The Serendipitous Extragalactic X-Ray Source Identification ( SEXSI ) Program : I . Characteristics of the Hard X-Ray Sample

@inproceedings{Harrison2003TheSE,
  title={The Serendipitous Extragalactic X-Ray Source Identification ( SEXSI ) Program : I . Characteristics of the Hard X-Ray Sample},
  author={F A Harrison and Megan E. Eckart and Peter H. Mao and David J. Helfand and Daniel Stern},
  year={2003}
}
The Serendipitous Extragalactic X-ray Source Identification (SEXSI) Program is designed to extend greatly the sample of identified extragalactic hard X-ray (2 – 10 keV) sources at intermediate fluxes (∼ 10−13−10−15 erg cm s). SEXSI, which studies sources selected from more than 2 deg, provides an essential complement to the Chandra Deep Fields, which reach… CONTINUE READING