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Query : 2018A&A...609A...4K |
2018A&A...609A...4K - Astronomy and Astrophysics, volume 609A, 4-4 (2018/1-1)
Simulating the exoplanet yield of a space-based mid-infrared interferometer based on Kepler statistics.
KAMMERER J. and QUANZ S.P.
Abstract (from CDS):
Abstract Copyright: © ESO, 2017
Journal keyword(s): planets and satellites: detection - planets and satellites: terrestrial planets - instrumentation: high angular resolution - instrumentation: interferometers - methods: numerical
Simbad objects: 20
Number of rows : 20 |
N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2024 |
#notes |
---|---|---|---|---|---|---|---|---|---|---|---|---|
1 | HD 225213 | Er* | 00 05 24.4284351777 | -37 21 26.507931505 | 11.074 | 10.022 | 8.562 | 7.589 | 6.432 | M2V | 206 | 0 |
2 | HD 1326 | Er* | 00 18 22.8849799680 | +44 01 22.637951588 | 10.120 | 7.3 | M2V | 542 | 0 | |||
3 | * zet Tuc | PM* | 00 20 04.2586334956 | -64 52 29.257190108 | 4.82 | 4.80 | 4.23 | 3.73 | 3.40 | F9.5V | 380 | 0 |
4 | * eta Cas | PM* | 00 49 06.2945942922 | +57 48 54.638239716 | 4.04 | 4.02 | 3.44 | 2.94 | 2.58 | F9V | 637 | 0 |
5 | * alf CMa | SB* | 06 45 08.91728 | -16 42 58.0171 | -1.51 | -1.46 | -1.46 | -1.46 | -1.43 | A0mA1Va | 1529 | 0 |
6 | * alf CMi | SB* | 07 39 18.11950 | +05 13 29.9552 | 0.82 | 0.79 | 0.37 | -0.05 | -0.28 | F5IV-V+DQZ | 1864 | 0 |
7 | HD 79210 | SB* | 09 14 22.7748624830 | +52 41 11.791503353 | 9.388 | 6.8 | K7V | 309 | 0 | |||
8 | HD 95735 | Er* | 11 03 20.1948195942 | +35 58 11.576182057 | 10.030 | 8.960 | 7.520 | 5.99 | 4.79 | M2+V | 715 | 0 |
9 | HD 119850 | Er* | 13 45 43.7755597223 | +14 53 29.471707437 | 10.989 | 9.894 | 8.50 | 7.465 | 6.363 | M2V | 352 | 0 |
10 | * alf Cen B | PM* | 14 39 35.06311 | -60 50 15.0992 | 2.89 | 2.21 | 1.33 | K1V | 1024 | 2 | ||
11 | * alf Cen A | SB* | 14 39 36.49400 | -60 50 02.3737 | 0.96 | 0.72 | 0.01 | G2V | 1280 | 1 | ||
12 | BD-12 4523 | BY* | 16 30 18.0583947383 | -12 39 45.321217732 | 12.829 | 11.638 | 10.072 | 8.917 | 7.421 | M3V | 315 | 0 |
13 | * alf Lyr | dS* | 18 36 56.33635 | +38 47 01.2802 | 0.03 | 0.03 | 0.03 | 0.07 | 0.10 | A0Va | 2686 | 1 |
14 | HD 173739 | PM* | 18 42 46.7043860406 | +59 37 49.409446059 | 10.43 | 8.93 | M3V | 382 | 1 | |||
15 | * alf Aql | dS* | 19 50 46.99855 | +08 52 05.9563 | 1.07 | 0.98 | 0.76 | 0.62 | 0.49 | A7Vn | 875 | 1 |
16 | * del Pav | PM* | 20 08 43.6088716052 | -66 10 55.442769229 | 4.78 | 4.32 | 3.56 | 2.95 | 2.61 | G8IV | 390 | 0 |
17 | HD 191849 | PM* | 20 13 53.3962498530 | -45 09 50.470550834 | 10.627 | 9.419 | 7.966 | 7.053 | 6.124 | M0V | 166 | 0 |
18 | HD 204961 | PM* | 21 33 33.9751191976 | -49 00 32.399427028 | 11.359 | 10.176 | 8.672 | 7.665 | 6.479 | M2/3V | 290 | 1 |
19 | * alf PsA | PM* | 22 57 39.04625 | -29 37 20.0533 | 1.31 | 1.25 | 1.16 | 1.11 | 1.09 | A4V | 1236 | 3 |
20 | HD 217987 | PM* | 23 05 52.0357857091 | -35 51 11.055185039 | 8.83 | 7.39 | M2V | 273 | 0 |
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