KELT-25 b and KELT-26 b: A Hot Jupiter and a Substellar Companion Transiting Young A Stars Observed by TESS

被引:30
|
作者
Martinez, Romy Rodriguez [1 ]
Gaudi, B. Scott [1 ]
Rodriguez, Joseph E. [2 ]
Zhou, George [2 ]
Labadie-Bartz, Jonathan [3 ]
Quinn, Samuel N. [2 ]
Penev, Kaloyan [4 ]
Tan, Thiam-Guan [5 ]
Latham, David W. [2 ]
Paredes, Leonardo A. [6 ]
Kielkopf, John F. [7 ]
Addison, Brett [8 ]
Wright, Duncan J. [8 ]
Teske, Johanna [9 ]
Howell, Steve B. [10 ]
Ciardi, David [11 ]
Ziegler, Carl [12 ]
Stassun, Keivan G. [13 ,14 ]
Johnson, Marshall C. [15 ]
Eastman, Jason D. [2 ]
Siverd, Robert J. [16 ]
Beatty, Thomas G. [17 ,18 ]
Bouma, Luke [19 ]
Bedding, Timothy [20 ]
Pepper, Joshua [21 ]
Winn, Joshua [19 ]
Lund, Michael B. [11 ]
Villanueva, Steven, Jr. [22 ,23 ]
Stevens, Daniel J. [24 ,25 ]
Jensen, Eric L. N. [26 ]
Kilby, Coleman [26 ]
Crane, Jeffrey D. [9 ,27 ]
Tokovinin, Andrei [28 ]
Everett, Mark E. [29 ]
Tinney, C. G. [30 ]
Fausnaugh, Michael [22 ,23 ]
Cohen, David H. [26 ]
Bayliss, Daniel [31 ,32 ]
Bieryla, Allyson [2 ]
Cargile, Phillip A. [2 ]
Collins, Karen A. [2 ]
Conti, Dennis M. [33 ]
Colon, Knicole D. [34 ]
Curtis, Ivan A. [35 ]
Depoy, D. L. [36 ,37 ]
Evans, Phil [38 ]
Feliz, Dax L. [13 ]
Gregorio, Joao [39 ,40 ]
Rothenberg, Jason [41 ]
James, David J. [2 ,42 ]
机构
[1] Ohio State Univ, Dept Astron, 140 West 18th Ave, Columbus, OH 43210 USA
[2] Harvard & Smithsonian, Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
[3] Univ Sao Paulo, Inst Astron Geofis & Ciencias Atmosfer, Rua Matao 1226,Cidade Univ, BR-05508900 Sao Paulo, SP, Brazil
[4] Univ Texas Dallas, Dept Phys, 800 West Campbell Rd, Richardson, TX 75080 USA
[5] Perth Exoplanet Survey Telescope, Perth, WA, Australia
[6] Georgia State Univ, Dept Phys & Astron, Atlanta, GA 30302 USA
[7] Univ Louisville, Dept Phys & Astron, Louisville, KY 40292 USA
[8] Univ Southern Queensland, Ctr Astrophys, West St, Toowoomba, Qld 4350, Australia
[9] Carnegie Inst Sci, The Observatories, 813 Santa Barbara St, Pasadena, CA 91101 USA
[10] NASA, Ames Res Ctr, Moffett Field, CA 94035 USA
[11] CALTECH IPAC NASA Exoplanet Sci Inst, 1200 East Calif Ave, Pasadena, CA 91125 USA
[12] Univ Toronto, Dunlap Inst Astron & Astrophys, Toronto, ON M5S 3H4, Canada
[13] Vanderbilt Univ, Dept Phys & Astron, Nashville, TN 37235 USA
[14] Fisk Univ, Dept Phys, 1000 17th Ave North, Nashville, TN 37208 USA
[15] Cumbres Observ, 6740 Cortona Dr,Suite 102, Goleta, CA 93117 USA
[16] Northern Operat Ctr, Gemini Observ, 670 North Aohoku Pl, Hilo, HI 96720 USA
[17] Univ Arizona, Dept Astron, Tucson, AZ 85721 USA
[18] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA
[19] Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA
[20] Univ Sydney, Sch Phys, Sydney Inst Astron SIfA, Sydney, NSW 2006, Australia
[21] Lehigh Univ, Dept Phys, 16 Mem Dr East, Bethlehem, PA 18015 USA
[22] MIT, Dept Phys, Cambridge, MA 02139 USA
[23] MIT, Kavli Inst Astrophys & Space Res, Cambridge, MA 02139 USA
[24] Penn State Univ, Dept Astron & Astrophys, 525 Davey Lab, University Pk, PA 16802 USA
[25] Penn State Univ, Ctr Exoplanets & Habitable Worlds, 525 Davey Lab, University Pk, PA 16802 USA
[26] Swarthmore Coll, Dept Phys & Astron, Swarthmore, PA 19081 USA
[27] Carnegie Inst Sci, Dept Terr Magnetism, 5241 Broad Branch Rd NW, Washington, DC 20015 USA
[28] Cerro Tololo Interamer Observ, Casilla 603, La Serena, Chile
