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1“...We examine the distributions of eccentricity and host star metallicity of exoplanets as a function...”
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2“...We examine the distributions of eccentricity and host star metallicity of exoplanets as a function...”
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3“...Abstract. We examine the distributions of eccentricity and host star metallicity of exoplanets as a...”
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4by Bakos, G. A., Penev, K., Bayliss, D., Hartman, J. D., Zhou, G., Brahm, R., Mancini, L., de Val-Borro, M., Bhatti, W., Jordan, A., Rabus, M., Espinoza, N., Csubry, Z., Howard, A. W., Fulton, B. J., Buchhave, L. A., Ciceri, S., Henning, T., Schmidt, B., Isaacson, H., Noyes, R. W., Marcy, G. W., Suc, V., Howe, A. R., Burrows, A. S., Lazar, J., Papp, I., Sari, P.“... from that of Saturn, which has 75% of its mass in H2-He. Based on a sample of transiting exoplanets...”
Published in The Astrophysical Journal (2015)
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5by Bakos, G. Á., Penev, K., Bayliss, D., Hartman, J. D., Zhou, G., Brahm, R., Mancini, L., de Val-Borro, M., Bhatti, W., Jordán, A., Rabus, M., Espinoza, N., Csubry, Z., Howard, A. W., Fulton, B. J., Buchhave, L. A., Ciceri, S., Henning, T., Schmidt, B., Isaacson, H., Noyes, R. W., Marcy, G. W., Suc, V., Howe, A. R., Burrows, A. S., Lázár, J., Papp, I., Sári, P.“... that of Saturn, which has 75% of its mass in H2-He. Based on a sample of transiting exoplanets with accurately...”
Published 2015
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6“... of transiting exoplanets with accurately (<20%) determined parameters, we establish approximate power-law...”
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7by Bakos, G. Á., Penev, K., Bayliss, D., Hartman, J. D., Zhou, G., Brahm, R., Mancini, L., de Val-Borro, M., Bhatti, W., Jordán, A., Rabus, M., Espinoza, N., Csubry, Z., Howard, A. W., Fulton, B. J., Buchhave, L. A., Ciceri, S., Henning, T., Schmidt, B., Isaacson, H., Noyes, R. W., Marcy, G. W., Suc, V., Howe, A. R., Burrows, A. S., Lázár, J., Papp, I., Sári, P.“... that of Saturn, which has 75% of its mass in H2-He. Based on a sample of transiting exoplanets with accurately...”
Published in The Astrophysical Journal (2015)
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8by Bakos, G. A., Penev, K., Bayliss, Daniel, Hartman, J. D., Zhou, Guyin (George), Brahm, R., Mancini, L., De Val-Borro, M., Bhatti, Waqas, Jordan, A., Rabus, M., Espinoza, N., Csubry, Z., Howard, Andrew, Fulton, B. J., Buchhave, L. A., Ciceri, Simona, Henning, T., Schmidt, Brian, Isaacson, H., Noyes, R. W., Marcy, G. W., Suc, V., Howe, A. R., Burrows, A., Lazar, J., Papp, I., Sari, P.“... from that of Saturn, which has 75% of its mass in H2-He. Based on a sample of transiting exoplanets...”
Published in The Astrophysical Journal
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9by Bakos G. A., Penev K., Bayliss D., Hartman J. D., Zhou G., Brahm R., Mancini L., De Val-Borro M., Bhatti W., Jordan A., Rabus M., Espinoza N., Csubry Z., Howard A. W., Fulton B. J., Buchhave L. A., Ciceri S., Henning T., Schmidt B., Isaacson H., Noyes R. W., Marcy G. W., Suc V., Howe A. R., Burrows A. S., Lazar J., Papp I., Sari P.“... of transiting exoplanets with accurately (<20%) determined parameters, we establish approximate power-law...”
Published in The Astrophysical Journal (2015)
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10“... of transiting exoplanets with accurately (<20%) determined parameters, we establish approximate power-law...”
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