LBT/LBC z-band image of the field. The coverage of different surveys/instruments is shown, including the forthcoming JWST/NIRCam mosaic. The entire field is also covered by XMM, VLA, JVLA, MUSYC wide, and Spitzer/IRAC.
Multi-band data
| Band | Survey/Instrument | Area | Depth(5σ) | Status/Refs/Notes |
|---|---|---|---|---|
| X-ray 0.5-7 keV | Chandra/ACIS-I | 17' x 17' | 1.7 x 10-16 erg/cm2/s | Nanni+18, Gilli+19, Nanni+20, Marchesi+21, Peca+21 |
| X-ray 0.3-10 keV | XMM | 30' diameter | 1.0 x 10-15 erg/cm2/s | Farrah+04 - reanalyzed data |
| Opt - U B V R i z | MUSYC Wide | 30' x 30' | mAB = 25-26 | Blanc+08 |
| Opt - g | LBT/LBC | 23' x 25' | mAB = 27.0 | PI Mignoli (observed, May 2021) |
| Opt - r i z | LBT/LBC | 23' x 25' | mAB = 25, 26, 27.5 | Morselli+14 |
| Opt - r i z | Subaru/Suprime-Cam | 27' x 34' | mAB = 26-28 | Diaz+14 |
| Opt - F775W F850LP | HST/ACS | 3.3' x 3.3' | mAB = 27.5 | Stiavelli+05, Kim+09 |
| NIR - Y J | WIRCAM/CFHT | 24' x 24' | mAB = 24 | Balmaverde+17 |
| NIR - Ks | WIRCAM/CFHT | 24' x 24' | mAB = 24 | PI Mignoli (observed, Feb 2022, Jan 2023) |
| NIR - Ks | LBT/LUCI+SOUL (AO) | 2 x (30" x 30") | mAB ~ 26 | PI Gilli (observed, Apr 2022, Apr 2023) |
| NIR - J H K | MUSYC Deep | 10' x 10' | mAB = 23 | Quadri+07 |
| NIR - K | MUSYC Wide | 30' x 30' | mAB = 21 | Blanc+08 |
| NIR - F160W | HST/WFC3 | 2' x 2' | mAB = 27.5 | HST archive - D'Amato+20 |
| MIR 3.6-8.0μm | Spitzer/IRAC | ~35' x 35' | [3.6] = 22.5 | Annunziatella+18 |
| MIR 24μm | Spitzer/MIPS | ~10' x 16' | [24] = 19.5 | IRSA archive |
| FIR - 100,160μm | Herschel/PACS | ~4' x 7' | ~10 mJy | IRSA archive; see also Leipski+14 |
| FIR - 250,350,500μm | Herschel/SPIRE | ~16' x 16' | ~30 mJy | IRSA archive; see also Leipski+14 |
| FIR - 1.1mm | AzTEC | 212.6 arcmin2 | 2.6 mJy | Zeballos+18 |
| FIR - 1.2mm | ALMA | 25'' FWHM | 230 μJy | Decarli+18 |
| FIR - 1.2mm | ALMA | 25'' FWHM | 300 μJy | PI Mignoli (observed, May 2022) |
| FIR - 3.0mm | ALMA | 1' x 2' | 35 μJy | D'Amato+20 |
| Radio - 1.4GHz | VLA | 30' FWHM | 90 μJy | Petric+03 - reanalyzed data |
| Radio - 1.4GHz | JVLA | 30' FWHM | 12.5 μJy | D'Amato+22 |
| Radio - 400,650MHz | uGMRT | 80,40' FWHM | 125,50 μJy | PI Brienza (observed, Oct 2021) |
| Radio - 150MHz | LOFAR | 3o FWHM | 650 μJy | Brienza+23 |
Spectroscopic data
| Band | Telescope/Instrument/Mode | # slits/targets | Emission line sensitivity (5σ) | Status/Refs/Notes |
|---|---|---|---|---|
| Opt | LBT/MODS/MOS | MOS | 10-17 erg/cm2/s | Mignoli+20, Marchesi+21 |
| Opt | LBT/MODS/MOS | MOS | 10-17 erg/cm2/s | Marchesi+23 |
| Opt | Keck/DEIMOS/MOS | MOS | 10-17 erg/cm2/s | Decarli+19, Marchesi+21 |
| Opt | Keck/DEIMOS/MOS | MOS | 10-17 erg/cm2/s | Meyer+20 |
| Opt | VLT/MUSE/IFU | IFU | 2 x 10-18 erg/cm2/s | Mignoli+20, Meyer+20, Diaz+21 |
| Opt | VLT/FORS2 | MOS | 6 x 10-18 erg/cm2/s | Mignoli+20, Marchesi+21 |
| NIR | LBT/LUCI/Long Slit | Long Slit | 2 x 10-17 erg/cm2/s | Gilli+19 |
| mm | Noema | single pointing | 0.5 Jy km/s | Decarli+19 |
Last modified: 10 Apr 2023