TESS Eclipsing Binary Stars. I. Short-cadence Observations of 4584 Eclipsing Binaries in Sectors 1-26

Bibcode
2022ApJS..258...16P
DOI
10.3847/1538-4365/ac324a
Prša, Andrej; Kochoska, Angela; Conroy, Kyle E.; Eisner, Nora; Hey, Daniel R.; IJspeert, Luc; Kruse, Ethan; Fleming, Scott W.; Johnston, Cole; Kristiansen, Martti H.; LaCourse, Daryll; Mortensen, Danielle; Pepper, Joshua; Stassun, Keivan G.; Torres, Guillermo; Abdul-Masih, Michael; Chakraborty, Joheen; Gagliano, Robert; Guo, Zhao; Hambleton, Kelly; Hong, Kyeongsoo; Jacobs, Thomas; Jones, David; Kostov, Veselin; Lee, Jae Woo; Omohundro, Mark; Orosz, Jerome A.; Page, Emma J.; Powell, Brian P.; Rappaport, Saul; Reed, Phill; Schnittman, Jeremy; Schwengeler, Hans Martin; Shporer, Avi; Terentev, Ivan A.; Vanderburg, Andrew; Welsh, William F.; Caldwell, Douglas A.; Doty, John P.; Jenkins, Jon M.; Latham, David W.; Ricker, George R.; Seager, Sara; Schlieder, Joshua E.; Shiao, Bernie; Vanderspek, Roland; Winn, Joshua N.
Referencia bibliográfica

The Astrophysical Journal Supplement Series

Fecha de publicación:
1
2022
Número de autores
47
Número de autores del IAC
1
Número de citas
67
Número de citas referidas
49
Descripción
In this paper we present a catalog of 4584 eclipsing binaries observed during the first two years (26 sectors) of the TESS survey. We discuss selection criteria for eclipsing binary candidates, detection of hitherto unknown eclipsing systems, determination of the ephemerides, the validation and triage process, and the derivation of heuristic estimates for the ephemerides. Instead of keeping to the widely used discrete classes, we propose a binary star morphology classification based on a dimensionality reduction algorithm. Finally, we present statistical properties of the sample, we qualitatively estimate completeness, and we discuss the results. The work presented here is organized and performed within the TESS Eclipsing Binary Working Group, an open group of professional and citizen scientists; we conclude by describing ongoing work and future goals for the group. The catalog is available from http://tessEBs.villanova.edu and from MAST.
Proyectos relacionados
Izquierda - Imagen RGB de la nebulosa de Orión y M43 obtenida filtros estrechos con la cámara WFC en el INT: H alfa (rojo), [S II] 6716+30 (verde), [O III] 5007 (azul). Derecha - Imagen en falso color de la nebulosa planetaria NGC 6778. En azul se ve la emisión en la línea de O II tomada con el filtro sintonizable azul del instrumento OSIRIS en el GTC; en verde imagen con el filtro estrecho de [O III] del Nordic Optical Telescope (NOT).
Física de Nebulosas Ionizadas

Este proyecto mantiene dos líneas principales de investigación activas: 1) Estudio de la estructura, condiciones físicas y composición química de las nebulosas ionizadas, tanto galácticas como extragalácticas, a través del análisis detallado y modelización de sus espectros. Investigación de los gradientes de composición química a lo largo del disco

Jorge
García Rojas
En ejecución
Tipo
Con árbitro
Física estelar e interestelar (FEEI)
La Vía Láctea y el Grupo Local (MWLG)

Te puede interesar

  • Con árbitro
    The variability patterns of the TeV blazar PG 1553 + 113 from a decade of MAGIC and multiband observations

    PG 1553 + 113 is one of the few blazars with a convincing quasi-periodic emission in the gamma-ray band. The source is also a very high energy (VHE; >100 GeV) gamma-ray emitter. To better understand its properties and identify the underlying physical processes driving its variability, the MAGIC Collaboration initiated a multiyear, multiwavelength

    Abe, H. et al.

    Fecha de publicación:

    4
    2024
    Bibcode
    2024MNRAS.529.3894A
    Número de citas
    0
  • Con árbitro
    First characterization of the emission behavior of Mrk 421 from radio to very high-energy gamma rays with simultaneous X-ray polarization measurements

    Aims: We have performed the first broadband study of Mrk 421 from radio to TeV gamma rays with simultaneous measurements of the X-ray polarization from IXPE. Methods: The data were collected as part of an extensive multiwavelength campaign carried out between May and June 2022 using MAGIC, Fermi-LAT, NuSTAR, XMM-Newton, Swift, and several optical

    Abe, S. et al.

    Fecha de publicación:

    4
    2024
    Bibcode
    2024A&A...684A.127A
    Número de citas
    0
  • Con árbitro
    Effects of density and temperature variations on the metallicity of Mrk 71

    In a very recent work, [1] claim that the scenario of temperature inhomogeneities proposed by [2] ($t2$ > 0) is not able to explain the O$^{2+}$/H$^{+}$ abundance discrepancy observed between the calculations based on the optical [OIII] collisional excited lines (CELs) and the OII recombination lines (RLs) in the star forming galaxy Mrk71. In this

    Méndez-Delgado, J. Eduardo et al.

    Fecha de publicación:

    3
    2024
    Bibcode
    2024NatAs...8..275M
    Número de citas
    2