Analysis of soft X-ray excesses of quasi-stellar objects by using their IPC spectra

1992 ◽  
Vol 400 ◽  
pp. 430 ◽  
Author(s):  
Y. Y. Zhou ◽  
K. N. Yu
2019 ◽  
Vol 15 (S356) ◽  
pp. 95-95
Author(s):  
Itziar Aretxaga

AbstractWe present MIR spectroscopy and photometry obtained with CanariCam on the 10.4 m Gran Telescopio CANARIAS for a sample of 20 nearby, MIR bright and X-ray luminous quasi-stellar objects (QSOs). We find that for the majority of QSOs the MIR emission is unresolved at angular scales ∼0.3 arcsec. We derive the properties of the dusti tori that surround the nucleus based on these observations and find significant differences in the parameters compared with a sample of Seyfert 1 and 2 nuclei. We also find evidence for polycyclic aromatic hydrocarbon (PAH) features in the spectra, indicative of star formation, more centrally peaked (on scales of a few hundred pc) than previously believed.


1987 ◽  
Vol 314 ◽  
pp. 111 ◽  
Author(s):  
Scott F. Anderson ◽  
Bruce Margon

2000 ◽  
Vol 528 (2) ◽  
pp. 637-649 ◽  
Author(s):  
W. N. Brandt ◽  
A. Laor ◽  
Beverley J. Wills

2004 ◽  
Vol 352 (2) ◽  
pp. 523-534 ◽  
Author(s):  
K. L. Page ◽  
N. Schartel ◽  
M. J. L. Turner ◽  
P. T. O'Brien

1986 ◽  
Vol 119 ◽  
pp. 51-52
Author(s):  
A. Hewitt ◽  
G. Burbidge

We have prepared a new catalogue of QSOs and BL Lac objects containing approximately 3400 entries. A complete update of the Hewitt-Burbidge (1980) catalogue has been made with approximately another 2000 objects with known redshifts added. The references to discovery, magnitudes, redshifts, color, spectra and polarimetry have been updated for the objects listed in 1980, and complete new references are included for the new objects. In addition to the basic optical information, the new catalogue also contains X-ray, radio and infrared information for all objects. Absorption redshifts are listed when they are available. A supplementary catalogue which is now in preparation will contain similar information for objects described variously as Seyfert galaxies, N systems and AGNs. In doubtful cases we have used the operational dividing line ƶ = 0.1. All objects with ƶ < 0.1 are put in the supplementary catalogue unless their discoverers have unambiguously defined them as QSOs. With approximately twice as many objects included it is interesting to note that: a)There are still very few genuine BL Lac objects, ∼100.b)The largest number of additions has come from identifications using the objective prism-grism techniques.


2005 ◽  
Vol 360 (2) ◽  
pp. 610-618 ◽  
Author(s):  
J. A. Stevens ◽  
M. J. Page ◽  
R. J. Ivison ◽  
F. J. Carrera ◽  
J. P. D. Mittaz ◽  
...  

2014 ◽  
Vol 446 (3) ◽  
pp. 2394-2417 ◽  
Author(s):  
M. Brusa ◽  
A. Bongiorno ◽  
G. Cresci ◽  
M. Perna ◽  
A. Marconi ◽  
...  

2016 ◽  
Vol 464 (4) ◽  
pp. 4586-4592 ◽  
Author(s):  
M. J. Page ◽  
F. J. Carrera ◽  
M. Ceballos ◽  
A. Corral ◽  
J. Ebrero ◽  
...  

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