Qatar Exoplanet Survey: Qatar-3b, Qatar-4b, and Qatar-5b

Khalid Alsubai; Dimitris Mislis; Zlatan I. Tsvetanov; David W. Latham; Allyson Bieryla; Lars A. Buchhave; Gilbert A. Esquerdo; D. M. Bramich; Stylianos Pyrzas; Nicolas P.E. Vilchez; Luigi Mancini; John Southworth; Daniel F. Evans; Thomas Henning; Simona Ciceri

doi:10.3847/1538-3881/aa6340

Qatar Exoplanet Survey: Qatar-3b, Qatar-4b, and Qatar-5b

Khalid Alsubai
, Dimitris Mislis
, Zlatan I. Tsvetanov
, David W. Latham
, Allyson Bieryla
, Lars A. Buchhave
, Gilbert A. Esquerdo
, D. M. Bramich
, Stylianos Pyrzas
, Nicolas P.E. Vilchez
, Luigi Mancini
, John Southworth
, Daniel F. Evans
, Thomas Henning
, Simona Ciceri

Research output: Contribution to journal › Article › peer-review

20 Citations (Scopus)

Abstract

We report the discovery of Qatar-3b, Qatar-4b, and Qatar-5b, three new transiting planets identified by the Qatar Exoplanet Survey. The three planets belong to the hot Jupiter family, with orbital periods of P_Q3b=2.50792 days, P_Q4b=1.80539 days, and P_Q5b=2.87923 days. Follow-up spectroscopic observations reveal the masses of the planets to be M_Q3b=4.31±0.47 M_J, M_Q4b=6.10±0.54 M_J, and M_Q5b=4.32±0.18 M_J, while model fits to the transit light curves yield radii of R_Q3b=1.096±0.14 R_J, R_Q4b=1.135±0.11 R_J, and R_Q5b= 1.107±0.064 R_J. The host stars are low-mass main sequence stars with masses and radii M_Q3= 1.145±0.064 Ṁ, M_Q4=0.896±0.048Ṁ, M_Q5=1.128±0.056 Ṁ and R_Q3=1.272±0.14 RṀ, R_Q4=0.849±0.063 R , and R_Q5=1.076±0.051 Ṙ for Qatar-3, 4, and 5 respectively. The V magnitudes of the three host stars are V_Q3=12.88, V_Q4=13.60, and V_Q5=12.82. All three new planets can be classified as heavy hot Jupiters (M > 4 M_J).

Original language	English
Article number	200
Journal	Astronomical Journal
Volume	153
Issue number	4
DOIs	https://doi.org/10.3847/1538-3881/aa6340
Publication status	Published - Apr 2017

Keywords

planetary systems
planets and satellites: gaseous planets

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10.3847/1538-3881/aa6340

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Alsubai, K., Mislis, D., Tsvetanov, Z. I., Latham, D. W., Bieryla, A., Buchhave, L. A., Esquerdo, G. A., Bramich, D. M., Pyrzas, S., Vilchez, N. P. E., Mancini, L., Southworth, J., Evans, D. F., Henning, T., & Ciceri, S. (2017). Qatar Exoplanet Survey: Qatar-3b, Qatar-4b, and Qatar-5b. Astronomical Journal, 153(4), Article 200. https://doi.org/10.3847/1538-3881/aa6340

@article{f979b92771b04069bb73383b168f33b9,

title = "Qatar Exoplanet Survey: Qatar-3b, Qatar-4b, and Qatar-5b",

abstract = "We report the discovery of Qatar-3b, Qatar-4b, and Qatar-5b, three new transiting planets identified by the Qatar Exoplanet Survey. The three planets belong to the hot Jupiter family, with orbital periods of PQ3b=2.50792 days, PQ4b=1.80539 days, and PQ5b=2.87923 days. Follow-up spectroscopic observations reveal the masses of the planets to be MQ3b=4.31±0.47 MJ, MQ4b=6.10±0.54 MJ, and MQ5b=4.32±0.18 MJ, while model fits to the transit light curves yield radii of RQ3b=1.096±0.14 RJ, RQ4b=1.135±0.11 RJ, and RQ5b= 1.107±0.064 RJ. The host stars are low-mass main sequence stars with masses and radii MQ3= 1.145±0.064 Ṁ, MQ4=0.896±0.048Ṁ, MQ5=1.128±0.056 Ṁ and RQ3=1.272±0.14 RṀ, RQ4=0.849±0.063 R , and RQ5=1.076±0.051 Ṙ for Qatar-3, 4, and 5 respectively. The V magnitudes of the three host stars are VQ3=12.88, VQ4=13.60, and VQ5=12.82. All three new planets can be classified as heavy hot Jupiters (M > 4 MJ).",

