Table 3
Stars in the SHINE statistical sample observed as special targets (highest priority).
| Target | Priority | Remarks | Discovery paper | SPHERE paper |
|---|---|---|---|---|
| β Pic | P1 | Known planet and disk | Lagrange et al. (2009) | Lagrange et al. (2019) |
| HR 8799 | P1 | Known planet | Marois et al. (2008) | Zurlo et al. (2016) |
| HD 95086 | P1 | Known planet | Rameau et al. (2013b) | Chauvin et al. (2018) |
| Fomalhaut | P2 | Known planet and disk | Kalas et al. (2008) | – |
| FomalhautB | P3 | Companion to P0 star | – | – |
| PZ Tel | P1 | Known brown dwarf | Biller et al. (2010) | Maire et al. (2016) |
| HIP 107412 | P4 | Known brown dwarf | Milli et al. (2017) | Delorme et al. (2017); Grandjean et al. (2019) |
| 51 Eri | P1 | Known planet | Macintosh et al. (2015) | Samland et al. (2017); Maire et al. (2019) |
| AB Pic | P1 | Known brown dwarf | Chauvin et al. (2005b) | – |
| TYC 8047-0232-1 | P1 | Known brown dwarf | Chauvin et al. (2005a) | – |
| HIP 78530 | P1 | Known brown dwarf | Lafrenière et al. (2011) | – |
| HD 61005 | P1 | Known disk | Hines et al. (2007) | Olofsson et al. (2016) |
| HR 4796 | P1 | Known disk | Schneider et al. (1999) | Milli et al. (2017, 2019) |
| AU Mic | P1 | Known disk | Liu (2004) | Boccaletti et al. (2015, 2018) |
| HD 30477 | P1 | Known disk | Soummer et al. (2014) | |
| TWA 7 | P1 | Known disk | Choquet et al. (2016) | Olofsson et al. (2018) |
| HD 141943 | P2 | Known disk | Soummer et al. (2014) | Boccaletti et al. (2019) |
| ζ Lep | P2 | Known disk | Moerchen et al. (2010) | |
| ρ Vir | P1 | Known disk | Booth et al. (2013) | – |
| HIP 71724 | P3 | Known low-mass comp. | Hinkley et al. (2015) | – |
| HIP 73990 | P3 | Known low-mass comp. | Hinkley et al. (2015) | – |
| HD 115600 | P3 | Known disk | Currie et al. (2015) | – |
| HD 377 | P2 | Known disk | Choquet et al. (2016) | – |
Notes. The originalpriority in the selection of the statistical sample, the motivation for priority upgrade, and the references to discovery papers and individual SPHERE papers are listed. SAM stands for sparse aperture masking (e.g., Tuthill et al. 2006).
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