E1 1031 Rauer et al. (2009A&A...506..281R)
E2 0165 Leger et al. (2009A&A...506..287L); Queloz et al. (2009A&A...506..303Q, 
E2 0165  Cat. J/A+A/506/303); Hatzes et al. (2010A&A...520A..93H); Bruntt et al.
E2 0165  (2010A&A...519A..51B); Pont et al. (2011MNRAS.411.1953P); 
E2 0165  Hatzes et al. (2011ApJ...743...75H)
E2 3459 Gillon et al. (2010A&A...520A..97G)
E2 5277 IAC 80 confirms the transit is on target. HARPS and HIRES RV data 
E2 5277  confirm a hot-Jupiter planet with Mp~~2MJup transiting an F8 IV star 
E2 5277  with Teff~~6100K and logg~~3.5dex (Patzold et al., in prep.).
E1 0544 Classified as F7 V by AAOmega. According to SOPHIE RV measurements, the 
E1 0544  star is a fast rotator and shows no RV variation down to a precision of
E1 0544  50m/s. EulerCam and IAC 80 photometry reveals that a ~4mag fainter 
E1 0544  star, located 9" west of the main target, contaminates the lightcurve 
E1 0544  with deep eclipses (D~~20%).
E1 0561 gamma-Doradus variable star, classified as an A7IV/V star by AAOmega. 
E1 0561  SOPHIE finds a low-contrast single peak CCF with an RV variation of 
E1 0561  about 52km/s, in anti-phase with the CoRoT ephemeris. A single epoch 
E1 0561  UVES spectrum reveals an SB3 system.
E1 2890 IAC 80 observations find that a ~3.2mag fainter star, located ~12" 
E1 2890  southeast of the target, shows a 40% deep eclipse. Taking into account 
E1 2890  the light contamination inside the photometric mask, the observed 
E1 2890  variation is consistent with the CoRoT transit-like signal.
E1 3666 IAC 80 and CHFT observations find that a ~0.5mag fainter star, located 
E1 3666  ~8" west of the target, exhibits a 1.5% deep eclipse. Taking into 
E1 3666  account the light contamination inside the photometric mask, the 
E1 3666  observed variation is consistent with the CoRoT transit-like signal.
E1 5015 Transit duration of 10h indicates an eclipsing binary at photometric 
E1 5015  detection level. ESA-OGS observes the transit on target. Two HARPS RV 
E1 5015  measurements confirm a binary system with low-mass companion 
E1 5015  (K=16.3km/s if e=0; M2~~0.18M_{sun}_ if M1=1M_{sun}_).
E1 4353 EulerCam finds that the transit-like signal is caused by a 5% deep 
E1 4353  eclipse in a nearby contaminant star (CoRoT ID: 0102691690, V=16.7mag).
E1 4353  CEB scenario confirmed by IAC 80.
E2 1123 Wise and IAC 80 observe the transit on target. CORALIE, UVES, and HARPS 
E2 1123  show an active K5 V star with no detected RV variation at a level of 
E2 1123  about 50m/s. UVES spectra reveal 3 emission components in the core of 
E2 1123  the CaII H & K lines. The RVs of 2 components vary in phase at twice 
E2 1123  the transit period and with a maximum velocity difference of 67km/s. 
E2 1123  Blend scenario: suspected hierarchical triple system consisting of an 
E2 1123  active K-dwarf orbited by two eclipsing active M-type stars.
E2 1145 Also known as IRa01 E1 1873. Classified as A9 IV/V by AAOmega. SOPHIE 
E2 1145  finds an RV variation with a semi-aplitude K=23.5km/s (assuming e=0) 
E2 1145  in anti-phase with the CoRoT ephemeris.
E2 1897 Hints of a secondary eclipse are found in the lightcurve. Contamination 
E2 1897  by an eclipsing binary located ~3" northeast from the main CoRoT 
E2 1897  target is found by CFHT photometry.
E2 2249 K0 III/IV star based on AA0mega spectra. SOPHIE finds an RV 
E2 2249  semi-amplitude K=12.2km/s (assuming e=0) consistent with a binary 
E2 2249  system with low-mass companion (M2~~0.17M_{sun}_ if M1=1M_{sun}_).
E2 2481 Also a mono-transit candidate in IRa01, known as IRa01 E1 2046. AAOmega 
E2 2481  and SOPHIE identify this candidate as an SB2 system.
E2 2694 SOPHIE and HARPS find no CCF, HeI absorption lines, and strong emission 
E2 2694  Balmer lines. AAOmega identifies the star as a B3 Ve star. If on 
E2 2694  target, the observed transit signal is caused by an eclipsing star.
E2 4129 Wise observations are inconclusive. EulerCam reveals a 7% drop in the 
E2 4129  flux of a contaminating star located ~4.5" north-northeast from the 
E2 4129  CoRoT target and responsible for the detected transit-like signal.
