Table 1
Statistical overview of the analyzed LAMOST spectra that have been obtained before the end of the 2014 observation season for the Kepler FOV.
| Field | RA(2000) | Dec(2000) | Date | # | Spectra | KO |
|
|
||||||
| LK01 | 19:03:39.26 | +39:54:39.2 | 110 530 | 1 | 939 | 411 |
| 110 608 | 2 | 711 | 370 | |||
| 140 602 | 2 | 3386 | 1846 | |||
| LK02a | 19:36:37.98 | +44:41:41.8 | 120 604 | 1 | 382 | 247 |
| 140 913 | 2 | 5439 | 3469 | |||
| LK03b | 19:24:09.92 | +39:12:42.0 | 120 615 | 3 | 4614 | 3381 |
| LK04c | 19:37:08.86 | +40:12:49.6 | 120 617 | 3 | 4206 | 2769 |
| LK05 | 19:49:18.14 | +41:34:56.8 | 131 005 | 2 | 3271 | 2247 |
| 140 522 | 1 | 1170 | 865 | |||
| LK06 | 19:40:45.38 | +48:30:45.1 | 130 522 | 1 | 1774 | 1317 |
| 130 914 | 1 | 2234 | 1530 | |||
| LK07 | 19:21:02.82 | +42:41:13.1 | 130 519 | 1 | 1778 | 1340 |
| 130 926 | 1 | 2324 | 1772 | |||
| LK08d | 19:59:20.42 | +45:46:21.1 | 130 925 | 2 | 4330 | 1759 |
| 131 002 | 1 | 100 | 31 | |||
| 131 017 | 1 | 1674 | 660 | |||
| 131 025 | 1 | 2147 | 821 | |||
| LK09 | 19:08:08.34 | +44:02:10.9 | 131 004 | 1 | 2462 | 1702 |
| LK10 | 19:23:14.83 | +47:11:44.8 | 140 520 | 2 | 2041 | 1395 |
| LK11 | 19:06:51.50 | +48:55:31.8 | 140 918 | 1 | 2589 | 1649 |
| LK12 | 18:50:31.04 | +42:54:43.7 | 131 007 | 1 | 2111 | 1170 |
| LK13 | 18:51:11.99 | +46:44:17.5 | 140 502 | 1 | 1921 | 1075 |
| 140 529 | 2 | 3410 | 1841 | |||
| LK14 | 19:23:23.79 | +50:16:16.6 | 140 917 | 1 | 2588 | 1397 |
| 140 927 | 1 | 1814 | 974 | |||
| 140 929 | 1 | 2338 | 1158 | |||
|
|
||||||
| Total | 61 753 | 37 196 | ||||
| Unique | 51 385 | 30 213 | ||||
| 1× | 42 553 | 24 303 | ||||
| 2× | 7569 | 5007 | ||||
| 3× | 1079 | 784 | ||||
| 4× | 117 | 81 | ||||
| +5× | 67 | 38 | ||||
Notes. The top lines give the specifications of the LK fields that have been observed. For each LK field, we give the right ascension (RA(2000)) and declination (DE(2000)) of the centrum, date of observation (YYMMDD; Date), number of plates that were used to observe the LK field (#), number of spectra for which we derived the atmospheric parameters with the ROTFIT code (Spectra), and number of spectra that correspond to a target that was observed by the Kepler mission (KO). The bottom lines give the summary of the observations of all LK fields together. We give the total number of spectra for which we derived the atmospheric parameters with the ROTFIT code (Total), number of different objects that were analyzed (Unique), and number of targets for which we obtained one (1×), two (2×), three (3×), four (4×), and at least five (+5×) sets of atmospheric parameters.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.