Disk Detective Talk
A #mstar with #I-IR-E
F Star - possible contamination from the star at 6 o'clock
#i-ir-e
M star YSOc. Vetted to round three user added
A #late type star, M by color. I-IR-E but passes ruler test. Vetted to Mdwarf spreadsheet
#I-IR-E
V* V360 Aur -- Long-period variable star... likely #MGiant
A #late type star, M by color. PM 2.8 / -5.9
A G8 YSOc - vetted to round three.
A #late type star that is highly variable, Vamp around .92 - factoring in fairly low PM and probably a #MGiant
Haro 5-17 -- Emission-line Star
Vetted to round 3
IRAS 05363-1115 -- Star
A #late type M star. PM 8.3/1.8 and vmag 15.005.
IRAS 23384+5307 -- Star
A #late type star, M by color. Vmag 14.102 and PM 5/5.4 (Finch 2016)
LAMOST J070240.89+114104.0 -- Star
A #late type star. CSS LC shows a variable star, and MACIEJEWSKI list it as a variable star as well. Probably an #MGiant
GSC 02772-01244 -- Star
A #late type object with #I-IR-E and doesn't pass ruler test. Not a good candidate.
A #late type star, M by color. W1-W4=1.7 with PM -9/1.8 (Zacharias 2017).
2MASS J19183916+3345453 -- Asymptotic Giant Branch Star (He-burning)
IRAS 17392-1225 -- Infra-Red source
A #late type star, M by color. W1-W4=1.4 and PM 2.4/2 (Zacharias 2012)
A #late type star with distance of 4166pc (Kunder 2017).... #MGiant
UCAC2 4716143 -- Star
A #late type star, M by color. W1-W4=1 with -8.4/-1.9 (Zacharias 2015)
A #late type star, M by color. CSS LC is very tight. W1-W4=2.1 and PM -.8/-2.1 (Zacharias 2015)
RAVE J113411.6-491450 -- Star
#I-IR-E and fails ruler test
A #late type star, M by color. W1-W4=.98 and PM 2.7/6.6 (Zacharias 2015).
A #late type star, M by color. W1-W4=1.1 and PM -11.1/.2 (Zacharias 2012)
A #late type star, M by color. W1-W4=1.49 and CSS LC shows variation around .75 - PM 4.5/-5.7 (Zacharias 2012)
A #ate type star. W1-W4=1.63 - PM -2.9/=10.1(Zacharias 2015)
A #late type star M by color. CSS LC shows limited variability. W1-W4=1.48 and PM -3.5/-11.1 (Zacharias 2015) Vmag=14.81 (AAVSO)
IRAS 17066-0627 -- Star
A #late type star, M by color. W1-W4=1.61 and PM 7.1/1.5 (URAT 1)
V* MX Gem -- Long-period variable star
A # late type star, M by color. PM -.2/13 UCAC4 and Vmag 14.54.
HD 250160 -- Emission-line Star
A #late type star, M by color. PM -2.9/1 per UCAC5 and Vmag12.974 per AAVSO.
A #late type star, M by color. PM 13.5/9.8 URAT 5 and Vmag 14.957 AAVSO
A #late type star, M by color. PM .1/-5.5 UCAC4.
vetted to mdwarf sheet!!!
A #late type star, M by color. PM 6.2/-17.1 (Zacharias 2015)
2MASS J17112377-0237127 -- Star
A #late type star, M by color. PM 2.2/.7 (Zacharias 2017) and vmag: 14.097 per AAVSO.
A #late type star, M by color. PM 4.8/-4.3 (Zacharias 2015) and Vmag: 16.515 in AAVSO.
M by color...distance 1086pc (Pojmanski+, 2002-2005) .... #MGiant
UCAC2 3432932 -- Star
A #late type star, M by color. PM -4.6/-7.2 (Zacharias 2012) with vmag: 12.54 (GSC2.3) (STScI, 2006). W1-W4 = 1.668
A #late type star, M by color. PM 1.3/-9.7 (Zacharias+, 2012) with vmag 13.514 (AAVSO). CSS LC is very tight.
V* W Hyi -- Variable Star of Mira Cet type
A #late type star, M by color. #I-IR-E but passes ruler test. PM -6.4/5.4 (Zacharias+ 2015). CSS LC is fairly tight.
A #late type star, M by color. PM -3.1/-.7 (Zacharias 2012) with vmag: 13.67 (Nascimbeni+, 2016)
A #late type star with distance of 5263pc. A #MGiant
UCAC2 11987742 -- Star
A late type star with #I-IR-E
A #late type star, M by color. Vamp per ASAS is 1.32. Definite #MGiant
A #late type star, M by color. PM -5.2/-.3 (zacharias 2012) vmag 16.6.
A #late type star, M by color. PM -9.6/-7.8 (Zacharias 2017). Vmag 15.360. Vetted to Mdwarf sheet!
A #late type star, M by color. Does have some W4 #extension. PM -7.7/-3.2 (Zacahrias 2017). CSS LC is fairly tight.
