#variable . A significant change in the 31 day study.Possible #binary star .I suppose the presence of a giant star at the spot from time to time the brightness of the star decreases its
Star is probably active. The light curve shows that the star can be the #starspot#flare
#transiningplanet probably warm jupiter Msin=2.134 Mj .the exact parameters of the possible planet can not be established and the object can be as large and smaller mass
On the basis of the corrected data, we can assume that the presence of this star #eclipsingbinary companion to a short periodic orbit .
After some time there is a chaotic activity of outbreaks which also zaknichavetsya a certain period of time a powerful burst of energy
interesting feature observed during the passage of the companion around the star. After 19 days of the study, after the transit is observed powerful flash
with potential partners as well as at the time of the passage of a possible stellar companion star is also visible around the #flare
The possible existence of transiting planets .but it is appropriate based on the adjusted data have no observable periodicity. The complexity of the study of this object in that it is a red dwarf
The possible existence of transiting planets .but quite appropriate on the basis of adjusted data there is no observed periodicity. The difficulty of studying this object also in the fact that it is a red dwarf.
KOI 1384 .It is #possibletransit a brown dwarf in a short orbit, but it is probably a false positive
Q10-1 #variable #transiting
#rotatingstars
#gap #glitch #noisy
Q1-21 #possibletransitingplanet #noise #glitch
Q9-2 #longvariable #transit
Q12-1 #noisy #longwariable #manytransits
Q1-1 possible #transit on @24.91 day
Detection is possible planet is highly unlikely . Looking more sensitive equipment
Q11-3 #gap #noise .Possible #transitingplanet . AU 0242 RJ≈0.816 MJ≈0.923 Inclination 85.007
Q3-2 #iregular possible #transitingplanet
Q8-3 #noise mayde #variable #transit
Q1-1 #transitingplanet
Probably no gas giants ≥1 M(sin)J , but do not exclude less massinve orbit
Q6-1 #semiregular #gap #glitch
Q14-1 mayde #longvariables #glitch #noise
Q16-2 KID 7377033 (KOI 882) Kepler Favorite http://oldtalk.planethunters.org/discussions/DPH100i9j2
Q4-3 #iregular .Possible #trasit(s)
mayde #Semiiregular
mayde #RRLyrae
Q12-1 #pulsating #starspots
Q1-4 #glitch possible #transit
Q1-2 #glitch #gap possible #flare
Q-15 #transit red dwarf
Q1-4 possible #transit @ 6.25
Q1-1 #glitch #gap
Q1-4 regular #transitingplanet or #eclpsingbnary
Q14-1 #variable #glitch #gap
Q6-2 #variable #noise #glitch #gap
Q11-3 #noisy #gap
Q10-3 #noisy
Q11-4 Perhaps semiregular variable. Possible #transit , but it is probably still a #glitch. #Noisy
Q1-2 #transitingplanet(s) . Water govian planet ?
B 17-1 #glitch #noisy possible #variable
Q12 possible #transit #var iable #noise #glitch
Q15-3 #glitch #noisy
possible #multiplanet system
possible #transit BKJD 2233 2295.88
Also, there are changes that can have both a transit and nature and actually be glitches 2243.03 2252.2
It is quite possible #transitingplanet BKJD 2235.08
mayde #flare. Possible #asteroids
Mayde #transitingplanet type hot jupiter
possible #transitingplanet BJD 2273
HD 24465 is possible because the planet and EB according to a survey of XO http://arxiv.org/abs/1006.2139
The noise is caused by flare star HD 24465
#eclipsingbinary . Possible #transitingplanet BJD 2287.13
very good #transitingplanet
#ecipsinbinary.BJD 2240 probably #heartbeatstar #flare
possible #transitingplanet at BJD 2289.88 (day 20.20)
TYC 1257-432-1 star - http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=TYC+1257-432-1&submit=SIMBAD+search
#noise ang #glitch .Possible #transit . https://www.cfa.harvard.edu/~avanderb/k2c4/ep210765308.html
possible #transiting planets
#eclipsingbinary big #starspots #flare
#pulsating , possible #transit
Possible #transitingplanet day 1.25 7
probably #variable
#noise
Q1-2 probably #dwarfnova
Probably mira type #variable
possible #transtinigplanet. the signal borders on the edge glitch. Days 4.64 4.97 5.7 6.3 14.5 18.4 23.2 24.8 31.2 32.15 32.6
possible #transitingplanet pobably 30 day
#transitingplanet at 25.6 day
#eclipsingbinary
possible #transit(s) BJD 2779 2287.64
possible #transit BJD 2287.75
#interesting.probably #glitch .The star of spectral type F2V so it is possible that the bug is probably caused by the brightness of the star
#transitingplanet
ID 2268.22 possible #transit .
