2018AJ....155..112B


Query : 2018AJ....155..112B

2018AJ....155..112B - Astron. J., 155, 112-112 (2018)

HATS-43b, HATS-44b, HATS-45b, and HATS-46b: four short-period transiting giant planets in the Neptune-Jupiter mass range.

BRAHM R., HARTMAN J.D., JORDAN A., BAKOS G.A., ESPINOZA N., RABUS M., BHATTI W., PENEV K., SARKIS P., SUC V., CSUBRY Z., BAYLISS D., BENTO J., ZHOU G., MANCINI L., HENNING T., CICERI S., DE VAL-BORRO M., SHECTMAN S., CRANE J.D., ARRIAGADA P., BUTLER P., TESKE J., THOMPSON I., OSIP D., DIAZ M., SCHMIDT B., LAZAR J., PAPP I. and SARI P.

Abstract (from CDS):

We report the discovery of four short-period extrasolar planets transiting moderately bright stars from photometric measurements of the HATSouth network coupled to additional spectroscopic and photometric follow-up observations. While the planet masses range from 0.26 to 0.90 MJ, the radii are all approximately a Jupiter radii, resulting in a wide range of bulk densities. The orbital period of the planets ranges from 2.7 days to 4.7 days, with HATS-43b having an orbit that appears to be marginally non-circular (e = 0.173 ± 0.089). HATS-44 is notable for having a high metallicity ([Fe/H] = 0.320 ± 0.071). The host stars spectral types range from late F to early K, and all of them are moderately bright (13.3 < V < 14.4), allowing the execution of future detailed follow-up observations. HATS-43b and HATS-46b, with expected transmission signals of 2350 ppm and 1500 ppm, respectively, are particularly well suited targets for atmospheric characterization via transmission spectroscopy.

Abstract Copyright: © 2018. The American Astronomical Society. All rights reserved.

Journal keyword(s): planetary systems - stars: individual: (HATS-43, HATS-44, HATS-45, HATS-46)

VizieR on-line data: <Available at CDS (J/AJ/155/112): stars.dat table6.dat table7.dat>

Simbad objects: 26

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Number of rows : 26
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 HATS-46 * 00 26 48.5936508600 -56 18 58.080378456   14.42 13.63 13.68   ~ 16 0
2 HATS-46b Pl 00 26 48.5936508600 -56 18 58.080378456           ~ 20 0
3 HAT-P-19b Pl 00 38 04.0135699416 +34 42 41.553538560           ~ 74 1
4 HAT-P-48b Pl? 02 57 53.0159860416 +30 37 32.337459192           ~ 7 0
5 WASP-139b Pl 03 18 14.9435473104 -41 18 07.661940624           ~ 33 0
6 HATS-5b Pl 04 28 53.4832441440 -21 28 55.061983848           ~ 27 0
7 HATS-43 * 05 22 09.1675085784 -30 58 15.010622904   14.47 13.59 13.40   ~ 18 0
8 HATS-43b Pl 05 22 09.1675085784 -30 58 15.010622904           ~ 20 0
9 HATS-44 * 05 37 18.4239766680 -27 58 21.275663520   15.49 14.43 14.24   ~ 13 0
10 HATS-44b Pl 05 37 18.4239766680 -27 58 21.275663520           ~ 13 0
11 HATS-45b Pl 06 47 58.6224879696 -21 54 38.618349336           ~ 15 0
12 HATS-45 * 06 47 58.6224879696 -21 54 38.618349336   13.85 13.31 13.27   ~ 18 0
13 HAT-P-9b Pl 07 20 40.4564614032 +37 08 26.342829060           ~ 73 1
14 K2-98b Pl 08 25 57.1878020136 +11 30 40.081742604           ~ 19 0
15 CD-23 9677 PM* 11 01 35.8978277184 -23 51 38.386984896   11.05 10.28 10.21 9.66 ~ 75 1
16 CD-23 9677b Pl 11 01 35.8978277184 -23 51 38.386984896           ~ 59 1
17 K2-27b Pl 11 26 03.6414933480 +01 13 50.660984604           ~ 31 0
18 WASP-107b Pl 12 33 32.8441110816 -10 08 46.225572324           ~ 289 0
19 HATS-7b Pl 13 55 25.6669039416 -21 12 27.724490244           ~ 39 0
20 HAT-P-26b Pl 14 12 37.5331103311 +04 03 36.116569918           ~ 200 1
21 WASP-39b Pl 14 29 18.4151689656 -03 26 40.204480380           ~ 345 1
22 Kepler-101b Pl 18 53 01.3205511624 +48 21 18.784380528           ~ 52 0
23 HATS-8b Pl 19 39 46.0127465208 -25 44 54.008422008           ~ 35 0
24 Kepler-89d Pl 19 49 19.9343204784 +41 53 28.006017936           ~ 93 1
25 BD-05 5432b Pl 21 00 06.1968214728 -05 05 40.034944176           ~ 219 1
26 CD-40 15273b Pl 23 51 31.0839097560 -39 54 24.258188484           ~ 88 1

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