Colección SciELO Chile

Departamento Gestión de Conocimiento, Monitoreo y Prospección
Consultas o comentarios: productividad@anid.cl
Búsqueda Publicación
Búsqueda por Tema Título, Abstract y Keywords



The TESS-Keck Survey. XVIII. A Sub-Neptune and Spurious Long-period Signal in the TOI-1751 System
Indexado
WoS WOS:001196732200001
Scopus SCOPUS_ID:85189921129
DOI 10.3847/1538-3881/AD29EE
Año 2024
Tipo artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


Abstract



We present and confirm TOI-1751 b, a transiting sub-Neptune orbiting a slightly evolved, solar-type, metal-poor star (T eff = 5996 +/- 110 K, log ( g ) = 4.2 +/- 0.1 , V = 9.3 mag, [Fe/H] = -0.40 +/- 0.06 dex) every 37.47 days. We use TESS photometry to measure a planet radius of 2.77 - 0.07 + 0.15 R circle plus . We also use both Keck/HIRES and APF/Levy radial velocities (RV) to derive a planet mass of 14.5 - 3.14 + 3.15 M circle plus , and thus a planet density of 3.6 +/- 0.9 g cm-3. There is also a long-period (similar to 400 days) signal that is observed in only the Keck/HIRES data. We conclude that this long-period signal is not planetary in nature and is likely due to the window function of the Keck/HIRES observations. This highlights the role of complementary observations from multiple observatories to identify and exclude aliases in RV data. Finally, we investigate the potential compositions of this planet, including rocky and water-rich solutions, as well as theoretical irradiated ocean models. TOI-1751 b is a warm sub-Neptune with an equilibrium temperature of similar to 820 K. As TOI-1751 is a metal-poor star, TOI-1751 b may have formed in a water-enriched formation environment. We thus favor a volatile-rich interior composition for this planet.

Revista



Revista ISSN
Astronomical Journal 0004-6256

Métricas Externas



PlumX Altmetric Dimensions

Muestra métricas de impacto externas asociadas a la publicación. Para mayor detalle:

Disciplinas de Investigación



WOS
Astronomy & Astrophysics
Scopus
Sin Disciplinas
SciELO
Sin Disciplinas

Muestra la distribución de disciplinas para esta publicación.

Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional



Muestra la distribución de colaboración, tanto nacional como extranjera, generada en esta publicación.


