All of the dispersive elements in COS are holographically-ruled, ion-etched diffraction gratings with excellent scattered light properties and reflectivities. The gratings have Al+MgF2 coatings, except the G225M and G285M gratings, which have bare Al coatings.
Further details can be obtained in sections 3.2.3, 5.11, and 13.3 of the COS Instrument Handbook.
|
Grating
|
Useful wavelength range (Å)1
|
Bandpass per exposure (Å)
|
Resolving
Power2 R = λ/Δλ |
Dispersion
(mÅ pixel-1) |
|---|---|---|---|---|
|
FUV Channel
|
||||
G130M |
1150 -1450 |
2923 |
20,000 - 24,000 |
9.97 |
G160M |
1405 - 1775 |
3604 |
20,000 - 24,000 |
12.23 |
G140L |
1230 - 2050 |
>820 |
2,000 - 5,000 |
80.3 |
|
NUV Channel
|
||||
G185M |
1700 - 2100 |
3 × 35 |
16,000 - 20,000 |
37 |
G225M |
2100 - 2500 |
3 × 35 |
20,000 - 24,000 |
33 |
G285M |
2500 - 3200 |
3 × 41 |
20,000 - 24,000 |
40 |
G230L |
1650 - 32005 |
(1 or 2) × 398 |
1,550 - 2,900 |
390 |
| Grating | Central Wavelength (Å) | FP-POS | Recorded Wavelengths | |
|---|---|---|---|---|
| Segment B | Segment A | |||
|
Wavelength Ranges for G140L
|
||||
| G140L | 1105 | 3 | No value for Seg B | 1120 - 2246 |
| 1250 | 3 | <900 - 1155 | 1260 - 2385 | |
|
Wavelength Ranges for G130M
|
||||
| G130M | 1291 | 3 | 1134 - 1274 | 1290 - 1430 |
| 1300 | 3 | 1144 - 1284 | 1300 - 1400 | |
| 1309 | 3 | 1153 - 1294 | 1309 - 1449 | |
| 1318 | 3 | 1163 - 1303 | 1319 - 1459 | |
| 1327 | 3 | 1173 - 1313 | 1328 - 1468 | |
|
Wavelength Ranges for G160M
|
||||
| G160M | 1577 | 3 | 1386 - 1559 | 1577 - 1749 |
| 1589 | 3 | 1398 - 1571 | 1589 - 1761 | |
| 1600 | 3 | 1410 - 1581 | 1601 - 1772 | |
| 1611 | 3 | 1421 - 1594 | 1612 - 1784 | |
| 1623 | 3 | 1433 - 1606 | 1625 - 1796 | |