Search Publications

The Sizes of z ∼ 9-10 Galaxies Identified in the Brightest of Reionizing Galaxies (BoRG) Survey
DOI: 10.3847/1538-3881/aba617 Bibcode: 2020AJ....160..154H

Holwerda, Benne W.; Bradley, Larry; Livermore, Rachael +5 more

Redshift z = 9-10 object selection is the effective limit of Hubble Space Telescope (HST) imaging capability, even when confirmed with Spitzer. If only a few photometry data points are available, it becomes attractive to add criteria based on their morphology in these J- and H-band images. One could do so through visual inspection, a size criterio…

2020 The Astronomical Journal
eHST 12
Using the "Ghost Front" to Predict the Arrival Time and Speed of CMEs at Venus and Earth
DOI: 10.3847/1538-4357/aba95a Bibcode: 2020ApJ...899..143C

Wang, Yuming; Shen, Chenglong; Lockwood, Mike +7 more

Using in situ measurements and remote-sensing observations, we study two coronal mass ejections (CMEs) that left the Sun on 2012 June 13-14 and impacted both Venus and Earth while the planets were in close radial alignment. The two CMEs generate multiple fronts in Solar Terrestrial Relations Observatory (STEREO)/Heliospheric Imager (HI) images, wh…

2020 The Astrophysical Journal
SOHO VenusExpress 12
Isochrone fitting of Galactic globular clusters - II. NGC 6205 (M13)
DOI: 10.1093/mnras/staa1694 Bibcode: 2020MNRAS.497.3674G

Gontcharov, George A.; Mosenkov, Aleksandr V.; Khovritchev, Maxim Yu

We present new isochrone fits to colour-magnitude diagrams of the Galactic globular cluster NGC 6205 (M13). We utilize 34 photometric bands from the ultraviolet to mid-infrared by use of data from the HST, Gaia DR2, SDSS, unWISE, Pan-STARRS DR1, and other photometric sources. In our isochrone fitting we use the PARSEC, MIST, DSEP, BaSTI, and IAC-B…

2020 Monthly Notices of the Royal Astronomical Society
Gaia eHST 12
Star Formation and Evolution of Blister-type H II Region Sh2-112
DOI: 10.3847/1538-4357/abc42e Bibcode: 2020ApJ...905...61P

Bhatt, B. C.; Dewangan, L. K.; Ojha, D. K. +4 more

We report the observational findings of the Sh2-112 H II region by using the multiwavelength data analysis ranging from optical to radio wavelengths. This region is powered by the massive O8V-type star BD +45 3216. The surface density distribution and minimum spanning tree analyses of the young stellar object (YSO) candidates in the region reveal …

2020 The Astrophysical Journal
AKARI Gaia 12
Cross-correlation of Far-infrared Background Anisotropies and CMB Lensing from Herschel and Planck Satellites
DOI: 10.3847/1538-4357/abada1 Bibcode: 2020ApJ...901...34C

Gong, Yan; Cooray, Asantha; Chen, Xuelei +3 more

The cosmic infrared background (CIB) anisotropies and cosmic microwave background (CMB) lensing are powerful measurements for exploring cosmological and astrophysical problems. In this work, we measure the autocorrelation power spectrum of the CIB anisotropies in the Herschel-SPIRE HerMES Large Mode Survey (HeLMS) field, and the cross-power spectr…

2020 The Astrophysical Journal
Herschel 12
Spectroscopy of hot γ Doradus and A-F hybrid Kepler candidates close to the hot border of the δ Scuti instability strip
DOI: 10.1093/mnras/staa399 Bibcode: 2020MNRAS.493.4518K

Handler, G.; Poretti, E.; Rainer, M. +4 more

If γ Dor-type pulsations are driven by the convective blocking mechanism, a convective envelope at a sufficient depth is essential. There are several hot γ Dor and hybrid star candidates in which there should not be an adequate convective envelope to excite the γ Dor-type oscillations. The existence of these hot objects needs an explanation. There…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 12
Artificial Intelligence-Assisted Inversion (AIAI) of Synthetic Type Ia Supernova Spectra
DOI: 10.3847/1538-4365/ab9a3b Bibcode: 2020ApJS..250...12C

Wang, Lifan; Hu, Lei; Chen, Xingzhuo

We generate ∼100,000 model spectra of Type 1a supernovae (SNe Ia) to form a spectral library for the purpose of building an artificial intelligence-assisted inversion (AIAI) algorithm for theoretical models. As a first attempt, we restrict our studies to the time around B-band maximum and compute theoretical spectra with a broad spectral wavelengt…

2020 The Astrophysical Journal Supplement Series
eHST 12
Identifying new X-ray binary candidates in M31 using random forest classification
DOI: 10.1093/mnras/staa207 Bibcode: 2020MNRAS.492.5075A

Barmby, P.; Vulic, N.; Arnason, R. M.

Identifying X-ray binary (XRB) candidates in nearby galaxies requires distinguishing them from possible contaminants including foreground stars and background active galactic nuclei. This work investigates the use of supervised machine learning algorithms to identify high-probability XRB candidates. Using a catalogue of 943 Chandra X-ray sources i…

2020 Monthly Notices of the Royal Astronomical Society
eHST 12
A deep Chandra survey for faint X-ray sources in the Galactic globular cluster M30, and searches for optical and radio counterparts
DOI: 10.1093/mnras/staa2927 Bibcode: 2020MNRAS.499.3338Z

Strader, Jay; Bahramian, Arash; Maccarone, Thomas J. +11 more

We present a deep (~330 ks) Chandra survey of the Galactic globular cluster M30 (NGC 7099). Combining the new Cycle 18 with the previous Cycle 3 observations we report a total of 10 new X-ray point sources within the 1${_{.}^{\prime}}$03 half-light radius, compiling an extended X-ray catalogue of a total of 23 sources. We incorporate imaging obser…

2020 Monthly Notices of the Royal Astronomical Society
Gaia eHST 12
The assembly history of the nearest S0 galaxy NGC 3115 from its kinematics out to six half-light radii
DOI: 10.1093/mnras/staa1080 Bibcode: 2020MNRAS.495.1321D

Forbes, Duncan A.; Romanowsky, Aaron J.; Brodie, Jean P. +6 more

Using new and archival data, we study the kinematic properties of the nearest field S0 galaxy, NGC 3115, out to ∼6.5 half-light radii (Re) from its stars (integrated starlight), globular clusters (GCs), and planetary nebulae (PNe). We find evidence of three kinematic regions with an inner transition at ∼0.2 Re from a dispersi…

2020 Monthly Notices of the Royal Astronomical Society
eHST 12