VizieR Online Data Catalog: PS1 z>5.6 QSO Survey. II. 55 quasars follow-up (Banados+, 2023)

In Table 3 we report follow-up photometry, spanning 2013-09-28 to 2020-11-20, for our quasar candidates obtained in the following filters and telescopes: I#705 (I_E) and Z#623 (Z_E) with the ESO Faint Object Spectrograph and Camera (EFOSC2) at the NTT telescope in La Silla, J_G and H_G with the GROND camera at the MPG 2.2m telescope in La Silla, Js Hs Ks with SOFI at the NTT telescope in La Silla, and YR with the RetroCam camera at the Du Pont telescope in Las Campanas Observatory. For completeness, in Table 3 we also report IZYHK magnitudes from public surveys or published papers when available. See Section 2.3.

The discovery of the 55 quasars presented in this work has been a large effort, involving multiple observatories in the time frame 2013-11-19 to 2022-09-28. A few of these quasars have been part of multiple follow-up campaigns, and some of their properties have been presented in the literature; see Section 3.3.

The spectrographs/telescopes used for the discovery of these quasars are the Double Spectrograph (DBSP) on the 200 inch (5m) Hale telescope at Palomar Observatory (P200), the Low Dispersion Survey Spectrograph (LDSS3) at the Clay Magellan telescope at Las Campanas Observatory, the Multi-Object Double Spectrograph (MODS) at the Large Binocular Telescope (LBT), EFOSC2 at the NTT telescope in La Silla, the Low Resolution Imaging Spectrometer (LRIS) at the Keck telescope on Maunakea, the Gemini Multi-Object Spectrographs (GMOS) on the Gemini-North telescope, the Red Channel Spectrograph on the 6.5m MMT Telescope, and the FOcal Reducer/low dispersion Spectrograph 2 (FORS2) at the Very Large Telescope (VLT). The spectroscopic observations log is listed in Table 1.

(3 data files).