Auxiliary Information on results for the paper  "TeV flaring activity of the AGN PKS 0625-354 in November 2018" (HESS Collaboration, Astronomy & Astrophysics, 683, A70)


Fig. 1. Nightly-binned light curve above 200 GeV measured with the H.E.S.S. telescopes in November 2018.

# MJD dMJD Flux[cm^-2 s^-1] dFlux_low[cm^-2 s^-1] dFlux_high[cm^-2 s^-1] 
58424.0057655 0.01646567531861 2.4335e-11 4.5547e-12 4.9419e-12 
58424.99445876 0.06292619765736 4.9132e-12 1.8745e-12 2.0405e-12 
58426.02857409 0.05806286400184 6.6102e-12 1.6346e-12 1.7496e-12 
58426.99709292 0.06911130272783 5.1797e-12 1.6764e-12 1.8048e-12  
58428.04207649 0.0681616992224 9.8331e-12 2.0399e-12 2.1868e-12 
58429.02785259 0.06724617839791 1.5966e-12 1.2612e-12 1.3488e-12   
58430.02852523 0.08380158059299 7.051e-13 2.0845e-12 2.4048e-12  
58431.01608481 0.09050669288263 -9.4647e-13 1.6689e-12 1.879e-12 
58432.02925955 0.05418581864797 3.5764e-14 1.3375e-12 1.4671e-12   
58432.96819997 0.01974438712932 -2.3588e-12 2.2796e-12 2.6551e-12  



Fig. 2. Spectral energy distributions  measured with the H.E.S.S. telescopes in 2018 - spectral points.

average spectrum:
#Energy  ErrHigh ErrLow Flux ErrHigh ErrLow 
#[TeV]  [TeV]  [TeV]	[TeV cm-2 s-1] 	[TeV cm-2 s-1] [TeV cm-2 s-1]
1.864e-01 2.908e-02 3.958e-02 8.180e-11 3.177e-11 2.959e-11
2.675e-01 4.875e-02 5.203e-02 2.035e-11 6.812e-12 6.476e-12
3.821e-01 8.206e-02 6.587e-02 8.943e-12 2.398e-12 2.274e-12
5.601e-01 1.212e-01 9.592e-02 3.042e-12 8.887e-13 8.292e-13
8.890e-01 3.225e-01 2.077e-01 8.078e-13 2.502e-13 2.316e-13

high state spectrum: 
#Energy  ErrHigh ErrLow Flux ErrHigh ErrLow 
#[TeV]  [TeV]  [TeV]	[TeV cm-2 s-1] 	[TeV cm-2 s-1] [TeV cm-2 s-1]
2.946e-01 5.348e-02 5.745e-02 1.063e-10 3.302e-11 2.881e-11
4.183e-01 9.256e-02 7.027e-02 1.633e-11 9.813e-12 8.075e-12
6.139e-01 1.360e-01 1.030e-01 1.020e-11 4.742e-12 3.855e-12
9.383e-01 2.732e-01 1.884e-01 2.481e-12 1.600e-12 1.226e-12 

low state spectrum:
Energy  ErrHigh ErrLow Flux ErrHigh ErrLow 
[TeV]  [TeV]  [TeV]	[TeV cm-2 s-1] 	[TeV cm-2 s-1] [TeV cm-2 s-1]
1.862e-01 2.920e-02 3.947e-02 8.168e-11 3.172e-11 2.954e-11
2.667e-01 4.957e-02 5.121e-02 1.511e-11 6.812e-12 6.459e-12
3.819e-01 8.229e-02 6.564e-02 7.652e-12 2.419e-12 2.288e-12
5.597e-01 1.216e-01 9.555e-02 2.517e-12 8.878e-13 8.248e-13
8.876e-01 3.239e-01 2.063e-01 6.505e-13 2.483e-13 2.287e-13 




Fig. 3. Light curve and flux upper limits measured with Fermi-LAT in 2018 between 100 MeV and 500 GeV.  

#flux,flux_err,flux_ul95,ts,index,index_err,tmin,tmax,mjd,mjd_err,ul
#[10^{-8} cm^-2 s^-1],[10^{-8} cm^-2 s^-1],[10^{-8} cm^-2 s^-1], , , , , , , ,
0.8537752822032689,0.44505843347723945,1.3695223262807579,26.481889000016963,1.7113146217395143,0.20638695622286465,536457605,541641605,58149.00005787037,30.0,False
0.17124793677983757,0.174864437727625,0.36011420233229263,23.446717752551194,1.3489649039945335,0.34547458209063175,541641605,546825605,58209.00005787037,30.0,False
0.2748783954202438,0.28158456350901223,0.6329587801908849,6.843677279219264,1.7307330912484375,0.3799767273830494,546825605,552009605,58269.00005787037,30.0,True
4.256063117203727,1.5815111629255765,6.221240318428374,19.301459140937368,2.5768772556613095,0.3083197560608138,552009605,554601605,58314.00005787037,15.0,False
0.9480846609293854,1.3215388031394082,2.9031823900059837,0.865886400169984,2.605490427496777,1.1738437374880684,554601605,557193605,58344.00005787037,15.0,True
0.00023153601529587382,0.14740589150259994,2.9142569927978856,-4.25938269472681e-05,2.7980219294640407,133.95702718984808,557193605,559785605,58374.00005787037,15.0,True
1.0972184964957834,0.5421040808080724,1.7266803916744518,49.892373907598085,1.5935819141665024,0.18716842661882488,559785605,562377605,58404.00005787037,15.0,False
6.915169982498934,2.3094518704724734,9.908693187896207,21.507781770822476,2.6304073390348974,0.27049134005013675,562377605,564969605,58434.00005787037,15.0,False
1.6065263027049193,2.013324567037071,4.47064412289045,0.8782508037766092,2.75213764807652,0.7418847863492646,564969605,567561605,58464.00005787037,15.0,True