Three FITS format images of the Galactic center made by the Green Bank Telescope. Radio continuum emission was observed in L, C, and X bands (1.4, 5, and 8 GHz frequencies) over roughly the central degree of the Galaxy. Calibration and image processing has been applied, as discussed in the original publication. The flux scale is accurate on small size scales, but image filtering has removed the large-scale emission (along with many calibration artifacts)
The Galactic center (GC) lobe is a degree-tall shell seen in radio continuum images of the GC region...
Abstract. This paper presents the revised sample of 373 extragalactic radio sources brighter than 0....
We observed 64 newly identified galactic bulge planetary nebulae in the radio continuum at 3 and 6 c...
We describe the results of a radio continuum survey of the central 4° × 1° with the 100 m Green Bank...
This is a high-quality survey of the Galactic center region carried out from Chile, where the center...
In the fall of 1986 the Galactic Radio Patrol began total power observations with the new seven feed...
Available data are raw, interpolated, and moment-masked versions of a large (1.3 GB) FITS cube conta...
We use absolutely calibrated data from the ARCADE 2 flight in 2006 July to model Galactic emission a...
The Galactic center (GC) is a dense and chaotic region filled with unusual sources, such as intense ...
The Galactic center (GC) lobe is a degree-tall shell of gas that spans the central degree of our Gal...
The Galactic center (GC) is a dense and chaotic region filled with unusual sources, such as intense ...
We consider the calibration of flux densities of radio bursts from decametric to kilometric wavelen...
The Rhodes/HartRAO SKYMAP survey is the highest frequency (2326 MHz) and highest resolution (20 arcm...
The Bolocam Galactic Plane Survey (BGPS) data for a 6 deg(2) region of the Galactic plane containing...
Description: Data were taken May-June 2003 and 2005. Flux units are in mJy per 31 arcsecond beam. ...
The Galactic center (GC) lobe is a degree-tall shell seen in radio continuum images of the GC region...
Abstract. This paper presents the revised sample of 373 extragalactic radio sources brighter than 0....
We observed 64 newly identified galactic bulge planetary nebulae in the radio continuum at 3 and 6 c...
We describe the results of a radio continuum survey of the central 4° × 1° with the 100 m Green Bank...
This is a high-quality survey of the Galactic center region carried out from Chile, where the center...
In the fall of 1986 the Galactic Radio Patrol began total power observations with the new seven feed...
Available data are raw, interpolated, and moment-masked versions of a large (1.3 GB) FITS cube conta...
We use absolutely calibrated data from the ARCADE 2 flight in 2006 July to model Galactic emission a...
The Galactic center (GC) is a dense and chaotic region filled with unusual sources, such as intense ...
The Galactic center (GC) lobe is a degree-tall shell of gas that spans the central degree of our Gal...
The Galactic center (GC) is a dense and chaotic region filled with unusual sources, such as intense ...
We consider the calibration of flux densities of radio bursts from decametric to kilometric wavelen...
The Rhodes/HartRAO SKYMAP survey is the highest frequency (2326 MHz) and highest resolution (20 arcm...
The Bolocam Galactic Plane Survey (BGPS) data for a 6 deg(2) region of the Galactic plane containing...
Description: Data were taken May-June 2003 and 2005. Flux units are in mJy per 31 arcsecond beam. ...
The Galactic center (GC) lobe is a degree-tall shell seen in radio continuum images of the GC region...
Abstract. This paper presents the revised sample of 373 extragalactic radio sources brighter than 0....
We observed 64 newly identified galactic bulge planetary nebulae in the radio continuum at 3 and 6 c...