output
19912026
most citedSciPy 1.0--Fundamental Algorithms for Scientific Computing in Python

40.2k citations

Showing 2020 · astro-ph.HEShow all

60 papers · 2 filters

astro-ph.HE2020★ 6 cited

Detection of X-ray pulsations at the lowest observed luminosity of Be/X-ray binary pulsar EXO 2030+375 with AstroSat

Gaurava K. Jaisawal, Sachindra Naik, Shivangi Gupta +4

We present the results obtained from timing and spectral studies of Be/X-ray binary pulsar EXO 2030+375 using observations with the Large Area Xenon Proportional Counters and Soft…

astro-ph.HE2020★ 3 cited

Broadband Modelling of Orphan Gamma Ray Flares

S. R. Patel, D. Bose, N. Gupta +1

Blazars, a class of highly variable active galactic nuclei, sometimes exhibit Orphan -ray flares. These flares having high flux only in -ray energies do not show significant…

astro-ph.HE2020★ 20 cited

Double-peaked Lines, Dual VLBI Components, and Precessing Jets in J1328+2751

S. Nandi, A. Caproni, P. Kharb +2

In this work, we report a radio galaxy with precessing jets, double-peaked emission lines and the presence of two compact radio components with a projected separation of ~6 parsec…

astro-ph.HE2020★ 1 cited

Observations of bright stars with AstroSat Soft X-ray Telescope

K. P. Singh, G. Stewart, S. Chandra +5

We present observations of four bright stars observed with the AstroSat Soft X-ray Telescope (SXT). Visible light from bright stars like these can leak through the very thin filter…

astro-ph.HE2020★ 51 cited

Diving below the spin-down limit: Constraints on gravitational waves from the energetic young pulsar PSR J0537-6910

The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1589

We present a search for continuous gravitational-wave signals from the young, energetic X-ray pulsar PSR J0537-6910 using data from the second and third observing runs of LIGO and…

astro-ph.HE2020★ 180 cited

LOFAR Detection of 110-188 MHz Emission and Frequency-Dependent Activity from FRB 20180916B

Z. Pleunis, D. Michilli, C. G. Bassa +32

FRB 20180916B is a well-studied repeating fast radio burst source. Its proximity (~150 Mpc), along with detailed studies of the bursts, have revealed many clues about its nature --…

astro-ph.HE2020★ 45 cited

Fast Optical Transients from Stellar-Mass Black Hole Tidal Disruption Events in Young Star Clusters

Kyle Kremer, Wenbin Lu, Anthony L. Piro +3

Observational evidence suggests that the majority of stars may have been born in stellar clusters or associations. Within these dense environments, dynamical interactions lead to h…

astro-ph.HE2020★ 34 cited

First discovery of new pulsars and RRATs with CHIME/FRB

D. C. Good, B. C. Andersen, P. Chawla +20

We report the discovery of seven new Galactic pulsars with the Canadian Hydrogen Intensity Mapping Experiment's Fast Radio Burst backend (CHIME/FRB). These sources were first ident…

astro-ph.HE2020★ 17 cited

AstroSat view of IGR J17091-3624 and GRS 1915+105: decoding the 'pulse' in the 'Heartbeat State'

Tilak Katoch, Blessy E. Baby, Anuj Nandi +3

IGR J17091--3624 is a transient galactic black hole which has a distinct quasi-periodic variability known as `heartbeat', similar to the one observed in GRS 1915+105. In this paper…

astro-ph.HE2020★ 31 cited

Mode changing, subpulse drifting and nulling in four component conal pulsar PSR J2321+6024

Sk. Minhajur Rahaman, Rahul Basu, Dipanjan Mitra +1

In this study, we report on a detailed single pulse polarimetric analysis of the radio emission from the pulsar J2321+6024 (B2319+60) observed with the Giant Metrewave Radio Telesc…

astro-ph.HE2020★ 7 cited

Radio counterparts of gamma-ray sources in the Cygnus region

Paula Benaglia, C. H. Ishwara-Chandra, Josep M. Paredes +3

The view of the gamma-ray universe is being continuously expanded by space high energy (HE) and ground based very-high energy (VHE) observatories. Yet, the angular resolution limit…

astro-ph.HE2020★ 12 cited

The Search for Fast Transients with CZTI

Y. Sharma, A. Marathe, V. Bhalerao +9

The Cadmium Zinc Telluride Imager on AstroSat has proven to be a very effective all-sky monitor in the hard X-ray regime, detecting over three hundred GRBs and putting highly compe…

astro-ph.HE2020★ 94 cited

The 60 pc Environment of FRB 20180916B

Shriharsh P. Tendulkar, Armando Gil de Paz, Aida Yu. Kirichenko +18

Fast Radio Burst FRB 20180916B in its host galaxy SDSS J015800.28+654253.0 at 149 Mpc is by far the closest-known FRB with a robust host galaxy association. The source also exhibit…

astro-ph.HE2020

Constraining millisecond pulsar geometry using time-aligned radio and gamma-ray pulse profile