#starspot
#variable #eclipsingbinary
#noise
possible #transit 23.14 day . Another possible #transits days 17 21.5 27.3
#GAP
probably a #glitch
probably hot jupiter
#variable
Search for planets around this star is complicated pulsating stars
#cepheid
possible #eclipsingbinary
#pulsating #starspot
The probable age of the star 3.5 billion years.
possible #transit (s) 0.45 1.15 days
#starspots #flare
#variable . A significant change in the 31 day study.Possible #binary star .I suppose the presence of a giant star at the spot from time to time the brightness of the star decreases its
brightening
probably #glitch and #nouse
possible #transit @ 21.95 32.95 days
#nouse #variable #starspot
possible #transit 4.5 5.249 20.25
#noise
beatiful
#variable #starspot
possible #transitingplanet @ 27.9-28.5 30.95? 31.15
possible #transitingplanet at 3.25-3.5 day , but probably it is a #glitch of the telescope . #starspot
possible #transit 30.998 days
With the passage of a planet across the disk of the star recorded the #starspot
#variable big #starspot . #transitingplanet @ 4.25-4.5 8 days
The probable age of the star - 500 million years
possible #transit 32.45
#variable #starspot . Possible #multiplanet system @ 3.9 4.67 4.95 6.95 8.05 9.35 10.10 10.6 11.75 12.9 22.5 22.55 25.5 25.7 31.5
#multiplanet system ?
The probable age of the star less than 1 billion years
#transitingplanet and #starspots
#dip @ 25
#transitingplanet ID 2240 . Probably #eclipsingbinary
#pulsating #flare #starspots
The incredible mass of 2.823 Mj
#transtingplanet at ID 2281.64-2287.40
long periodic #flare 6 day
#multiplanet system ?
Perhaps the age of stars no more than 2 billion years old
ID 2241-2269.9 very interesting .Maybe #glitch #debrisdisk
O3 2283-2286 possible 2236.85 2274.26 2288.45 2290 2290.3 2293 . 2293.99
object1( O )2281-2282 . O2 2287-2288 ( probably #eclipsingbinary )
likely #glitch . Probably #transit
#semiregular #variable #starspots
eclipsing binary probably transit ( s ) S1 4.88-7.9 days S2 2.25-10 days
#pulsating . The probability to detect the transit of very low activity due to the star
beuatiful ! #eclipsingbinary
posible small #tansitingplanet p 25 days
#glitch
#possibletransit
#pulsating #flare #starspot . #eclpsingbinary ?
periodic #flare
#eclipsingbinary 4d
#variable #starspots . #eclipsingbinary ?
possible #transit
#variable #starspots
#pulsating #eclipsingbinary
#starspot #variable #flare
#transitingplanet
#eclipsingbinary #flare
#pulsating
probably #variable
#variable
Probably #cepheid
no anomaly . #pulsating #variable
possible #starspots
probably #variable δ Sct
#glitch
maybe #cv
possible long-lived #flare
#pulsating #starspots #variable
wow.what is it ?
possible #cv #varible big #starspots
posible #transit #pulsating big #starspots
#pulsating #eclipsingbinary
Star is probably active. The light curve shows that the star can be the #starspot #flare
#transiningplanet probably warm jupiter Msin=2.134 Mj .the exact parameters of the possible planet can not be established and the object can be as large and smaller mass
Not Cepheid as it is likely a red giant #eclipsingbinary
#pulsating #flare , probably very #starspot
this star probably has a #debrisdisk
Based on this reference http://iopscience.iop.org/article/10.1088/0004-637X/705/2/1646/meta;jsessionid=6E102A3D94F4CEB8D8B923F7BA98A135.c2.iopscience.cld.iop.org
V* V718 Sco -Eclipsing binary of Algol type http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HD+145718&submit=SIMBAD+search
is very similar Delta Scuti #variable
It may be dust disk?