A #late type star, M by color. CSS LC is fairly tight. PM -6.8/-.9 and vmag 14.839. Vetted to round three
#repeat
A #late type star, M by color. Vamp: .46 (ASAS). PM -2.2/-3.9 (Zacharias 2017)
A #late type star, M by color. PM -.4/2.4 and Vmag 17.72
A #late type star, M by color. PM -2.6/-4 (Zacharias 2012) with vmag 14.915 (AAVSO).
[VV98] J073218.7+615906 -- Quasar
A #late type star, M by color. PM -.6/-2.3 (Zacharias 2015). Vmag 14.66
Vetted to round three DDOI
2MASS J19234475+3541512 -- Variable Star
A #late type star, M by color. PM -4.4/3.2 vmag 17.83.
A #late type star, M by color. PM -5.8/-3 and vamp between .36 and .56 (CSS LC shows regular variability). #I-IR-E
Added to user added faint DDOi
A #late type star, M by color. PM -8.3/2.4 (Zacharias 2015). CSS LC is tight > .4 variation. Possible #Mdwarfc with #diskc
IRAS 15516-4710 -- Star
A #late type star, M by color. PM 3/4.9 and Vmag 12.863
A #late type star with #I-IR-E
2MASS J19562478+4555018 -- Long-period variable star
A #late type star, M by color. PM -5.3/14.4 (zacharias 2012)
Already vetted to round three
A #late type star, M by color. Distance of 7142 pc (Kunder+, 2017) means a definite #MGiant
2MASS J19184925-6559282 -- Star
Vetted to round three
#AGB
2MASS J20184753+5620129 -- Asymptotic Giant Branch Star (He-burning)
A #late type star. No vmag or CSS LC. Decent PM 1.3/-18.9 (Zacharias+, 2012). W1-W4~1.5
2MASS J04202494+4540381 -- Carbon Star
UCAC2 8668888 -- Star
A #late type star, M by color. PM -5.9/2.3 (Zacharias+, 2012). W1-W4=1.636
IRAS 12587-7810 -- Star
A #late type star, M by color. Distance of 1500 pc (Kunder+, 2017) means a definite #MGiant
A #late type star, M by color with very high proper motion and fairly faint star indicate possible #mdwarf with #diskc. Vetted to round 3!
IRAS 17153-5335 -- Star
A #late type star, M by color. PM -11.9/-7.5. W1-W4=1.74
LPV combined with high vamp 1.44 (Pojmanski+, 2002-2005) means most likely a #MGiant
V* DN Lib -- Long-period variable star
A #late type star, M by color. #I-IR-E and CSS LC shows var ~.8 with PM -1.8/-5.9. Appears to be a likely #MGiant
V* IM Lyr -- Long-period variable star
No followup on Slow Irregular Red stars #MGiant
ASAS J173708-4708.0 -- Variable Star
A #late type star, M by color. PM -5.9/-8.1 (Zacharias 2012). #I-IR-E of .875
A #late type star, M by color. Low PM -3.2/3.1 (Zacharias 2012) and CSS LC shows variance of ~.85. Likely #MGiant
2MASS J15253932+4224508 -- Carbon Star
A #late type star, M by color. PM 4.8/.2 (Zacharias 2012). #I-IR-E of .81
A #late type star, my by color. Distance of 4672 pc means a definite #MGiant
UCAC2 21523741 -- Star
HD 60757 -- Be Star... no further follow up needed on Be stars
A #late type star, M by color. PM (-1.2/-2.4... Zacharias 2012). CSS LC is very tight ~ .1 variability.
Appears either a nebula or a galaxy
Already vetted to main DD Vetting List
V* V350 Ori -- Emission-line Star
A #late type star, M by color. Extremely low PM -.2/.7 (Zacharias+, 2012) and #I-IR-E
UCAC2 23761786 -- Star
A #late type star, M by color. PM 1.3/-7.3 (Zacharias+, 2012) and #I-IR-E. Not a good candidate
2MASS J01113415+6012228 -- Asymptotic Giant Branch Star (He-burning)
A #late type star, M by color. PM -6.1/3.8 (Zacharias+, 2012). W1-W4=1.7
slightly extended and very low PM
A #late type star, M by color. PM -.5/-11.2 (Zacharias 2012). VAMP .33 (Pojmanski 2005). #I-IR-E W1-W4=.55
A #early star, A2 per simbad. Vetted to Round Three as poss new early type star with disk.
A late type star, M by color. Very low PM indicates likely M Giant.
A #late type star, M by color. Low PM .7/-1 (Zacharias 2012).
a #late type star, M by color. Vmag 16.5, with PM -6.7/-8 (Zacharias+, 2012).
#notagoodcandidate
A #late type star, M by color. PM -7.3/3.6 (Zacharias+, 2012). Vmag: 16.09. W1-W4=1.172
CSS LC shows regular fairly constrained variation (0.5 or less). Low PM -1.7/1.0 (UCAC4).
