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Table 1

Selected sample of δ Scuti stars observed by CoRoT.

Run Star ID CoRoT ID SpT mv log Teff (K) MV v sin i (km s−1) Obs. time (d)
IRa01 HD 508441 123 A2 9.1 3.88 1.31 64 57.713
SRc01 HD 1749362 7613 A2 8.58 3.9 1.88 170 27.194
SRc01 HD 1749663 7528 A3 7.72 3.88 1.95 125 27.197
LRc01 HD 181555⋆,4 8669 A5 V 7.52 3.85 −0.72 200 156.645
LRa01 HD 494345 100 F1 V 5.74 3.86 2.74 87 136.890
LRc02 HD 1721896,7 8170 A2 8.73 3.89 1.04 78 149.013
SRc02 HD 174532⋆,8 7655 A2 6.90 3.86 1.38 32 26.239
SRc02 HD 174589 7663 F2 III 6.09 3.85 1.45 100 26.168
LRa02 HD 51722 1022 A5 7.53 3.86 1.13 127 117.375
LRa02 HD 51359 1320 A5 8.50 3.9 0.89 117.41
LRa02 HD 508709 546 F0 8.88 3.88 1.67 17 114.413
LRc0506 HD 1706999 8301 A2 6.95 3.88 1.49 270 89.282
IRLRa04 GSC 00144–030311,10 21960 A8 10.1 3.89 79.133
IRLRa05 HD 41641 5685 A5 7.9 3.882 1.92 28 94.432
SRa05 HD 48784 3619 F0 6.66 3.84 1.87 108 25.305

Notes. From left to right: observing run, HD number, CoRoT number, spectral type, visual magnitude, effective temperature, absolute magnitude, rotational velocity and observation interval.

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