Thermally emitting isolated neutron star candidates from the srg/erosita all-sky survey

HIGHLIGHTS

• What: In the following, the authors assess the efficiency of the method at selecting XDINS candidates from the eRASS catalogues based on the completeness and reliability of the sample. The authors show the resulting cumulative distribution of non-matching probabilities (blue) in Fig 4. To give an impression on the quality of the eROSITA spectra and the resulting fits, the authors show the spectrum and subsequent best-fit BB model for J13472 in Fig 6. In Fig 8 the authors compare the resulting X-ray-to-optical flux ratio values to those of the most abundant contaminants . . .
  

   

  

  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.