A #late type star, M by color. Fairly low PM -4.2/3.8 (UCAC4). W1-W4=2.681
A #late type star, M by color. Distance of 3067pc (Kunder+, 2017) indicated a definite #MGiant
AKARI-IRC-V1 J1131139-502320 -- Star
A #late type star, M by color. Low PM -1.9/-4.1 UCAC4. W1-W4=1.085
probably #MGiant
A #late type star, M by color. Vmag=15.213. PM = 7.7/-2 (UCAC4). W1-W4=1.745. CSS LC is fairly tight.
2MASS J04451111+1937028 -- Infra-Red source
Low PM. CSS LC shows variability. Probably #MGiant
A #late type star, M by color. Low PM 6.4/-4.5 (UCAC4). Vmag 13.611. CSS LC is fairly constrained. #I-IR-E W1-W4=.618 #notagoodcandidate
A #late type star, M by color. Low PM -4.5/.6 (UCAC4). Vmag 14.6. Most likely a #MGiant
A #late type, M by color. Fairly high PM, but extremely insufficient excess.
A #late type star, M by color. Low PM -6.2/1.3 UCAC4 and excess W1-W4=1.022.
V* V963 Cas -- Long Period Variable candidate
A #late type star, M by color. Decent PM of 7.0/-9.6 (Zacharias+, 2012). Vmag = 15.1 (Zacharias+ 2005). W1-W4=2.43
IRAS 10582-6604 -- Star
A #late type star, M by color. Low PM -2.4/-.2 (Zacharias+, 2012)
A #late type star, M by color. Low PM. Most likely a #MGiant
A #late type star, M by color. Distance is 2127 pc (Gaia Collaboration, 2016). A definite #MGiant
TYC 2632-454-1 -- Star
already vetted to DD vetting list
vetted to Round Three! User added.
A #late type star, M by color. PM -3.2/-4.8 (Zacharias+, 2012). W1-W4=1.577
A #late type star, M by color. Distance 3964pc (Kunder+, 2017) A #MGiant and not a good candidate.
A #late type star, M by color. Low PM.
V* OW Cas -- Long-period variable star
Previously vetted to DDOI Main
A #late type star, M by color. Fairly low PM (.1/2.3 per Zacharias 2012) with W1-W4=1.173
A #late type star, an LPV in SIMBAD. A #mgiant star and not a good candidate.
V* V1075 Oph -- Long-period variable star
EM* MWC 43 -- Emission-line Star
A #LPV, most likely a #MGiant
A #late type star, M by color. Low Vamp .368 (Williams+, 2004). Decent PM (-4.5/-.7 per UCAC4). Paired with faint star, possible #Mdwarf
A #late type star, M by color. Catalina light curve shows large variability. Probable #MGiant
Already vetted to DD Vetting List
A #late type star, M by color. Catalina light curve shows large variability. Paired with fairly low PM, probably #MGiant in my opinion.
A #late type star, M by color. PMRA = -.9 and PMDE = -7.5. Paired with fairly bright star V=14.5 indicates possible #MGiant
A #LPV most likely #MGiant
A #late type star, M by color. Fairly bright star with lower PM (-4/2.1 per UCAC4) indicates most likely #MGiant
A #late type star, M7 in SIMBAD. Most likely a LPV, #MGiant
A #late type star, M by color. A definite #Mgiant based on distance of 25,000 pc (Gaia 2016). Not a good candidate.
A #late type star, M by color. Low PM, and Insufficient Excess W1-W4=.576
A #late type star, M by color. RMS PM = 5.3 and W1-W4 = 1.787
A #late type star, M by color. Decent PM with RMS 14.8, W1-W4=2.277
#MGiant
A #late type star, M by color. Low PM. W1-W4=.915
A #late type star, M by color. Low PM and W1-W4=1.237. SED shows poss #ysoc
A #late type star, M by color. Low PM. I-IR-E W1-W4=.54. Not a good candidate.
A #late type star, M by color. Catalina variability suggest #MGiant
#MGiant not a good candidate
LPV most likely a #MGiant. Not a good candidate.
A #late type star, M by color. Catalina variability indicates a highly probably #MGiant.
IRAS 20201-2849
A #late type star, M by color. Low PM. Good W1-W4=2.232
A #late type star, M by color. With distance of 1676 pc (Kordopatis+, 2013), a definite #MGiant.
A #late type star, M by color. Variability in Catalina survey makes this a probable #MGiant.
Vetted to test sheet!
A #late type star, M class by color. Low Vamp(0.49 (Pojmanski+, 2002-2005) ). Low PM and #I-IR-E W1-W4=.574
A #late type star, M5 (GIGOYAN K.S. et all, 2003). At a distance of 3301 pc, a definite #MGiant
A #late type star, M by color. Low PM. I-IR-E w1-w4=.554
A #late type star, M4.5 (GIGOYAN K.S. et all, 2003). Low PM. W1-W4=1.266
A #late type star, M class by color. With a distance of 2582 pc, a definite #MGiant
A #late type star, M by color. Catalina Sky Survey shows variability, most likely consistent with an #Mgiant along with low PM.