keywords = "planetary systems, planets and satellites: gaseous planets",

author = "Khalid Alsubai and Dimitris Mislis and Tsvetanov, \{Zlatan I.\} and Latham, \{David W.\} and Allyson Bieryla and Buchhave, \{Lars A.\} and Esquerdo, \{Gilbert A.\} and Bramich, \{D. M.\} and Stylianos Pyrzas and Vilchez, \{Nicolas P.E.\} and Luigi Mancini and John Southworth and Evans, \{Daniel F.\} and Thomas Henning and Simona Ciceri",

note = "Publisher Copyright: {\textcopyright} 2017 Published by Elsevier B.V.",

year = "2017",

month = apr,

doi = "10.3847/1538-3881/aa6340",

language = "English",

volume = "153",

journal = "Astronomical Journal",

issn = "0004-6256",

publisher = "American Astronomical Society",

number = "4",

}

TY - JOUR

T1 - Qatar Exoplanet Survey

T2 - Qatar-3b, Qatar-4b, and Qatar-5b

AU - Alsubai, Khalid

AU - Mislis, Dimitris

AU - Tsvetanov, Zlatan I.

AU - Latham, David W.

AU - Bieryla, Allyson

AU - Buchhave, Lars A.

AU - Esquerdo, Gilbert A.

AU - Bramich, D. M.

AU - Pyrzas, Stylianos

AU - Vilchez, Nicolas P.E.

AU - Mancini, Luigi

AU - Southworth, John

AU - Evans, Daniel F.

AU - Henning, Thomas

AU - Ciceri, Simona

PY - 2017/4

Y1 - 2017/4

N2 - We report the discovery of Qatar-3b, Qatar-4b, and Qatar-5b, three new transiting planets identified by the Qatar Exoplanet Survey. The three planets belong to the hot Jupiter family, with orbital periods of PQ3b=2.50792 days, PQ4b=1.80539 days, and PQ5b=2.87923 days. Follow-up spectroscopic observations reveal the masses of the planets to be MQ3b=4.31±0.47 MJ, MQ4b=6.10±0.54 MJ, and MQ5b=4.32±0.18 MJ, while model fits to the transit light curves yield radii of RQ3b=1.096±0.14 RJ, RQ4b=1.135±0.11 RJ, and RQ5b= 1.107±0.064 RJ. The host stars are low-mass main sequence stars with masses and radii MQ3= 1.145±0.064 Ṁ, MQ4=0.896±0.048Ṁ, MQ5=1.128±0.056 Ṁ and RQ3=1.272±0.14 RṀ, RQ4=0.849±0.063 R , and RQ5=1.076±0.051 Ṙ for Qatar-3, 4, and 5 respectively. The V magnitudes of the three host stars are VQ3=12.88, VQ4=13.60, and VQ5=12.82. All three new planets can be classified as heavy hot Jupiters (M > 4 MJ).

AB - We report the discovery of Qatar-3b, Qatar-4b, and Qatar-5b, three new transiting planets identified by the Qatar Exoplanet Survey. The three planets belong to the hot Jupiter family, with orbital periods of PQ3b=2.50792 days, PQ4b=1.80539 days, and PQ5b=2.87923 days. Follow-up spectroscopic observations reveal the masses of the planets to be MQ3b=4.31±0.47 MJ, MQ4b=6.10±0.54 MJ, and MQ5b=4.32±0.18 MJ, while model fits to the transit light curves yield radii of RQ3b=1.096±0.14 RJ, RQ4b=1.135±0.11 RJ, and RQ5b= 1.107±0.064 RJ. The host stars are low-mass main sequence stars with masses and radii MQ3= 1.145±0.064 Ṁ, MQ4=0.896±0.048Ṁ, MQ5=1.128±0.056 Ṁ and RQ3=1.272±0.14 RṀ, RQ4=0.849±0.063 R , and RQ5=1.076±0.051 Ṙ for Qatar-3, 4, and 5 respectively. The V magnitudes of the three host stars are VQ3=12.88, VQ4=13.60, and VQ5=12.82. All three new planets can be classified as heavy hot Jupiters (M > 4 MJ).

KW - planetary systems

KW - planets and satellites: gaseous planets

UR - https://www.scopus.com/pages/publications/85017324019

U2 - 10.3847/1538-3881/aa6340

DO - 10.3847/1538-3881/aa6340

M3 - Article

AN - SCOPUS:85017324019

SN - 0004-6256

VL - 153

JO - Astronomical Journal

JF - Astronomical Journal

IS - 4

M1 - 200

ER -

Qatar Exoplanet Survey: Qatar-3b, Qatar-4b, and Qatar-5b

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