E2 5084 HARPS reveals an SB1 system with a K=37.2km/s RV curve (assuming e=0) 
E2 5084  in anti-phase with the CoRoT ephemeris.
E2 5184 Also in IRa01 as IRa01 E1 4108. CFHT confirms the transit on target. 
E2 5184  HARPS spectra yield Teff=5000+/-100K, logg=4.4+/-0.1dex, 
E2 5184  [M/H]=0.07+/-0.06dex, vsini=1.5+/-0.5km/s, and SpT=K0 V. Strong HARPS 
E2 5184  CCF bisector-RV correlation identifies the candidate as a blend.
E2 5747 Also in IRa01 as IRa01 E1 4617. Transit duration (14.13h) and 
E2 5747  depth (3.64%) implies stellar companion. HARPS finds no CCF. Target 
E2 5747  star identified as a rapidly rotating A-type star. If on target, the 
E2 5747  observed transit signal is caused by an eclipsing star.
E2 3739 Also a mono-transit candidate in IRa01, known as IRa01 E1 4014. Transit 
E2 3739  depth (2.93%), duration (6.97h), and shape indicate grazing stellar 
E2 3739  eclipses. Transit observed by EulerCam 0.15 days after the predicted 
E2 3739  time, but still consistent with the transit event being on target. 
E2 3739  HARPS spectroscopy shows no CCF and a rapidly rotating A-type star. 
E2 3739  The observed transit signal is caused by an eclipsing star.
E2 5756 Deep transit signal (2.72%) with steep ingress/egress. Transit on target
E2 5756  according to IAC 80 observations. HARPS finds no CCF and a rapidly 
E2 5756  rotating A-type star. The observed transit signal is caused by an 
E2 5756  eclipsing star.
E1 0286 Sandiford, HARPS, SOPHIE, HIRES, and FIES RV measurements show that the 
E1 0286  G8/9 IV primary star (Teff=5250+/-80K, logg=3.75+/-0.10dex, 
E1 0286  [M/H]=-0.10+/-0.05dex, vsini=3.0+/-1.0km/s) belongs to a stellar binary
E1 0286  system (P=337.52+/-0.20-days, e~~0.01, K=6.22+/-0.18km/s, 
E1 0286  yielding M2~~0.22M_{sun}_ if M1=1.10M_{sun}_). No RV variation in phase
E1 0286  with the CoRoT ephemeris is found in the RV residuals down to 5m/s. 
E1 0286  CFHT and EulerCam photometric observations are not conclusive but might
E1 0286  suggest a CEB scenario. The candidate is still under investigation.
E1 2101 The lightcurve shows a spot-induced 2% flux modulation with a period 
E1 2101  of ~11 days. The transit signal is only found in the CoRoT red channel 
E1 2101  because its depth is below the noise level in the green and blue 
E1 2101  channels. Combined measurements with CFHT and MONET-North exclude CEB. 
E1 2101  HARPS reveals K6 V star with Teff~~4250K and logg~~4.5dex. Six HARPS RV
E1 2101  measurements show no significant sinusoidal variation down to a 
E1 2101  precision of 18m/s. The candidate is still under investigation.
E1 2240 Asymmetric transit shape. Owing to the low S/N ratio this is not 
E1 2240  conclusive to rule out the candidate.
E1 3216 It shows shallow out-of-transit variations.
E1 3221 V-shaped transit. Pulsations with periods of 0.78 and 8.75 days, typical
E1 3221  of a giant, are detected in the lightcurve, in disagreement with the 
E1 3221  A5 V classification reported in Exo-Dat.
E1 4423 V-shaped transit. The lightcurve is strongly affected by instrumental 
E1 4423  effects (jumps).
E1 4594 The 6.62h transit duration suggests an evolved host star. IAC 80 
E1 4594  excludes nearby CEBs. The transit is concluded to be on target.
E1 4667 Wise photometric observations are inconclusive because of bad weather. 
E1 4667  IAC 80 photometry excludes contamination by background eclipsing 
E1 4667  binaries. Two HARPS spectra unveil a G0 V star and show an RV variation
E1 4667  of 84m/s, which is comparable to the error bars (~70m/s). The 
E1 4667  spectroscopic follow-up is still on-going.
E1 4719 V-shaped and asymmetric transit shape. EulerCam follow-up might have 
E1 4719  missed the transit owing to the timing errors (2h) at the time of the 
E1 4719  observations (28 October 2010). Nevertheless, large photometric 
E1 4719  variations from nearby contaminant stars are probably not the cause for
E1 4719  the observed transit event.
E1 4820 According to OGS-ESA observations, the transit is on target. The 
E1 4820  lightcurve analysis indicates possible out-of-transit variations and 
E1 4820  depth differences between even and odd transits.
E1 5320 Uncertain detection. The transit-like signal is only identified in the 
E1 5320  phase-folded lightcurve.