2MASS J14082402-4600307 -- Star
A #late type star, M by color. W1-W4=1.835 with low PM.
Vetted to Round Three!
A #late type star, M class by color. Poss #YSOc. W1-W4=1.456 and low PM
Vetted to main DDOI Round Three
A #late type star, M class by color. Low PM. W1-W4=1.026
A #late type star, M class by color. I-IR-E W1-W4=.633
#ysoc
Cepheid variable Star
A #late type star, M class by color. Low PM. W1-W4=1.101
A #late type star, M class by color. Low PM. Low IR-E W1-W4=.411
A #late type star, M class by color. Low PM. #I-IR-E W1-W4=.355
A #late type star, M class by color with low Vamp=.34. Low PM. I-IR-E = .514
A #late type star, M class by color. Vamp=.31 W1-W4=1.398. Low PM. Possible #mdwarf
A #late type star, M class by color. Very low amp .067 (Feldmeier+, 2011). Low PM. Poss #mdwarf
A #late type star, M class by color. Low PM. W1-W4=1.347
A #late type star, M class (V-K). Low PM. W1-W4=1.58
A #late type #carbonstar. #H-alpha present (12.68). Low PM. W1-W4=.976
IRAS 03086+5253 -- Carbon Star
A #late type star, M class (V-K). Low PM. W1-W4=1.497
A #late type star, a likely #MGiant due to (V-K) and high Variability=1.404 (Williams+ 2004). W1-W4=2.28. Low PM.
HD 91273 -- Be Star
A #MGiant
V* V940 Per -- Long Period Variable candidate
A probable #late type star, M class (V-K). High variability (vamp=1.95) indicates #MGiant.
UCAC2 19387126 -- Star
A #goodcandidate probable #YSO with W1-W4=4.87. Low PM
One A0V and one F5III
V* V395 Aur -- Spectroscopic binary
A #early type star, class A0. W1-W4=.703. Low PM and PLX 446.42 pc.
HD 42617 -- Star
CCDM J05053+2740AB -- Double or multiple star
A #late type star #MGiant based on high PLX (5555 pc) and (V-K). Low PM. W1-W4=1.319.
UCAC2 3405742 -- Star
A #goodcandidate #early type Be #emission-line star. Low PM. W1-W4=2.111
EM* MWC 462 -- Emission-line Star
A #late type star, M type (V-K). W1-W4=1.769. Low PM.
IRAS 00507+6440 -- Star
GSC 01009-00236 -- Variable Star
A #variable #late type star, M class (V-K). W1-W4=1.126 with low PM.
A #late type star, M class based on (V-K). Low W1-W4=.569 and low PM.
A #goodcandidate #late type star, M class based on (V-K). W1-W4=1.962 with very low PM.
A #late type star. V-K indicates M type with low W1-W4=.737
A #early type star class A0V. W1-W4=.575. #spitzer observed.
A #late type star and V-K suggests definite M type. W1-W4=2.833.
IRAS 19569-1829 -- Star
A #late type star. V-K shows M star with very small W1-W4=.406
IRAS 05398-1335 -- Star
A #late type star. (V-K) suggest M type. W1-W4=1.094.
A #late type star, M class (using V-K). W1-W4=1.082.
W1-W4=4.872.
#T-tau star candidate
V* V953 Per -- Long-period variable star
A #Variable #MGiant
SED suggest #late type star. Very low PM and W1-W4=1.649.
#galaxy
SED suggest #late type star. Low PM with PLX=.61 and W1-W4=.802
TYC 2651-761-1 -- Star
#late type star
V* UZ Tel -- Variable Star of Mira Cet type
#goodcandidate. #variable #MGiant. Low PM. W1-W4=1.575.
SED suggest #YSO. W1-W4=.59
#goodcandidate. SED suggest #late type star. Low PM. W1-W4 = 1.41
SP77 28-13 M0.5 TYPE
#goodcandidate, #late type star. #MGiant.
HD 68554 -- B9V STAR
#goodcandidate. SED suggest #EARLY type star. Low PM. W1-W4 = 1.186
A #GOODCANDIDATE #MGIANT THAT IS #VARIABLE
V* FZ Gem -- Variable Star of Mira Cet type
A #goodcandidate #YSOc with W1-W4=2.457. Low PM.
A STRONG #YSO WITH #H-ALPHA
#POSSIBLEYSO BUT WITH FAINT MULTIPLE
GALAXY
POSSIBLE YSO
HV 2424 -- Variable Star
LATE STAR OR YSO
FIRST J094804.7+363041 -- Radio-source
POSSIBLE YSO OR LATE TYPE
V2001 Sgr -- Variable Star of Mira Cet type
#YSO
#possibleYSO
#latetype
#latestar
A #mstar with #I-IR-E
F Star - possible contamination from the star at 6 o'clock
#i-ir-e
#i-ir-e
#i-ir-e
#i-ir-e
M star YSOc. Vetted to round three user added
A #late type star, M by color. I-IR-E but passes ruler test. Vetted to Mdwarf spreadsheet
#I-IR-E
V* V360 Aur -- Long-period variable star... likely #MGiant
A #late type star, M by color. PM 2.8 / -5.9
A G8 YSOc - vetted to round three.
