Search Publications

New Physical Insights about Tidal Disruption Events from a Comprehensive Observational Inventory at X-Ray Wavelengths
DOI: 10.3847/1538-4357/aa633b Bibcode: 2017ApJ...838..149A

Ramirez-Ruiz, Enrico; Auchettl, Katie; Guillochon, James

We perform a comprehensive study of the X-ray emission from 70 transient sources that have been classified as tidal disruption events (TDEs) in the literature. We explore the properties of these candidates, using nearly three decades of X-ray observations to quantify their properties and characteristics. We find that the emission from X-ray TDEs i…

2017 The Astrophysical Journal
XMM-Newton 227
Simultaneous X-Ray, Gamma-Ray, and Radio Observations of the Repeating Fast Radio Burst FRB 121102
DOI: 10.3847/1538-4357/aa8456 Bibcode: 2017ApJ...846...80S

Ransom, S. M.; Chatterjee, S.; Cordes, J. M. +19 more

We undertook coordinated campaigns with the Green Bank, Effelsberg, and Arecibo radio telescopes during Chandra X-ray Observatory and XMM-Newton observations of the repeating fast radio burst FRB 121102 to search for simultaneous radio and X-ray bursts. We find 12 radio bursts from FRB 121102 during 70 ks total of X-ray observations. We detect no …

2017 The Astrophysical Journal
XMM-Newton 127
X-Ray Brightening and UV Fading of Tidal Disruption Event ASASSN-15oi
DOI: 10.3847/2041-8213/aaa0c2 Bibcode: 2017ApJ...851L..47G

Cenko, S. B.; Arcavi, I.; Gezari, S.

We present late-time observations by Swift and XMM-Newton of the tidal disruption event (TDE) ASASSN-15oi that reveal that the source brightened in the X-rays by a factor of ∼10 one year after its discovery, while it faded in the UV/optical by a factor of ∼100. The XMM-Newton observations measure a soft X-ray blackbody component with {{kT}}{b…

2017 The Astrophysical Journal
XMM-Newton 121
iPTF Discovery of the Rapid “Turn-on” of a Luminous Quasar
DOI: 10.3847/1538-4357/835/2/144 Bibcode: 2017ApJ...835..144G

Cenko, S. B.; Kulkarni, S. R.; Nugent, P. E. +13 more

We present a radio-quiet quasar at z = 0.237 discovered “turning on” by the intermediate Palomar Transient Factory (iPTF). The transient, iPTF 16bco, was detected by iPTF in the nucleus of a galaxy with an archival Sloan Digital Sky Survey spectrum with weak narrow-line emission characteristic of a low-ionization nuclear emission-line region (LINE…

2017 The Astrophysical Journal
XMM-Newton 121
X-Ray Morphological Analysis of the Planck ESZ Clusters
DOI: 10.3847/1538-4357/aa855f Bibcode: 2017ApJ...846...51L

Lovisari, Lorenzo; Andrade-Santos, Felipe; Jones, Christine +7 more

X-ray observations show that galaxy clusters have a very large range of morphologies. The most disturbed systems, which are good to study how clusters form and grow and to test physical models, may potentially complicate cosmological studies because the cluster mass determination becomes more challenging. Thus, we need to understand the cluster pr…

2017 The Astrophysical Journal
Planck XMM-Newton 106
Pulsator-like Spectra from Ultraluminous X-Ray Sources and the Search for More Ultraluminous Pulsars
DOI: 10.3847/1538-4357/836/1/113 Bibcode: 2017ApJ...836..113P

Mereghetti, S.; Stella, L.; Wolter, A. +3 more

Ultraluminous X-ray sources (ULXs) are a population of extragalactic objects whose luminosity exceeds the Eddington limit for a 10 M black hole (BH). Their properties have been widely interpreted in terms of accreting stellar-mass or intermediate-mass BHs. However at least three neutron stars (NSs) have been recently identified in ULX…

2017 The Astrophysical Journal
XMM-Newton 104
Constraints on Axion-like Particles from X-Ray Observations of NGC1275
DOI: 10.3847/1538-4357/aa8b16 Bibcode: 2017ApJ...847..101B

Berg, Marcus; Conlon, Joseph P.; Day, Francesca +4 more

Axion-like particles (ALPs) can induce localized oscillatory modulations in the spectra of photon sources passing through astrophysical magnetic fields. Ultra-deep Chandra observations of the Perseus cluster contain over 5× {10}5 counts from the active galactic nucleus (AGN) of the central cluster galaxy NGC1275 and represent a data set…

2017 The Astrophysical Journal
XMM-Newton 90
Spectral Changes in the Hyperluminous Pulsar in NGC 5907 as a Function of Super-orbital Phase
DOI: 10.3847/1538-4357/834/1/77 Bibcode: 2017ApJ...834...77F

Harrison, F. A.; Stern, D.; Bachetti, M. +5 more

We present broadband, multi-epoch X-ray spectroscopy of the pulsating ultra-luminous X-ray source (ULX) in NGC 5907. Simultaneous XMM-Newton and NuSTAR data from 2014 are best described by a multicolor blackbody model with a temperature gradient as a function of accretion disk radius significantly flatter than expected for a standard thin accretio…

2017 The Astrophysical Journal
XMM-Newton 77
General Physical Properties of CGRaBS Blazars
DOI: 10.3847/1538-4357/aa98e1 Bibcode: 2017ApJ...851...33P

Ajello, M.; Rao, A. R.; Hartmann, D. +4 more

We present the results of a multi-frequency, time-averaged analysis of blazars included in the Candidate Gamma-ray Blazar Survey catalog. Our sample consists of 324 γ-ray detected (γ-ray loud) and 191 γ-ray undetected (γ-ray quiet) blazars; we consider all the data up to 2016 April 1. We find that both the γ-ray loud and γ-ray quiet blazar populat…

2017 The Astrophysical Journal
XMM-Newton 76
X-Ray and Radio Observations of the Magnetar SGR J1935+2154 during Its 2014, 2015, and 2016 Outbursts
DOI: 10.3847/1538-4357/aa899a Bibcode: 2017ApJ...847...85Y

Göğüş, Ersin; Kouveliotou, Chryssa; Lin, Lin +10 more

We analyzed broadband X-ray and radio data of the magnetar SGR J1935+2154 taken in the aftermath of its 2014, 2015, and 2016 outbursts. The source soft X-ray spectrum <10 keV is well described with a blackbody+power-law (BB+PL) or 2BB model during all three outbursts. Nuclear Spectroscopic Telescope Array observations revealed a hard X-ray tail…

2017 The Astrophysical Journal
XMM-Newton 74