Search Publications

Superorbital Modulation in the High-mass X-Ray Binary 4U 1538-52 and Possible Modulation in IGR J16393-4643
DOI: 10.3847/1538-4357/abc477 Bibcode: 2021ApJ...906...13C

Roche, Paul; Pottschmidt, Katja; Corbet, Robin H. D. +2 more

Hard X-ray observations with the Neil Gehrels Swift Observatory Burst Alert Telescope (BAT) reveal superorbital modulation in the wind-accreting supergiant high-mass X-ray binary (HMXB) 4U 1538-52 at a period of 14.9130 ± 0.0026 days that is consistent with four times the 3.73 day orbital period. These periods agree with a previously suggested cor…

2021 The Astrophysical Journal
INTEGRAL 6
Investigation and application of fitting models for centering algorithms in astrometry
DOI: 10.1007/s10509-021-03965-z Bibcode: 2021Ap&SS.366...59L

Lin, F. R.; Peng, Q. Y.; Zheng, Z. J. +2 more

To determine the precise positions of stars in CCD frames, various centering algorithms have been proposed for astrometry. The effective point spread function (ePSF) and the Gaussian centering algorithms are two representative centering algorithms. This paper compares in detail and investigates these two centering algorithms in performing data red…

2021 Astrophysics and Space Science
Gaia 6
NGTS and HST insights into the long-period modulation in GW Librae
DOI: 10.1093/mnras/staa4015 Bibcode: 2021MNRAS.502..581C

Reichart, D. E.; Hermes, J. J.; Gänsicke, B. T. +17 more

Light curves of the accreting white dwarf pulsator GW Librae spanning a 7.5-month period in 2017 were obtained as part of the Next-Generation Transit Survey. This data set comprises 787 h of photometry from 148 clear nights, allowing the behaviour of the long (hours) and short-period (20 min) modulation signals to be tracked from night to night ov…

2021 Monthly Notices of the Royal Astronomical Society
eHST 6
Ultraviolet Imaging Telescope (UVIT) observation of the Galactic globular cluster NGC 7492
DOI: 10.1093/mnras/staa4032 Bibcode: 2021MNRAS.502..313K

Pradhan, Ananta C.; Mohapatra, Abhisek; Parthasarathy, M. +4 more

We present detailed photometric observations of the Galactic globular cluster NGC 7492 using the data obtained with two far-ultraviolet (FUV; 1300-1800 Å) and three near-ultraviolet (NUV; 2000-3000 Å) filters of Ultraviolet Imaging Telescope (UVIT) onboard the AstroSat satellite. We confirmed the cluster membership of the extracted sources using G…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 6
Star cluster survival in dark matter haloes: an old cluster in Eridanus II?
DOI: 10.1093/mnras/stab1322 Bibcode: 2021MNRAS.505.2074A

Alzate, Jairo A.; Bruzual, Gustavo; Lomelí-Núñez, Luis +2 more

The star formation history and the internal dynamics of Milky Way satellite galaxies are often complicated. In the last years, a substantial fraction of the known faint dwarf satellites have been studied. Some of them show embedded stellar substructures, such as star clusters and even globular star clusters. In this work, we study Eridanus II, a d…

2021 Monthly Notices of the Royal Astronomical Society
eHST 6
Revisiting the Spectral Features of Ellerman Bombs and UV Bursts. I. Radiative Hydrodynamic Simulations
DOI: 10.3847/1538-4357/ac1ba0 Bibcode: 2021ApJ...921...50H

Ding, M. D.; Li, Ying; Hong, Jie +1 more

Ellerman bombs (EBs) and UV bursts are both small-scale solar activities that occur in active regions. They are now believed to form at different heights in the lower atmosphere. In this paper, we use one-dimensional radiative hydrodynamic simulations to calculate various line profiles in response to heating in different atmospheric layers. We con…

2021 The Astrophysical Journal
IRIS 6
Science Commissioning of NIHTS: The Near-infrared High Throughput Spectrograph on the Lowell Discovery Telescope
DOI: 10.1088/1538-3873/abe2f4 Bibcode: 2021PASP..133c5001G

Cushing, Michael C.; Gustafsson, Annika; Moskovitz, Nicholas +3 more

The Near-Infrared High Throughput Spectrograph (NIHTS) is in operation on the 4.3 m Lowell Discovery Telescope (LDT) in Happy Jack, AZ. NIHTS is a low-resolution spectrograph (R ∼ 200) that operates from 0.86 to 2.45 microns. NIHTS is fed by a custom dichroic mirror which reflects near-infrared wavelengths to the spectrograph and transmits the vis…

2021 Publications of the Astronomical Society of the Pacific
eHST 6
Exploring the pulsational properties of two ZZ Ceti stars
DOI: 10.1051/0004-6361/202140338 Bibcode: 2021A&A...651A..14B

Sódor, Á.; Kalup, Cs.; Bognár, Zs.

Context. We continued our ground-based observing project with the season-long observations of ZZ Ceti stars at the Konkoly Observatory. Our present targets are the newly discovered PM J22299+3024 and the already known LP 119-10 variables. LP 119-10 was also observed by the TESS space telescope in 120-second cadence mode.
Aims: Our main aims a…

2021 Astronomy and Astrophysics
Gaia 6
Effects of the chromospheric Lyα line profile shape on the determination of the solar wind H I outflow velocity using the Doppler dimming technique
DOI: 10.1051/0004-6361/202039821 Bibcode: 2021A&A...652A..85C

Sasso, C.; Romoli, M.; Andretta, V. +15 more

Context. The determination of solar wind H I outflow velocity is fundamental to shedding light on the mechanisms of wind acceleration occurring in the corona. Moreover, it has implications in various astrophysical contexts, such as in the heliosphere and in cometary and planetary atmospheres.
Aims: We aim to study the effects of the chromosph…

2021 Astronomy and Astrophysics
SOHO SolarOrbiter 6
Constraints on Optical Emission of FAST-detected FRB 20181130B with GWAC Synchronized Observations
DOI: 10.3847/1538-4357/ac1daf Bibcode: 2021ApJ...922...78X

Huang, L.; Wang, J.; Li, H. L. +17 more

Multiwavelength simultaneous observations are essential to the constraints on the origin of fast radio bursts (FRBs). However, it is a significant observational challenge due to the nature of FRBs as transients with a radio millisecond duration, which occur randomly in the sky regardless of time and position. Here, we report the search for short-t…

2021 The Astrophysical Journal
Gaia 6