| Optics | Wolter Type-I |
| Mirror coatings | Iridium |
| Mirror outer diameters (1, 3, 4, 6) | 1.23, 0.99, 0.87, 0.65 m |
| Mirror lengths | 84 cm |
| Unobscured clear aperture | 1145 cm2 |
| Focal length | 10.066 m |
| Plate scale | 48.8 µm/arcsec |
| PSF FWHM (with detector) | 0.5 arcsec |
| Ghost-free field of view | 30 arcmin diameter |
| Effective Area: | |
| @ 0.25 keV | 800 cm2 |
| @ 5.0 keV | 400 cm2 |
| @ 8.0 keV | 100 cm2 |
| Read more in the HRMA chapter of the Proposer's Observatory Guide | |
| Focal plane arrays: | |
| I-array (ACIS-I) | 4 CCDs placed to lie tangent to the focal surface, used for imaging |
| S-array (ACIS-S) | 6 CCDs in a linear
array tangent to the grating Rowland circle, used for either imaging or as a grating readout |
| CCD format | 1024 by 1024 pixels |
| Pixel size | 24.0 µm (0.492 ± 0.0001 arcsec) |
| ACIS-I array size | 16.9 by 16.9 arcmin |
| ACIS-S array size | 8.3 by 50.6 arcmin |
| On-axis effective area of frontside illuminated (FI) chips (integrated over the PSF to >99% encircled energy): | |
| @ 0.5 keV | 110 cm2 |
| @ 1.5 keV | 600 cm2 |
| @ 8.0 keV | 40 cm2 |
| Quantum efficiency for FI chips: | |
| 3.0 - 5.0 keV | > 80% |
| 0.8 - 8.0 keV | > 30% |
| Quantum efficiency for backside illuminated (BI) chips: | |
| 0.8 - 6.5 keV | > 80% |
| 0.3 - 8.0 keV | > 30% |
| Maximum readout rate per channel | ~ 100 kpix/sec |
| Minimum row readout time | 2.8 ms |
| Nominal frame time | 3.2 sec (full frame) |
| Allowable frame times | 0.2 to 10.0 sec |
| Frame transfer time | 41 µs (per row) |
| Point-source sensitivity | 4 X 10-15 ergs/cm2/s in 104 s (0.4 to 6.0 keV) |
| Read more in the ACIS chapter of the Proposer's Observatory Guide | |
| Focal plane arrays: | |
| HRC-I: | CsI-coated microchannel plate pairs, 90 X 90 mm |
| HRC-S: | CsI-coated microchannel plate pairs, 3-100 X 20 mm |
| Field of view: | |
| HRC-I | ~ 30 X 30 arcmin |
| HRC-S | 6 X 90 arcmin |
| Spatial resolution, FWHM: | ~ 20 µm, ~ 0.4 arcsec |
| Energy range: | 0.08 - 10.0 keV |
| Spectral resolution (E/dE): | ~ 1 @ 1 keV |
| Quantum efficiency: | |
| @ 1.0 keV | 30% |
| @ 8.0 keV | 30% |
| On-axis effective area: | |
| HRC-I @ 0.277 keV | 133 cm2 |
| HRC-I @ 1 keV | 227 cm2 |
| Time resolution | 16 µs |
| Limiting sensitivity   (point source, 3 sigma detection in 3 X 105 s) | 9 X 10-16erg/cm2/s |
| On-orbit quiescent background (before ground processing): | |
| HRC-I | 9 X 10-6cts/s/arcsec2 |
| HRC-S | 1.8 X 10-4cts/s/(res. elm.) |
| Read more in the HRC chapter of the Proposer's Observatory Guide | |
| HETGS range: | 0.4 - 10.0 keV (31 - 1.2 Å) |
| High Energy Grating (HEG) range: | 0.8 - 10.0 keV (15 - 1.2 Å) |
| Medium Energy Grating (MEG) range: | 0.4 - 5.0 keV (31 - 2.5 Å) |
| Effective area (MEG+HEG first orders, with ACIS-S): | |
| @ 0.5 keV | 7 cm2 |
| @ 1.0 keV | 59 cm2 |
| @ 1.5 keV | 200 cm2 |
| @ 6.5 keV | 28 cm2 |
| Resolving power (E/dE): | |
| HEG: | 65 - 1070 (1000 @ 1 keV, 12.4 Å) |
| MEG: | 80 - 970 (660 @ 0.826 keV, 15 Å) |
| Resolution: | |
| d lambda, HEG: | 0.012 Å FWHM |
| d lambda, MEG: | 0.023 Å FWHM |
| Absolute wavelength accuracy: | |
| HEG: | ± 0.006 Å |
| MEG: | ± 0.011 Å |
| Wavelength scale: | |
| HEG: | 0.0055595 Å / ACIS pixel |
| MEG: | 0.0111185 Å / ACIS pixel |
| Read more in the HETG chapter of the Proposer's Observatory Guide | |
| Wavelength range: | |
| HRC-S | 1.7 - 170 Å |
| ACIS-S | 1.4 - 63 Å |
| Energy range: | |
| HRC-S | 0.07 - 7.29 keV |
| ACIS-S | 0.20 - 8.86 keV |
| Resolution: (d lambda, FWHM) | 0.05 Å |
| Resolving power: (E/dE) | |
| 50 - 160 Å | >= 1000 |
| 3 - 50 Å | ~ 20 ⨉ λ |
| Dispersion | 1.148 Å/mm |
| Plate scale | 48.80 µm/arcsec |
| Effective area (with HRC-S): | |
| 125 - 170 Å | 1 - 2 cm2 |
| 60 - 120 Å | 3 - 7 cm2 |
| 44 - 60 Å | 7 - 12 cm2 |
| 19 - 40 Å | 4 - 8 cm2 |
| 6 - 18 Å | 10 - 25 cm2 |
| 2 - 5 Å | 3 - 5 cm2 |
| Background (quiescent) | |
| HRC-S, on-orbit | 0.12 counts/pixel/100-ksec |
| HRC-S, after filtering | ~ 0.04 counts/pixel/100-ksec |
| ACIS-S, on-orbit | « 0.01 counts/pixel/100-ksec |
| Read more in the LETG chapter of the Proposer's Observatory Guide | |
Last modified: 01/08/21