B | C | D | E | F | G | H | I | J | K | L | M | N | O | P | Q | R | S | T | U | V | W | X | Y | Z | |
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1 | ID | User First Name | User Last Name | User Institution | Title | ||||||||||||||||||||
2 | 2 | Abhishek | Desai | University of Wisconsin Madison | Studying the AGN radio-neutrino correlation using IceCube and MOJAVE+RFC catalogs | ||||||||||||||||||||
3 | 3 | Michael | Corcoran | Catholic University of America | The Expansion of the X-ray Nebula Around Eta Carinae | ||||||||||||||||||||
4 | 4 | Erik | Kuulkers | ESA/ESTEC | Cygnus X-1's fast X-ray variability behaviour in the 70s revisited: never throw away old data! | ||||||||||||||||||||
5 | 5 | Miguel Angel | Martinez | Northwestern University | Retention and Ejection of Intermediate Mass Black Holes from Dense Star Clusters by Fewbody Scattering | ||||||||||||||||||||
6 | 6 | Fulya | Kiroglu | Northwestern University | Tidal disruption events of stars by intermediate-mass black holes | ||||||||||||||||||||
7 | 8 | Carter | Rhea | University of Montreal | A New Paradigm in X-ray Spectral Analysis | ||||||||||||||||||||
8 | 9 | Giacomo | Fragione | Northwestern University | Intermediate-mass black holes: past, present, future | ||||||||||||||||||||
9 | 10 | Mason | Ng | MIT | Discovery of a 7.8 Hz QPO from the High-Intensity Outburst of Dipping NS LMXB 1A 1744-361 | ||||||||||||||||||||
10 | 13 | Dana | Kullgren | University of Delaware / Northwestern University | Constraining the Stellar Initial Mass Function with Gravitational Wave Data | ||||||||||||||||||||
11 | 14 | Elena | Gonzalez | Northwestern University | Intermediate-mass Black Holes on the Run from Young Star Clusters | ||||||||||||||||||||
12 | 16 | Cosmin | Ilie | Colgate University | The first stars in the universe as Dark Matter laboratories | ||||||||||||||||||||
13 | 18 | Meicun | Hou | Kavli Institute for Astronomy and Astrophysics, Peking University | X-Ray Constraints on the Hot Gas Content of Member Galaxies in Virgo | ||||||||||||||||||||
14 | 27 | Tyler | Parsotan | UMBC/Goddard/CRESST | BatAnalysis - A Comprehensive Python Pipeline for Swift BAT Survey Analysis | ||||||||||||||||||||
15 | 32 | Lailani | Kenoly | DeAnza College | Studying r-process mixing in the Early Universe | ||||||||||||||||||||
16 | 33 | Andrea | Antoni | University of California, Berkeley | Random angular momentum in convection: delayed explosions of red supergiants following “failed” supernovae | ||||||||||||||||||||
17 | 79 | Vanessa | Lopez-Barquero | University of Cambridge | Low-Frequency QPOs, Self-Oscillations, and the Corona. | ||||||||||||||||||||
18 | 88 | Tyler | Parsotan | UMBC/Goddard/CRESST | Demystifying the Prompt Emission of Gamma Ray Bursts | ||||||||||||||||||||
19 | 89 | William | Brandt | Pennsylvania State University | X-ray Coverage of the LSST Deep-Drilling Fields: Current XMM-SERVS Results and Future Prospects | ||||||||||||||||||||
20 | 90 | Simon | Guichandut | McGill University | Impact of compositional gradients on X-ray burst lightcurves | ||||||||||||||||||||
21 | 95 | Shuo | Zhang | Bard College | Twenty-year-long X-ray monitoring of the Galactic Center: echoes of past Sgr A* outbursts | ||||||||||||||||||||
22 | 96 | Julia | Sisk-Reynes | Institute of Astronomy, University of Cambridge, UK | Probing Physics Beyond the Standard Model with current and next-generation X-ray observatories: A case for Very-Light Axion-Like Particles. | ||||||||||||||||||||
23 | 97 | Zhijie (Jay) | Xu | Pacific Northwest National Laboratory | New models and critical length scales for co-evolution between supermassive black holes and host galaxies | ||||||||||||||||||||
24 | 99 | Stephen | Kerby | Penn State University | A Study of Newly-Identified Low-Luminosity Blazars from the Fermi-LAT Unassociated Sources | ||||||||||||||||||||
25 | 100 | Nickolas | Solomey | Wichita State Univ. | A neutrino and dark matter detector in space | ||||||||||||||||||||
26 | 101 | Tong | Bao | Nanjing University | Periodic X-ray sources in globular clusters: diagnosing dynamical formation and evolution of cataclysmic variables | ||||||||||||||||||||
