Abstract Preliminary investigation of GALEX images of the diffuse ultraviolet background radiation suggests that part of the diffuse background represents red-shifted Lyman α recom-bination radiation from the intergalactic medium, which in turn would require, to maintain the observed high degree of ionization of the intergalactic medium, that the non-baryonic dark matter decay with the emission of an ionizing photon. Techniques for verifying this and for treating the data are described in some detail. Key words: techniques: ultraviolet – cosmology: diffuse backgroun
SummaryWe have studied the diffuse UV emission from Lockman Hole using 23 Deep Imaging Surveys (DIS)...
The imaging instrumentation on the Dynamics Explorer 1 satellite is used to measure the intensity of...
Abstract. The upcoming TAUVEX mission is expected to provide us with high quality data from observat...
ABSTRACT. I review the nature of the diffuse cosmic ultraviolet background radiation. The ultraviole...
Abstract. Diffuse ultraviolet background radiation may contain important information concerning the ...
We have observed a region of nebulosity first identified as starlight scattered by interstellar dust...
We have studied small-scale (2′) spatial variation of the diffuse ultraviolet (UV) radiation using a...
The diffuse cosmic background radiation in the Galaxy Evolution Explorer far-ultraviolet (FUV, 1300–...
Abstract. I report on progress in my ongoing work with Professor Jayant Murthy con-cerning the origi...
The diffuse far-ultraviolet (FUV) background has received considerable attention from astronomers si...
The cosmic X-ray background was discovered at the dawn of the X-ray astronomy: during the first succ...
A new determination of the upper limit to the cosmic diffuse background radiation, at »110 nm, of 30...
"Diffuse" gamma rays consist of several components: truly diffuse emission from the interstellar med...
We have previously calculated the intergalactic background light (IBL) as a function of redshift in ...
The diffuse high-latitude Hα background is widely believed to be predomi-nantly the result of in-sit...
SummaryWe have studied the diffuse UV emission from Lockman Hole using 23 Deep Imaging Surveys (DIS)...
The imaging instrumentation on the Dynamics Explorer 1 satellite is used to measure the intensity of...
Abstract. The upcoming TAUVEX mission is expected to provide us with high quality data from observat...
ABSTRACT. I review the nature of the diffuse cosmic ultraviolet background radiation. The ultraviole...
Abstract. Diffuse ultraviolet background radiation may contain important information concerning the ...
We have observed a region of nebulosity first identified as starlight scattered by interstellar dust...
We have studied small-scale (2′) spatial variation of the diffuse ultraviolet (UV) radiation using a...
The diffuse cosmic background radiation in the Galaxy Evolution Explorer far-ultraviolet (FUV, 1300–...
Abstract. I report on progress in my ongoing work with Professor Jayant Murthy con-cerning the origi...
The diffuse far-ultraviolet (FUV) background has received considerable attention from astronomers si...
The cosmic X-ray background was discovered at the dawn of the X-ray astronomy: during the first succ...
A new determination of the upper limit to the cosmic diffuse background radiation, at »110 nm, of 30...
"Diffuse" gamma rays consist of several components: truly diffuse emission from the interstellar med...
We have previously calculated the intergalactic background light (IBL) as a function of redshift in ...
The diffuse high-latitude Hα background is widely believed to be predomi-nantly the result of in-sit...
SummaryWe have studied the diffuse UV emission from Lockman Hole using 23 Deep Imaging Surveys (DIS)...
The imaging instrumentation on the Dynamics Explorer 1 satellite is used to measure the intensity of...
Abstract. The upcoming TAUVEX mission is expected to provide us with high quality data from observat...