A #late type star that is highly variable, Vamp around .92 - factoring in fairly low PM and probably a #MGiant
#I-IR-E
#I-IR-E
Haro 5-17 -- Emission-line Star
Vetted to round 3
IRAS 05363-1115 -- Star
A #late type M star. PM 8.3/1.8 and vmag 15.005.
IRAS 23384+5307 -- Star
A #late type star, M by color. Vmag 14.102 and PM 5/5.4 (Finch 2016)
LAMOST J070240.89+114104.0 -- Star
A #late type star. CSS LC shows a variable star, and MACIEJEWSKI list it as a variable star as well. Probably an #MGiant
GSC 02772-01244 -- Star
A #late type object with #I-IR-E and doesn't pass ruler test. Not a good candidate.
#I-IR-E
A #late type star, M by color. W1-W4=1.7 with PM -9/1.8 (Zacharias 2017).
2MASS J19183916+3345453 -- Asymptotic Giant Branch Star (He-burning)
#I-IR-E
IRAS 17392-1225 -- Infra-Red source
A #late type star, M by color. W1-W4=1.4 and PM 2.4/2 (Zacharias 2012)
A #late type star with distance of 4166pc (Kunder 2017).... #MGiant
UCAC2 4716143 -- Star
A #late type star, M by color. W1-W4=1 with -8.4/-1.9 (Zacharias 2015)
A #late type star, M by color. CSS LC is very tight. W1-W4=2.1 and PM -.8/-2.1 (Zacharias 2015)
RAVE J113411.6-491450 -- Star
#I-IR-E and fails ruler test
A #late type star, M by color. W1-W4=.98 and PM 2.7/6.6 (Zacharias 2015).
A #late type star, M by color. W1-W4=1.1 and PM -11.1/.2 (Zacharias 2012)
A #late type star, M by color. W1-W4=1.49 and CSS LC shows variation around .75 - PM 4.5/-5.7 (Zacharias 2012)
A #ate type star. W1-W4=1.63 - PM -2.9/=10.1(Zacharias 2015)
A #late type star M by color. CSS LC shows limited variability. W1-W4=1.48 and PM -3.5/-11.1 (Zacharias 2015) Vmag=14.81 (AAVSO)
IRAS 17066-0627 -- Star
A #late type star, M by color. W1-W4=1.61 and PM 7.1/1.5 (URAT 1)
V* MX Gem -- Long-period variable star
A # late type star, M by color. PM -.2/13 UCAC4 and Vmag 14.54.
#I-IR-E
HD 250160 -- Emission-line Star
A #late type star, M by color. PM -2.9/1 per UCAC5 and Vmag12.974 per AAVSO.
A #late type star, M by color. PM 13.5/9.8 URAT 5 and Vmag 14.957 AAVSO
A #late type star, M by color. PM .1/-5.5 UCAC4.
vetted to mdwarf sheet!!!
A #late type star, M by color. PM 6.2/-17.1 (Zacharias 2015)
2MASS J17112377-0237127 -- Star
A #late type star, M by color. PM 2.2/.7 (Zacharias 2017) and vmag: 14.097 per AAVSO.
A #late type star, M by color. PM 4.8/-4.3 (Zacharias 2015) and Vmag: 16.515 in AAVSO.
M by color...distance 1086pc (Pojmanski+, 2002-2005) .... #MGiant
UCAC2 3432932 -- Star
#I-IR-E
A #late type star, M by color. PM -4.6/-7.2 (Zacharias 2012) with vmag: 12.54 (GSC2.3) (STScI, 2006). W1-W4 = 1.668
A #late type star, M by color. PM 1.3/-9.7 (Zacharias+, 2012) with vmag 13.514 (AAVSO). CSS LC is very tight.
V* W Hyi -- Variable Star of Mira Cet type
A #late type star, M by color. #I-IR-E but passes ruler test. PM -6.4/5.4 (Zacharias+ 2015). CSS LC is fairly tight.
A #late type star, M by color. PM -3.1/-.7 (Zacharias 2012) with vmag: 13.67 (Nascimbeni+, 2016)
A #late type star with distance of 5263pc. A #MGiant
UCAC2 11987742 -- Star
A late type star with #I-IR-E
A #late type star, M by color. Vamp per ASAS is 1.32. Definite #MGiant
A #late type star, M by color. PM -5.2/-.3 (zacharias 2012) vmag 16.6.
A #late type star, M by color. PM -9.6/-7.8 (Zacharias 2017). Vmag 15.360. Vetted to Mdwarf sheet!
A #late type star, M by color. Does have some W4 #extension. PM -7.7/-3.2 (Zacahrias 2017). CSS LC is fairly tight.
