velocity ionized filament in the First Galactic Quadrant
- Velocity measurement in the extensive [OIII] emission region 1.2° south-east of M31
- A Possible Supernova Remnant high above the Galactic Disk
- Study of the Cosmic Rays and Interstellar Medium in Local HI Clouds using Fermi-LAT Gamma-Ray Observations
- Arc-minute-scale studies of the interstellar gas towards HESSJ1804216: Still an unidentified TeV -ray source
- Constraining the Anomalous Microwave Emission Mechanism in the S140 Star Forming Region with Spectroscopic Observations Between 4 and 8 GHz at the Green Bank Telescope
- The Lyman alpha Sky as Observed by New Horizons
- RMS Radio Source Contributions to the Microwave Sky
- Modeling the H Emission Surrounding Spica using the Lyman Continuum from a Gravity-darkened Central Star
- Low-Frequency Carbon Recombination Lines in the Orion Molecular Cloud Complex
- Nearly Full-Sky Low-Multipole Cosmic Microwave Temperature Anisotropy: I. Foreground Cleaned Maps
- Explaining the extended GeV gamma-ray emission adjacent to HESS J1825-137
- Extreme Starlight Polarization Efficiency Toward Ophiuchi: A Case for Line-of-Sight Foreground Subtraction
- Long, depolarising H-filament towards the Monogem ring
- Construction of a far ultraviolet all sky map from an incomplete survey: Application of a deep learning algorithm
- Space Missions for Astronomy and Astrophysics in Korea: Past, Present, and Future
- Far-infrared to centimeter emission of very nearby galaxies with archival data
- Implications of scattering for CMB foreground emission modelling
- A characterization of the diffuse Galactic emissions in the anti-center of the Galaxy
- A look at the high energy aspects of the supernova remnant G309.8+00.0 with eROSITA and Fermi-LAT
- Pulsar scattering as a probe for structures in the interstellar medium
- New Radio Observations of the Supernova Remnant CTA 1
- Young Stars in the Camelopardalis Dust and Molecular Clouds. I. The Cam OB1 Association
- Gamma-ray emission toward supergiant shells in the Large Magellanic Cloud
- Radio properties of the optically identified supernova remnant G107.0+9.0
- Directional quantum scattering transducer in cooperative Rydberg metasurfaces
- A characterization of the diffuse Galactic emissions at large angular scales using the Tenerife data
- A Monte Carlo Implementation of Galactic Free-Free Emission for the EoR Foreground Models
- MIRIS Paα Galactic Plane Survey. II. The Catalog of Paα Emission-line Sources
- Magnetic field properties of the SNR HB 9
- A new wideband radio polarization observation of the Supernova Remnant G315.42.3
- Correlation Analysis between Tibet AS- TeV Cosmic Ray and WMAP Nine-year Data
- Multi-Wavelength Correlation Studies Of Diffuse Emission From The Aquila Rift