Free Access
Table 1
List of facilities, instruments and methods employed to determine the full spectral energy distribution of Proxima.
| λ range (nm) | Facility/Instrument | Dataset | Section | Method |
|
|
||||
| 0.7–3.8 | XMM-Newton/RGS | 0551120201, 0551120301, 0551120401 | 2.1 | Combined spectrum, energetic flare correction |
| 3.8–10 | ROSAT/PSPC | RP200502N00, RP200502A01, RP200502A02, RP200502A03 | 2.2 | Plasma fit, combined spectrum, energetic flare correction |
| 10–40 | EUVE | proxima_cen__9305211911N | 2.3 | Spectrum, energetic flare correction |
| 40–92 | Model | 2.4 | Scaled from H Lyman α | |
| 92–117 | FUSE | D1220101000 | 2.5 | Spectrum, geocoronal correction |
| 117–121.4 and | HST/STIS E140M | O5EO01010, O5EO01020, O5EO01030, O5EO01040 | 2.6 | Combined spectrum |
| 121.7–170 | O5EO02010, O5EO02020, O5EO02040 | |||
| 121.4–121.7 | HST/STIS E140M | O5EO01010, O5EO01020, O5EO01030, O5EO01040 | 2.6 | Fit to H Lyman α wings to correct for ISM absorption |
| 170–1000 | HST/STIS G230LB, | OCR7QQANQ, OCR7QQAOQ, OCR7QQARQ, OCR7QQASQ, | 2.7 | Spectrum |
| G430L,G750L | OCR7QQAMQ, OCR7QQAPQ, OCR7QQAQQ | |||
| 1000–30 000 | Model | IR photometry (Table 4) | 2.8 | Fit using BT-Settl models |
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.