E1 5536 Although CFHT observed a 0.40+/-0.25% deep transit on target compatible 
E1 5536  with the CoRoT signal, some of the nearby background stars could not be
E1 5536  excluded as possible contaminants. Observations are considered 
E1 5536  inconclusive.
E2 3156 The transit is only seen in the red CoRoT channel because its depth is 
E2 3156  below the noise level in the green and blue channels. It is V-shaped 
E2 3156  and has a long duration (~2h) for a planetary object. According to 
E2 3156  IAC 80 observations, background contaminants are probably excluded. 
E2 3156  There is a 20-30% chance of missed transit owing to timing errors. 
E2 3156  HARPS & HIRES find no RV variation down to a precision of 10m/s. The 
E2 3156  candidate is still under investigation.
E2 3619 Also in IRa01 as IRa01 E1 2060. G8 V star according to Exo-Dat. 
E2 3619  Classified as a G0 IV/V star by low-resolution AAOmega observations. 
E2 3619  CoRoT photometry shows multi-periodic variations with frequency spacing
E2 3619  consistent with a giant. True spectral type unclear.
E2 4519 EulerCam and IAC 80 observations show no photometric variations in any 
E2 4519  of the nearby stars. However, the transit might have been missed owing 
E2 4519  to the timing errors (1.5h) at the time of the observations 
E2 4519  (Nov-Dec 2010). Still, the transit-like signal is considered to arise 
E2 4519  from the target.
E1 2970 V-shaped transit signal detected only in the red channel. No significant
E1 2970  detection in the blue and green channels. Hints of secondary eclipse 
E1 2970  in the red lightcurve. Suspected CEB.
E1 3617 Several frequencies coherent with the transit period point to activities
E1 3617  induced by a massive companion. Hints of secondary eclipses in the 
E1 3617  lightcurve. Suspected eclipsing binary.
E1 3674 V-shaped transit with long duration (3.38h) seen only in the red 
E1 3674  channel. No significant detection in the blue and green lightcurve. 
E1 3674  Suspected CEB.
E1 4272 ESA-OGS confirms the transit signal to be on target. Out-of-transit 
E1 4272  variations detected in the lightcurve. Suspected eclipsing binary.
E1 4777 V-shaped transit with long duration (3.90h) and depth differences by 
E1 4777  more than 1{sigma} in the three color channels. No transit detected by 
E1 4777  IAC 80, possibly owing to underestimated transit timing error at the 
E1 4777  time of the observations (February 2011).
E1 4836 V-shaped signal with significant (12{sigma}) depth difference between 
E1 4836  even and odd transits. Suspected eclipsing binary.
E1 5450 Asymmetric transit shape. Duration too long (9.23h) to be consistent 
E1 5450  with a transiting planet.
E2 2185 Also in IRa01 as IRa01 E1 1319. V-shaped long transit signal (3.57h). 
E2 2185  Faint secondary eclipse at phase 0.5 and depth differences between even
E2 2185  and odd transits suggest an eclipsing binary.
E2 2597 The signal is only present in the blue channel. No significant detection
E2 2597  in the green and red lightcurve. Classified as a G6 III/IV star by 
E2 2597  AAOmega. FLAMES yields Teff=4991+/-140K, logg=3.24+/-0.30dex, 
E2 2597  [M/H]=-0.29+/-0.15dex, and vsini=4.8+/-2.0km/s. Suspected CEB.
E2 2627 V-shaped transit signal found only in the CoRoT blue channel. No 
E2 2627  significant detection in the green and red channels. Classified as an 
E2 2627  F4 V star by AAOmega. Suspected CEB.
E2 3157 V-shaped signal found only in the red channel with significant 
E2 3157  (5{sigma}) depth differences between even and odd transits. 
E2 3157  Suspected CEB.
E2 4494 Asymmetric transit signal with long duration (2.81h).
E2 4910 Also in IRa01 as IRa01 E1 1531. Classified as an F7/8 V star according 
E2 4910  to AAOmega. IAC 80 observes the transit on target. Secondary eclipses 
E2 4910  found in the lightcurve. Suspected eclipsing binary.
E2 5194 Transit duration too long (2.79h) for a planetary companion. 
E2 5194  Suspected eclipsing binary.
E1 2960 Transit-like signal detected only in the CoRoT red channel. Instrumental
E1 2960  effects (jumps) in the lightcurve might mimic the transit-like signal.
E2 3389 Instrumental effects (jumps) in the lightcurve might mimic the 
E2 3389  transit-like signal.
E2 3612 Asymmetric transit shape. Instrumental effects (jumps) in the lightcurve
E2 3612  might mimic the transit-like signal.
E2 0928 Transit signal too deep (2.60%) for a planetary candidate if spectral 
E2 0928  type is A5 IV (Exo-Dat). It needs spectral type confirmation.
E2 5678 Transit signal too deep (4.33%) for a planetary candidate if spectral 
E2 5678  type is F8 V (Exo-Dat). It needs spectral type confirmation.