Erosita (erass1) study of the canis major overdensity: developing a multi-wavelength algorithm for classifying faint x-ray sources

HIGHLIGHTS

• What: For those sources, which the analysis has identified as potential members of CMa OD (see Sect 4), the authors applied the more strict criterion of ML ≥ 10 (>4σ). The source No is the ID of the sources in the catalogue of this work, see Appendix A.2. and IR properties of maximum three counterparts of the Xray source were collected for further analysis (see Sect 4). The survey presents the optical data in 5 bands of grizy (495.7, 621.1, 752.2, 867.1, and 970.7 nm, respectively). The aim of this work is . . .
  

   

  

  If you want to have access to all the content you need to log in!

  Thanks :)

  Username or Email

  Password

  Remember me

  Lost your password?

  If you don't have an account, you can create one here.