Autores - Afiliación



Ord. Autor Género Institución - País
1 Desai, Anmol - UNIV CALIF BERKELEY - Estados Unidos
University of California, Berkeley - Estados Unidos
2 Turtelboom, Emma V. - UNIV CALIF BERKELEY - Estados Unidos
University of California, Berkeley - Estados Unidos
3 Harada, Caleb K. Hombre UNIV CALIF BERKELEY - Estados Unidos
University of California, Berkeley - Estados Unidos
4 Dressing, Courtney D. Mujer UNIV CALIF BERKELEY - Estados Unidos
University of California, Berkeley - Estados Unidos
5 Rice, David R. - Open Univ Israel - Israel
The Open University of Israel - Israel
6 Murphy, Joseph M.A. Hombre Univ Calif Santa Cruz - Estados Unidos
University of California, Santa Cruz - Estados Unidos
7 Brinkman, Casey L. - Univ Hawaii - Estados Unidos
University Hawaii Institute for Astronomy - Estados Unidos
8 Chontos, Ashley Mujer Princeton Univ - Estados Unidos
Princeton University - Estados Unidos
9 Pearce, Logan Hombre UNIV KANSAS - Estados Unidos
University of Kansas - Estados Unidos
10 Dai, Fei - Div Geol & Planetary Sci - Estados Unidos
CALTECH - Estados Unidos
Division of Geological and Planetary Sciences - Estados Unidos
California Institute of Technology - Estados Unidos
11 Hill, Michelle L. Mujer Univ Calif Riverside - Estados Unidos
University of California, Riverside - Estados Unidos
12 Fetherolf, Tara Mujer Univ Calif Riverside - Estados Unidos
Calif State Univ - Estados Unidos
University of California, Riverside - Estados Unidos
California State University San Marcos - Estados Unidos
13 Giacalone, Steven Hombre CALTECH - Estados Unidos
California Institute of Technology - Estados Unidos
14 Howard, Andrew W. Hombre CALTECH - Estados Unidos
California Institute of Technology - Estados Unidos
15 Huber, Daniel Hombre Univ Hawaii - Estados Unidos
UNIV SYDNEY - Australia
University Hawaii Institute for Astronomy - Estados Unidos
The University of Sydney - Australia
16 Isaacson, Howard Hombre UNIV CALIF BERKELEY - Estados Unidos
Univ Southern Queensland - Australia
University of California, Berkeley - Estados Unidos
University of Southern Queensland - Australia
17 Kane, Stephen R. Hombre Univ Calif Riverside - Estados Unidos
University of California, Riverside - Estados Unidos
18 Lubin, Jack - Univ Calif Irvine - Estados Unidos
University of California, Riverside - Estados Unidos
University of California, Irvine - Estados Unidos
19 MacDougall, Mason G. Hombre UNIV CALIF LOS ANGELES - Estados Unidos
University of California, Los Angeles - Estados Unidos
20 Mayo, Andrew W. Hombre UNIV CALIF BERKELEY - Estados Unidos
Univ Copenhagen - Dinamarca
University of California, Berkeley - Estados Unidos
Statens Naturhistoriske Museum - Dinamarca
21 Mocnik, Teo - Gemini Observ NSFs NOIRLab - Estados Unidos
Gemini Observatory - Estados Unidos
22 Polanski, Alex S. Hombre UNIV KANSAS - Estados Unidos
University of Kansas - Estados Unidos
23 Rice, Malena Mujer YALE UNIV - Estados Unidos
Yale University - Estados Unidos
24 Robertson, Paul Hombre Univ Calif Irvine - Estados Unidos
University of California, Riverside - Estados Unidos
University of California, Irvine - Estados Unidos
25 Rubenzahl, Ryan A. Hombre CALTECH - Estados Unidos
California Institute of Technology - Estados Unidos
26 Van Zandt, Judah Hombre UNIV CALIF LOS ANGELES - Estados Unidos
University of California, Los Angeles - Estados Unidos
27 Weiss, Lauren M. Mujer UNIV NOTRE DAME - Estados Unidos
University of Notre Dame - Estados Unidos
28 Bieryla, Allyson Mujer Ctr Astrophys Harvard & Smithsonian - Estados Unidos
Harvard-Smithsonian Center for Astrophysics - Estados Unidos
29 Buchhave, L. A. Hombre Tech Univ Denmark - Dinamarca
Technical University of Denmark - Dinamarca
30 JENKINS, JAMES STEWART Hombre NASA Ames Res Ctr - Estados Unidos
NASA Ames Research Center - Estados Unidos
31 Kostov, Veselin Hombre NASA Goddard Space Flight Ctr - Estados Unidos
SETI Inst - Estados Unidos
SETI Institute - Estados Unidos
NASA Goddard Space Flight Center - Estados Unidos
32 Levine, Alan M. Hombre Kavli Inst Astrophys & Space Res - Estados Unidos
MIT Kavli Institute for Astrophysics and Space Research - Estados Unidos
33 Lillo-Box, J. Hombre Ctr Astrobiol CAB - España
European Space Astronomy Centre - España
34 Paegert, Martin Hombre Ctr Astrophys Harvard & Smithsonian - Estados Unidos
Harvard-Smithsonian Center for Astrophysics - Estados Unidos
35 Rabus, M. Hombre Universidad Católica de la Santísima Concepción - Chile
36 Stalport, M. Hombre Kavli Inst Astrophys & Space Res - Estados Unidos
MIT - Estados Unidos
Dept Aeronaut & Astronaut - Estados Unidos
MIT Kavli Institute for Astrophysics and Space Research - Estados Unidos
37 Stassun, Keivan - Vanderbilt Univ - Estados Unidos
38 Ting, Eric B. Hombre NASA Ames Res Ctr - Estados Unidos
NASA Ames Research Center - Estados Unidos
39 Watanabe, David Hombre Planetary Discoveries - Estados Unidos
40 Hart, R. Hombre Princeton Univ - Estados Unidos
Princeton University - Estados Unidos

Muestra la afiliación y género (detectado) para los co-autores de la publicación.

Financiamiento



Fuente
National Science Foundation
Australian Research Council
University of California
National Aeronautics and Space Administration
W. M. Keck Foundation
David and Lucile Packard Foundation
Alfred P. Sloan Foundation
University of California Berkeley
Heising-Simons Foundation
Science Mission Directorate
Heising-Simons Foundation (HSF)https://doi.org/10.13039/100014155
UC Berkeley Physics
FINESST Planetary Science Division

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos



Agradecimiento
Some of the data presented in this paper were obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation. The authors wish to recognize and acknowledge the very significant cultural role and reverence that the summit of Maunakea has always had within the indigenous Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this sacred mountain which is now colonized land.
This paper made use of data collected by the TESS mission and is publicly available from the Mikulski Archive for Space Telescopes (MAST) operated by the Space Telescope Science Institute (STScI; MAST Team ). Funding for the TESS mission is provided by NASA's Science Mission Directorate. We acknowledge the use of public TESS data from pipelines at the TESS Science Office and at the TESS Science Processing Operations Center. Resources supporting this work were provided by the NASA High-End Computing (HEC) Program through the NASA Advanced Supercomputing (NAS) Division at Ames Research Center for the production of the SPOC data products.
Some of the data presented in this paper were obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation. The authors wish to recognize and acknowledge the very significant cultural role and reverence that the summit of Maunakea has always had within the indigenous Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this sacred mountain which is now colonized land.
This paper made use of data collected by the TESS mission and is publicly available from the Mikulski Archive for Space Telescopes (MAST) operated by the Space Telescope Science Institute (STScI; MAST Team ). Funding for the TESS mission is provided by NASA's Science Mission Directorate. We acknowledge the use of public TESS data from pipelines at the TESS Science Office and at the TESS Science Processing Operations Center. Resources supporting this work were provided by the NASA High-End Computing (HEC) Program through the NASA Advanced Supercomputing (NAS) Division at Ames Research Center for the production of the SPOC data products.

Muestra la fuente de financiamiento declarada en la publicación.