Gliese 12 b: A Temperate Earth-sized Planet at 12 pc Ideal for Atmo...

Ad

Ad

Ad

Ad

Ad

Ad

Ad

Ad

Ad

Ad

Ad

Ad

Gliese 12 b: A Temperate Earth-sized Planet at 12 pc Ideal for Atmospheric
Transmission Spectroscopy
Masayuki Kuzuhara1,2,...

42
Institute of Engineering, Tokyo University of Agriculture and Technology, 2-24-16, Nakacho, Koganei, Tokyo, 184-8588, J...

Currently, TRAPPIST-1 (Gillon et al. 2017) is the only
known M dwarf within 30 pc transited by terrestrial planets
with in...

dwarfs to search for exoplanets using the RV technique
(Harakawa et al. 2022). Although the RV signal of Gliese 12 b
is to...

Advertisement

3.1. AO Imaging
Gliese 12 was observed with the NIRI imager of the Gemini-
North telescope (Hodapp et al. 2003) with the A...

Beichman). The images of Gliese 12 were corrected by the AO
system for NIRC2, where we adopted PyWFS (Bond et al.
2020) as...

spectrograph based on the same procedures as used in the
previous IRD papers (e.g., Kuzuhara et al. 2018; Hirano et al.
20...

estimation, we performed a Monte Carlo simulation adopted by
Harakawa et al. (2022).
The Teff, bolometric luminosity (Lbol...

and the Stefan–Boltzmann law, Lbol was calculated to be
7.28 ± 0.15 × 10−3
Le. We summarize the derived stellar
parameter ...

Advertisement

approximate Matérn 3/2 kernel implemented in the celer-
ite package with hyperparameters of s
ln and r
ln , where σ
and ρ ...

T = 18.4 ± 0.8 mag (ΔT < 8.1 ± 0.8 mag). Then, we converted
the detected source’s J-band magnitude to its T magnitude
unde...

each instrument σjit, IRD and σjit, CAR, where CAR stands for
CARMENES.
The parameters for the transit model are the same ...

varied P
log orb from 0 to 3 with 0.05 increments and ( )
m i
log sin
from 0 to 2 with 0.05 increments. We randomly sample...

20% of the total simulations were able to detect a planet as
massive as ∼4 M⊕ at Porb = 5 days. For 10 days < Porb <
30 da...

Advertisement

determination, we followed Kempton et al. (2018) to determine
the transmission spectroscopy metric (TSM) value of
Gliese 1...

public TESS data from pipelines at the TESS Science Ofﬁce
and at the TESS Science Processing Operations Center
(SPOC). Res...

Observatory staffs. Their support was essential in achieving
this discovery, especially amidst the many difﬁculties asso-
...

consistent results regardless of the adopted functions. A total of
99% of the measurements are consistent within 0.05 mag,...

Appendix C
Odd–Even Transit Plot for the TESS Data
The phase-folded TESS light curves of the odd- and even-
numbered trans...

Advertisement

Appendix D
Priors and Posteriors of the Light-curve Analyses
Table 4 summarizes the priors and posteriors of the transit
m...

Appendix E
Posteriors of the Joint-ﬁt Parameters
Figure 12 shows a corner plot for the posterior probability
distributions...

ORCID iDs
Masayuki Kuzuhara https:/
/orcid.org/0000-0002-
4677-9182
Akihiko Fukui https:/
/orcid.org/0000-0002-4909-5763
J...

Aoi Takahashi https:/
/orcid.org/0000-0003-3881-3202
Huan-Yu Teng https:/
/orcid.org/0000-0003-3860-6297
Motohide Tamura h...

Reid, I. N., Hawley, S. L., & Gizis, J. E. 1995, AJ, 110, 1838
Reiners, A., Zechmeister, M., Caballero, J. A., et al. 2018...

Share Slideshare

LinkedIn
Facebook
Twitter

Embed

Size (px)

Show related Slideshows at end

WordPress Shortcode

Link

Share
Email

2024 Trend Updates: What Really Wor... by Search Engine Jou... 1050381 views
Storytelling For The Web: Integrate... by Chiara Aliotta 965124 views
Artificial Intelligence, Data and C... by OECD Directorate ... 896563 views
How to Leverage AI to Boost Employe... by SocialHRCamp 378582 views
2024 State of Marketing Report – by... by Marius Sescu 214693 views
Everything You Need To Know About C... by Expeed Software 233000 views

View on Slideshare

1 of 24 Ad

View on Slideshare

1 of 24 Ad