All Tables

Table 1: Objects with I-J>3.5 found in this survey.
Table 2: Objects with photometry suggesting they are L dwarfs. Our photometric spectral classifications are based on the colours in Kirkpatrick et al. (2000).
Table 3: SIPS objects which share common proper motions with other SIPS objects. PA = Position Angle. For NLTT objects see Luyten, for LEHPM objects see Pokorny et al. (2003), for WT objects see Wroblewski & Torres (1991) and for ¹ see Giclas et al. (1971). Pairs marked with * were identified as binaries by Luyten (1988). The pair marked with ** was found simulatiously by Artigau et al. (2007).
Table 4: SIPS objects which share common proper motions with objects found in other studies which are not themselves SIPS objects. These pairings were found during the cross referencing process and should not be regarded as a complete list. PA = Position Angle. For LEHPM objects see Pokorny (2003), for NLTT objects see NLTT, ¹ see Lasker et al. (1990), ² see Gizis et al. (2000) and ³ see Schonfeld (1886). All pairs marked * were identified as common proper motion pairs by Luyten (1988).
Table 5: Objects in this sample with proper motions in the range $\rm0.1''/yr<\mu <0.5''/yr$ which have estimated distances closer that 20 pc.
Table 6: Objects in this sample with proper motions above 0.5''/yr which have estimated distances closer that 20 pc.
Table 7: An example section of Table 7 which contains all objects in the survey with $\rm0.1''/yr>\mu >0.5''/yr$ . The full version of Table 7 along with a citation key is available from CDS.
Table 8: An example section of Table 8 which contains all objects in our overspill sample which have $\rm\mu >0.5''$ /yr. The full version of Table 8 along with a citation key is available from CDS.