O. Benli, J. Petri, Dipanjan Mitra

Since the launch of the Fermi Gamma-Ray Space Telescope, several hundred gamma-ray pulsars have been discovered, some being radio-loud and some radio-quiet with time-aligned radio…

astro-ph.HE2020★ 70 cited

Discovery of a Gamma-ray Black Widow Pulsar by GPU-accelerated Einstein@Home

L. Nieder, C. J. Clark, D. Kandel +39

We report the discovery of 1.97 ms period gamma-ray pulsations from the 75 minute orbital-period binary pulsar now named PSR J1653-0158. The associated Fermi Large Area Telescope g…

astro-ph.HE2020★ 2 cited

Search for Off-pulse emission in Long Period Pulsars

Rahul Basu, Dipanjan Mitra, George I. Melikidze

We have revisited the problem of off-pulse emission in pulsars, where detailed search for the presence of low level radio emission outside the pulse window is carried out. The pres…

astro-ph.HE2020★ 26 cited

AstroSat Observations of the first Galactic ULX Pulsar Swift J0243.6+6124

Aru Beri, Sachindra Naik, K. P Singh +11

SwiftJ0243.6+6124, the first Galactic ultra-luminous X-ray pulsar, was observed during its 2017-2018 outburst with \emph{AstroSat} at both sub- and super-Eddington levels of accret…

astro-ph.HE2020★ 41 cited

Multi-waveband quasi-periodic oscillations in the light curves of blazar CTA 102 during its 2016-2017 optical outburst

Arkadipta Sarkar, Pankaj Kushwaha, Alok C. Gupta +2

Quasi-periodic fluctuations in the light curves of blazars can provide insight into the underlying emission process. This type of flux modulation hints at periodic physical process…

astro-ph.HE2020★ 51 cited

AstroSat view of GRS 1915+105 during the Soft State: Detection of HFQPOs and estimation of Mass and Spin

Sreehari H., Anuj Nandi, Santabrata Das +4

We report the results of AstroSat observations of GRS 1915105 obtained using 100 ks guaranteed-time (GT) during the soft state. The Color-Color Diagram (CCD) indicates a variabi…

astro-ph.HE2020★ 39 cited

Search for Gravitational Waves Associated with Gamma-Ray Bursts Detected by Fermi and Swift During the LIGO-Virgo Run O3a

The LIGO Scientific Collaboration, the Virgo Collaboration, R. Abbott +1250

We search for gravitational-wave transients associated with gamma-ray bursts detected by the Fermi and Swift satellites during the first part of the third observing run of Advanced…

astro-ph.HE2020★ 10 cited

Population Properties of Compact Objects from the Second LIGO-Virgo Gravitational-Wave Transient Catalog

The LIGO Scientific Collaboration, the Virgo Collaboration, R. Abbott +1338

We report on the population of the 47 compact binary mergers detected with a false-alarm rate 1/yr in the second LIGO--Virgo Gravitational-Wave Transient Catalog, GWTC-2. We observ…

astro-ph.HE2020★ 14 cited

Improved early warning of compact binary mergers using higher modes of gravitational radiation: A population study

Mukesh Kumar Singh, Shasvath J. Kapadia, Md Arif Shaikh +2

A gravitational-wave (GW) early-warning of a compact-binary coalescence event, with a sufficiently tight localisation skymap, would allow telescopes to point in the direction of th…

astro-ph.HE2020★ 9 cited

Scintillation of PSR B1508+55 -- the view from a 10,000-km baseline

V. R. Marthi, D. Simard, R. A. Main +6

We report on the simultaneous Giant Metrewave Radio Telescope (GMRT) and Algonquin Radio Observatory (ARO) observations at 550-750 MHz of the scintillation of PSR B1508+55, resulti…

astro-ph.HE2020★ 38 cited

A Possible -ray Quasi-periodic Oscillation of 314 days in the Blazar OJ 287

Pankaj Kushwaha, Arkadipta Sarkar, Alok C. Gupta +3

We report the detection of a probable -ray quasi-periodic oscillation (QPO) of around 314 days in the monthly binned 0.1 -- 300 GeV -ray {\it Fermi}-LAT light curve of the we…