output
20112026
most citedEstimating the sample mean and standard deviation from commonly reported quantiles in meta-analysis

932 citations

Showing astro-ph.HEShow all

8 papers · 1 filter

astro-ph.HE2025

ELAIS-N1 deep field uGMRT Band-2: constraints on diffuse Galactic synchrotron emission power spectrum

Rashmi Sagar, Abhirup Datta, Arnab Chakraborty +13

We present high sensitivity, low radio frequency continuum observations of the ELAIS-N1 field with 32 hours of observations of the uGMRT Band-2 ( MHz) covering $5.86\,\tex…

astro-ph.HE2024★ 4 cited

Hydrodynamical simulations of proton ingestion flashes in Type I X-ray Bursts

Simon Guichandut, Michael Zingale, Andrew Cumming

We perform the first multidimensional fluid simulations of thermonuclear helium ignition underneath a hydrogen-rich shell. This situation is relevant to Type I X-ray bursts on neut…

astro-ph.HE2023★ 7 cited

The imprint of convection on Type I X-ray bursts: Pauses in photospheric radius expansion lightcurves

Simon Guichandut, Andrew Cumming

Motivated by the recent observation by NICER of a type I X-ray burst from SAX J1808.4-3658 with a distinct "pause" feature during its rise (Bult et al. 2019), we show that bursts w…

astro-ph.HE2022★ 11 cited

Fast neutrino cooling in the accreting neutron star MXB 1659-29

Melissa Mendes, Farrukh J. Fattoyev, Andrew Cumming +1

Modelling of crust heating and cooling across multiple accretion outbursts of the low mass X-ray binary MXB 1659-29 indicates that the neutrino luminosity of the neutron star core…

astro-ph.HE2021★ 13 cited

Expanded atmospheres and winds in Type I X-ray bursts from accreting neutron stars

Simon Guichandut, Andrew Cumming, Maurizio Falanga +2

We calculate steady-state models of radiation-driven super-Eddington winds and static expanded envelopes of neutron stars caused by high luminosities in type I X-ray bursts. We use…

astro-ph.HE2016★ 21 cited

Swift observations of two outbursts from the magnetar 4U 0142+61

R. F. Archibald, V. M. Kaspi, P. Scholz +3

4U 0142+61 is one of a small class of persistently bright magnetars. Here we report on a monitoring campaign of 4U 0142+61 from 2011 July 26 - 2016 June 12 using the Swift X-ray Te…

astro-ph.HE2016★ 105 cited

A Magnetar-like Outburst from a High-B Radio Pulsar

R. F. Archibald, V. M. Kaspi, S. P. Tendulkar +1

Radio pulsars are believed to have their emission powered by the loss of rotational kinetic energy. By contrast, magnetars show intense X-ray and gamma-ray radiation whose luminosi…

astro-ph.HE2015

The link between coherent burst oscillations, burst spectral evolution and accretion state in 4U 1728-34

Guobao Zhang, Mariano Mendez, Michael Zamfir +1

Coherent oscillations and the evolution of the X-ray spectrum during thermonuclear X-ray bursts in accreting neutron-star X-ray binaries have been studied intensively but separatel…