a  WISEA J000533.57+280705.8: M6 V (Kirkpatrick et al. 1994, J/ApJS/94/749).
b  WISEA J004326.26+222124.0: Although only ~26 arcsec from LSPM J0043+222, source does not share common proper motion with the LSPM object.
c  WISEA J005718.26-404534.2: Candidate white dwarf binary (Day-Jones et al. 2008MNRAS.388..838D).
d  WISEA J010308.35+450929.1: M9 (Cruz et al. 2007, J/AJ/133/439).
e  WISEA J010704.09+243523.8: M9 (Cruz et al. 2003, J/AJ/126/2421).
f  WISEA J015209.73+340033.8: M6.5 V (Kirkpatrick et al. 1997, J/ApJ/476/311).
g  WISEA J021159.43+042150.7: New common proper motion companion to BD+03 301.
h  WISEA J025521.64+194614.9: M0.5-1 V (Luhman 2001ApJ...560..287L).
i  WISEA J025754.85+411130.5: M9? (Cruz et al. 2003, J/AJ/126/2421).
j  WISEA J031606.54-374215.4: New common-proper-motion companion to TYC 7561-77-1.
k  WISEA J032644.74+191926.3: M8.5 (Reid et al. 2008, J/AJ/136/1290).
l  WISEA J035227.56-315105.2: New common-proper-motion companion to LHS 1609.
m  WISEA J035334.72+074818.6: M2 (Robertson 1984AJ.....89.1229R).
n  WISEA J041036.35-145925.2: M8.5 (Rajpurohit et al. 2013, J/A+A/556/A15)
o  WISEA J044350.89-482003.8: New common-proper-motion companion to LTT 2077.
p  WISEA J045958.61-033311.7: M4 (Riaz et al. 2006, J/AJ/132/866).
q  WISEA J051723.88-345121.8: New common-proper-motion companion to omicron Columbae.
r  WISEA J054318.95+642250.2: L1 (Reid et al. 2008, J/AJ/136/1290).
s  WISEA J062352.84+513701.5: M8 (Reid et al. 2008, J/AJ/136/1290).
t  WISEA J065448.82+131002.5: New common-proper-motion companion to 38 Geminorum AB.
u  WISEA J065829.45-125942.7: Appears not to be a common-proper-motion companion to Gliese 256, located 51 arcsec away.
v  WISEA J070720.50+170532.7: Published in Wright et al. (2014AJ....147...61W) as the first AllWISE motion discovery.
w  WISEA J075748.44+503935.0: K5 (Stephenson 1986AJ.....92..139S).
x  WISEA J082149.69+453156.3: M7.5 (Cruz et al. 2007, J/AJ/133/439).
y  WISEA J082852.10-243536.5: New common-proper-motion companion to WT 1549.
z  WISEA J084834.45-785347.5: M5e (Lawson et al. 2002MNRAS.329L..29L).
aa WISEA J091245.46+242546.2: M7 (Cruz et al. 2003, J/AJ/126/2421).
ab WISEA J100231.88+324406.0: M9 (West et al. 2008, J/AJ/135/785).
ac WISEA J100532.08+133113.9: K5 (Stephenson 1986, III/123).
ad WISEA J101958.20+732408.6: M8.5 (Cruz et al. 2003, J/AJ/126/2421).
ae WISEA J102205.98-140032.7: In the 2MASS and DSS images, there appears to be a blue common-proper-motion companion (possibly a white dwarf) ~6 arcsec to the SE of the WISE motion source.
af WISEA J103213.77-420858.6: M7 (Gizis 2002ApJ...575..484G).
ag WISEA J103405.88+035014.1: L0 (Schmidt et al. 2010, J/AJ/139/1808).
ah WISEA J103949.78-383156.0: M1 (Bidelman 1985ApJS...59..197B).
ai WISEA J105407.62-850459.4: M8 (Gizis 2002ApJ...575..484G).
aj WISEA J105536.09-575042.1: New common-proper-motion companion to UPM J1056-5750.
