Search Publications

PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter
DOI: 10.3847/2041-8213/ab50c5 Bibcode: 2019ApJ...887L..24M

Harding, A. K.; Ray, P. S.; Wood, K. S. +18 more

Neutron stars are not only of astrophysical interest, but are also of great interest to nuclear physicists because their attributes can be used to determine the properties of the dense matter in their cores. One of the most informative approaches for determining the equation of state (EoS) of this dense matter is to measure both a star’s equatoria…

2019 The Astrophysical Journal
XMM-Newton 1379
An Embedded X-Ray Source Shines through the Aspherical AT 2018cow: Revealing the Inner Workings of the Most Luminous Fast-evolving Optical Transients
DOI: 10.3847/1538-4357/aafa01 Bibcode: 2019ApJ...872...18M

Berger, E.; Hurley, K.; Götz, D. +42 more

We present the first extensive radio to γ-ray observations of a fast-rising blue optical transient, AT 2018cow, over its first ∼100 days. AT 2018cow rose over a few days to a peak luminosity L pk ∼ 4 × 1044 erg s-1, exceeding that of superluminous supernovae (SNe), before declining as L ∝ t -2. Initial s…

2019 The Astrophysical Journal
INTEGRAL XMM-Newton 225
1ES 1927+654: An AGN Caught Changing Look on a Timescale of Months
DOI: 10.3847/1538-4357/ab39e4 Bibcode: 2019ApJ...883...94T

Filippenko, Alexei V.; Remillard, Ronald A.; Rest, Armin +21 more

We study the sudden optical and ultraviolet (UV) brightening of 1ES 1927+654, which until now was known as a narrow-line active galactic nucleus (AGN). 1ES 1927+654 was part of the small and peculiar class of “true Type-2” AGNs that lack broad emission lines and line-of-sight obscuration. Our high-cadence spectroscopic monitoring captures the appe…

2019 The Astrophysical Journal
XMM-Newton eHST 153
Constraining the Neutron Star Mass-Radius Relation and Dense Matter Equation of State with NICER. I. The Millisecond Pulsar X-Ray Data Set
DOI: 10.3847/2041-8213/ab53eb Bibcode: 2019ApJ...887L..25B

Steiner, James F.; Remillard, Ronald A.; Enoto, Teruaki +27 more

We present the set of deep Neutron Star Interior Composition Explorer (NICER) X-ray timing observations of the nearby rotation-powered millisecond pulsars PSRs J0437-4715, J0030+0451, J1231-1411, and J2124-3358, selected as targets for constraining the mass-radius relation of neutron stars and the dense matter equation of state (EoS) via modeling …

2019 The Astrophysical Journal
XMM-Newton 148
Improved Dynamical Constraints on the Masses of the Central Black Holes in Nearby Low-mass Early-type Galactic Nuclei and the First Black Hole Determination for NGC 205
DOI: 10.3847/1538-4357/aafe7a Bibcode: 2019ApJ...872..104N

Pechetti, Renuka; Neumayer, Nadine; Strader, Jay +17 more

We improve the dynamical black hole (BH) mass estimates in three nearby low-mass early-type galaxies: NGC 205, NGC 5102, and NGC 5206. We use new Hubble Space Telescope (HST)/STIS spectroscopy to fit the star formation histories of the nuclei in these galaxies, and use these measurements to create local color-mass-to-light ratio (M/L) relations. W…

2019 The Astrophysical Journal
XMM-Newton eHST 143
Short GRB 160821B: A Reverse Shock, a Refreshed Shock, and a Well-sampled Kilonova
DOI: 10.3847/1538-4357/ab38bb Bibcode: 2019ApJ...883...48L

Pian, E.; Greiner, J.; Fruchter, A. S. +31 more

We report our identification of the optical afterglow and host galaxy of the short-duration gamma-ray burst sGRB 160821B. The spectroscopic redshift of the host is z = 0.162, making it one of the lowest redshift short-duration gamma-ray bursts (sGRBs) identified by Swift. Our intensive follow-up campaign using a range of ground-based facilities as…

2019 The Astrophysical Journal
Gaia XMM-Newton eHST 136
X-Ray Properties of SPT-selected Galaxy Clusters at 0.2 < z < 1.5 Observed with XMM-Newton
DOI: 10.3847/1538-4357/aaf230 Bibcode: 2019ApJ...871...50B

Miller, Eric D.; Schrabback, Tim; Holzapfel, W. L. +22 more

We present measurements of the X-ray observables of the intracluster medium (ICM), including luminosity L X , ICM mass M ICM, emission-weighted mean temperature T X , and integrated pressure Y X , that are derived from XMM-Newton X-ray observations of a Sunyaev-Zel’dovich effect (SZE) selected sample …

2019 The Astrophysical Journal
XMM-Newton 109
The Analogous Structure of Accretion Flows in Supermassive and Stellar Mass Black Holes: New Insights from Faded Changing-look Quasars
DOI: 10.3847/1538-4357/ab3c1a Bibcode: 2019ApJ...883...76R

Green, Paul J.; Anderson, Scott F.; Eracleous, Michael +5 more

Despite their factor of ∼108 difference in black hole mass, several lines of evidence suggest possible similarities between black hole accretion flows in active galactic nuclei (AGN) and Galactic X-ray binaries. However, it is still unclear whether the geometry of the disk-corona system in X-ray binaries directly scales up to AGN and wh…

2019 The Astrophysical Journal
XMM-Newton 108
A New Class of Changing-look LINERs
DOI: 10.3847/1538-4357/ab3a38 Bibcode: 2019ApJ...883...31F

Cenko, S. Bradley; Duev, Dmitry A.; Rusholme, Ben +28 more

We report the discovery of six active galactic nuclei (AGNs) caught “turning on” during the first nine months of the Zwicky Transient Facility (ZTF) survey. The host galaxies were classified as low-ionization nuclear emission-line region galaxies (LINERs) by weak narrow forbidden line emission in their archival SDSS spectra, and detected by ZTF as…

2019 The Astrophysical Journal
XMM-Newton eHST 101
The First Tidal Disruption Flare in ZTF: From Photometric Selection to Multi-wavelength Characterization
DOI: 10.3847/1538-4357/aafe0c Bibcode: 2019ApJ...872..198V

Cenko, S. Bradley; Riddle, Reed; Rusholme, Ben +37 more

We present Zwicky Transient Facility (ZTF) observations of the tidal disruption flare AT2018zr/PS18kh reported by Holoien et al. and detected during ZTF commissioning. The ZTF light curve of the tidal disruption event (TDE) samples the rise-to-peak exceptionally well, with 50 days of g- and r-band detections before the time of maximum light. We al…

2019 The Astrophysical Journal
XMM-Newton 97