activity
19962023
most citedA study of fundamental limitations to statistical detection of redshifted HI from the epoch of reionization

165 citations · 743 across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.HE2023

Rapid dimming followed by a state transition: a study of the highly variable nuclear transient AT 2019avd over 1000+ days

Yanan Wang, Dheeraj R. Pasham, Diego Altamirano +16

The tidal disruption of a star around a supermassive black hole (SMBH) offers a unique opportunity to study accretion onto a SMBH on a human-timescale. We present results from our…

astro-ph.HE2021★ 19 cited

NICER observations of the black hole candidate MAXI J0637430 during the 2019-2020 Outburst

Arghajit Jana, Gaurava K. Jaisawal, Sachindra Naik +5

We present detailed timing and spectral studies of the black hole candidate MAXI J0637430 during its 2019-2020 outburst using observations with the {\em Neutron Star Interior Co…

astro-ph.HE2020★ 39 cited

A NICER View of a Highly-Absorbed Flare in GRS 1915+105

J. Neilsen, J. Homan, J. F. Steiner +4

After 26 years in outburst, the black hole X-ray binary GRS 1915+105 dimmed considerably in early 2018; its flux dropped sharply in mid-2019, and it has remained faint ever since.…

astro-ph.HE2019★ 35 cited

The SUrvey for Pulsars and Extragalactic Radio Bursts IV: Discovery and polarimetry of a 12.1-second radio pulsar

V. Morello, E. F. Keane, T. Enoto +19

We report the discovery of PSR~J22513711, a radio pulsar with a spin period of 12.1 seconds, the second longest currently known. Its timing parameters imply a characteristic age…

astro-ph.HE2018★ 75 cited

A NICER Spectrum of MAXI J1535-571: Near-Maximal Black Hole Spin and Potential Disk Warping

J. M. Miller, K. Gendreau, R. M. Ludlam +10

We report on a NICER observation of the Galactic X-ray binary and stellar-mass black hole candidate, MAXI J1535-571. The source was likely observed in an "intermediate" or "very hi…

astro-ph.HE2018★ 18 cited

A Persistent Disk Wind in GRS 1915+105 with NICER

Joey Neilsen, E. Cackett, R. A. Remillard +13

The bright, erratic black hole X-ray binary GRS 1915+105 has long been a target for studies of disk instabilities, radio/infrared jets, and accretion disk winds, with implications…

astro-ph.IM2015★ 28 cited

A Digital-Receiver for the Murchison Widefield Array

Thiagaraj Prabu, K. S. Srivani, D. Anish Roshi +55

An FPGA-based digital-receiver has been developed for a low-frequency imaging radio interferometer, the Murchison Widefield Array (MWA). The MWA, located at the Murchison Radio-ast…

astro-ph.GA2013★ 67 cited

A survey for transients and variables with the Murchison Widefield Array 32-tile prototype at 154 MHz

M. E. Bell, T. Murphy, D. L. Kaplan +55

We present a search for transient and variable radio sources at 154 MHz with the Murchison Widefield Array 32-tile prototype. Fifty-one images were obtained that cover a field of v…

astro-ph.CO2013★ 165 cited

A study of fundamental limitations to statistical detection of redshifted HI from the epoch of reionization

Nithyanandan Thyagarajan, N. Udaya Shankar, Ravi Subrahmanyan +46

In this paper we explore for the first time the relative magnitudes of three fundamental sources of uncertainty, namely, foreground contamination, thermal noise and sample variance…

astro-ph.CO2013★ 27 cited

The giant lobes of Centaurus A observed at 118 MHz with the Murchison Widefield Array

B. McKinley, F. Briggs, B. M. Gaensler +50

We present new wide-field observations of Centaurus A (Cen A) and the surrounding region at 118 MHz with the Murchison Widefield Array (MWA) 32-tile prototype, with which we invest…

astro-ph.CO2012★ 41 cited

Low Frequency Observations of the Moon with the Murchison Widefield Array

B. McKinley, F. Briggs, D. L. Kaplan +49

A new generation of low frequency radio telescopes is seeking to observe the redshifted 21 cm signal from the Epoch of Reionization (EoR), requiring innovative methods of calibrati…

astro-ph.IM2012★ 70 cited

The EoR Sensitivity of the Murchison Widefield Array

A. P. Beardsley, B. J. Hazelton, M. F. Morales +48

Using the final 128 antenna locations of the Murchison Widefield Array (MWA), we calculate its sensitivity to the Epoch of Reionization (EoR) power spectrum of red- shifted 21 cm e…

astro-ph.IM2012★ 29 cited

A new layout optimization technique for interferometric arrays, applied to the MWA

A. P. Beardsley, B. J. Hazelton, M. F. Morales +46

Antenna layout is an important design consideration for radio interferometers because it determines the quality of the snapshot point spread function (PSF, or array beam). This is…

astro-ph2004★ 45 cited

X1908+075: A Pulsar Orbiting in the Stellar Wind of a Massive Companion

A. M. Levine, S. Rappaport, R. Remillard +1

We have observed the persistent but optically unidentified X-ray source X1908+075 with the PCA and HEXTE instruments on RXTE. The binary nature of this source was established by We…

astro-ph2000★ 46 cited

Faint Infrared Flares from the Microquasar GRS 1915+105

S. Eikenberry, K. Matthews, M. Muno +3

We present simultaneous infrared and X-ray observations of the Galactic microquasar GRS 1915+105 using the Palomar 5-m telescope and Rossi X-ray Timing Explorer on July 10, 1998 UT…

astro-ph1997★ 25 cited

Rxte Observations of a New X-Ray Transient: GRS 1737-31

Wei Cui, W. A. Heindl, J. H. Swank +4

We present the results from RXTE observations of a new X-ray transient, GRS 1737-31, near the Galactic center during an outburst. Over a span of two weeks, the source was seen to v…

astro-ph1996★ 14 cited

Anticorrelated Hard/Soft X-Ray Emission from the X-Ray Burster 4U 0614+091

E. Ford, P. Kaaret, M. Tavani +6

We have detected transient X-ray activity from the X-ray burster 4U~0614+091 simultaneously with BATSE/CGRO (20-100 keV) and ASM/RXTE (1-12 keV). The peak fluxes reach approximatel…