Table 3.
Observing information of the QSO2 sample observed with OSIRIS/GTC.
| Short name | IP FWHM | Slit width | Seeing (slit width) | Seeing | DIMM seeing | Airmass |
|---|---|---|---|---|---|---|
| SDSS/PA | (Å) | (″) | (″) | (″) | (″) | (″) |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) |
| 0741+3020 | 5.29 ± 0.08 | 1.5 | 1.40 ± 0.04 | 1.47 ± 0.04 | 1.6 | 1.17 |
| 0818+3958 | 5.32 ± 0.08 | 1.5 | 1.69 ± 0.06 | 1.84 ± 0.07 | 1.6 | 1.04 |
| 0834+5534/34 | 5.50 ± 0.46 | 1.5 | 0.98 ± 0.02 | 1.00 ± 0.02 | 1.5 | 1.23 |
| 0834+5534/145 | 5.99 ± 0.69 | 1.5 | 0.78 ± 0.02 | 0.84 ± 0.02 | 1.5 | 1.32 |
| 0902+5459/83 | 5.31 ± 0.15 | 1.5 | 1.67 ± 0.08 | 1.87 ± 0.09 | 1.7 | 1.14 |
| 0902+5459/138 | 5.24 ± 0.08 | 1.5 | 1.88 ± 0.07 | 2.16 ± 0.08 | 1.7 | 1.20 |
| 0956+5735 | 5.25 ± 0.28 | 1.5 | 1.72 ± 0.15 | 2.10 ± 0.18 | 1.6 | 1.20 |
| 1101+4004 | 4.46 ± 0.05 | 1.2 | 2.59 ± 0.12 | 2.64 ± 0.12 | 1.5 | 1.12 |
Notes. Column (1): short name of the source. The slit PA is also quoted, except when only one slit is used for the observations (see Table 1). Column (2): FWHM of the IP as derived from several sky lines. Column (3): slit width in arcsec. Column (4): seeing computed using an aperture equivalent to the slit width. Column (5): seeing computed from several stars in the acquisition image. Column (6): differential image motion monitor seeing value. It gives an approximate estimate of the real seeing during the night. Column (7): airmass during the observations.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.