Extended Data Table 1 Emission line fluxes in various regions

From: Directly imaging the cooling flow in the Phoenix cluster

  1. *The ionization energy required to create ions of the given species, obtained from NIST.
  2. †The integrated flux within an elliptical aperture covering the region of extended emission to the north of the nucleus, with the QSO contribution subtracted.
  3. ‡The integrated flux within a circular aperture with a 1″ radius centered on the nucleus, including the QSO contribution.
  4. §The integrated flux throughout the full channel 2 FOV, with the QSO contribution subtracted.
  5. ∥3σ upper limits are derived by integrating a gaussian with an amplitude of 3 times the continuum RMS at the ___location of the line, with a width of 1000 km s−1.
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