2010AJ....139..757K


Query : 2010AJ....139..757K

2010AJ....139..757K - Astron. J., 139, 757-764 (2010/February-0)

The Taiwan-American Occultation Survey project stellar variability. I. Detection of low-amplitude δ Scuti stars.

KIM D.-W., PROTOPAPAS P., ALCOCK C., BYUN Y.-I., KYEONG J., LEE B.-C., WRIGHT N.J., AXELROD T., BIANCO F.B., CHEN W.-P., COEHLO N.K., COOK K.H., DAVE R., KING S.-K., LEE T., LEHNER M.J., LIN H.-C., MARSHALL S.L., PORRATA R., RICE J.A., SCHWAMB M.E., WANG J.-H., WANG S.-Y., WEN C.-Y. and ZHANG Z.-W.

Abstract (from CDS):

We analyzed data accumulated during 2005 and 2006 by the Taiwan-American Occultation Survey (TAOS) in order to detect short-period variable stars (periods of ≲1 hr) such as δ Scuti. TAOS is designed for the detection of stellar occultation by small-size Kuiper Belt Objects and is operating four 50 cm telescopes at an effective cadence of 5 Hz. The four telescopes simultaneously monitor the same patch of the sky in order to reduce false positives. To detect short-period variables, we used the fast Fourier transform algorithm (FFT) in as much as the data points in TAOS light curves are evenly spaced. Using FFT, we found 41 short-period variables with amplitudes smaller than a few hundredths of a magnitude and periods of about an hour, which suggest that they are low-amplitude δ Scuti stars. The light curves of TAOS δ Scuti stars are accessible online at the Time Series Center Web site (http://timemachine.iic.harvard.edu).

Abstract Copyright: ∼

Journal keyword(s): stars: variables: delta Scuti - methods: data analysis - surveys

Nomenclature: Table 3: [KPA2010] NN (Nos 1-41) = TAOS FFF.NNNNN N=41.

