| Observable . | Frequency/en.range . | Instrument . | Detection threshold . | Note . |
|---|---|---|---|---|
| X-ray emission | 0.3–2.0 keV | eROSITA | |$\approx \!2 \times 10^{-15} \rm erg\, s^{-1} \,cm^2$| | 10 ks (polar region survey) |
| X-ray emission | 0.3–2.0 keV | ATHENA-WFI | |$\approx \!5 \times 10^{-16} \rm erg\, s^{-1} \,cm^2$| | 100 ks |
| Differential H i Temperature | 1400 MHz | ASKAP | |$\approx \!10^{-3} \rm \,K$| | Possum |
| Differential H i Temperature | 1000 MHz | SKA-MID | |$\approx \!10^{-5} \rm \,K$| | Phase II survcey |
| Radio emission | 200 MHz | LOFAR-HBA | |$\approx \!1.0 \rm\, \mu Jy\, arcsec^{-2}$| | Tier I survey |
| Radio emission | 200 MHz | SKA-LOW | |$\approx \!0.2 \rm \, \mu Jy\, arcsec^{-2}$| | 2 years survey |
| Radio emission | 180 MHz | MWA | |$\approx \!0.28 \rm \, \mu Jy\, arcsec^{-2}$| | MWA Phase I |
| Faraday Rotation | 1400 MHz | ASKAP/Meerkat | |$\approx \!1\, \rm rad\, m^{-2}$| | Possum/Mightee-Pol |
| Faraday Rotation | 1000 MHz | SKA-MID | |$\approx \!0.1\, \rm rad\, m^{-2}$| | Phase II |
| Compton Y-param. | 220 GHz | PLANCK | ≈2890 | |
| Compton Y-param. | 21 GHz | AtlAS | ≈1000 |
| Observable . | Frequency/en.range . | Instrument . | Detection threshold . | Note . |
|---|---|---|---|---|
| X-ray emission | 0.3–2.0 keV | eROSITA | |$\approx \!2 \times 10^{-15} \rm erg\, s^{-1} \,cm^2$| | 10 ks (polar region survey) |
| X-ray emission | 0.3–2.0 keV | ATHENA-WFI | |$\approx \!5 \times 10^{-16} \rm erg\, s^{-1} \,cm^2$| | 100 ks |
| Differential H i Temperature | 1400 MHz | ASKAP | |$\approx \!10^{-3} \rm \,K$| | Possum |
| Differential H i Temperature | 1000 MHz | SKA-MID | |$\approx \!10^{-5} \rm \,K$| | Phase II survcey |
| Radio emission | 200 MHz | LOFAR-HBA | |$\approx \!1.0 \rm\, \mu Jy\, arcsec^{-2}$| | Tier I survey |
| Radio emission | 200 MHz | SKA-LOW | |$\approx \!0.2 \rm \, \mu Jy\, arcsec^{-2}$| | 2 years survey |
| Radio emission | 180 MHz | MWA | |$\approx \!0.28 \rm \, \mu Jy\, arcsec^{-2}$| | MWA Phase I |
| Faraday Rotation | 1400 MHz | ASKAP/Meerkat | |$\approx \!1\, \rm rad\, m^{-2}$| | Possum/Mightee-Pol |
| Faraday Rotation | 1000 MHz | SKA-MID | |$\approx \!0.1\, \rm rad\, m^{-2}$| | Phase II |
| Compton Y-param. | 220 GHz | PLANCK | ≈2890 | |
| Compton Y-param. | 21 GHz | AtlAS | ≈1000 |
Note: We associate to each observable a reference instrument, which loosely corresponds to the adopted observational cut.
| Observable . | Frequency/en.range . | Instrument . | Detection threshold . | Note . |
|---|---|---|---|---|
| X-ray emission | 0.3–2.0 keV | eROSITA | |$\approx \!2 \times 10^{-15} \rm erg\, s^{-1} \,cm^2$| | 10 ks (polar region survey) |
| X-ray emission | 0.3–2.0 keV | ATHENA-WFI | |$\approx \!5 \times 10^{-16} \rm erg\, s^{-1} \,cm^2$| | 100 ks |
| Differential H i Temperature | 1400 MHz | ASKAP | |$\approx \!10^{-3} \rm \,K$| | Possum |
| Differential H i Temperature | 1000 MHz | SKA-MID | |$\approx \!10^{-5} \rm \,K$| | Phase II survcey |
| Radio emission | 200 MHz | LOFAR-HBA | |$\approx \!1.0 \rm\, \mu Jy\, arcsec^{-2}$| | Tier I survey |
| Radio emission | 200 MHz | SKA-LOW | |$\approx \!0.2 \rm \, \mu Jy\, arcsec^{-2}$| | 2 years survey |
| Radio emission | 180 MHz | MWA | |$\approx \!0.28 \rm \, \mu Jy\, arcsec^{-2}$| | MWA Phase I |
| Faraday Rotation | 1400 MHz | ASKAP/Meerkat | |$\approx \!1\, \rm rad\, m^{-2}$| | Possum/Mightee-Pol |
| Faraday Rotation | 1000 MHz | SKA-MID | |$\approx \!0.1\, \rm rad\, m^{-2}$| | Phase II |
| Compton Y-param. | 220 GHz | PLANCK | ≈2890 | |
| Compton Y-param. | 21 GHz | AtlAS | ≈1000 |
| Observable . | Frequency/en.range . | Instrument . | Detection threshold . | Note . |
|---|---|---|---|---|
| X-ray emission | 0.3–2.0 keV | eROSITA | |$\approx \!2 \times 10^{-15} \rm erg\, s^{-1} \,cm^2$| | 10 ks (polar region survey) |
| X-ray emission | 0.3–2.0 keV | ATHENA-WFI | |$\approx \!5 \times 10^{-16} \rm erg\, s^{-1} \,cm^2$| | 100 ks |
| Differential H i Temperature | 1400 MHz | ASKAP | |$\approx \!10^{-3} \rm \,K$| | Possum |
| Differential H i Temperature | 1000 MHz | SKA-MID | |$\approx \!10^{-5} \rm \,K$| | Phase II survcey |
| Radio emission | 200 MHz | LOFAR-HBA | |$\approx \!1.0 \rm\, \mu Jy\, arcsec^{-2}$| | Tier I survey |
| Radio emission | 200 MHz | SKA-LOW | |$\approx \!0.2 \rm \, \mu Jy\, arcsec^{-2}$| | 2 years survey |
| Radio emission | 180 MHz | MWA | |$\approx \!0.28 \rm \, \mu Jy\, arcsec^{-2}$| | MWA Phase I |
| Faraday Rotation | 1400 MHz | ASKAP/Meerkat | |$\approx \!1\, \rm rad\, m^{-2}$| | Possum/Mightee-Pol |
| Faraday Rotation | 1000 MHz | SKA-MID | |$\approx \!0.1\, \rm rad\, m^{-2}$| | Phase II |
| Compton Y-param. | 220 GHz | PLANCK | ≈2890 | |
| Compton Y-param. | 21 GHz | AtlAS | ≈1000 |
Note: We associate to each observable a reference instrument, which loosely corresponds to the adopted observational cut.
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