A #late type star, M by color. CSS LC is fairly tight. PM -6.8/-.9 and vmag 14.839. Vetted to round three
#repeat
A #late type star, M by color. Vamp: .46 (ASAS). PM -2.2/-3.9 (Zacharias 2017)
A #late type star, M by color. PM -.4/2.4 and Vmag 17.72
A #late type star, M by color. PM -2.6/-4 (Zacharias 2012) with vmag 14.915 (AAVSO).
[VV98] J073218.7+615906 -- Quasar
A #late type star, M by color. PM -.6/-2.3 (Zacharias 2015). Vmag 14.66
Vetted to round three DDOI
2MASS J19234475+3541512 -- Variable Star
A #late type star, M by color. PM -4.4/3.2 vmag 17.83.
A #late type star, M by color. PM -5.8/-3 and vamp between .36 and .56 (CSS LC shows regular variability). #I-IR-E
Added to user added faint DDOi
A #late type star, M by color. PM -8.3/2.4 (Zacharias 2015). CSS LC is tight > .4 variation. Possible #Mdwarfc with #diskc
IRAS 15516-4710 -- Star
A #late type star, M by color. PM 3/4.9 and Vmag 12.863
A #late type star with #I-IR-E
2MASS J19562478+4555018 -- Long-period variable star
A #late type star, M by color. PM -5.3/14.4 (zacharias 2012)
Already vetted to round three
A #late type star, M by color. Distance of 7142 pc (Kunder+, 2017) means a definite #MGiant
2MASS J19184925-6559282 -- Star
Vetted to round three
#AGB
2MASS J20184753+5620129 -- Asymptotic Giant Branch Star (He-burning)
A #late type star. No vmag or CSS LC. Decent PM 1.3/-18.9 (Zacharias+, 2012). W1-W4~1.5
2MASS J04202494+4540381 -- Carbon Star
A #late type star with #I-IR-E
UCAC2 8668888 -- Star
A #late type star, M by color. PM -5.9/2.3 (Zacharias+, 2012). W1-W4=1.636
IRAS 12587-7810 -- Star
A #late type star, M by color. Distance of 1500 pc (Kunder+, 2017) means a definite #MGiant
A #late type star, M by color with very high proper motion and fairly faint star indicate possible #mdwarf with #diskc. Vetted to round 3!
IRAS 17153-5335 -- Star
A #late type star, M by color. PM -11.9/-7.5. W1-W4=1.74
LPV combined with high vamp 1.44 (Pojmanski+, 2002-2005) means most likely a #MGiant
V* DN Lib -- Long-period variable star
A #late type star, M by color. #I-IR-E and CSS LC shows var ~.8 with PM -1.8/-5.9. Appears to be a likely #MGiant
V* IM Lyr -- Long-period variable star
#I-IR-E
No followup on Slow Irregular Red stars #MGiant
ASAS J173708-4708.0 -- Variable Star
A #late type star, M by color. PM -5.9/-8.1 (Zacharias 2012). #I-IR-E of .875
A #late type star, M by color. Low PM -3.2/3.1 (Zacharias 2012) and CSS LC shows variance of ~.85. Likely #MGiant
2MASS J15253932+4224508 -- Carbon Star
A #late type star, M by color. PM 4.8/.2 (Zacharias 2012). #I-IR-E of .81
A #late type star, my by color. Distance of 4672 pc means a definite #MGiant
UCAC2 21523741 -- Star
HD 60757 -- Be Star... no further follow up needed on Be stars
A #late type star, M by color. PM (-1.2/-2.4... Zacharias 2012). CSS LC is very tight ~ .1 variability.
Appears either a nebula or a galaxy
Already vetted to main DD Vetting List
V* V350 Ori -- Emission-line Star
A #late type star, M by color. Extremely low PM -.2/.7 (Zacharias+, 2012) and #I-IR-E
UCAC2 23761786 -- Star
A #late type star, M by color. PM 1.3/-7.3 (Zacharias+, 2012) and #I-IR-E. Not a good candidate
2MASS J01113415+6012228 -- Asymptotic Giant Branch Star (He-burning)
A #late type star, M by color. PM -6.1/3.8 (Zacharias+, 2012). W1-W4=1.7
slightly extended and very low PM
A #late type star, M by color. PM -.5/-11.2 (Zacharias 2012). VAMP .33 (Pojmanski 2005). #I-IR-E W1-W4=.55
A #early star, A2 per simbad. Vetted to Round Three as poss new early type star with disk.
A late type star, M by color. Very low PM indicates likely M Giant.
A #late type star, M by color. Low PM .7/-1 (Zacharias 2012).
a #late type star, M by color. Vmag 16.5, with PM -6.7/-8 (Zacharias+, 2012).
#notagoodcandidate
A #late type star, M by color. PM -7.3/3.6 (Zacharias+, 2012). Vmag: 16.09. W1-W4=1.172
CSS LC shows regular fairly constrained variation (0.5 or less). Low PM -1.7/1.0 (UCAC4).