[29] Natl Opt Astron Observ, 950 North Cherry Ave, Tucson, AZ 85719 USA
[30] UNSW Sydney, Sch Phys, Exoplanetary Sci UNSW, Sydney, NSW 2052, Australia
[31] Univ Warwick, Dept Phys, Gibbet Hill Rd, Coventry CV4 7AL, W Midlands, England
[32] Univ Warwick, Ctr Exoplanets & Habitabil, Gibbet Hill Rd, Coventry CV4 7AL, W Midlands, England
[33] Amer Assoc Variable Star Observers, 49 Bay State Rd, Cambridge, MA 02138 USA
[34] NASA, Exoplanets & Stellar Astrophys Lab, Goddard Space Flight Ctr, Code 667, Greenbelt, MD 20771 USA
[35] Ivan Curtis Private Observ, Adelaide, SA, Australia
[36] Texas A&M Univ, George P & Cynthia Woods Mitchell Inst Fundamenta, College Stn, TX 77843 USA
[37] Texas A&M Univ, Dept Phys & Astron, College Stn, TX 77843 USA
[38] El Sauce Observ, Rio Hurtado, Coquimbo, Chile
[39] Atalaia Grp, Portalegre, Portugal
[40] CROW Observ, Portalegre, Portugal
[41] Univ Wyoming, Dept Phys & Astron, 1000 East Univ Ave,Dept 3905, Laramie, WY 82071 USA
[42] Harvard Univ, Black Hole Initiat, 20 Garden St, Cambridge, MA 02138 USA
[43] Brigham Young Univ, Dept Phys & Astron, Provo, UT 84602 USA
[44] South African Astron Observ, POB 9, ZA-7935 Cape Town, South Africa
[45] Southern African Large Telescope, POB 9, ZA-7935 Cape Town, South Africa
[46] Spot Observ, Nashville, TN 37206 USA
[47] Wellesley Coll, Dept Astron, Wellesley, MA 02481 USA
[48] Louisiana State Univ, Dept Phys & Astron, Baton Rouge, LA 70803 USA
[49] Kutztown State Univ, Dept Phys Sci, Kutztown, PA 19530 USA
[50] Hazelwood Observ, Churchill, Vic, Australia
来源
ASTRONOMICAL JOURNAL | 2020年 / 160卷 / 03期
基金
澳大利亚研究理事会; 美国国家航空航天局; 巴西圣保罗研究基金会;
关键词
ROTATIONAL VELOCITIES; PLANET; DWARF; EXOPLANETS; SOUTH; SUN; ATMOSPHERES; ABUNDANCE; SELECTION; PROJECT;
D O I
10.3847/1538-3881/ab9f2d
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the discoveries of KELT-25 b (TIC 65412605, TOI-626.01) and KELT-26 b (TIC 160708862, TOI1337.01), two transiting companions orbiting relatively bright, early A stars. The transit signals were initially detected by the KELT survey and subsequently confirmed by Transiting Exoplanet Survey Satellite (TESS) photometry. KELT-25 b is on a 4.40 day orbit around the V = 9.66 star CD-24 5016 (T-eff = 8280(-180)(+440) K, M-star = 2.18(-0.11)(+0.12) M-circle dot), while KELT-26 b is on a 3.34 day orbit around the V = 9.95 star HD 134004 (T-eff = 8640(-240)(+500) K, M-circle dot = 1.93(-0.16)(+0.14) M-circle dot), which is likely an Am star. We have confirmed the substellar nature of both companions through detailed characterization of each system using ground-based and TESS photometry, radial velocity measurements, Doppler tomography, and high-resolution imaging. For KELT-25, we determine a companion radius of R-P = 1.64(-0.043)(+0.039) R-J and a 3 sigma upper limit on the companion's mass of similar to 64 M-J. For KELT-26 b, we infer a planetary mass and radius of M-P = 1.41(-0.51)(+0.43) M-J and R-P = 1.94(-0.058)(+0.060) R-J. From Doppler tomographic observations, we find KELT-26 b to reside in a highly misaligned orbit. This conclusion is weakly corroborated by a subtle asymmetry in the transit light curve from the TESS data. KELT-25 b appears to be in a well-aligned, prograde orbit, and the system is likely a member of the cluster Theia 449.
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页数:21
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