27 | 102 | Ross | Silver | Clemson University | Using Machine Learning to find Heavily Obscured AGN with X-rays and Infrared Data | ||||||||||||||||||||
28 | 103 | Adrien | Picquenot | UMD / NASA | Observation of the narrowing of the synchrotron filaments with energy in Cassiopeia A | ||||||||||||||||||||
29 | 104 | Fabio | Pacucci | Harvard University and Smithsonian Astrophysical Observatory | Accretion from Winds of Red Giant Branch Stars May Reveal the Supermassive Black Hole in Leo I | ||||||||||||||||||||
30 | 105 | Alyssa | Cassity | University of British Columbia | The Chandra X-ray Galaxy Catalog with CSC2 | ||||||||||||||||||||
31 | 106 | Juan | Martinez Galarza | Smithsonian Astrophysical Observatory | New avenues for multi-messenger discoveries in high energy astrophysics using machine learning | ||||||||||||||||||||
32 | 108 | David | Wang | University of Washington | An Optical Search for Outbursting X-Ray Binaries | ||||||||||||||||||||
33 | 109 | Hayk | Hakobyan | Princeton Plasma Physics Laboratory | Radiative reconnection-powered TeV flares from the black hole magnetosphere in M87 | ||||||||||||||||||||
34 | 110 | Eliza | Neights | George Washington University | Introduction to COSI Data Analysis | ||||||||||||||||||||
35 | 111 | Simon | Bandler | NASA/GSFC | The Line Emission Mapper (LEM) Microcalorimeter Spectrometer | ||||||||||||||||||||
36 | 113 | Zack | Andalman | Yale University | Understanding Broad Line Emission in Tidal Disruption Events | ||||||||||||||||||||
37 | 115 | Isaiah | Cox | Clemson University | Using X-ray Hardness Ratios to Predict NH Variability in Nearby AGN | ||||||||||||||||||||
38 | 116 | Zachary | Metzler | University of Maryland | Calibration of the anti-coincidence detector subsystem for the Compton Pair balloon instrument | ||||||||||||||||||||
39 | 117 | Steven | Rossland | University of Utah | Characterization of the Background Components of NuSTAR to Measure the Cosmic X-Ray Background in the ~3--30 keV Energies. | ||||||||||||||||||||
40 | 123 | Jose | Arita-Escalante | NASA Goddard Space Flight Center | Optimizing the Resolution of Hydrodynamic Simulations for MCRaT Radiative Transfer Calculations | ||||||||||||||||||||
41 | 126 | Aravind | Ravi | University of Texas at Arlington | Latest Evolution of the X-ray Remnant of SN 1987A: Beyond the Inner Ring | ||||||||||||||||||||
42 | 127 | Gokul | Srinivasaragavan | University of Maryland College Park | A Study of Broad-Lined Type Ic Supernovae from the Zwicky Transient Facility | ||||||||||||||||||||
43 | 128 | Chris | Fryer | Los Alamos National Laboratory | Compact Remnant Properties and the Supernova Engine | ||||||||||||||||||||
44 | 129 | Valeria | Olivares | University of Kentucky | Unveiling the relationship between the optical H-alpha and X-ray filaments in cooling flow clusters | ||||||||||||||||||||
45 | 130 | Robin | Corbet | University of Maryland- Baltimore County | Orbital Modulation and Long-Term Variability in MAXI J0903-531 and XTE J1829-098 from Swift BAT, Fermi GBM, MAXI and RXTE PCA Observations | ||||||||||||||||||||
46 | 131 | Laurence | Arcadias | Maryland Institute College of Art | Workshopping Art/Science Activities for a Guerrilla Astro-Animation STEM Exhibition | ||||||||||||||||||||
47 | 134 | Jiachen | Jiang | Institute of Astronomy, University of Cambridge | The Densities of Black Hole Accretion Discs and Their Implications in X-ray Data | ||||||||||||||||||||
48 | 135 | Ioanna | Psaradaki | University of Michigan | Mineralogy of interstellar dust in the X-ray regime | ||||||||||||||||||||
49 | 136 | Nazma | Islam | NASA GSFC and UMBC | Superorbital modulations in supergiant High Mass X-ray binaries | ||||||||||||||||||||
50 | 140 | Amanda | Steinhebel | NASA/GSFC | AstroPix: Monolithic Active Pixelated Silicon Detectors for Future Space-Based Gamma-Ray Telescopes | ||||||||||||||||||||
51 | 143 | Congyao | Zhang | The University of Chicago | X-ray Bubbles in Galaxy Clusters and their Role in Generating Internal Gravity Waves and Shaping Ha Filaments | ||||||||||||||||||||
