An X-ray spectral measurement of the quasar 3C 273 with the HEAO-A2 experiment in June/July 1978 is reported. The best power law fit to the photon flux over the range 2-60 keV gives a slope of 1.41 + or - 0.02. However, structure is observed, indicating a slope of 1.52 between 2 keV and 9 keV and a slight flattening between 9 keV and 30 keV. Observations with the same experiment in December 1977 and OSO-8 in June 1976 allows confirmation of 40% intensity variability on the time scale of months, although within limits provided by the poorer statistical quality of the additional data no spectral change is discerned. Absorption from the source is found to be low, with the 1978 data yielding a 90% confidence upper limit to the hydrogen column d...
Using new deep VLA and HST observations of the large-scale jet in 3C273 matched to 0.3" resolution, ...
The quasar 3C 273 was detected by the Compton Observatory Satellite (COS-B) in the 1970's. Energetic...
The quasar 3C273 has been detected by all instruments on CGRO. The emission from this source is moni...
The aim of this paper is to study the evolution of the broadband spectrum of one of the brightest an...
We present absolutely calibrated FUV spectra of the quasar 3C~273 covering 900- 1800 A. Our ~3 A res...
The properties of 3C 273 are reviewed and an attempt is made to find an answer to the question why 3...
An X-ray spectrum of the quasi-stellar object 3C 273 in the interval 0.25 to 10 KeV was obtained by ...
We present the results of our 1994 January and 1995 January observations of the quasar 3C 273 obtain...
The COMPTEL experiment aboard the Compton Gamma Ray Observatory, sensitive in the energy range from ...
We present results from a 244 ks NuSTAR observation of 3C 273 obtained during a cross-calibration ca...
We present images from five observations of the quasar 3C 273 with the Chandra X-ray Observatory. Th...
HEAO-1 experiment A-2 observations of the BL Lac object MK421 in May 1978 show a marked spectral cha...
An X-ray burst source was discovered near the X-ray source 3U1915-05. The continuum spectra of both ...
We report the results of a 3-week multi-wavelength campaign targeting the flat spectrum radio quasar...
We present a wide multi-wavelength database of most observations of the quasar 3C 273 obtained durin...
Using new deep VLA and HST observations of the large-scale jet in 3C273 matched to 0.3" resolution, ...
The quasar 3C 273 was detected by the Compton Observatory Satellite (COS-B) in the 1970's. Energetic...
The quasar 3C273 has been detected by all instruments on CGRO. The emission from this source is moni...
The aim of this paper is to study the evolution of the broadband spectrum of one of the brightest an...
We present absolutely calibrated FUV spectra of the quasar 3C~273 covering 900- 1800 A. Our ~3 A res...
The properties of 3C 273 are reviewed and an attempt is made to find an answer to the question why 3...
An X-ray spectrum of the quasi-stellar object 3C 273 in the interval 0.25 to 10 KeV was obtained by ...
We present the results of our 1994 January and 1995 January observations of the quasar 3C 273 obtain...
The COMPTEL experiment aboard the Compton Gamma Ray Observatory, sensitive in the energy range from ...
We present results from a 244 ks NuSTAR observation of 3C 273 obtained during a cross-calibration ca...
We present images from five observations of the quasar 3C 273 with the Chandra X-ray Observatory. Th...
HEAO-1 experiment A-2 observations of the BL Lac object MK421 in May 1978 show a marked spectral cha...
An X-ray burst source was discovered near the X-ray source 3U1915-05. The continuum spectra of both ...
We report the results of a 3-week multi-wavelength campaign targeting the flat spectrum radio quasar...
We present a wide multi-wavelength database of most observations of the quasar 3C 273 obtained durin...
Using new deep VLA and HST observations of the large-scale jet in 3C273 matched to 0.3" resolution, ...
The quasar 3C 273 was detected by the Compton Observatory Satellite (COS-B) in the 1970's. Energetic...
The quasar 3C273 has been detected by all instruments on CGRO. The emission from this source is moni...