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Table A.1

Observations and flux values for all epochs.

Epoch Observing dates Instrument Grating Exposure avg F1350a Fit F 1350 b fit α c

2013_v1 2013 June 22 HST:COS G130M 1.8 ks 1.95 ± 0.36
G160M 2.1 ks
2013_v2 2013 July 12 HST:COS G130M 5.0 ks 2.22 ± 0.34
G160M 2.2 ks
2013_v3 2013 July 24 HST:COS G130M 2.0 ks 3.70 ± 0.44
G160M 2.2 ks
2013_v4 2013 July 30 HST:COS G130M 2.0 ks 3.51 ± 0.44
G160M 2.2 ks
2013_v5 2013 August 01 HST:COS G130M 2.0 ks 3.28 ± 0.40
G160M 2.2 ks
2013_v6 2013 December 20 HST:COS G130M 2.0 ks 3.26 ± 0.40 3.14 ± 0.02 0.79 ± 0.03
G160M 2.2 ks
2013_v345 2013 July 24 to 2013 August 01 HST:COS G130M 6.0 ks 3.51 ± 0.24 3.44 ± 0.03 0.776 ± 0.014
G160M 6.6 ks
2013_v12345 2013 June 22 to 2013 August 01 HST:COS G130M 12.8 ks 3.11 ± 0.19 3.051 ± 0.015 0.736 ± 0.026
G160M 11.0 ks
2011 2011 June 16 HST:COS G130M 1.9 ks 6.17 ± 0.52 6.13 ± 0.05 0.86 ± 0.07
G160M 2.4 ks
2004 2004 February 10 to 2004 February 13 HST:STIS E140M 52.2 ks 0.25 ± 0.07 0.203 ± 0.017 1.86 ± 0.29
2002 2002 January 22 to 2002 January 23 HST:STIS E140M 15.3 ks 1.80 ± 0.18 1.80 ± 0.04 1.46 ± 0.06
1998 1998 March 11 HST:STIS E140M 4.75 ks 6.41 ± 0.75 6.43 ± 0.12 1.51 ± 0.13

Notes. .

(a)

Flux at rest-frame 1350 Å in units of 10-14 erg s-1 cm-2 Å-1.

(b)

Flux from a power-law fit of the form F(λ) = F1350(λ/ 1350)α.

(c)

Spectral index from the above power-law fit

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