ak WISEA J112453.24+132251.8: M5.5 (Cruz et al. 2003, J/AJ/126/2421).
al WISEA J113333.67-414016.7: New common-proper-motion companion to CD-40 6796.
am WISEA J120247.90+380231.6: M7 (West et al. 2008, J/AJ/135/785).
an WISEA J120623.80-401709.7: M8 (Gizis 2002ApJ...575..484G).
ao WISEA J121058.26-461204.5: New common-proper-motion companion to CD-45 7595 (LTT 4560).
ap WISEA J121841.95-060912.7: M4.5 (Riaz et al. 2006, J/AJ/132/866).
aq WISEA J122338.35-460620.4: M4 (Riaz et al. 2006, J/AJ/132/866).
ar WISEA J122644.61+471422.8: K4 (Maheswar et al. 2003, J/A+A/402/963).
as WISEA J123836.98-270337.0: M2.5 (Riaz et al. 2006, J/AJ/132/866).
at WISEA J124014.80+204752.7: New common-proper-motion companion to BD+21 2442 (G 59-32).
au WISEA J124154.87-315258.4: M6.5 (Gizis 2002ApJ...575..484G).
av WISEA J124726.75-434441.8: New common-proper-motion companion to CD-43 7881 (LTT 4892).
aw WISEA J125453.59-723631.1: Possible new common-proper-motion companion to TYC 7772-1225-1.
ax WISEA J125623.02+283044.7: M7.5 (Kirkpatrick et al. 1997, J/ApJ/476/311).
ay WISEA J131932.24-424531.8: M1 (Riaz et al. 2006, J/AJ/132/866).
az WISEA J132240.60-290536.2: DA3.0 (Gianninas et al. 2011, J/ApJ/743/138).
ba WISEA J132405.16-350806.2: M6 (Gizis 2002ApJ...575..484G).
bb WISEA J132557.78-362035.7: M5 (Gizis 2002ApJ...575..484G).
bc WISEA J133825.35-251647.2: M3.5 (Riaz et al. 2006, J/AJ/132/866).
bd WISEA J134457.17-453537.2: New common-proper-motion companion to LTT 5330.
be WISEA J135425.73-081045.5: K7 (Stephenson 1986, III/123).
bf WISEA J135858.88-005355.5: M9 (West et al. 2008, J/AJ/135/785).
bg WISEA J140350.20-592348.0: New common-proper-motion companion to L 197-165 (NLTT 36089).
bh WISEA J140924.56-305534.1: New common-proper-motion companion to LHS 2807.
bi WISEA J141248.55-162957.3: M3 (Riaz et al. 2006, J/AJ/132/866).
bj WISEA J142053.60-050137.8: New common-proper-motion companion to BD-04 3668.
bk WISEA J142505.52+613116.2: M5 (West et al. 2008, J/AJ/135/785).
bl WISEA J160431.22+090838.9: M8 (Reid et al. 2008, J/AJ/136/1290).
bm WISEA J160741.27-110309.1: M4 (Riaz et al. 2006, J/AJ/132/866).
bn WISEA J161412.96+821139.2: M8 (Cruz et al. 2003, J/AJ/126/2421).
bo WISEA J164611.36+501950.5: M7 (Cruz et al. 2003, J/AJ/126/2421).
bp WISEA J165537.70+045430.2: M8 (Gizis 2002ApJ...575..484G).
bq WISEA J165909.60+205817.6: M3 (Riaz et al. 2006, J/AJ/132/866).
br WISEA J171826.98-224543.5: New common-proper-motion system with WISEA J171828.99-224630.2.
bs WISEA J171828.99-224630.2: New common-proper-motion system with WISEA J171826.98-224543.5.
bt WISEA J172230.07-695119.2: Possible new common-proper-motion system with WISEA J172237.14-695112.2.
bu WISEA J172237.14-695112.2: Possible new common-proper-motion system with WISEA J172230.07-695119.2.
bv WISEA J172615.23-031132.0: M4.5 (Riaz et al. 2006, J/AJ/132/866).
bw WISEA J180811.16-001719.5: K4 (Stephenson 1986, III/123).
