Search Publications

Measuring the Hubble constant and spatial curvature from supernova apparent magnitude, baryon acoustic oscillation, and Hubble parameter data
DOI: 10.1007/s10509-019-3627-8 Bibcode: 2019Ap&SS.364..134P

Park, Chan-Gyung; Ratra, Bharat

Cosmic microwave background (CMB) anisotropy (spatial inhomogeneity) data provide the tightest constraints on the Hubble constant, matter density, spatial curvature, and dark energy dynamics. Other data, sensitive to the evolution of only the spatially homogeneous part of the cosmological model, such as Type Ia supernova apparent magnitude, baryon…

2019 Astrophysics and Space Science
eHST 86
Observational constraints on the tilted flat-XCDM and the untilted nonflat XCDM dynamical dark energy inflation parameterizations
DOI: 10.1007/s10509-019-3567-3 Bibcode: 2019Ap&SS.364...82P

Park, Chan-Gyung; Ratra, Bharat

We constrain tilted spatially-flat and untilted nonflat XCDM dynamical dark energy inflation parameterizations using Planck 2015 cosmic microwave background (CMB) anisotropy data and recent baryonic acoustic oscillations distance measurements, Type Ia supernovae data, Hubble parameter observations, and growth rate measurements. Inclusion of the fo…

2019 Astrophysics and Space Science
eHST 86
CCD UBV photometric and Gaia astrometric study of eight open clusters—ASCC 115, Collinder 421, NGC 6793, NGC 7031, NGC 7039, NGC 7086, Roslund 1 and Stock 21
DOI: 10.1007/s10509-019-3640-y Bibcode: 2019Ap&SS.364..152Y

Paunzen, E.; Güver, T.; Bilir, S. +8 more

In this study, we carried out CCD UBV photometry of eight open clusters, ASCC 115, Collinder 421, NGC 6793, NGC 7031, NGC 7039, NGC 7086, Roslund 1, Stock 21, and determined their reddening, metallicity, distance, age, and mass functions. We used new Gaia Data Release 2 (DR2) astrometric data to separate cluster member stars from the field stars a…

2019 Astrophysics and Space Science
Gaia 21
Radio emission from interstellar shocks: Young type Ia supernova remnants and the case of N 103B in the Large Magellanic Cloud
DOI: 10.1007/s10509-019-3696-8 Bibcode: 2019Ap&SS.364..204A

Haberl, F.; Filipović, M. D.; Rowell, G. +19 more

We investigate young type Ia supernova remnants (SNRs) in our Galaxy and neighbouring galaxies in order to understand their properties and early stage of their evolution. Here we present a radio continuum study based on new and archival data from the Australia Telescope Compact Array (ATCA) towards N 103B, a young (≤1000 yrs) spectroscopically con…

2019 Astrophysics and Space Science
eHST 14
A young multipolar planetary nebula in the making—IRAS 21282+5050
DOI: 10.1007/s10509-019-3523-2 Bibcode: 2019Ap&SS.364...32H

Zhang, Yong; Kwok, Sun; Hsia, Chih-Hao +1 more

We present high-angular-resolution Hubble Space Telescope (HST) optical and near-infrared imaging of the compact planetary nebula (PN) IRAS 21282+5050. Optical images of this object reveal several complex morphological structures including three pairs of bipolar lobes and an elliptical shell lying close to the plane of the sky. From near-infrared …

2019 Astrophysics and Space Science
AKARI Gaia ISO eHST 10
Implication of kinetic Alfvén waves to magnetic field turbulence spectra: Earth's magnetosheath
DOI: 10.1007/s10509-019-3592-2 Bibcode: 2019Ap&SS.364..101D

Khodachenko, M. L.; Kumar, S.; Echim, M. +5 more

In the present paper, we investigate the power-law behaviour of the magnetic field spectra in the Earth's magnetosheath region using Cluster spacecraft data under solar minimum condition. The power spectral density of the magnetic field data and spectral slopes at various frequencies are analysed. Propagation angle,

2019 Astrophysics and Space Science
Cluster 9
The analysis of effective galaxies number count for Chinese Space Station Optical Survey (CSS-OS) by image simulation
DOI: 10.1007/s10509-019-3501-8 Bibcode: 2019Ap&SS.364....9Z

Zhang, Xin; Meng, Xianmin; Cao, Li

The Chinese Space Station Optical Survey (CSS-OS) is a mission to explore the vast universe. This mission will equip a 2-meter space telescope to perform a multi-band NUV-optical large area survey (over 40% of the sky) and deep survey (

2019 Astrophysics and Space Science
eHST 8
Optical spectroscopic classification of 35 hard X-ray sources from the Swift-BAT 70-month catalogue
DOI: 10.1007/s10509-019-3642-9 Bibcode: 2019Ap&SS.364..153M

Palazzi, E.; Minniti, D.; Masetti, N. +15 more

The nature of a substantial percentage (about one fifth) of hard X-ray sources discovered with the BAT instrument onboard the Neil Gehrels Swift Observatory (hereafter Swift) is unknown because of the lack of an identified longer-wavelength counterpart. Without such follow-up, an X-ray catalogue is of limited astrophysical value: we therefore emba…

2019 Astrophysics and Space Science
XMM-Newton 7
Metallicity and absolute magnitude calibrations for F-G type main-sequence stars in the Gaia era
DOI: 10.1007/s10509-019-3659-0 Bibcode: 2019Ap&SS.364..172C

Bilir, S.; Ak, T.; Yontan, T. +3 more

In this study, photometric metallicity and absolute magnitude calibrations were derived using F-G spectral type main-sequence stars in the Solar neighbourhood with precise spectroscopic, photometric and Gaia astrometric data for UBV photometry. The sample consists of 504 main-sequence stars covering the temperature, surface gravity and colour inde…

2019 Astrophysics and Space Science
Gaia 4
Prospect for UV observations from the Moon. III. Assembly and ground calibration of Lunar Ultraviolet Cosmic Imager (LUCI)
DOI: 10.1007/s10509-019-3538-8 Bibcode: 2019Ap&SS.364...53M

Brosch, Noah; Mathew, Joice; Sreejith, A. G. +14 more

The Lunar Ultraviolet Cosmic Imager (LUCI) is a near-ultraviolet (NUV) telescope with all-spherical mirrors, designed and built to fly as a scientific payload on a lunar mission with Team Indus—the original Indian entry to the Google Lunar X-Prize. Observations from the Moon provide a unique opportunity of a stable platform with an unobstructed vi…

2019 Astrophysics and Space Science
IUE 3