Search Publications

Solar-metallicity gas in the extended halo of a galaxy at z ∼ 0.12
DOI: 10.1093/mnras/staa184 Bibcode: 2020MNRAS.493..250P

Pradeep, Jayadev; Narayanan, Anand; Khaire, Vikram +4 more

We present the detection and analysis of a weak low-ionization absorber at z = 0.121 22 along the sightline of the blazar PG 1424+240, using spectroscopic data from both HST/COS and STIS. The absorber is a weak Mg II analogue, with an incidence of weak C II and Si II, along with multicomponent C IV and O VI. The low ions are tracing a dense (n

2020 Monthly Notices of the Royal Astronomical Society
eHST 4
Magnetic Flux Emergence in a Coronal Hole
DOI: 10.1007/s11207-020-01629-9 Bibcode: 2020SoPh..295...64P

Denker, Carsten; Temmer, Manuela; Veronig, Astrid +13 more

A joint campaign of various space-borne and ground-based observatories, comprising the Japanese Hinode mission (Hinode Observing Plan 338, 20 - 30 September 2017), the GREGOR solar telescope, and the Vacuum Tower Telescope (VTT), investigated numerous targets such as pores, sunspots, and coronal holes. In this study, we focus on the coronal hole r…

2020 Solar Physics
Hinode 4
Electromagnetic counterparts to gravitational wave events from Gaia
DOI: 10.1093/mnras/staa436 Bibcode: 2020MNRAS.493.3264K

Harrison, D. L.; Koposov, S. E.; Evans, D. W. +15 more

The recent discoveries of gravitational wave events and in one case also its electromagnetic (EM) counterpart allow us to study the Universe in a novel way. The increased sensitivity of the LIGO and Virgo detectors has opened the possibility for regular detections of EM transient events from mergers of stellar remnants. Gravitational wave sources …

2020 Monthly Notices of the Royal Astronomical Society
Gaia 4
A comparative analysis of denoising algorithms for extragalactic imaging surveys
DOI: 10.1051/0004-6361/201936278 Bibcode: 2020A&A...643A..43R

Castellano, M.; Merlin, E.; Fontana, A. +4 more


Aims: We present a comprehensive analysis of the performance of noise-reduction (denoising) algorithms to determine whether they provide advantages in source detection, mitigating noise on extragalactic survey images.
Methods: The methods we analyze here are representative of different algorithmic families: Perona-Malik filtering, bilate…

2020 Astronomy and Astrophysics
eHST 4
Characterizing continuum variability in the radio-loud narrow-line Seyfert 1 galaxy IRAS 17020+4544
DOI: 10.1093/mnras/staa1735 Bibcode: 2020MNRAS.496.3708G

Fabian, A. C.; Gallo, L. C.; Alston, W. N. +4 more

We present results of temporal and spectral analyses on four XMM-Newton EPIC pn observations of IRAS 17020+4544, a narrow-line Seyfert 1 galaxy with evidence of a radio jet. Analysis of the light curves reveals that this radio-loud source does not behave like the bulk population of its radio-quiet counterparts. A trend of spectral hardening with i…

2020 Monthly Notices of the Royal Astronomical Society
XMM-Newton 4
Shape model and spin state of non-principal axis rotator (5247) Krylov
DOI: 10.1051/0004-6361/201936808 Bibcode: 2020A&A...635A.137L

Duffard, R.; Marciniak, A.; Ďurech, J. +12 more

Context. The study of non-principal axis (NPA) rotators can provide important clues to the evolution of the spin state of asteroids. However, very few studies to date have focused on NPA-rotating main belt asteroids (MBAs). One MBA known to be in an excited rotation state is asteroid (5247) Krylov.
Aims: By using disk-integrated photometric d…

2020 Astronomy and Astrophysics
AKARI 4
Multiwavelength classification of X-ray selected galaxy cluster candidates using convolutional neural networks
DOI: 10.1093/mnras/staa1723 Bibcode: 2020MNRAS.496.4141K

Kendrew, Sarah; Valtchanov, Ivan; Werner, Norbert +15 more

Galaxy clusters appear as extended sources in XMM-Newton images, but not all extended sources are clusters. So, their proper classification requires visual inspection with optical images, which is a slow process with biases that are almost impossible to model. We tackle this problem with a novel approach, using convolutional neural networks (CNNs)…

2020 Monthly Notices of the Royal Astronomical Society
XMM-Newton 4
Fundamental parameters of Ap-star HD 108662
DOI: 10.26087/INASAN.2020.5.4.010 Bibcode: 2020INASR...5..219R

Romanovskaya, A. M.; Ryabchikova, T. A.; Shulyak, D. V.

We present the results of self-consistent spectroscopic analysis of the atmosphere of Ap-star HD 108662 based on high resolution spectrum and spectrophotometric observations in a wide wavelength range. Magnetic field effects were taking into account. Abundances of 24 chemical elements were derived, and stratification of Fe which lines make the mai…

2020 INASAN Science Reports
Gaia IUE 4
HD 93795: a late-B supergiant star with a square circumstellar nebula
DOI: 10.1093/mnras/stz3612 Bibcode: 2020MNRAS.492.2383G

Katkov, I. Y.; Gvaramadze, V. V.; Castro, N. +1 more

We report the discovery of a square axisymmetric circumstellar nebula around the emission-line star HD 93795 in the archival Spitzer Space Telescope 24 {µ m} data. We classify HD 93795 as a B9 Ia star using optical spectra obtained with the Southern African Large Telescope (SALT). A spectral analysis carried out with the stellar atmosphere c…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 4
Investigation of the coronal heating through phase relation of solar activity indexes
DOI: 10.1017/pasa.2019.43 Bibcode: 2020PASA...37....1L

Li, K. J.; Xu, J. C.; Yin, Z. Q. +2 more

The coronal heating problem is a long-standing perplexing issue. In this study, 13 solar activity indexes are used to investigate their phase relation with the sunspot number (SSN). Only three of them are found to statistically significantly lag the SSN (large-scale magnetic activity) by about one solar rotation period; the three indexes are total…

2020 Publications of the Astronomical Society of Australia
SOHO 4