2023ApJS..265....1Y

Query : 2023ApJS..265....1Y

2023ApJS..265....1Y - Astrophys. J., Suppl. Ser., 265, 1-32 (2023/March-0)

The TESS Grand Unified Hot Jupiter Survey. II. Twenty New Giant Planets.

YEE S.W., WINN J.N., HARTMAN J.D., BOUMA L.G., ZHOU G., QUINN S.N., LATHAM D.W., BIERYLA A., RODRIGUEZ J.E., COLLINS K.A., ALFARO O., BARKAOUI K., BEARD C., BELINSKI A.A., BENKHALDOUN Z., BENNI P., BERNACKI K., BOYLE A.W., BUTLER R.P., CALDWELL D.A., CHONTOS A., CHRISTIANSEN J.L., CIARDI D.R., COLLINS K.I., CONTI D.M., CRANE J.D., DAYLAN T., DRESSING C.D., EASTMAN J.D., ESSACK Z., EVANS P., EVERETT M.E., FAJARDO-ACOSTA S., FORES-TORIBIO R., FURLAN E., GHACHOUI M., GILLON M., HELLIER C., HELM I., HOWARD A.W., HOWELL S.B., ISAACSON H., JEHIN E., JENKINS J.M., JENSEN E.L.N., KIELKOPF J.F., LALOUM D., LEONHARDES-BARBOZA N., LEWIN P., LOGSDON S.E., LUBIN J., LUND M.B., MacDOUGALL M.G., MANN A.W., MASLENNIKOVA N.A., MASSEY B., McLEOD K.K., MUNOZ J.A., NEWMAN P., ORLOV V., PLAVCHAN P., POPOWICZ A., POZUELOS F.J., PRITCHARD T.A., RADFORD D.J., REEFE M., RICKER G.R., RUDAT A., SAFONOV B.S., SCHWARZ R.P., SCHWEIKER H., SCOTT N.J., SEAGER S., SHECTMAN S.A., STOCKDALE C., TAN T.-G., TESKE J.K., THOMAS N.B., TIMMERMANS M., VANDERSPEK R., VERMILION D., WATANABE D., WEISS L.M., WEST R.G., VAN ZANDT J., ZEJMO M. and ZIEGLER C.

Abstract (from CDS):

NASA's Transiting Exoplanet Survey Satellite (TESS) mission promises to improve our understanding of hot Jupiters by providing an all-sky, magnitude-limited sample of transiting hot Jupiters suitable for population studies. Assembling such a sample requires confirming hundreds of planet candidates with additional follow-up observations. Here we present 20 hot Jupiters that were detected using TESS data and confirmed to be planets through photometric, spectroscopic, and imaging observations coordinated by the TESS Follow-up Observing Program. These 20 planets have orbital periods shorter than 7 days and orbit relatively bright FGK stars (10.9 < G < 13.0). Most of the planets are comparable in mass to Jupiter, although there are four planets with masses less than that of Saturn. TOI-3976b, the longest-period planet in our sample (P = 6.6 days), may be on a moderately eccentric orbit (e = 0.18 ± 0.06), while observations of the other targets are consistent with them being on circular orbits. We measured the projected stellar obliquity of TOI-1937A b, a hot Jupiter on a 22.4 hr orbit with the Rossiter-McLaughlin effect, finding the planet's orbit to be well aligned with the stellar spin axis (∣λ∣ = 4.°0 ± 3.°5). We also investigated the possibility that TOI-1937 is a member of the NGC 2516 open cluster but ultimately found the evidence for cluster membership to be ambiguous. These objects are part of a larger effort to build a complete sample of hot Jupiters to be used for future demographic and detailed characterization work.

Abstract Copyright: © 2023. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Exoplanets - Hot Jupiters - Radial velocity - Exoplanet detection methods - Transit photometry

VizieR on-line data: <Available at CDS (J/ApJS/265/1): table1.dat table3.dat table4.dat table5.dat table7.dat table8.dat fig15a.dat fig15b.dat fig15c.dat fig5/*>