bx WISEA J183223.83-443512.5: M6 (Gizis 2002ApJ...575..484G).
by WISEA J185216.88+525715.1: M8 (Cruz et al. 2003, J/AJ/126/2421).
bz WISEA J185225.68-373037.2: M4.5 (Riaz et al. 2006, J/AJ/132/866).
ca WISEA J193904.59-423929.2: M9: (Reid et al. 2008, J/AJ/136/1290).
cb WISEA J194324.81-372212.8: M3.5 (Riaz et al. 2006, J/AJ/132/866).
cc WISEA J201605.71-115838.5: New common-proper-motion system with WISEA J201605.96-115916.7.
cd WISEA J201605.96-115916.7: New common-proper-motion system with WISEA J201605.71-115838.5.
ce WISEA J202218.30-582110.5: This source is likely to be LHS 3541, although it is 62 arcsec away from the J2000 position of LHS 3541 given in SIMBAD.
cf WISEA J205414.99-532957.6: SIMBAD identifies another bright source 31 arcsec away from this WISE source as the motion object BPM 27068.  However, the source identified as BPM 27068 appears not to be moving.  It is thus likely that the WISE motion source is actually BPM 27068 itself.
cg WISEA J210055.27-413146.6: M4 (Riaz et al. 2006, J/AJ/132/866).
ch WISEA J210630.56-382606.1: New common-proper-motion system with WISEA J210632.73-382640.4.
ci WISEA J210632.73-382640.4: New common-proper-motion system with WISEA J210630.56-382606.1.
cj WISEA J211221.80+842733.4: M8 (Reid et al. 2008, J/AJ/136/1290).
ck WISEA J213322.99-061102.8: This WISE object appears to be common proper motion with LP 698-4 (aka the DC white dwarf WD 2130-064), which is 52" distant. The white dwarf is not detected in WISE.
cl WISEA J214728.36+252308.5: Images indicate that this is a common-proper-motion binary. Only the brighter primary is detected in WISE because the secondary is lost in the brighter star's halo.
cm WISEA J214736.41-135335.4: New common-proper-motion companion to Ross 208.
cn WISEA J215027.06-122811.8: M2.5 (Riaz et al. 2006, J/AJ/132/866).
co WISEA J221839.91-532640.1: M2.5 (Riaz et al. 2006, J/AJ/132/866).
cp WISEA J224909.81+320547.0: L5 (Cruz et al. 2007, J/AJ/133/439).
cq WISEA J230226.16+801241.8: New common-proper-motion companion to BD+79 762.
cr WISEA J235459.79-185222.4: L2 (Martin et al. 2010A&A...517A..53M).
cs WISEA J235908.50+233827.1: M9 (Reid et al. 2008, J/AJ/136/1290).
ct WISEA J085510.74-071442.5: This object is 28" from the radio source 3C 209, which has the identifier WISEA J085509.46-071502.9. Although the WISE imaging data show a clear photocentric shift between the two epochs of data, additional imaging is needed to confirm the motion measure.
cu WISEA J151813.45+311515.8: Brightest in W3 band (11.073+/-0.097mag) but also faintly visible at W1 and W2.
cv WISEA J163139.17-244942.7: May correspond to the embedded, sub-mm source JCMTSE J163138.6-244950 in the {rho} Oph star formation complex.
da WISEA J021159.43+042150.7: Using the 2MASS-to-WISE time baseline we obtain a motion, ({mu}{alpha}, {mu}{delta}), of (-140.5+/-10.2, -65.8+/-9.3)mas/yr for this object. The other component, BD+03 301, has a published motion of (-144.70+/-1.64, -78.66+/-1.18)mas/yr (van Leeuwen 2007, I/311). These motions are identical within their 2{sigma} errors, so this is likely a common-proper-motion system.
db WISEA J031606.54-374215.4: Using the 2MASS-to-WISE time baseline we obtain a motion, ({mu}{alpha}, {mu}{delta}), of (48.0+/-11.3, 36.3+/-10.4)mas/yr for this object. The other component, TYC 7561-77-1, has a published motion of (57.4+/-2.2, 30.6+/-2.1)mas/yr (Hog et al. 2000, I/259). Although small, these motions are identical within their 1{sigma} errors, so this is likely a common-proper-motion system.
