2009PASP..121.1096K

Query : 2009PASP..121.1096K

2009PASP..121.1096K - Publ. Astron. Soc. Pac., 121, 1096-1103 (2009/October-0)

Exoplanetary transit constraints based upon secondary eclipse observations.

KANE S.R. and VON BRAUN K.

Abstract (from CDS):

Transiting extrasolar planets provide an opportunity to study the mass-radius relation of planets as well as their internal structure. The existence of a secondary eclipse enables further study of the thermal properties of the the planet by observing at infrared wavelengths. The probability of an observable secondary eclipse depends upon the orbital parameters of the planet, particularly eccentricity and argument of periastron. Here we provide analytical expressions for these probabilities, investigate their properties, and calculate their values for the known extrasolar planets. We furthermore quantitatively discuss constraints on existence and observability of primary transits if a secondary eclipse is observed. Finally, we calculate the a posteriori transit probabilities of the known extrasolar planets, and we present several case studies in which orbital constraints resulting from the presence of a secondary eclipse may be applied in observing campaigns.

Abstract Copyright: ∼

Journal keyword(s):

Simbad objects: 53

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Number of rows : 53
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 * 54 Psc b Pl 00 39 21.8053928046 +21 15 01.712899720           ~ 61 2
2 HD 4113b Pl 00 43 12.5955916128 -37 58 57.477720936           ~ 37 1
3 HD 6434b Pl 01 04 40.1502696688 -39 29 17.584220159           ~ 42 1
4 * ups And d Pl 01 36 47.8415443907 +41 24 19.651368029           ~ 171 1
5 HD 13445b Pl 02 10 25.9181700303 -50 49 25.465181208           ~ 110 1
6 HD 17156 PM* 02 49 44.4871034544 +71 45 11.629235988   8.78 8.16     F9V 195 2
7 BD+20 518 PM* 03 11 14.2301712744 +21 05 50.493993288   9.26 8.50     G6V 127 1
8 HD 27894b Pl 04 20 47.0461066173 -59 24 39.024646358           ~ 32 1
9 HD 33283b Pl 05 08 01.0123084872 -26 47 50.894113344           ~ 35 1
10 HD 37605b Pl 05 40 01.7283246192 +06 03 38.072512008           ~ 42 1
11 HD 38529b Pl 05 46 34.9131388488 +01 10 05.502949860           ~ 90 1
12 HD 41004B * 05 59 49.6531151 -48 14 23.428302   13.85 12.33     M 67 1
13 HD 46375b Pl 06 33 12.6224391648 +05 27 46.528531452           ~ 75 1
14 HD 49674b Pl 06 51 30.5162069160 +40 52 03.924103260           ~ 56 1
15 HD 68988b Pl 08 18 22.1728652088 +61 27 38.595044628           ~ 52 1
16 HD 69830b Pl 08 18 23.9469682407 -12 37 55.817187530           ~ 76 1
17 HD 69830c Pl 08 18 23.9469682407 -12 37 55.817187530           ~ 65 1
18 HD 73256b Pl 08 36 23.0165447400 -30 02 15.446225796           ~ 47 1
19 HD 74156b Pl 08 42 25.1219511432 +04 34 41.145751740           ~ 69 1
20 HD 75289b Pl 08 47 40.3893739728 -41 44 12.455319264           ~ 93 1
21 * rho01 Cnc e Pl 08 52 35.8111044043 +28 19 50.954994470           ~ 682 1
22 * rho01 Cnc b Pl 08 52 35.8111044043 +28 19 50.954994470           ~ 267 1
23 HD 76700b Pl 08 53 55.5161171358 -66 48 03.575953228           ~ 42 1
24 HD 80606 PM* 09 22 37.5768032712 +50 36 13.435326684   9.78 9.00     G8V 366 2
25 HD 80606b Pl 09 22 37.5768032712 +50 36 13.435326684           ~ 369 1
26 HD 83443b Pl 09 37 11.8275201048 -43 16 19.933774320           ~ 74 1
27 HD 86081b Pl 09 56 05.9184616896 -03 48 30.325874184           ~ 36 1
28 HD 88133b Pl 10 10 07.6764870792 +18 11 12.728406552           ~ 50 1
29 BD-10 3166b Pl 10 58 28.7841138528 -10 46 13.394735436           ~ 44 1
30 * 83 Leo Bb Pl 11 26 46.2783265113 +03 00 22.756723728           ~ 45 1
31 Ross 905b Pl 11 42 11.0933350978 +26 42 23.650782778           ~ 913 1
32 HD 102117b Pl 11 44 50.4608641248 -58 42 13.357947852           ~ 29 1
33 HD 102195b Pl 11 45 42.2928676296 +02 49 17.324140440           ~ 62 1
34 HD 108147b Pl 12 25 46.2673666032 -64 01 19.516186956           ~ 58 1
35 HD 117618b Pl 13 32 25.5556238328 -47 16 16.913213976           ~ 28 1
36 HD 118203b Pl 13 34 02.5393988472 +53 43 42.698012376           ~ 54 1
37 * tau Boo b Pl 13 47 15.7381720026 +17 27 24.809555600           ~ 312 1
38 HD 130322b Pl 14 47 32.7262287384 -00 16 53.307811560           ~ 67 1
39 HD 147506b Pl 16 20 36.3576063720 +41 02 53.106772488           ~ 274 1
40 CD-46 11540b Pl 17 28 39.9455781571 -46 53 42.688095874           ~ 58 1
41 HD 162020b Pl 17 50 38.3557484304 -40 19 06.072311784           ~ 60 1
42 HD 168746b Pl 18 21 49.7826927816 -11 55 21.652464900           ~ 53 1
43 HD 179949b Pl 19 15 33.2300695008 -24 10 45.671448072           ~ 135 1
44 HD 185269b Pl 19 37 11.7411563088 +28 29 59.507007072           ~ 42 1
45 HD 187123b Pl 19 46 58.1122487784 +34 25 10.281404460           ~ 94 1
46 HD 190360c Pl 20 03 37.4050868074 +29 53 48.492435887           ~ 62 1
47 HD 192263b Pl 20 13 59.8455790536 -00 52 00.769626768           ~ 68 1
48 HD 195019b Pl 20 28 18.6366815627 +18 46 10.180434472           ~ 74 1
49 HD 209458b Pl 22 03 10.7727465312 +18 53 03.549393384           ~ 2037 1
50 BD-15 6290c Pl 22 53 16.7325836486 -14 15 49.304052185           ~ 202 1
51 * 51 Peg b Pl 22 57 27.9804852576 +20 46 07.797040104           ~ 744 1
52 HD 217107b Pl 22 58 15.5408995872 -02 23 43.383234768           ~ 101 1
53 HD 224693b Pl 23 59 53.8317247296 -22 25 41.216257992           ~ 31 1

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