Simbad objects: 55

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Number of rows : 55
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 2MASS J02370750+5451089 * 02 37 07.4996168788 +54 51 09.105956931           ~ 1 0
2 TOI-3688b Pl 02 37 07.7271832800 +54 51 04.551214968           ~ 2 0
3 TOI-3688 * 02 37 07.7271832800 +54 51 04.551214968   12.92 12.24     ~ 7 0
4 TOI-4145 * 02 37 43.0668700440 +80 16 02.791327692   12.94 12.08     ~ 9 0
5 TOI-4145b Pl 02 37 43.0668700440 +80 16 02.791327692           ~ 4 0
6 Gaia DR3 568619417628568704 * 02 37 43.5205135270 +80 16 04.149839466           ~ 1 0
7 Cl Melotte 22 OpC 03 46 38.0 +24 10 41           ~ 3679 0
8 NAME HIP 21974 Cluster OpC 04 37 00.6 +71 16 52           ~ 62 0
9 TOI-2796 * 05 36 36.6499716930 +00 53 46.562962102   13.162 12.514 12.389   ~ 12 0
10 TOI-2796b Pl 05 36 36.6499716930 +00 53 46.562962102           ~ 2 0
11 TOI-2364b Pl 05 56 31.1936699267 -05 00 43.067307526           ~ 3 0
12 TOI-2364 * 05 56 31.1936699267 -05 00 43.067307526   13.128 12.289 12.103   ~ 10 0
13 TOI-2803b Pl 06 12 27.5367024693 -23 29 33.168403163           ~ 2 0
14 TOI-2803 * 06 12 27.5367024693 -23 29 33.168403163   13.044 12.544 12.486   ~ 10 0
15 UCAC4 333-011270 * 06 12 28.3784885611 -23 29 17.433447683       12.845   ~ 2 0
16 TOI-2842 * 07 12 10.6061580255 -10 38 21.688639730   13.253 12.598 12.509   ~ 7 0
17 TOI-2842b Pl 07 12 10.6061580255 -10 38 21.688639730           ~ 2 0
18 TOI-4791b Pl 07 17 33.2272340736 -19 49 44.275483272           ~ 2 0
19 TOI-4791 * 07 17 33.2272340736 -19 49 44.275483272   12.083 11.471 11.320   ~ 6 0
20 TOI-2587b Pl 07 43 43.5877776648 -01 04 23.606559984           ~ 2 0
21 TOI-2587 * 07 43 43.5877776648 -01 04 23.606559984   12.13 11.54     ~ 6 0
22 UCAC4 445-040797 * 07 43 44.1359126985 -01 04 26.975139153       13.744   ~ 1 0
23 ** CTI 1217B * 07 45 28.9627703552 -52 22 57.430146133           ~ 3 0
24 TOI-1937b Pl 07 45 28.9826465707 -52 22 59.906654197           ~ 7 0
25 TOI-1937 * 07 45 28.9826465707 -52 22 59.906654197     13.246 13.027   ~ 15 0
26 TOI-2818 * 07 56 14.3640216669 -35 07 00.017957398   12.639 11.962 11.853   ~ 11 0
27 TOI-2818b Pl 07 56 14.3640216669 -35 07 00.017957398           ~ 3 0
28 NGC 2516 OpC 07 58 00.5 -60 46 36           ~ 793 0
29 TOI-3819b Pl 08 07 27.1889299621 +29 23 19.472233911           ~ 2 0
30 TOI-3819 * 08 07 27.1889299621 +29 23 19.472233911   13.178 12.516 12.441   ~ 5 0
31 NGC 2548 OpC 08 13 34.0 -05 43 11           ~ 227 0
32 NGC 2632 OpC 08 39 58.4 +19 36 33           ~ 1733 0
33 TOI-3807 * 09 16 27.0174552768 +69 04 26.881770648   12.878 12.112 12.079   ~ 7 0
34 TOI-3807b Pl 09 16 27.0174552768 +69 04 26.881770648           ~ 2 0
35 TOI-2977b Pl 09 35 42.4094996425 -60 21 27.237693261           ~ 2 0
36 TOI-2977 * 09 35 42.4094996425 -60 21 27.237693261   13.268 12.531 12.374   ~ 5 0
37 TOI-3364b Pl 09 38 09.1068931392 -49 20 07.018813500           ~ 1 0
38 TOI-3364 * 09 38 09.1068931392 -49 20 07.018813500   12.200 11.450 11.305   ~ 6 0
39 TOI-3023 PM* 11 01 16.0250174148 -72 21 24.534977525   13.068 12.240 12.109   ~ 7 0
40 TOI-3023b Pl 11 01 16.0250174148 -72 21 24.534977525           ~ 2 0
41 NGC 3532 OpC 11 05 33.9 -58 42 13           ~ 414 0
42 TOI-3912b Pl 14 23 12.3501833250 +24 04 35.635525863           ~ 2 0
43 TOI-3912 * 14 23 12.3501833250 +24 04 35.635525863   13.148 12.398 12.396   ~ 6 0
44 TOI-4087b Pl 14 31 42.3348223800 +83 22 21.579944052           ~ 4 0
45 TOI-4087 * 14 31 42.3348223800 +83 22 21.579944052   12.208 11.741 11.761   ~ 11 0
46 2MASS J14572504+4416237 * 14 57 24.9511330722 +44 16 23.510362766           ~ 1 0
47 TOI-3976 * 14 57 25.4706362982 +44 16 27.403568068   12.988 12.318 12.343   ~ 6 0
48 TOI-3976b Pl 14 57 25.4706362982 +44 16 27.403568068           ~ 2 0
49 TOI-2583b Pl 18 09 04.0755444806 +45 20 12.761012482           ~ 1 0
50 TOI-2583 * 18 09 04.0755444806 +45 20 12.761012482   13.095 12.616 12.491   ~ 6 0
51 2MASS J18090425+4520078 * 18 09 04.2506617454 +45 20 07.838966016           ~ 1 0
52 HD 349013 PM* 18 37 25.9564928208 +18 43 47.043130476   11.64 11.04     F5 10 0
53 HD 349013b Pl 18 37 25.9564928208 +18 43 47.043130476           ~ 3 0
54 HD 349013B PM* 18 37 26.7194341437 +18 43 43.595466331           ~ 1 0
55 NGC 6811 OpC 19 37 21.8 +46 22 43   7.47 6.8     ~ 435 0

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