Search Publications

The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems I: High-contrast Imaging of the Exoplanet HIP 65426 b from 2 to 16 µm
DOI: 10.3847/2041-8213/acd93e Bibcode: 2023ApJ...951L..20C

Henning, Thomas; Fortney, Jonathan J.; Carter, Aarynn L. +108 more

We present JWST Early Release Science coronagraphic observations of the super-Jupiter exoplanet, HIP 65426b, with the Near-Infrared Camera (NIRCam) from 2 to 5 µm, and with the Mid-Infrared Instrument (MIRI) from 11 to 16 µm. At a separation of ~0.″82 (87 ${}_{-31}^{+108}$ au), HIP 65426b is clearly detected in all seven of our observa…

2023 The Astrophysical Journal
AKARI Gaia JWST 75
Patchy Forsterite Clouds in the Atmospheres of Two Highly Variable Exoplanet Analogs
DOI: 10.3847/1538-4357/acab58 Bibcode: 2023ApJ...944..138V

Marley, Mark; Faherty, Jacqueline K.; Morley, Caroline V. +12 more

We present an atmospheric retrieval analysis of a pair of highly variable, ~200 Myr old, early T type planetary-mass exoplanet analogs SIMP J01365662+0933473 and 2MASS J21392676+0220226 using the Brewster retrieval framework. Our analysis, which makes use of archival 1-15 µm spectra, finds almost identical atmospheres for both objects. For b…

2023 The Astrophysical Journal
AKARI 32
Evolved massive stars at low-metallicity. V. Mass-loss rate of red supergiant stars in the Small Magellanic Cloud
DOI: 10.1051/0004-6361/202244770 Bibcode: 2023A&A...676A..84Y

Tian, Hao; Yang, Ming; Bonanos, Alceste Z. +17 more

The mass-loss rate (MLR) is one of the most important parameters in astrophysics, because it impacts many areas of astronomy, such as ionizing radiation, wind feedback, star-formation rates, initial mass functions, stellar remnants, supernovae, and so on. However, the most important modes of mass loss are also the most uncertain, as the dominant p…

2023 Astronomy and Astrophysics
AKARI Gaia 31
GOALS-JWST: Small Neutral Grains and Enhanced 3.3 µm PAH Emission in the Seyfert Galaxy NGC 7469
DOI: 10.3847/2041-8213/ad0387 Bibcode: 2023ApJ...957L..26L

Inami, Hanae; Böker, Torsten; Law, David R. +37 more

We present James Webb Space Telescope (JWST) Near Infrared Spectrograph (NIRSpec) integral field spectroscopy of the nearby luminous infrared galaxy NGC 7469. We take advantage of the high spatial/spectral resolution and wavelength coverage of JWST/NIRSpec to study the 3.3 µm neutral polycyclic aromatic hydrocarbon (PAH) grain emission on ~2…

2023 The Astrophysical Journal
AKARI JWST 29
Hard X-Ray to Radio Multiwavelength SED Analysis of Local U/LIRGs in the GOALS Sample with a Self-consistent AGN Model including a Polar-dust Component
DOI: 10.3847/1538-4365/acb349 Bibcode: 2023ApJS..265...37Y

Imanishi, Masatoshi; Tanimoto, Atsushi; Ueda, Yoshihiro +7 more

We conduct hard X-ray to radio multiwavelength spectral energy distribution (SED) decomposition for 57 local luminous and ultraluminous infrared galaxies observed with the Nuclear Spectroscopic Telescope Array and/or Swift/Burst Alert Telescope in the GOALS sample. We modify the latest SED-fitting code X-CIGALE by implementing the infrared (IR) CL…

2023 The Astrophysical Journal Supplement Series
AKARI Herschel XMM-Newton 26
Corrected SFD: A More Accurate Galactic Dust Map with Minimal Extragalactic Contamination
DOI: 10.3847/1538-4357/acf4a1 Bibcode: 2023ApJ...958..118C

Chiang, Yi-Kuan

The widely used Milky Way dust-reddening map, the Schlegel-Finkbeiner-Davis (SFD) map, was found to contain extragalactic large-scale structure (LSS) imprints. Such contamination is inherent in maps based on infrared emission, which pick up not only Galactic dust but also the cosmic infrared background (CIB). When SFD is used for extinction correc…

2023 The Astrophysical Journal
AKARI Gaia 22
Hunting for C-rich long-period variable stars in the Milky Way's bar-bulge using unsupervised classification of Gaia BP/RP spectra
DOI: 10.1093/mnras/stad574 Bibcode: 2023MNRAS.521.2745S

Matsunaga, Noriyuki; Sanders, Jason L.

The separation of oxygen- and carbon-rich asymptotic giant branch sources is crucial for their accurate use as local and cosmological distance and age/metallicity indicators. We investigate the use of unsupervised learning algorithms for classifying the chemistry of long-period variables from Gaia DR3's BP/RP spectra. Even in the presence of signi…

2023 Monthly Notices of the Royal Astronomical Society
AKARI Gaia 21
GOALS-JWST: Revealing the Buried Star Clusters in the Luminous Infrared Galaxy VV 114
DOI: 10.3847/2041-8213/acb335 Bibcode: 2023ApJ...944L..55L

Inami, Hanae; Böker, Torsten; Kemper, Francisca +30 more

We present the results of a James Webb Space Telescope NIRCam investigation into the young massive star cluster (YMC) population in the luminous infrared galaxy VV 114. We identify 374 compact YMC candidates with signal-to-noise ratios ≥ 3, 5, and 5 at F150W, F200W, and F356W, respectively. A direct comparison with our HST cluster catalog reveals …

2023 The Astrophysical Journal
AKARI eHST JWST 20
A New Study on a Type Iax Stellar Remnant and its Probable Association with SN 1181
DOI: 10.3847/1538-4357/acb138 Bibcode: 2023ApJ...944..120L

Hillier, D. John; Parker, Quentin A.; Ritter, Andreas +4 more

We report observations and modeling of the stellar remnant and presumed double-degenerate merger of Type Iax supernova Pa 30, which is the probable remnant of SN 1181 AD. It is the only known bound stellar SN remnant and the only star with Wolf-Rayet features that is neither a planetary nebula central star nor a massive Population I progenitor. We…

2023 The Astrophysical Journal
AKARI Gaia INTEGRAL XMM-Newton eHST 16
Confirmation of an He I evaporating atmosphere around the 650-Myr-old sub-Neptune HD 235088 b (TOI-1430 b) with CARMENES
DOI: 10.1051/0004-6361/202346445 Bibcode: 2023A&A...677A..56O

Sánchez-López, A.; López-Puertas, M.; Nagel, E. +31 more

HD 235088 (TOI-1430) is a young star known to host a sub-Neptune-sized planet candidate. We validated the planetary nature of HD 235088 b with multiband photometry, refined its planetary parameters, and obtained a new age estimate of the host star, placing it at 600-800 Myr. Previous spectroscopic observations of a single transit detected an exces…

2023 Astronomy and Astrophysics
AKARI XMM-Newton 16