With observed FIR-color $\sim$1, Haro11 falls within the large spread of L$\rm{_{[C~II]}}$/L$\rm{_{TIR}}$ values and is not particularly \[C [ii]{}\] deficient nor \[C [ii]{}\] excessive, as often seen in low metallicity galaxies [@madden-2012b].

Photometry data
---------------

For the discussion on the SED of Haro11 in Section \[sect:sed\], we use broad-band data available from the X-ray to the radio regime, to assess how the models perform in reproducing the continuum emission. The photometry is taken from NED. In addition, we use the [*Spitzer*]{}/MIPS photometry from [@bendo-2012], the [*Herschel*]{}/PACS and SPIRE photometry from [@remy-2012], and the [*Spitzer*]{}/IRAC and LABOCA 870 $\mu$m photometry from [@galametz-2009]. All fluxes are summarized in Table \[table:phot\].

  --------- -------------- ---------- ---------- ------
                                                 
                                                 
  Chandra      2-10 keV     9.17e-09   1.03e-09   (1)
  Chandra     0.5-2 keV     3.21e-08   0.43e-08   (1)
  ROSAT       0.1-2 keV     4.41e-08   0.55e-08   (2)
  FUSE          1150 Å      2.30e-03   0.33e-03   (3)
  GALEX         1530 Å      3.63e-03    7e-05     (4)
  GALEX         2315 Å      4.37e-03    4e-05     (4)
  Cousins    0.439 $\mu$m   8.03e-03   0.69e-03   (5)
  Cousins    0.639 $\mu$m    0.012      0.001     (5)
  2MASS      1.25 $\mu$m     0.013      0.001     (6)
  2MASS      1.64 $\mu$m     0.013      0.001     (6)
  2MASS      2.17 $\mu$m     0.014      0.001     (6)
  IRAC        3.6 $\mu$m     0.023      0.002     (7)
  IRAC        4.5 $\mu$m     0.029      0.003     (7)
  IRAC       5.8  $\mu$m     0.073      0.007     (7)
  IRAC         8 $\mu$m      