#mira-type . Interesting ligth curve , probably #gitch
probably #variable
Based on this reference http://iopscience.iop.org/article/10.1086/426937/meta this star immet debris disk
V* V1229 Tau -- Eclipsing binary of Algol type (detached) http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HD+23642&submit=SIMBAD+search
#variable #eclipsingbinary #starspot #flare
#pulsating
#variable #flare #starspots .Finding planets is very difficult because of the large number of star spots
#varable #starspots #flare #megaflare
#variable #flare
Posible transit at 0.8 1? 1.25? 3.45?
Q1-2 posible #transitingplatet
Probably red dwarf . #pulsating #variable #flare #starspot
#Possible transit 3.84 the nature of which can be low-mass brown dwarf Mj=16.708
#pulsating. Star probably not cepfeid ,as it is a red giant. #starspot #flare #variable
#transitingplanet probably hot jovian type or brown dwarf at 8.95 23.9 days. Probably mass 6.21Jr before 68 Jr
Red Star probably gigant . Probably #variable SRC type. #qasi-transits #flare .Change the light curve of the star can be seen in particular ID 2270
but this is unlikely because the object is under the monstrous temperatures and likely prichny this change may be the most active star
if there is likely to transit its can cause a brown dwarf with a slight eccentricity in the short periodic orbit
Possible transit and micro-transit 1.10&
#variable #pulsating #heartbeatstar #flare #starspot
probably #starspot
#pulsating probably #cv
probably #eclipsingbinary
typical #eclipsinbinary
Interesting. #eclipsingbinary #pulsating as the star most likely a red giant that does not apply to the type of RR Lyrae stars and Cepheid
#variable
#variable #flare
Perfect #eclipsingbinary .Star TYC 6784-662-1 http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=TYC+6784-662-1&submit=SIMBAD+search
strange and #interesting .Probably #mira #variable
Posible #glitch . #flare . Although theoretically possible variant of #eclipsingbinariy
Perfect #eclipsingbinary
#variable #starspot
#flare #variable . Changes in the light curve may be due to finding the star in the nebula IC 4592
possible #transit at 6 days . Transit at 5.95 days ?
#flare #variable #glitch , quasi - transit at 23 days.
#variable . Quasi-transit . Possible #transits at 2 days
#glitch
#eclipsingbinary . Perhaps this companion star is a red dwarf young for a short periodic orbit
posible #transit . #eclipsinbinary ? #glitch
On the basis of the corrected data, we can assume that the presence of this star #eclipsingbinary companion to a short periodic orbit .
After some time there is a chaotic activity of outbreaks which also zaknichavetsya a certain period of time a powerful burst of energy
interesting feature observed during the passage of the companion around the star. After 19 days of the study, after the transit is observed powerful flash
with potential partners as well as at the time of the passage of a possible stellar companion star is also visible around the #flare
interesting and short #eclipsingbinary . #flare
probably a wrong turn.
Mira type?
#flare #starspot . Possible transits and micro-transts 3.15? 3.5-3.75? 4.25? 4.75? 7.10-(кather stellar activity) 13.85? 16.2&
#orion type variable
Interesting enough #pulsating #flare . Possible #transit at 6.6 days but also such a change can be explained, and the most active star
#pulsating
#variable
#cepheid?
Possible micro-transins . Observed periodicity 8.48-21.75-23.15 On the verge of Gluck 15.75& 20. 23.5? 25.10? 29.25?