dc WISEA J035227.56-315105.2: Using the 2MASS-to-WISE time baseline we obtain a motion, ({mu}{alpha}, {mu}{delta}), of (196.6+/-11.0, -531.9+/-10.4)mas/yr for this object. The other component, LHS 1609, has a published motion of (219, -533)mas/yr (Luyten 1979a). These motions are identical to within 2{sigma}, so this is likely a common-proper-motion binary.
dd WISEA J044350.89-482003.8: Using the 2MASS-to-WISE time baseline we obtain a motion, ({mu}{alpha}, {mu}{delta}), of (-5.5+/-9.0, 263.4+/-8.8)mas/yr for this object. The other component, LTT 2077, has a published motion of (4.75+/-0.37, 276.85+/-0.43)mas/yr (van Leeuwen 2007, I/311). These motions are identical to within 2{sigma}, so this is likely a common-proper-motion binary.
de WISEA J051723.88-345121.8: Using the 2MASS-to-WISE time baseline we obtain a motion, ({mu}{alpha}, {mu}{delta}), of (86.7+/-8.2, -340.4+/-8.0)mas/yr for this object. The other component, o Columbae, has a published motion of (92.67+/-0.14, -336.23+/-0.22)mas/yr (van Leeuwen 2007, I/311). These motions are identical within their 1{sigma} errors, so this is very likely a common-proper-motion system.
df WISEA J065448.82+131002.5: Using the 2MASS-to-WISE time baseline we obtain a motion, ({mu}{alpha}, {mu}{delta}), of (63.7+/-9.2, -86.2+/-8.8)mas/yr for this object. The other component, 38 Geminorum AB, has a published motion of (68.48+/-1.78, -72.98+/-1.46)mas/yr (van Leeuwen 2007, I/311). These motions are identical within their 2{sigma} errors, so this is likely a common-proper-motion system.
dg WISEA J074021.62-172454.8: This object falls in a tile overlap region, so it was processed twice by AllWISE. The apparition chosen for inclusion in the AllWISE Source Catalog, whose values are listed in the table above, was selected over the other apparition because the former is further from the tile edge. The other apparition, which appears in the AllWISE Reject Table as WISEAR J074021.62-172454.8, has motion values of 1563+/-50mas/yr and -608+/-52mas/yr in R.A. and Decl., respectively. The values for the AllWISE Reject source are <1{sigma} discrepant from either apparition of the primary, LHS 235. Because the same underlying frames are used for both tiles, it is unclear why the motion for one of the apparitions of LHS 234 is so wildly discrepant in R.A.
dh WISEA J082852.10-243536.5: Using the 2MASS-to-WISE time baseline we obtain a motion, ({mu}{alpha}, {mu}{delta}), of (157.6+/-10.8, -137.5+/-10.7)mas/yr for this object. The other component, WT 1549, has a published motion of (151+/-13, -140+/-13)mas/yr (Wroblewski & Torres 1996). These motions are identical within their 1{sigma} errors, so this is very likely a common-proper-motion system.
di WISEA J105536.09-575042.1: Using the 2MASS-to-WISE time baseline we obtain a motion, ({mu}{alpha}, {mu}{delta}), of (-196.5+/-9.3, 128.2+/-9.3)mas/yr for this object. The other component, UPM J1056-5750, has a published motion of (-194.4+/-7.4, 121.9+/-6.9)mas/yr (Finch et al. 2010, J/AJ/140/844). These motions are identical within their 1{sigma} errors, so this is very likely a common-proper-motion system.
dj WISEA J113333.67-414016.7: Using the 2MASS-to-WISE time baseline we obtain a motion, ({mu}{alpha}, {mu}{delta}), of (-152.9+/-9.2, -120.1+/-8.5)mas/yr for this object. The other component, CD-40 6796, has a published motion of (-169.7+/-1.9, -117.3+/-1.7)mas/yr (Hog et al. 2000, I/259). These motions are identical within their 2{sigma} errors, so this is likely a common-proper-motion system.
