Search Publications

High-resolution Spectroscopic Monitoring Observations of FU Orionis-type Object, V960 Mon
DOI: 10.3847/1538-4357/aba532 Bibcode: 2020ApJ...900...36P

Lee, Jeong-Eun; Pyo, Tae-Soo; Park, Sunkyung +9 more

We present the results of high-resolution (R ≥ 30,000) optical and near-infrared (NIR) spectroscopic monitoring observations of an FU Orionis-type object (FUor), V960 Mon, which underwent an outburst in 2014 November. We have monitored this object with the Bohyunsan Optical Echelle Spectrograph and the Immersion GRating INfrared Spectrograph since…

2020 The Astrophysical Journal
Gaia 19
Blazar Variability: A Study of Nonstationarity and the Flux-Rms Relation
DOI: 10.3847/1538-4357/ab91a8 Bibcode: 2020ApJ...897...25B

Bhattacharyya, Joy; Ghosh, Ritesh; Chatterjee, Ritaban +1 more

We analyze X-ray light curves of the blazars Mrk 421, PKS 2155-304, and 3C 273 using observations by the Soft X-ray Telescope on board AstroSat and archival XMM-Newton data. We use light curves of length 30-90 ks from three to four epochs for all three blazars. We apply the autoregressive integrated moving average model, which indicates the variab…

2020 The Astrophysical Journal
XMM-Newton 19
TESS Asteroseismic Analysis of the Known Exoplanet Host Star HD 222076
DOI: 10.3847/1538-4357/ab8f29 Bibcode: 2020ApJ...896...65J

Chaplin, William J.; Kane, Stephen R.; Stassun, Keivan G. +22 more

The Transiting Exoplanet Survey Satellite (TESS) is an all-sky survey mission aiming to search for exoplanets that transit bright stars. The high-quality photometric data of TESS are excellent for the asteroseismic study of solar-like stars. In this work, we present an asteroseismic analysis of the red-giant star HD 222076 hosting a long-period (2…

2020 The Astrophysical Journal
Gaia 19
A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies
DOI: 10.3847/1538-4357/ab94ac Bibcode: 2020ApJ...896...95O

Rakshit, Suvendu; Dewangan, Gulab Chand; Ojha, Vineet +1 more

We present a detailed comparative systematic study using a sample of 221 narrow-line Seyfert 1 (NLSy1) galaxies in comparison to a redshift-matched sample of 154 broad-line Seyfert 1 (BLSy1) galaxies based on their observations using ROSAT and/or XMM-Newton in soft X-ray band (0.1-2.0 keV). A homogeneous analysis is carried out to estimate their s…

2020 The Astrophysical Journal
XMM-Newton 19
First Solar Energetic Particles Measured on the Lunar Far-side
DOI: 10.3847/2041-8213/abbccc Bibcode: 2020ApJ...902L..30X

Wang, Yuming; Xu, Zigong; Guo, Jingnan +7 more

On 2019 May 6 the Lunar Lander Neutron & Dosimetry (LND) Experiment on board the Chang'E-4 lander on the far-side of the Moon detected its first solar energetic particle (SEP) event with proton energies up to 21 MeV. Combined proton energy spectra are studied based on the LND, SOHO/EPHIN, and ACE/EPAM measurements, which show that LND could pr…

2020 The Astrophysical Journal
SOHO 19
Far-infrared Photometric Redshifts: A New Approach to a Highly Uncertain Enterprise
DOI: 10.3847/1538-4357/aba528 Bibcode: 2020ApJ...900...68C

Casey, Caitlin M.

This paper presents a new approach to deriving far-infrared (FIR) photometric redshifts for galaxies based on their reprocessed emission from dust at rest-frame FIR through millimeter wavelengths. FIR photometric redshifts ("FIR-z") have been used over the past decade to derive redshift constraints for highly obscured galaxies that lack photometry…

2020 The Astrophysical Journal
Herschel 19
Accretion History of AGNs. II. Constraints on AGN Spectral Parameters Using the Cosmic X-Ray Background
DOI: 10.3847/1538-4357/ab5aef Bibcode: 2020ApJ...889...17A

Kirkpatrick, Allison; Marchesi, Stefano; Urry, C. Megan +5 more

We constrain X-ray spectral shapes for the ensemble of active galactic nuclei (AGNs) based on the shape of the cosmic X-ray background (CXB). Specifically, we rule out regions of X-ray spectral parameter space that do not reproduce the CXB in the energy range 1-100 keV. The key X-ray spectral parameters are the photon index, Γ; the cutoff energy, …

2020 The Astrophysical Journal
INTEGRAL 19
Is Superorbital Modulation in SMC X-1 Caused by Absorption in a Warped Precessing Accretion Disk?
DOI: 10.3847/1538-4357/ab8224 Bibcode: 2020ApJ...895...10P

Maitra, Chandreyee; Paul, Biswajit; Pradhan, Pragati

We present a broadband spectral-timing analysis of SMC X-1 at different intensity states of its superorbital variation using 10 Suzaku and 6 Nuclear Spectroscopic Telescope Array (NuSTAR) observations. The spectrum in all the states can be described by an absorbed power law with a high-energy cutoff and a blackbody component along with an iron emi…

2020 The Astrophysical Journal
Suzaku 18
The Flare-dominated Accretion Mode of a Radio-bright Candidate Transitional Millisecond Pulsar
DOI: 10.3847/1538-4357/ab8f28 Bibcode: 2020ApJ...895...89L

Strader, Jay; Chomiuk, Laura; Heinke, Craig O. +2 more

We report new simultaneous X-ray and radio continuum observations of 3FGL J0427.9-6704, a candidate member of the enigmatic class of transitional millisecond pulsars. These XMM-Newton and Australia Telescope Compact Array observations of this nearly edge-on, eclipsing low-mass X-ray binary were taken in the sub-luminous disk state at an X-ray lumi…

2020 The Astrophysical Journal
Gaia XMM-Newton 18
Surveying the Giant H II Regions of the Milky Way with SOFIA. II. M17
DOI: 10.3847/1538-4357/ab5fd0 Bibcode: 2020ApJ...888...98L

Lim, Wanggi; De Buizer, James M.; Radomski, James T.

We present our second set of results from our mid-infrared imaging survey of Milky Way giant H II regions. We used the FORCAST instrument on the Stratospheric Observatory For Infrared Astronomy (SOFIA) to obtain 20 and 37 µm images of the central ∼10' × 10' area of M17. We investigate the small- and large-scale properties of M17 using our da…

2020 The Astrophysical Journal
Herschel ISO 18