High precision X-ray log N ? log S distributions: implications for the obscured AGN population

MLA

Mateos, S., et al. “High Precision X-Ray Log N ? Log S Distributions: Implications for the Obscured AGN Population.” Astronomy and Astrophysics, vol. 492, no. 1, Dec. 2008, pp. 51–69. EBSCOhost, widgets.ebscohost.com/prod/customlink/proxify/proxify.php?count=1&encode=0&proxy=&find_1=&replace_1=&target=https://search.ebscohost.com/login.aspx?direct=true&site=eds-live&scope=site&db=edo&AN=ejs17494567&authtype=sso&custid=ns315887.

APA

Mateos, S., Warwick, R., Carrera, F., Stewart, G., Ebrero, J., Della Ceca, R., Caccianiga, A., Gilli, R., Page, M., Treister, E., Tedds, J., Watson, M., Lamer, G., Saxton, R., Brunner, H., & Page, C. (2008). High precision X-ray log N ? log S distributions: implications for the obscured AGN population. Astronomy and Astrophysics, 492(1), 51–69.

Chicago

Mateos, S., R. Warwick, F. Carrera, G. Stewart, J. Ebrero, R. Della Ceca, A. Caccianiga, et al. 2008. “High Precision X-Ray Log N ? Log S Distributions: Implications for the Obscured AGN Population.” Astronomy and Astrophysics 492 (1): 51–69. http://widgets.ebscohost.com/prod/customlink/proxify/proxify.php?count=1&encode=0&proxy=&find_1=&replace_1=&target=https://search.ebscohost.com/login.aspx?direct=true&site=eds-live&scope=site&db=edo&AN=ejs17494567&authtype=sso&custid=ns315887.