dk WISEA J121058.26-461204.5: Using the 2MASS-to-WISE time baseline we obtain a motion, ({mu}{alpha}, {mu}{delta}), of (101.3+/-8.3, 167.7+/-8.1)mas/yr for this object. The other component, CD-45 7595, has a published motion of (89.11+/-0.40, 168.15+/-0.47)mas/yr (van Leeuwen 2007, I/311). These motions are identical within their 2{sigma} errors, so this is likely a common-proper-motion system.
dl WISEA J124014.80+204752.7: Using the 2MASS-to-WISE time baseline we obtain a motion, ({mu}{alpha}, {mu}{delta}), of (205.6+/-10.6, -369.1+/-10.8)mas/yr for this object. The other component, BD+21 2442, has a published motion of (202.04+/-1.44, -368.45+/-0.99)mas/yr (van Leeuwen 2007, I/311). These motions are identical within their 1{sigma} errors, so this is very likely a common-proper-motion system.
dm WISEA J124726.75-434441.8: Using the 2MASS-to-WISE time baseline we obtain a motion, ({mu}{alpha}, {mu}{delta}), of (-182.0+/-7.1, -95.4+/-7.1)mas/yr for this object. The other component, CD-43 7881, has a published motion of (-196.60+/-0.80, -94.31+/-0.89)mas/yr (van Leeuwen 2007, I/311). These motions are identical within their 2{sigma} errors, so this is likely a common-proper-motion system.
dn WISEA J125435.54-381111.7: Using the 2MASS-to-WISE time baseline we obtain a motion, ({mu}{alpha}, {mu}{delta}), of (161.1+/-7.9, -25.4+/-7.8)mas/yr for this object. The other component, TYC 7772-1225-1, has a published motion of (149.6+/-2.8, -40.1+/-2.7)mas/yr (Hog et al. 2000, I/259). These motions are identical to within 2{sigma}, so this could be a common-proper-motion binary. In the UCAC4 Catalog this pair has listed motions of (147.6+/-0.7, -38.2+/-1.0)mas/yr for the brighter component and (144.5+/-0.8, -29.0+/-0.8)mas/yr for the fainter component. Although the 10{sigma} discrepancy in Decl. would seem to rule these out as a cpm pair, UCAC4 measurements can be unreliable and thus we still list this pair as a possible physical system.
do WISEA J134457.17-453537.2: Using the 2MASS-to-WISE time baseline we obtain a motion, ({mu}{alpha}, {mu}{delta}), of (-237.8+/-8.0, 35.7+/-8.0)mas/yr for this object. The other component, LTT 5330, has a published motion of (-240.51+/-13.1, 25.99+/-13.1)mas/yr (Roser et al. 2008, I/312). These motions are identical within their 1{sigma} errors, so this is very likely a common-proper-motion system.
dp WISEA J140350.20-592348.0: Using the 2MASS-to-WISE time baseline we obtain a motion, ({mu}{alpha}, {mu}{delta}), of (30.5+/-8.7, -494.3+/-8.5)mas/yr for this object. The other component, L 197-165, has a published motion of (33, -469)mas/yr (Luyten 1979b). The motion of the unpublished WISE object is identical within its 1{sigma} errors to the R.A. motion of the Luyten object but discrepant by ~3{sigma} from the Luyten Decl. measurement. Given the large motion in Decl. and the proximity of the sources, this is still likely a common-proper-motion system.
dq WISEA J140924.56-305534.1: Using the 2MASS-to-WISE time baseline we obtain a motion, ({mu}{alpha}, {mu}{delta}), of (-456.4+/-8.1, -213.8+/-8.0)mas/yr for this object. The other component, LHS 2807, has a published motion of (-460.60+/-3.68, -219.82+/-3.02)mas/yr (van Leeuwen 2007, I/311). These motions are identical to <1{sigma}, so this is likely a common-proper-motion system.