Simbad objects: 50

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Number of rows : 50
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 HD 5076 dS* 00 52 40.6238424696 +06 39 54.936149436   9.14 8.87     A2 8 0
2 V* V529 And gD* 01 27 26.6728869648 +41 06 04.177819368   6.711 6.425     A7m 89 0
3 TYC 2334-225-1 dS* 02 56 53.7471609552 +34 23 20.145659316   11.97 11.45     ~ 1 0
4 HD 22431 dS* 03 37 02.2536433680 +18 21 51.002015832   8.79 8.49     A2 5 0
5 TYC 1239-409-1 dS* 03 42 40.7047706424 +17 55 01.111075392   12.53 12.13     ~ 5 0
6 HD 23465 dS* 03 46 01.0016739576 +18 34 00.210123012 9.640 9.440 9.160     A5 22 0
7 HD 285349 dS* 04 03 21.9279260880 +19 21 31.047895332   11.2 11.03 10.8   A7 7 0
8 * gam Dor gD* 04 16 01.5866224848 -51 29 11.932714356   4.55 4.20     F1V 337 0
9 TYC 1277-1421-1 dS* 04 30 06.2462357136 +20 55 00.326487720   12.15 11.33     F0 3 0
10 HD 284788 dS* 04 48 36.9742685880 +21 10 32.827320012   11.62 11.44 11.3   F5 4 0
11 HD 31382 dS* 04 56 14.1977964288 +21 34 20.465637888   7.64 7.35     F0 11 0
12 TYC 1845-1089-1 dS* 05 08 38.2435294368 +22 49 37.340872320   12.14 11.85     ~ 5 0
13 [KPA2010] 11 dS* 05 09 23.8226875501 +23 16 05.335383817   12.29 11.40     ~ 2 0
14 HD 33233 dS* 05 09 40.8004447392 +21 50 05.267692608   9.24 9.00     A0 7 0
15 TYC 1846-1669-1 dS* 05 10 13.6265545536 +23 01 24.344146812   11.72 11.41     ~ 2 0
16 TYC 1846-2308-1 dS* 05 15 19.8483485640 +22 53 41.231069520   12.31 11.93     ~ 1 0
17 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 19090 0
18 M 37 OpC 05 52 18.6 +32 32 36           ~ 436 0
19 HD 250389 dS* 06 01 30.8594574672 +21 27 37.583586540   10.77 10.46     F0 11 0
20 HD 41140 dS* 06 04 05.7435530340 +21 29 38.902082250   7.98 7.77     A3 22 0
21 TYC 1325-761-1 dS* 06 04 26.0631511728 +21 21 54.961537716   11.12 10.96 10.93   ~ 2 0
22 TYC 1373-1436-1 dS* 07 39 07.0672951104 +21 39 19.983620196   11.59 11.14     kA7hA9mF0 5 0
23 TYC 1373-181-1 dS* 07 39 09.2392189800 +20 48 41.322657492   10.78 10.44     ~ 5 0
24 TYC 1373-2444-1 dS* 07 39 20.2197437424 +21 11 44.825582724   12.59 11.57     G0V 2 0
25 HD 64813A dS* 07 56 31.4057388624 +21 52 28.656536700   9.63 9.33 9.61   A5 15 0
26 TYC 1375-1698-1 dS* 07 58 26.5090554960 +21 36 23.674499892   11.0 10.85 10.7   ~ 2 0
27 BD+17 1919 dS* 08 43 26.8651937664 +16 52 59.765442636   9.05 8.80     F0 14 0
28 TYC 1393-458-1 dS* 08 43 45.5358828096 +17 24 59.869017720   10.88 10.60     ~ 3 0
29 HD 74362 dS* 08 44 07.2943724496 +15 55 50.529307764   8.69 8.57     A0 6 0
30 BD+18 2118 dS* 09 05 55.6748229840 +17 47 27.024136152   11.34 11.01     A5 4 0
31 BD+18 2132 dS* 09 09 53.6902674792 +17 41 07.604531448   10.36 10.18     A5 6 0
32 V* GM Leo dS* 10 04 08.3785722672 +11 37 42.647835324 7.330 7.310 7.130     A8VkA0mA0.5_lB 41 0
33 HD 114429 dS* 13 10 39.3140908056 -06 25 00.808370508   10.47 10.36     A3/5III 6 0
34 TYC 6195-826-1 dS* 15 58 40.2412812672 -19 27 13.672729512   12.0 11.62 11.2   ~ 6 0
35 BD+07 3260 dS* 16 51 54.5905380720 +07 36 43.578564696   11.09 10.74     A5 5 0
36 * del Sct dS* 18 42 16.4268984096 -09 03 09.188922060   5.04 4.71     F2II-III 507 0
37 V* HN Dra RR? 18 44 53.1326219016 +57 05 17.142065448   8.45 8.07     F2 23 0
38 HD 187592 dS* 19 51 30.9728803080 -22 23 03.290167788   10.11 9.86     A5/7III 11 0
39 ATO J301.1992-20.5350 dS* 20 04 47.8311592104 -20 32 05.829921528   12.22 11.63     ~ 2 0
40 TYC 1648-2182-1 dS* 21 01 43.6719741048 +16 39 37.194131556   11.51 11.20     ~ 1 0
41 [KPA2010] 34 dS* 21 03 25 +15 21.4   17.53 9.13     ~ 1 0
42 * bet Cep bC* 21 28 39.5968513 +70 33 38.574681 2.05 3.01 3.23 3.33 3.55 B0.5IIIs 756 0
43 [KPA2010] 35 dS* 21 54 03 +25 11.1   13.54 12.85     ~ 1 0
44 [KPA2010] 36 dS* 22 01 08 +24 44.5   13.42 13.01     ~ 1 0
45 ATO J330.4731-12.4811 dS* 22 01 53.5396312008 -12 28 51.953821500   12.23 12.25     ~ 6 0
46 BD+27 4253 dS* 22 05 55.2032103696 +28 02 31.733507004   9.95 9.48     A3 5 0
47 TYC 2216-1625-1 dS* 22 09 40.5398130840 +28 12 39.736944684   11.20 10.92     ~ 1 0
48 BD+36 4973 dS* 22 59 23.1741363840 +37 14 33.261869436   9.65 9.26     F2 4 0
49 TYC 2762-2049-1 dS* 23 02 06.8499860064 +36 30 28.552427892   11.84 11.51     ~ 2 0
50 V* SX Phe SX* 23 46 32.8928138474 -41 34 54.769886474   7.54 7.31     A3V 348 0

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