A #late type star, M by color. Fairly low PM -4.2/3.8 (UCAC4). W1-W4=2.681
A #late type star, M by color. Distance of 3067pc (Kunder+, 2017) indicated a definite #MGiant
AKARI-IRC-V1 J1131139-502320 -- Star
A #late type star, M by color. Low PM -1.9/-4.1 UCAC4. W1-W4=1.085
probably #MGiant
A #late type star, M by color. Vmag=15.213. PM = 7.7/-2 (UCAC4). W1-W4=1.745. CSS LC is fairly tight.
2MASS J04451111+1937028 -- Infra-Red source
Low PM. CSS LC shows variability. Probably #MGiant
A #late type star, M by color. Low PM 6.4/-4.5 (UCAC4). Vmag 13.611. CSS LC is fairly constrained. #I-IR-E W1-W4=.618 #notagoodcandidate
A #late type star, M by color. Low PM -4.5/.6 (UCAC4). Vmag 14.6. Most likely a #MGiant
A #late type, M by color. Fairly high PM, but extremely insufficient excess.
A #late type star, M by color. Low PM -6.2/1.3 UCAC4 and excess W1-W4=1.022.
V* V963 Cas -- Long Period Variable candidate
A #late type star, M by color. Decent PM of 7.0/-9.6 (Zacharias+, 2012). Vmag = 15.1 (Zacharias+ 2005). W1-W4=2.43
IRAS 10582-6604 -- Star
A #late type star, M by color. Low PM -2.4/-.2 (Zacharias+, 2012)
A #late type star, M by color. Low PM. Most likely a #MGiant
A #late type star, M by color. Distance is 2127 pc (Gaia Collaboration, 2016). A definite #MGiant
TYC 2632-454-1 -- Star
already vetted to DD vetting list
vetted to Round Three! User added.
A #late type star, M by color. PM -3.2/-4.8 (Zacharias+, 2012). W1-W4=1.577
A #late type star, M by color. Distance 3964pc (Kunder+, 2017) A #MGiant and not a good candidate.
A #late type star, M by color. Low PM.
V* OW Cas -- Long-period variable star
Previously vetted to DDOI Main
A #late type star, M by color. Fairly low PM (.1/2.3 per Zacharias 2012) with W1-W4=1.173
A #late type star, an LPV in SIMBAD. A #mgiant star and not a good candidate.
V* V1075 Oph -- Long-period variable star
EM* MWC 43 -- Emission-line Star
A #LPV, most likely a #MGiant
A #late type star, M by color. Low Vamp .368 (Williams+, 2004). Decent PM (-4.5/-.7 per UCAC4). Paired with faint star, possible #Mdwarf
A #late type star, M by color. Catalina light curve shows large variability. Probable #MGiant
Already vetted to DD Vetting List
A #late type star, M by color. Catalina light curve shows large variability. Paired with fairly low PM, probably #MGiant in my opinion.
A #late type star, M by color. PMRA = -.9 and PMDE = -7.5. Paired with fairly bright star V=14.5 indicates possible #MGiant
A #LPV most likely #MGiant
A #late type star, M by color. Fairly bright star with lower PM (-4/2.1 per UCAC4) indicates most likely #MGiant
A #late type star, M7 in SIMBAD. Most likely a LPV, #MGiant
A #late type star, M by color. A definite #Mgiant based on distance of 25,000 pc (Gaia 2016). Not a good candidate.
A #late type star, M by color. Low PM, and Insufficient Excess W1-W4=.576
A #late type star, M by color. RMS PM = 5.3 and W1-W4 = 1.787
Vetted to round three
A #late type star, M by color. Decent PM with RMS 14.8, W1-W4=2.277
#repeat
#MGiant
A #late type star, M by color. Low PM. W1-W4=.915
A #late type star, M by color. Low PM and W1-W4=1.237. SED shows poss #ysoc
#repeat
A #late type star, M by color. Low PM. I-IR-E W1-W4=.54. Not a good candidate.
#repeat
A #late type star, M by color. Catalina variability suggest #MGiant
#MGiant not a good candidate
LPV most likely a #MGiant. Not a good candidate.
A #late type star, M by color. Catalina variability indicates a highly probably #MGiant.
IRAS 20201-2849
A #late type star, M by color. Low PM. Good W1-W4=2.232
A #late type star, M by color. With distance of 1676 pc (Kordopatis+, 2013), a definite #MGiant.
A #late type star, M by color. Variability in Catalina survey makes this a probable #MGiant.
Vetted to test sheet!
A #late type star, M class by color. Low Vamp(0.49 (Pojmanski+, 2002-2005) ). Low PM and #I-IR-E W1-W4=.574
A #late type star, M5 (GIGOYAN K.S. et all, 2003). At a distance of 3301 pc, a definite #MGiant
#repeat
A #late type star, M by color. Low PM. I-IR-E w1-w4=.554
A #late type star, M4.5 (GIGOYAN K.S. et all, 2003). Low PM. W1-W4=1.266
A #late type star, M class by color. With a distance of 2582 pc, a definite #MGiant
A #late type star, M by color. Catalina Sky Survey shows variability, most likely consistent with an #Mgiant along with low PM.
2MASS J14082402-4600307 -- Star
#repeat
#repeat
A #late type star, M by color. W1-W4=1.835 with low PM.
