Search Publications

The Extremely Buried Nucleus of IRAS 17208-0014 Observed at Submillimeter and Near-infrared Wavelengths
DOI: 10.3847/1538-4357/ac57c2 Bibcode: 2022ApJ...928..184B

Onishi, Shusuke; Nakagawa, Takao; Baba, Shunsuke +6 more

The ultraluminous infrared galaxy IRAS 17208-0014 is a late-stage merger that hosts a buried active galactic nucleus (AGN). To investigate its nuclear structure, we performed high-spatial-resolution ( ~ 0.″04 ~ 32 pc) Atacama Large Millimeter/submillimeter Array (ALMA) observations in Band 9 (~450 µm or ~660 GHz), along with near-infrared AK…

2022 The Astrophysical Journal
AKARI Herschel ISO 10
Deblending Galaxies with Generative Adversarial Networks
DOI: 10.3847/1538-4357/aca1b8 Bibcode: 2022ApJ...941..141H

Mobasher, Bahram; Rhodes, Jason; Hemmati, Shoubaneh +6 more

Deep generative models including generative adversarial networks (GANs) are powerful unsupervised tools in learning the distributions of data sets. Building a simple GAN architecture in PyTorch and training on the CANDELS data set, we generate galaxy images with the Hubble Space Telescope (HST) resolution starting from a noise vector. We proceed b…

2022 The Astrophysical Journal
eHST 10
Shocks in the Outflow of the RS Oph 2021 Eruption Observed with X-Ray Gratings
DOI: 10.3847/1538-4357/ac8f46 Bibcode: 2022ApJ...938...34O

Luna, G. J. M.; Della Valle, M.; Behar, E. +9 more

The 2021 outburst of the symbiotic recurrent nova RS Oph was observed with the Chandra High Energy Transmission Gratings (HETG) on day 18 after optical maximum and with XMM-Newton and its Reflection Grating Spectrographs (RGS) on day 21, before the supersoft X-ray source emerged and when the emission was due to shocked ejecta. The absorbed flux in…

2022 The Astrophysical Journal
Gaia XMM-Newton 10
What Determines Active Region Coronal Plasma Composition?
DOI: 10.3847/1538-4357/ac6e40 Bibcode: 2022ApJ...933..245M

Long, David M.; Brooks, David H.; Baker, Deborah +4 more

The chemical composition of the solar corona is different from that of the solar photosphere, with the strongest variation being observed in active regions (ARs). Using data from the Extreme Ultraviolet (EUV) Imaging Spectrometer (EIS) on Hinode, we present a survey of coronal elemental composition as expressed in the first ionization potential (F…

2022 The Astrophysical Journal
Hinode 10
Decoding the X-Ray Flare from MAXI J0709-159 Using Optical Spectroscopy and Multiepoch Photometry
DOI: 10.3847/2041-8213/ac7b8a Bibcode: 2022ApJ...933L..34B

Arun, R.; Mathew, Blesson; Kartha, Sreeja S. +10 more

We present a follow-up study on the recent detection of two X-ray flaring events by MAXI/Gas Slit Camera observations in soft and hard X-rays from MAXI J0709-159 in the direction of HD 54786 (LY CMa), on 2022 January 25. The X-ray luminosity during the flare was around 1037 erg s-1 (MAXI), which got reduced to 1032

2022 The Astrophysical Journal
Gaia 10
HST Observations of the Globular Cluster NGC 6402 (M14) and Its Peculiar Multiple Populations
DOI: 10.3847/1538-4357/ac3a70 Bibcode: 2022ApJ...925..192D

D'Antona, Francesca; Milone, Antonino P.; Tailo, Marco +6 more

We present Hubble Space Telescope (HST) photometric results for NGC 6402, a highly reddened, very luminous Galactic globular cluster (GC). Recent spectroscopic observations of its red giant stars have shown a quite peculiar behavior in the chemistry of its multiple populations. These results have prompted UV and optical HST observations aimed at o…

2022 The Astrophysical Journal
eHST 10
The Directly Imaged Exoplanet Host Star 51 Eridani is a Gamma Doradus Pulsator
DOI: 10.3847/1538-4357/ac9229 Bibcode: 2022ApJ...938...49S

Li, Gang; Huber, Daniel; Bedding, Timothy R. +3 more

51 Eri is well known for hosting a directly imaged giant planet and for its membership to the β Pictoris moving group. Using 2 minute cadence photometry from the Transiting Exoplanet Survey Satellite (TESS), we detect multiperiodic variability in 51 Eri that is consistent with pulsations of Gamma Doradus (γ Dor) stars. We identify the most signifi…

2022 The Astrophysical Journal
Gaia 10
Compact Dust Emission in a Gravitationally Lensed Massive Quiescent Galaxy at z = 2.15 Revealed in 130 pc Resolution Observations by the Atacama Large Millimeter/submillimeter Array
DOI: 10.3847/1538-4357/ac9055 Bibcode: 2022ApJ...938..144M

Stiavelli, M.; Chiaberge, M.; Morishita, T. +3 more

We present new observations of MRG-M2129, a quiescent galaxy at z = 2.15, with the Atacama Large Millimeter/submillimeter Array (ALMA). With the combination of the effect of gravitational lensing by the foreground galaxy cluster and the angular resolution provided by ALMA, our data reveal 1.2 mm continuum emission at ~130 pc angular resolution. Co…

2022 The Astrophysical Journal
eHST 10
The Velocity Dispersion Function for Massive Quiescent and Star-forming Galaxies at 0.6 < z ≤ 1.0
DOI: 10.3847/1538-4357/ac9796 Bibcode: 2022ApJ...939...90T

Bell, Eric F.; Maseda, Michael V.; D'Eugenio, Francesco +10 more

We present the first direct spectroscopic measurement of the stellar velocity dispersion function (VDF) for massive quiescent and star-forming galaxies at 0.6 < z ≤ 1.0. For this analysis we use individual measurements of stellar velocity dispersion from high-signal-to-noise-ratio spectra from the public Large Early Galaxy Astrophysics Census (…

2022 The Astrophysical Journal
eHST 10
MHD Simulation of Homologous Eruptions from Solar Active Region 10930 Caused by Sunspot Rotation
DOI: 10.3847/1538-4357/ac8d0e Bibcode: 2022ApJ...938...61W

Feng, Xueshang; Duan, Aiying; Jiang, Chaowei +2 more

The relationship between solar eruption and sunspot rotation has been widely reported, and the underlying mechanism needs to be studied. Here we performed a full 3D MHD simulation using a data-constrained approach to study the mechanism of flare eruptions in active region (AR) NOAA 10930, which is characterized by continuous sunspot rotation and h…

2022 The Astrophysical Journal
Hinode 10