dr WISEA J142053.60-050137.8: Using the 2MASS-to-WISE time baseline we obtain a motion, ({mu}{alpha}, {mu}{delta}), of (-131.2+/-10.2, -55.4+/-10.0)mas/yr for this object. The other component, BD-04 3668, has a published motion of (-137.5+/-3.5, -58.0+/-3.2)mas/yr (Roeser & Bastian 1988). These motions are identical to <1{sigma}, so this is likely a common-proper-motion system.
ds WISEA J171828.99-224630.2 and WISEA J171826.98-224543.5: Using the 2MASS-to-WISE time baseline we obtain a motion, ({mu}{alpha}, {mu}{delta}), of (-149.3+/-8.9, -149.9+/-8.4)mas/yr for the brighter object and (-148.7+/-8.8, -148.8+/-8.3)mas/yr for the fainter one. These motions are identical to <1{sigma}, so this is very likely a common-proper-motion pair.
dt WISEA J172230.07-695119.2 and WISEA J172237.14-695112.2: Using the 2MASS-to-WISE time baseline we obtain a motion, ({mu}{alpha}, {mu}{delta}), of (-145.6+/-10.4, -217.6+/-8.7)mas/yr for the brighter object and (-37.6+/-11.5, -221.9+/-9.8)mas/yr for the fainter one. Although the (larger) Decl. motions are identical to <1{sigma}, the R.A. motions are discrepant by >9{sigma}. A visual check of the system more strongly supports common proper motion than do the actual measurements. We suspect that the WISE astrometry for the fainter source in the pair may be corrupted by a background object --seen at nearly equal magnitude in the earlier DSS2 images-- that lies near its position in the WISE data.
du WISEA J201605.71-115838.5 and WISEA J201605.96-115916.7: Both of these objects are listed in the UCAC4 Catalog, but no other literature is available. Using the 2MASS-to-WISE time baseline we obtain motions, ({mu}{alpha}, {mu}{delta}), of (-72.4+/-8.9, -141.1+/-7.5)mas/yr for the brighter component and (-69.4+/-9.0, -134.4+/-7.7)mas/yr for the dimmer component, which are identical within their 1{sigma} errors. In the UCAC4 Catalog this pair has listed motions of (-70.9+/-2.1, -135.6+/-2.2)mas/yr for the brighter component and (-57.3+/-2.1, -130.5+/-2.1)mas/yr for the fainter component. Although the 6.5{sigma} discrepancy in R.A. would seem to rule these out as a cpm pair, the secondary appears to be blended with another source of nearly equal magnitude in the DSS2 images. Because visual checks strongly suggest this is a co-moving system, we still list this as a possible physical pair.
dv WISEA J210630.56-382606.1 and WISEA J210632.73-382640.4: Using the 2MASS-to-WISE time baseline we obtain a motion, ({mu}{alpha}, {mu}{delta}), of (174.9+/-10.1, -323.4+/-10.1)mas/yr for the brighter object and (187.1+/-10.3, -323.3+/-10.2)mas/yr for the fainter one. The motions are identical to <2{sigma}, so these are likely a common-proper-motion pair.
dw WISEA J214736.41-135335.4: Using the 2MASS-to-WISE time baseline we obtain a motion, ({mu}{alpha}, {mu}{delta}), of (151.6+/-10.0, -300.2+/-9.3)mas/yr for this object. The other component, Ross 208, has a published motion of (152+/-5, -296+/-5)mas/yr (Salim & Gould 2003). These motions are identical within <1{sigma}, so this is very likely a common-proper-motion system.
dx WISEA J230226.16+801241.8: Using the 2MASS-to-WISE time baseline we obtain a motion, ({mu}{alpha}, {mu}{delta}), of (-68.1+/-9.9, 114.1+/-9.9)mas/yr for this object. The other component, BD+79 762, has a published motion of (-53.2+/-1.2, 127.2+/-1.2)mas/yr (Hog et al. 2000, I/259). These motions are identical within their 2{sigma} errors, so this is likely a common-proper-motion system.