Search Publications

Live to Die Another Day: The Rebrightening of AT 2018fyk as a Repeating Partial Tidal Disruption Event
DOI: 10.3847/2041-8213/ac9f36 Bibcode: 2023ApJ...942L..33W

Liu, Z.; Merloni, A.; Rau, A. +13 more

Stars that interact with supermassive black holes (SMBHs) can be either completely or partially destroyed by tides. In a partial tidal disruption event (TDE), the high-density core of the star remains intact, and the low-density outer envelope of the star is stripped and feeds a luminous accretion episode. The TDE AT 2018fyk, with an inferred blac…

2023 The Astrophysical Journal
XMM-Newton 67
The Jet Opening Angle and Event Rate Distributions of Short Gamma-Ray Bursts from Late-time X-Ray Afterglows
DOI: 10.3847/1538-4357/acf830 Bibcode: 2023ApJ...959...13R

Berger, E.; Chornock, R.; Laskar, T. +14 more

We present a comprehensive study of 29 short gamma-ray bursts (SGRBs) observed ≈0.8-60 days postburst using Chandra and XMM-Newton. We provide the inferred distributions of the SGRB jet opening angles and true event rates to compare against neutron star merger rates. We perform a uniform analysis and modeling of their afterglows, obtaining 10 open…

2023 The Astrophysical Journal
XMM-Newton 46
On the Cosmic Evolution of AGN Obscuration and the X-Ray Luminosity Function: XMM-Newton and Chandra Spectral Analysis of the 31.3 deg2 Stripe 82X
DOI: 10.3847/1538-4357/acac28 Bibcode: 2023ApJ...943..162P

Kirkpatrick, Allison; Marchesi, Stefano; LaMassa, Stephanie +11 more

We present X-ray spectral analysis of XMM-Newton and Chandra observations in the 31.3 deg2 Stripe-82X (S82X) field. Of the 6181 unique X-ray sources in this field, we analyze a sample of 2937 candidate active galactic nuclei (AGNs) with solid redshifts and sufficient counts determined by simulations. Our results show an observed populat…

2023 The Astrophysical Journal
XMM-Newton 34
IXPE and Multiwavelength Observations of Blazar PG 1553+113 Reveal an Orphan Optical Polarization Swing
DOI: 10.3847/2041-8213/acec3e Bibcode: 2023ApJ...953L..28M

Kaaret, Philip; Wu, Kinwah; Enoto, Teruaki +119 more

The lower-energy peak of the spectral energy distribution of blazars has commonly been ascribed to synchrotron radiation from relativistic particles in the jets. Despite the consensus regarding jet emission processes, the particle acceleration mechanism is still debated. Here, we present the first X-ray polarization observations of PG 1553+113, a …

2023 The Astrophysical Journal
XMM-Newton 32
X-Ray Polarization of BL Lacertae in Outburst
DOI: 10.3847/2041-8213/acd242 Bibcode: 2023ApJ...948L..25P

Kaaret, Philip; Wu, Kinwah; Enoto, Teruaki +128 more

We report the first >99% confidence detection of X-ray polarization in BL Lacertae. During a recent X-ray/γ-ray outburst, a 287 ks observation (2022 November 27-30) was taken using the Imaging X-ray Polarimetry Explorer (IXPE), together with contemporaneous multiwavelength observations from the Neil Gehrels Swift observatory and XMM-Newton in s…

2023 The Astrophysical Journal
XMM-Newton 27
X-Ray Polarization Observations of BL Lacertae
DOI: 10.3847/2041-8213/aca281 Bibcode: 2023ApJ...942L..10M

Wu, Kinwah; Masiero, Joseph R.; Tinyanont, Samaporn +144 more

Blazars are a class of jet-dominated active galactic nuclei with a typical double-humped spectral energy distribution. It is of common consensus that the synchrotron emission is responsible for the low frequency peak, while the origin of the high frequency hump is still debated. The analysis of X-rays and their polarization can provide a valuable …

2023 The Astrophysical Journal
XMM-Newton 27
UV-Optical Disk Reverberation Lags despite a Faint X-Ray Corona in the Active Galactic Nucleus Mrk 335
DOI: 10.3847/1538-4357/acbcd3 Bibcode: 2023ApJ...947...62K

Kaspi, Shai; Fabian, Andrew C.; Komossa, S. +37 more

We present the first results from a 100-day Swift, NICER, and ground-based X-ray-UV-optical reverberation mapping campaign of the Narrow-line Seyfert 1 Mrk 335, when it was in an unprecedented low X-ray flux state. Despite dramatic suppression of the X-ray variability, we still observe UV-optical lags as expected from disk reverberation. Moreover,…

2023 The Astrophysical Journal
XMM-Newton 26
The Hot Circumgalactic Medium of the Milky Way: New Insights from XMM-Newton Observations
DOI: 10.3847/1538-4357/acd337 Bibcode: 2023ApJ...952...41B

Mathur, Smita; Gupta, Anjali; Das, Sanskriti +2 more

We present XMM-Newton observations around the sight line of Mrk 421. The emission spectrum of the Milky Way (MW) circumgalactic medium (CGM) shows that a two-phase model is a better fit to the data compared to a single-phase model; in addition to the warm-hot virial phase at log (T/K) = 6.30 ± 0.02, a hot super-virial phase at log (T/K) = ${6.88}_…

2023 The Astrophysical Journal
XMM-Newton 25
X-Ray Polarization of the BL Lacertae Type Blazar 1ES 0229+200
DOI: 10.3847/1538-4357/ad05c4 Bibcode: 2023ApJ...959...61E

Kaaret, Philip; Wu, Kinwah; Enoto, Teruaki +111 more

We present polarization measurements in the 2-8 keV band from blazar 1ES 0229+200, the first extreme high synchrotron peaked source to be observed by the Imaging X-ray Polarimetry Explorer (IXPE). Combining two exposures separated by about two weeks, we find the degree of polarization to be ΠX = 17.9% ± 2.8% at an electric-vector positi…

2023 The Astrophysical Journal
XMM-Newton 25
Do Central Compact Objects have Carbon Atmospheres?
DOI: 10.3847/1538-4357/acaf55 Bibcode: 2023ApJ...944...36A

Halpern, J. P.; Alford, J. A. J.

Only three of the dozen central compact objects (CCOs) in supernova remnants (SNRs) show thermal X-ray pulsations due to nonuniform surface temperature (hot spots). The absence of X-ray pulsations from several unpulsed CCOs has motivated suggestions that they have uniform-temperature carbon atmospheres (UTCAs), which adequately fit their spectra w…

2023 The Astrophysical Journal
XMM-Newton 25