Axisymmetric parametrised metric of Konoplya, Rezzolla, and Zhidenko 2016 (PRD, 93, 064015) 4.e6 The black hole mass parameter m (which is not necessarily the same as the asymptotic mass M) 0. The black hole specific angular momentum parameter a (which is not necessarily the same as the asymptotic spin A) [0.,0.,0.,0.,0.,0.] Deformation parameters [δa01,δw01,δw21,δb01,δb21,δrot] to the Kerr metric constrainable at the black hole event horizon which coincide with the deviation functions of Ni et al. 2016 (JCAP 09, 014) [0.,0.,0.,0.,0.,0.] Deformation parameters [δepsilon0,ẟw00,ẟa00,ẟb00] to the Kerr metric constrainable asymptotically which coincide with the deviation functions B26-B27 of Cárdenas-Avendaño and Held 2024 (PRD 109, 064052) 6. Radius of the innermost stable circular orbit to be given by the user (not implemented in Gyoto)

         8
         30e3
         150
        Note: "microas" can be written "µas" in UTF-8 locales. We use the
        ASCII version here as automated systems are not always configured
        with a UTF-8 locales by default.
         90
        "degree" can be written "°" in UTF-8 locales.
         0
         0
         32

12
0 0 0
0
0.001
0
0.01
1e0
0.
Intensity
One can also specify a unit (if Gyoto was compiled with --with-udunits): Intensity[mJy/pix²] Intensity[mJy/µas²] Intensity[J.m-2.s-1.sr-1.Hz-1] Intensity[erg.cm-2.s-1.sr-1.Hz-1] Intensity[mJy.sr-1] Intensity[Jy.sr-1] The subscript "²" requires a UTF-8 locale. A normal "2" can be used instead.

12