activity
20092020
most citedBroad relativistic iron emission line observed in SAX J1808.4-3658

137 citations · 360 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.HE202025 cited

A Full Characterisation of the Supermassive Black Hole in IRAS 09149-6206

D. J. Walton, W. N. Alston, P. Kosec +11

We present new broadband X-ray observations of the type-I Seyfert galaxy IRAS 09149-6206, taken in 2018 with -, and . The source is highly complex, sho…

astro-ph.SR201922 cited

Using Multiwavelength Variability to Explore the Connection between X-ray Emission, the Far-Ultraviolet H2 Bump, and Accretion in T Tauri Stars

C. C. Espaillat, C. Robinson, S. Grant +1

The high-energy radiation fields of T Tauri stars (TTS) should affect the surrounding circumstellar disk, having implications for disk transport and heating. Yet, observational evi…

astro-ph.HE201935 cited

A Low-Flux State in IRAS 00521-7054 seen with NuSTAR and XMM-Newton: Relativistic Reflection and an Ultrafast Outflow

D. J. Walton, E. Nardini, L. C. Gallo +8

We present results from a deep, coordinated -+ observation of the Seyfert 2 galaxy IRAS 00521-7054. The data provide the first detection of this sourc…

astro-ph.HE201518 cited

Broad Iron Emission from Gravitationally Lensed Quasars Observed by Chandra

D. J. Walton, M. T. Reynolds, J. M. Miller +3

Recent work has demonstrated the potential of gravitationally lensed quasars to extend measurements of black hole spin out to high-redshift with the current generation of X-ray obs…

astro-ph.HE20159 cited

Are spectral and timing correlations similar in different spectral states in black hole X-ray binaries?

M. Kalamkar, M. T. Reynolds, M. van der Klis +2

We study the outbursts of the black hole X-ray binaries MAXI J1659-152, SWIFT J1753.5--0127 and GX 339-4 with the Swift X-ray Telescope. The bandpass of the X-ray Telescope has acc…

astro-ph.HE2009137 cited

Broad relativistic iron emission line observed in SAX J1808.4-3658

E. M. Cackett, D. Altamirano, A. Patruno +4

During the September-October 2008 outburst of the accreting millisecond pulsar SAX J1808.4-3658, the source was observed by both Suzaku and XMM-Newton approximately 1 day apart. Sp…