Vetted to Round Three!
A #late type star, M class by color. Poss #YSOc. W1-W4=1.456 and low PM
Vetted to main DDOI Round Three
A #late type star, M class by color. Low PM. W1-W4=1.026
A #late type star, M class by color. I-IR-E W1-W4=.633
#ysoc
Cepheid variable Star
A #late type star, M class by color. Low PM. W1-W4=1.101
A #late type star, M class by color. Low PM. Low IR-E W1-W4=.411
A #late type star, M class by color. Low PM. #I-IR-E W1-W4=.355
A #late type star, M class by color with low Vamp=.34. Low PM. I-IR-E = .514
A #late type star, M class by color. Vamp=.31 W1-W4=1.398. Low PM. Possible #mdwarf
A #late type star, M class by color. Very low amp .067 (Feldmeier+, 2011). Low PM. Poss #mdwarf
A #late type star, M class by color. Low PM. W1-W4=1.347
A #late type star, M class (V-K). Low PM. W1-W4=1.58
A #late type #carbonstar. #H-alpha present (12.68). Low PM. W1-W4=.976
IRAS 03086+5253 -- Carbon Star
A #late type star, M class (V-K). Low PM. W1-W4=1.497
A #late type star, a likely #MGiant due to (V-K) and high Variability=1.404 (Williams+ 2004). W1-W4=2.28. Low PM.
HD 91273 -- Be Star
A #MGiant
V* V940 Per -- Long Period Variable candidate
A probable #late type star, M class (V-K). High variability (vamp=1.95) indicates #MGiant.
UCAC2 19387126 -- Star
A #goodcandidate probable #YSO with W1-W4=4.87. Low PM
One A0V and one F5III
V* V395 Aur -- Spectroscopic binary
A #early type star, class A0. W1-W4=.703. Low PM and PLX 446.42 pc.
HD 42617 -- Star
CCDM J05053+2740AB -- Double or multiple star
A #late type star #MGiant based on high PLX (5555 pc) and (V-K). Low PM. W1-W4=1.319.
UCAC2 3405742 -- Star
A #goodcandidate #early type Be #emission-line star. Low PM. W1-W4=2.111
EM* MWC 462 -- Emission-line Star
A #late type star, M type (V-K). W1-W4=1.769. Low PM.
IRAS 00507+6440 -- Star
GSC 01009-00236 -- Variable Star
A #variable #late type star, M class (V-K). W1-W4=1.126 with low PM.
A #late type star, M class based on (V-K). Low W1-W4=.569 and low PM.
A #goodcandidate #late type star, M class based on (V-K). W1-W4=1.962 with very low PM.
A #late type star. V-K indicates M type with low W1-W4=.737
A #early type star class A0V. W1-W4=.575. #spitzer observed.
A #late type star and V-K suggests definite M type. W1-W4=2.833.
IRAS 19569-1829 -- Star
A #late type star. V-K shows M star with very small W1-W4=.406
IRAS 05398-1335 -- Star
A #late type star. (V-K) suggest M type. W1-W4=1.094.
A #late type star, M class (using V-K). W1-W4=1.082.
W1-W4=4.872.
#T-tau star candidate
V* V953 Per -- Long-period variable star
A #Variable #MGiant
SED suggest #late type star. Very low PM and W1-W4=1.649.
#galaxy
SED suggest #late type star. Low PM with PLX=.61 and W1-W4=.802
TYC 2651-761-1 -- Star
#late type star
V* UZ Tel -- Variable Star of Mira Cet type
#goodcandidate. #variable #MGiant. Low PM. W1-W4=1.575.
SED suggest #YSO. W1-W4=.59
#goodcandidate. SED suggest #late type star. Low PM. W1-W4 = 1.41
SP77 28-13 M0.5 TYPE
#goodcandidate, #late type star. #MGiant.
HD 68554 -- B9V STAR
#goodcandidate. SED suggest #EARLY type star. Low PM. W1-W4 = 1.186
A #GOODCANDIDATE #MGIANT THAT IS #VARIABLE
V* FZ Gem -- Variable Star of Mira Cet type
A #goodcandidate #YSOc with W1-W4=2.457. Low PM.
A STRONG #YSO WITH #H-ALPHA
#POSSIBLEYSO BUT WITH FAINT MULTIPLE
GALAXY
POSSIBLE YSO
HV 2424 -- Variable Star
LATE STAR OR YSO
FIRST J094804.7+363041 -- Radio-source
POSSIBLE YSO
POSSIBLE YSO OR LATE TYPE
POSSIBLE YSO
POSSIBLE YSO
POSSIBLE YSO
V2001 Sgr -- Variable Star of Mira Cet type
#YSO
#YSO
#YSO
#YSO
#YSO
#YSO
#YSO
#possibleYSO
#YSO
#possibleYSO
#latetype
#YSO
#YSO
#YSO
#YSO
#YSO
#YSO
#YSO
#YSO
#YSO
#latestar
#YSO
#YSO
#YSO
#YSO
#YSO