Search Publications

Superresolution Reconstruction of Severely Undersampled Point-spread Functions Using Point-source Stacking and Deconvolution
DOI: 10.3847/1538-4365/abcaa5 Bibcode: 2021ApJS..252...24S

Zemcov, Michael; Symons, Teresa; Bock, James +4 more

Point-spread function (PSF) estimation in spatially undersampled images is challenging because large pixels average fine-scale spatial information. This is problematic when fine-resolution details are necessary, as in optimal photometry where knowledge of the illumination pattern beyond the native spatial resolution of the image may be required. H…

2021 The Astrophysical Journal Supplement Series
Gaia 11
High-redshift Narrow-line Seyfert 1 Galaxies: A Candidate Sample
DOI: 10.3847/1538-4365/abd9bb Bibcode: 2021ApJS..253...28R

Stalin, C. S.; Rakshit, Suvendu; Shin, Jaejin +1 more

The study of narrow-line Seyfert 1 galaxies (NLS1s) is now mostly limited to low redshift (z < 0.8) because their definition requires the presence of the Hβ emission line, which is redshifted out of the spectral coverage of major ground-based spectroscopic surveys at z > 0.8. We studied the correlation between the properties of Hβ and Mg II …

2021 The Astrophysical Journal Supplement Series
XMM-Newton 11
WawHelioGlow: A Model of the Heliospheric Backscatter Glow. II. The Helioglow Buildup and the Potential Significance of the Anisotropy in the Solar EUV Output
DOI: 10.3847/1538-4365/abeb78 Bibcode: 2021ApJS..254...17K

Bzowski, M.; Kubiak, M. A.; Kowalska-Leszczynska, I. +1 more

The helioglow is the fluorescence of interstellar atoms inside the heliosphere, where they are excited by the solar EUV. Because the mean free path between collisions for interstellar gas is comparable to the size of the heliosphere, the distribution function of this gas inside the heliosphere strongly varies in space and with time and is non-Maxw…

2021 The Astrophysical Journal Supplement Series
SOHO 11
TIMES. I. A Systematic Observation in Multiple Molecular Lines toward the Orion A and Ophiuchus Clouds
DOI: 10.3847/1538-4365/ac090e Bibcode: 2021ApJS..256...16Y

Cho, Jungyeon; Choi, Minho; Choi, Yunhee +16 more

We have used the Taeduk Radio Astronomy Observatory to observe the Orion A and Ophiuchus clouds in the J = 1-0 lines of 13CO, C18O, HCN, HCO+, and N2H+ and the J = 2-1 line of CS. The fully sampled maps with uniform noise levels are used to create moment maps. The variations of the line intens…

2021 The Astrophysical Journal Supplement Series
Herschel 10
Chromospheric Activity of Periodic Variable Stars Based on the LAMOST Low- and Medium-resolution Spectral Survey
DOI: 10.3847/1538-4365/abe30b Bibcode: 2021ApJS..253...51L

Shi, Jianrong; Han, Xianming L.; Zhang, Li-yun +5 more

We present a catalog of 75,867 periodic variable stars from data release 7 of the Large Sky Area Multi-Object Fiber Spectroscopic Telescope. We calculated the chromospheric activity index, equivalent widths for 201,349 spectra, and excess fractional luminosity ( ${R}_{{\rm{H}}\alpha }^{{\prime} }$ ) for 130,796 spectra. Based on the intensity of t…

2021 The Astrophysical Journal Supplement Series
Gaia 10
Hubble Frontier Field Clusters and Their Parallel Fields: Photometric and Photometric Redshift Catalogs
DOI: 10.3847/1538-4365/abea9d Bibcode: 2021ApJS..256...27P

Mobasher, Bahram; Davidzon, I.; Sánchez, F. J. +1 more

We present a multiband analysis of the six Hubble Frontier Field clusters and their parallel fields, producing catalogs with measurements of source photometry and photometric redshifts. We release these catalogs to the public along with maps of intracluster light and models for the brightest galaxies in each field. This rich data set covers a wave…

2021 The Astrophysical Journal Supplement Series
eHST 10
Improved Atomic Transition Probabilities for UV and Optical Lines of Hf II and Determination of the Hf Abundance in Two Metal-poor Stars
DOI: 10.3847/1538-4365/abe861 Bibcode: 2021ApJS..254....5D

Roederer, I. U.; Lawler, J. E.; Den Hartog, E. A.

We report new branching fraction measurements for 199 UV and optical transitions of Hf II. These transitions range in wavelength (wavenumber) from 2068 to 6584 Å (48,322-15,183 cm-1) and originate in 17 odd-parity upper levels ranging in energy from 38,578 to 53,227 cm-1. The branching fractions are combined with radiative li…

2021 The Astrophysical Journal Supplement Series
eHST 10
The HASHTAG Project: The First Submillimeter Images of the Andromeda Galaxy from the Ground
DOI: 10.3847/1538-4365/ac23d0 Bibcode: 2021ApJS..257...52S

Ho, Luis C.; Lee, Chien-Hsiu; Clark, Christopher J. R. +46 more

Observing nearby galaxies with submillimeter telescopes on the ground has two major challenges. First, the brightness is significantly reduced at long submillimeter wavelengths compared to the brightness at the peak of the dust emission. Second, it is necessary to use a high-pass spatial filter to remove atmospheric noise on large angular scales, …

2021 The Astrophysical Journal Supplement Series
Herschel 8
X-Ray-to-radio Offset Inference from Low-count X-Ray Jets
DOI: 10.3847/1538-4365/abd8d7 Bibcode: 2021ApJS..253...37R

Georganopoulos, Markos; Meyer, Eileen T.; Reddy, Karthik

Observations of positional offsets between the location of X-ray and radio features in many resolved, extragalactic jets indicates that the emitting regions are not cospatial, an important piece of evidence in the debate over the origin of the X-ray emission on kiloparsec scales. The existing literature is nearly exclusively focused on jets with s…

2021 The Astrophysical Journal Supplement Series
eHST 8
Background Short-period Eclipsing Binaries in the Original Kepler Field
DOI: 10.3847/1538-4365/ac10c0 Bibcode: 2021ApJS..256...11B

Bódi, Attila; Szabó, Róbert; Forró, Adrienn +2 more

During the primary Kepler mission, between 2009 and 2013, about 150,000 preselected targets were observed with a 29.42 minute long cadence. However, a survey of background stars that fall within the field of view (FOV) of the downloaded apertures of the primary targets has revealed a number of interesting objects. In this paper, we present the res…

2021 The Astrophysical Journal Supplement Series
Gaia 8