#variable #flare
#gtch . Posible micro-transits 2 4.5? 4.7& 5.75? 6.25? 6.75& 7.2&
#flare #variable
posible #transins at 6 , 24 day
#flare
#pulsating #heartbeatstar
#eclipsngbnary
no Cephed , so this is likely a red giant . #pulsating
#T-tau
#Gitch . Posible transins 3? 1.7? 2.58& 3.75& 4.75?
#variable #pulsating #eclipsingbinary
#posible
Possible #eclpsingbinary
#RRLyrae ?
#rrlyrae
#eclipsingbinary
#eclipsingbinary
#transitingplanet and posible #eclipsingbinary
#pulsatng #starspot #flare #megaflare
#flare . On ID 2097.66 possible #transits @ 8 days
#rrlyrae
#pulsating
typical #eclpsingbinary
Q1-3 #transtngplanet Jupiter-like at 8 and 27 days
#glitch #flare
at 11.8? 13.95? 15.9? 16.67 16.85? 18.95? 20.6? 20.84 22.65? 22.8? 23.65? 23.8? 24.15? 24.25? 24.55 24.75? 25.05? 25.5
Possble planet (signals bordering on noise)
Possble #multplanetsystem #eclipsingbinary . Possible option and #multiplesystem
Q1-1 posible #transiitingplanet at 21-25.9 days ? #variable
Q1-3 #pulsating
Q1-1 posible #variable #gitch #flare
#variable #flare
Q1-1 #variable
Q1-3 possible #transitingplanet
Q1-2 #gap
Q1-1 #variable
Q1-1 #pulsating
Q1-2 #transit #flare
Q1-2 #cefeid ? #flare possible #transits
Q1-2 #variable
Q1-4 #pulsating
Q1-2 Perhaps #multiplesystem #flare . Is suspected #variable .In the 20 days possible #transitingplanet
#tranzit and #eclipsingbinary . Posible three different stellar eclipses
The possible existence of transiting planets .but it is appropriate based on the adjusted data have no observable periodicity. The complexity of the study of this object in that it is a red dwarf
Q1-3 #transitingplanet
Q1-3 #starspot #variable
Q1-1 #variable
Q1-1 #variable
Q1-3 #variable
#gitch
On the basis of the light curve of the star and its adjusted data possible transit of the planet for 28 days .
Q1-1 #RRLyrae
Q1-2 #variable #flare . Possible #transit at 15.9-17.1 days ?
Q1-3 #glirch posible #variiable . It is also possible the passage of the #transitplanet for 17 days
Q1-3 #variable #strarspot possible #transitinplanet(s)
Q1-3 #variable #starespot
#variable
Q1-3 #transit #variable #flare
Q1-3 #pulsating
Q1-3 possible #transitingplanet #variable
Q1-1 possible #transtingplanet #variable
Q1-2 posible #transit #flare. Suspicion of #eclipsingbinaries
Q1-2 #pulsating #variable
Q1-2 Posible #transits at 24 days
Q1-2 #transtingplanet at 20 days #gitch #flare
Q1-1 Probably #variable
Q1-1 Maybe #transit but probably #noise. It is also likely that a #variable star
Q1-3 Calm light curve of the star
Q1-3 #variable
Q1-2 #variable #flare
Q1-3 #RRLyrae #pulsating #flares
Q1-1 #cepheid
Q1-2 Beautiful curve #quietstars
Q1-2 #Variable #flare
Q1-2 #heartbeatstar
Q1-2 #pulsating
Q1-3 #flare #glitch
Q1-4 #cepheid
Q1-1 #variable at posible #tranzitingplanet
Q1-2 #variable #gap
#flare
Q1-1 #variable
Q1-2 #variable and #glitch
Q1-1 #variable
Q1-1 #variable
Q1-3 #variable #flare #eclipsingbinary
Q1-2 possible #transtingplanet
Q1-2 #eclipsingbinary #flare . Posible tranzitingplanet at 25.9 days ?
Q1-1 #pulsating #flare . Possible #transtingplanet at 15 days ?
