Search Publications

GROWTH on S190426c II: GROWTH-India Telescope search for an optical counterpart with a custom image reduction and candidate vetting pipeline
DOI: 10.1093/mnras/stac2516 Bibcode: 2022MNRAS.516.4517K

Kumar, Brajesh; De, Kishalay; Sharma, Yashvi +17 more

S190426c/GW190426_152155 was the first probable neutron star-black hole merger candidate detected by the LIGO-Virgo Collaboration. We undertook a tiled search for optical counterparts of this event using the 0.7-m GROWTH-India Telescope. Over a period of two weeks, we obtained multiple observations over a 22.1 deg2 area, with a 17.5 per…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 6
Discovery of quasi-periodic oscillations in the persistent X-ray emission of accreting binary X-ray pulsar LMC X-4
DOI: 10.1093/mnras/stac729 Bibcode: 2022MNRAS.512.4792R

Paul, Biswajit; Paul, K. T.; Rikame, Ketan +1 more

We report the discovery of quasi-periodic oscillations (QPOs) in the high-mass X-ray binary (HMXB) pulsar LMC X-4 in its non-flaring (persistent) state using observations with XMM-Newton. In addition to the 74 mHz coherent pulsations, the persistent emission light curve shows a QPO feature in the frequency range of 20-30 mHz. Quasi-periodic flares…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 6
Combining Rosetta's GIADA and MIDAS data: morphological versus dynamical properties of dust at 67P/Churyumov-Gerasimenko
DOI: 10.1093/mnras/stac2544 Bibcode: 2022MNRAS.516.5611L

Lasue, J.; Fulle, M.; Della Corte, V. +10 more

We related morphological (size/shape) and dynamical properties of the dust ejected from the 67P/Churyumov-Gerasimenko comet by combining data from two instruments onboard the ESA's Rosetta mission, i.e. the MIDAS atomic force microscope and the GIADA dust detector. The two instruments detected dust of different size (10-6-10-5

2022 Monthly Notices of the Royal Astronomical Society
Rosetta 6
Gravity Waves in Titan's Atmosphere: A Comparison Between Linearized Wave Model Calculations and HASI Observations
DOI: 10.1029/2022JE007310 Bibcode: 2022JGRE..12707310H

Cui, Jun; Huang, Jianping; Hao, Yongqiang +3 more

The Huygens Atmospheric Structure Instrument (HASI) detected wavelike temperature fluctuations from 500 to 1,000 km on Titan. However, these fluctuation structures have not been satisfactorily reproduced by any theoretical model to date. In this study, we construct a full-wave model to simulate the observed gravity wave structure. The model includ…

2022 Journal of Geophysical Research (Planets)
Huygens 6
Observation of a Flare and Filament Eruption in Lyman-α on 8 September 2011 by the PRoject for OnBoard Autonomy/Large Yield Radiometer (PROBA2/LYRA)
DOI: 10.1007/s11207-022-01963-0 Bibcode: 2022SoPh..297...36W

Kretzschmar, M.; Dammasch, I. E.; Dominique, M. +3 more

The Large Yield Radiometer (LYRA) instrument onboard the PRoject for OnBoard Autonomy (PROBA2) observes the solar irradiance in four channels in the UV-EUV. One of these channels is centered around the hydrogen line at 121.6 nm. The solar Lyman-α emission line is an optically thick line mostly formed in the chromosphere. Although it is one of the …

2022 Solar Physics
PROBA-2 SOHO 6
A survey for variable young stars with small telescopes - V. Analysis of TX Ori, V505 Ori, and V510 Ori, the HST ULLYSES targets in the σ Ori cluster
DOI: 10.1093/mnras/stab3450 Bibcode: 2022MNRAS.510.2883F

Eislöffel, Jochen; Hambsch, Franz-Josef; Froebrich, Dirk +2 more

Investigations of the formation of young stellar objects (YSOs) and planets require the detailed analysis of individual sources as well as statistical analysis of a larger number of objects. The Hubble UV Legacy Library of Young Stars as Essential Standards (ULLYSES) project provides such a unique opportunity by establishing a UV spectroscopic lib…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 6
Determination of Sodium Abundance Ratio from Low-resolution Stellar Spectra and Its Applications
DOI: 10.3847/1538-4357/ac3423 Bibcode: 2022ApJ...925...35K

Koo, Jae-Rim; Beers, Timothy C.; Lee, Young Sun +2 more

We present a method to determine sodium abundance ratios ([Na/Fe]) using the Na I D doublet lines in low-resolution (R ~ 2000) stellar spectra. As stellar Na I D lines are blended with those produced by the interstellar medium, we developed a technique for removing the interstellar Na I D lines using the relationship between extinction, which is p…

2022 The Astrophysical Journal
Gaia 6
Machine learning as a tool to classify extra-terrestrial landslides: A dossier from Valles Marineris, Mars
DOI: 10.1016/j.icarus.2022.114886 Bibcode: 2022Icar..37614886R

Rajaneesh, A.; Vishnu, C. L.; Oommen, T. +2 more

Many researchers studied Martian landslides, and most of these studies are in the Valles Marineris (VM). Those studies are mainly morphologic analysis, estimates of landslide deposit volumes, thermal properties of the landslides, spectral analyses, and mapping and classifying landslides. But, this study created a robust landslide inventory of 682 …

2022 Icarus
MEx 6
The SHARDDS survey: limits on planet occurrence rates based on point sources analysis via the Auto-RSM framework
DOI: 10.1051/0004-6361/202244145 Bibcode: 2022A&A...666A..33D

Marshall, J. P.; del Burgo, C.; Absil, O. +7 more

Context. In the past decade, high contrast imaging allowed the detection and characterisation of exoplanets, brown dwarfs, and circumstellar disks. Large surveys provided new insights about the frequency and properties of massive sub-stellar companions with separations from 5 to 300 au.
Aims: In this context, our study aims to detect and char…

2022 Astronomy and Astrophysics
Herschel 6
Quasi-stellar objects and galaxy mass density profiles derived using the submillimetre galaxies magnification bias
DOI: 10.1051/0004-6361/202244016 Bibcode: 2022A&A...667A.146C

Bonavera, L.; González-Nuevo, J.; Cueli, M. M. +3 more

Context. The magnification bias on the submillimetre galaxies (SMGs) is a gravitational lensing effect, where the SMGs are used as background lensed galaxies. This effect can be used to investigate the mass density profiles of different types of foreground lenses.
Aims: In this work, we want to exploit the magnification bias of the SMGs using…

2022 Astronomy and Astrophysics
Herschel 6