Table 1
Deep imaging surveys of young (<100 Myr) and intermediate-old to old (0.1−5 Gyr), close (<100 pc) stars that are dedicated to the search for planetary mass companions.
| Reference | Telescope | Instr. | Mode | Filter | FoV | # | SpT | Age | ||
( ) |
(Myr) | |||||||||
|
|
||||||||||
| Chauvin et al. (2003) | ESO3.6m | ADONIS | Cor-I | H,K | 13 × 13 | 29 | GKM | ≲50 | ||
| Neuhäuser et al. (2003) | NTT | Sharp | Sat-I | K | 11 × 11 | 23 | AFGKM | ≲50 | ||
| NTT | Sofi | Sat-I | H | 13 × 13 | 10 | AFGKM | ≲50 | |||
| Lowrance et al. (2005) | HST | NICMOS | Cor-I | H | 19 × 19 | 45 | AFGKM | 10−600 | ||
| Masciadri et al. (2005) | VLT | NaCo | Sat-I | H,K | 14 × 14 | 28 | KM | ≲200 | ||
| Biller et al. (2007) | VLT | NaCo | SDI | H | 5 × 5 | 45 | GKM | ≲300 | ||
| MMT | SDI | H | 5 × 5 | – | – | – | ||||
| Kasper et al. (2007) | VLT | NaCo | Sat-I | L ′ | 28 × 28 | 22 | GKM | ≲50 | ||
| Lafrenière et al. (2007) | Gemini-N | NIRI | ADI | H | 22 × 22 | 85 | 10–5000 | |||
| Apai et al. (2008)a | VLT | NaCo | SDI | H | 3 × 3 | 8 | FG | 12–500 | ||
| Chauvin et al. (2010) | VLT | NaCo | Cor-I | H,K | 28 × 28 | 88 | BAFGKM | ≲100 | ||
| Heinze et al. (2010a,b) | MMT | Clio | ADI | L ′ ,M | 15.5 × 12.4 | 54 | FGK | 100–5000 | ||
| Janson et al. (2011) | Gemini-N | NIRI | ADI | H,K | 22 × 22 | 15 | BA | 20–700 | ||
| Vigan et al. (2012) | Gemini-N | NIRI | ADI | H,K | 22 × 22 | 42 | AF | 10–400 | ||
| VLT | NaCo | ADI | H,K | 14 × 14 | – | – | – | |||
| Delorme et al. (2012) | VLT | NaCo | ADI | L ′ | 28 × 28 | 16 | M | ≲200 | ||
| Rameau et al. (2013c) | VLT | NaCo | ADI | L ′ | 28 × 28 | 59 | AF | ≲200 | ||
| Yamamoto et al. (2013) | Subaru | HiCIAO | ADI | H,K | 20 × 20 | 20 | FG | 125 ± 8 | ||
| Biller et al. (2013) | Gemini-S | NICI | Cor-ASDI | H | 18 × 18 | 80 | BAFGKM | ≲200 | ||
| Brandt et al. (2013) | Subaru | HiCIAO | ADI | H | 20 × 20 | 63 | AFGKM | ≲500 | ||
| Nielsen et al. (2013) | Gemini-S | NICI | Cor-ASDI | H | 18 × 18 | 70 | BA | 50–500 | ||
| Wahhaj et al. (2013)a | Gemini-S | NICI | Cor-ASDI | H | 18 × 18 | 57 | AFGKM | ~100 | ||
| Janson et al. (2013)a | Subaru | HiCIAO | ADI | H | 20 × 20 | 50 | AFGKM | ≲1000 | ||
Notes. We have indicated the telescope, the instrument, the imaging mode (Cor-I: coronagraphic imaging; Sat-I; saturated imaging; I: imaging; SDI: simultaneous differential imaging; ADI: angular differential imaging; ASDI: angular and spectral differential imaging), the filters, the field of view (FoV), the number of stars observed (#), their spectral types (SpT), and ages (Age).
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.