SIMBAD references

2012AJ....144...19B - Astron. J., 144, 19 (2012/July-0)

HAT-P-34b-HAT-P-37b: four transiting planets more massive than Jupiter orbiting moderately bright stars.

BAKOS G.A., HARTMAN J.D., TORRES G., BEKY B., LATHAM D.W., BUCHHAVE L.A., CSUBRY Z., KOVACS G., BIERYLA A., QUINN S., SZKLENAR T., ESQUERDO G.A., SHPORER A., NOYES R.W., FISCHER D.A., JOHNSON J.A., HOWARD A.W., MARCY G.W., SATO B., PENEV K., EVERETT M., SASSELOV D.D., FURESZ G., STEFANIK R.P., LAZAR J., PAPP I. and SARI P.

Abstract (from CDS):

We report the discovery of four transiting extrasolar planets (HAT-P-34b-HAT-P-37b) with masses ranging from 1.05 to 3.33 MJ and periods from 1.33 to 5.45 days. These planets orbit relatively bright F and G dwarf stars (from V = 10.16 to V = 13.2). Of particular interest is HAT-P-34b which is moderately massive (3.33 MJ), has a high eccentricity of e = 0.441±0.032 at a period of P = 5.452654±0.000016 days, and shows hints of an outer component. The other three planets have properties that are typical of hot Jupiters.

Abstract Copyright:

Journal keyword(s): planetary systems - stars: individual (HAT-P-34, GSC 1622-01261, HAT-P-35, GSC 0203-01079, HAT-P-36) - techniques: photometric - techniques: spectroscopic

VizieR on-line data: <Available at CDS (J/AJ/144/19): table2.dat table7.dat table8.dat table9.dat table10.dat table11.dat table12.dat table13.dat table14.dat>

Simbad objects: 23

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2020.01.23-00:37:06

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