Q1-3 #variable #transitingplanet at 25.9 days
Q1-2 #variable. Posible #ecliptingbinary
Q1-2 #pulsating nad #megaflare
Q1-1 posible #transitingplanet
Q1-3 #pulsating
Q1-1 #variable
Q1-1 #variable
Q1-1 #variable #megaflare
Q1-3 #flare posible #transitingplanet
Q1-3 #transitingplanet
Q1-1 #flare
Q1-2 #variable #flare posible #transitingplanet at 24,25,26 days
The possible existence of transiting planets .but quite appropriate on the basis of adjusted data there is no observed periodicity. The difficulty of studying this object also in the fact that it is a red dwarf.
Q1-1 #megaflare
Q1-3 possible #transtingplanet@2,5,14,24 days
Q1-3 #variable posible #eclipsingbinary and #transitingplanet #flare
Q1-2 #variable . Posible #eclipsingbinary and #tranzting planet at 6.5 days about neptune or minijovian planet type
Q1-3 #pulsating
Q1-3 #variable #transitingplanet
Q1-3 possible #transitingplanet type minineptune
Q1-4 #transitingplanet at posible #multiplanet sysnem
Q1-1 #Variable . Possible #tranztingplanet #flare
Q1-1 #flare
Q1-1 #Variable
Q1-4 #Variable RV Tauri and #flare
Q1-2 #Flare . Posible #transit 23.2 days ?
Q1-2 #flare #transitsitinplanet at 24 days
Q1-3 #variable
Q1-2 #transit .There are also #glitch #flare
Q1-2 #cepheid
Q1-2 #starspot #glitch
Q1-2 possible #transitinplanet at 6 days.
Q1-2 #Pulsarting
Q1-2 posible #tranziiting planet ?
Q1-1 #variable #flare at possible many #transits.
Q1-1 #transitingplanet #flare #eclipsingbinary #glitch
Q1-1 #flare.#Pulsarting.Possible #tranziting planet at 17+-1 days?
Q1-3 #transitingplanet ?
Q1-1 #Pulsating
Q1-2 #pulsating
Q1-1 #Pulsating.Posible #tranzit planet at 9.6 days?
Q1-4 Possible #transit Neptune 27 days
Q1-2 #pulsating
Q1-1 #pulsating #rrlyrae
Q1-1 #Pulsating
Q1-4 #transitingplanet #irregular
Q1-1 #Variable
Q1-2 #periodic #sinusoidal
Q1-1 The light curve of the star does not give any deviations
Q1-2 #transitingplanet
Q1-3 #Pulsating , #transitingplanet
Q1-1 #pulsating , #flares , #RRLirae
Q1-1 #Pulsating
Its posiible planet 23.9 days?
Q1-4 #Pulsating.Tak also possible option and #stars spots
Q1-4 #transitingplanet - #variable
Q1-2 #variable
Q1-2-1 Tak also possible option #eklipsing binary
Q1-2 35 day change is observed brightness of the star that may be caused by the passage # tranzitingplanets short period.
Q1-1 #Gap
Q1-1 #flare
Q1-2 #Gaps
Q1-1 #Pulsarting
Q1-2 # #possible ~68d
Q1-1 #flare
Q1-1 #tranziting planet #flare #starspot .
Q1-1 #Variable
Q1-1 #pulsating
Q1-1 #transitingplanet but likely #pulsating
Q1-1 #tranzit or #variable star
Q1-3 #Variable
Q1-3 #glitch
Q1-2 #Cepheid
Q1-4 #Gaps
Q1-2 #pulsating flares
#heartbeatstar
Q1-1 #GAPS
Q1-2 #variable
Q1-2 #pulsarting
Q1-2 #pulsating
Q1-4 #eclipsingbinary
Q1-2 #Variable star
Q1-2 #Flare
Q1-3 #Flare #eclipting binary and more example possible #transiting planet.It may also be (or) short-period planet
Q1-3 #variable star
Q1-2 #GAPS
Q1-4 #starspots
Q1-1#cv
#Flare and maybe pulsating star
Q1-2 #Glitch and maybe pulsating star
Q1-4 #flare
Q1-2 #starspot
Looking at the light curve of the star can be said that it has a chaotic frequency that concludes that the # variable star.