SummaryWe have studied the diffuse UV emission from Lockman Hole using 23 Deep Imaging Surveys (DIS) of GALEX mission in order to quantify different components of diffuse UV radiation and search for extragalactic emission. The region is important due to the presence of minimal amount of gas and dust and the GALEX images cover more than 10 square degrees in the region. The UV emissions in the region are compared with Infrared 100μm emission and we find a slight anti-correlation between UV and IR flux, which we attribute to the presence of extragalactic contribution in the diffuse background. Using the positional details of Spitzer – SERVS and SWIRE surveys, the contribution of extragalactic light was extracted as 192photonscm−2sr−1s−1Å−1 in ...
The Galaxy Evolution Explorer (GALEX) continues its surveys of the ultraviolet sky. GALEX surveys ha...
We combine wide and deep galaxy number-count data from the Galaxy And Mass Assembly, COSMOS/G10, Hub...
Funding: Australian Research Council via Discovery Project DP130103505 (SPD).We combine wide and dee...
SummaryWe have studied the diffuse UV emission from Lockman Hole using 23 Deep Imaging Surveys (DIS)...
Spectra are presented for the diffuse UV radiation field between 1250 to 3100 A from eight different...
We have observed a region of nebulosity first identified as starlight scattered by interstellar dust...
International audienceContext. The Virgo direction has been observed at many wavelengths in ...
The imaging instrumentation on the Dynamics Explorer 1 satellite is used to measure the intensity of...
The diffuse far-ultraviolet (FUV) background has received considerable attention from astronomers si...
The imaging instrumentation for the Dynamics Explorer Mission was designed primarily to obtain globa...
We have studied small-scale (2′) spatial variation of the diffuse ultraviolet (UV) radiation using a...
AbstractThe Galaxy Evolution Explorer (GALEX) has performed the first surveys of the sky in the ultr...
Far-UV observations in and near the Hubble Deep Fields demonstrate that the Space Telescope Imaging ...
The total ultraviolet (UV) flux (from 1412 to 2718 Å) of M101 is compared on a pixel-to-pixel basis ...
An analysis is presented for the spectra of the diffuse ultraviolet background taken during shuttle ...
The Galaxy Evolution Explorer (GALEX) continues its surveys of the ultraviolet sky. GALEX surveys ha...
We combine wide and deep galaxy number-count data from the Galaxy And Mass Assembly, COSMOS/G10, Hub...
Funding: Australian Research Council via Discovery Project DP130103505 (SPD).We combine wide and dee...
SummaryWe have studied the diffuse UV emission from Lockman Hole using 23 Deep Imaging Surveys (DIS)...
Spectra are presented for the diffuse UV radiation field between 1250 to 3100 A from eight different...
We have observed a region of nebulosity first identified as starlight scattered by interstellar dust...
International audienceContext. The Virgo direction has been observed at many wavelengths in ...
The imaging instrumentation on the Dynamics Explorer 1 satellite is used to measure the intensity of...
The diffuse far-ultraviolet (FUV) background has received considerable attention from astronomers si...
The imaging instrumentation for the Dynamics Explorer Mission was designed primarily to obtain globa...
We have studied small-scale (2′) spatial variation of the diffuse ultraviolet (UV) radiation using a...
AbstractThe Galaxy Evolution Explorer (GALEX) has performed the first surveys of the sky in the ultr...
Far-UV observations in and near the Hubble Deep Fields demonstrate that the Space Telescope Imaging ...
The total ultraviolet (UV) flux (from 1412 to 2718 Å) of M101 is compared on a pixel-to-pixel basis ...
An analysis is presented for the spectra of the diffuse ultraviolet background taken during shuttle ...
The Galaxy Evolution Explorer (GALEX) continues its surveys of the ultraviolet sky. GALEX surveys ha...
We combine wide and deep galaxy number-count data from the Galaxy And Mass Assembly, COSMOS/G10, Hub...
Funding: Australian Research Council via Discovery Project DP130103505 (SPD).We combine wide and dee...