52 | 144 | Congyao | Zhang | The University of Chicago | Evolution of Shocks and Splashback Boundaries in Cluster Outskirts | ||||||||||||||||||||
53 | 145 | Zuzana | Turonova | Los Alamos National Laboratory | Probing Black Hole Spin Orientations: the inner disk inclination angle in GRO J1655-40 | ||||||||||||||||||||
54 | 147 | Malgorzata | Sobolewska | Center for Astrophysics | Harvard and Smithsonian | Broadband X-ray spectra and X-ray variability of young radio sources | ||||||||||||||||||||
55 | 148 | Suraj | Poolakkil | University of Alabama in Huntsville | Exploring the viability of physically-motivated models to fit Gamma-ray Burst Spectrum | ||||||||||||||||||||
56 | 149 | Carolyn | Kierans | NASA/GSFC | The Compton Pair balloon instrument: A prototype for a next-generation gamma-ray observatory | ||||||||||||||||||||
57 | 150 | Elena | Bellomi | Harvard-Smithsonian Center for Astrophysics | Simulations of Large-Scale Cold Fronts and Subcluster Interactions in the Perseus Cluster | ||||||||||||||||||||
58 | 151 | Greg | Salvesen | Los Alamos National Laboratory | Spin-Orbit Misalignments in Black Hole X-ray Binaries | ||||||||||||||||||||
59 | 152 | Paul | Draghis | University of Michigan | Exploring the Spin Distribution of Stellar Mass Black Holes | ||||||||||||||||||||
60 | 153 | Greg | Salvesen | Los Alamos National Laboratory | An Electron-Scattering Time Delay in Black Hole Accretion Disks | ||||||||||||||||||||
61 | 154 | Gerrit | Schellenberger | Smithsonian Astrophysical Observatory | AGN feedback in two very different galaxy groups: NGC5044 and NGC6338 | ||||||||||||||||||||
62 | 155 | Gerrit | Schellenberger | Smithsonian Astrophysical Observatory | Using the XMM-Newton Small Window Mode to investigate systematic uncertainties in the particle background of X-ray CCD detectors | ||||||||||||||||||||
63 | 156 | Jeremiah | Paul | University of Nevada, Reno | Multiwavelength Scrutiny of the X-ray Weak Tail of Low-Mass Active Galactic Nuclei | ||||||||||||||||||||
64 | 157 | Ka Yui | Au | National Cheng Kung University | MULTI-WAVELENGTH OBSERVATIONS OF A NEW REDBACK MILLISECOND PULSAR 4FGL J1910.7-5320 | ||||||||||||||||||||
65 | 158 | John | Rankin | INAF/IAPS | Probing the geometry of binary systems through X-ray polarimetry | ||||||||||||||||||||
66 | 159 | Ann | Hornschemeier | NASA Goddard Space Flight Center | Time Domain Studies of Neutron Star and Black Hole Populations with the Athena WFI (Wide Field Instrument): X-ray Identification of Compact Object Types | ||||||||||||||||||||
67 | 162 | Wolfgang | Zober | Washington University in St. Louis | The Trans-Iron Galactic Element Recorder for the International Space Station (TIGERISS) | ||||||||||||||||||||
68 | 163 | Gerrit | Schellenberger | Smithsonian Astrophysical Observatory | Measuring the CGM to the virial radius with LEM mock observations | ||||||||||||||||||||
69 | 164 | Jason | Hinkle | University of Hawaii | The Growing Class of Ambiguous Nuclear Transients | ||||||||||||||||||||
70 | 166 | Chris | Irwin | RESCEU, University of Tokyo | Insights on the origin of low-luminosity GRBs from a revised shock breakout model for GRB 060218 | ||||||||||||||||||||
71 | 167 | Hongjun | An | Chungbuk National University | Investigation of the high-energy emission from the TeV gamma-ray binary HESS J0632+057 | ||||||||||||||||||||
72 | 168 | Jiachen | Jiang | Institute of Astronomy, University of Cambridge | Hybrid Plasma Emission in the Black Hole X-ray Binary MAXI J1535-571 | ||||||||||||||||||||
73 | 169 | Jiachen | Jiang | Institute of Astronomy, University of Cambridge | Reflection Spectra from a Thin Disc Model with Finite Thickness and Its Application to X-ray Spectral Data | ||||||||||||||||||||
74 | 171 | Jiachen | Jiang | Institute of Astronomy, University of Cambridge | Rapidly Alternating Flux States of GX 339-4 During its 2021 Outburst | ||||||||||||||||||||
75 | 172 | Jiachen | Jiang | Institute of Astronomy, University of Cambridge | A Highly Accreting Low-Mass Black Hole Hidden in the Dust | ||||||||||||||||||||
76 | 173 | Jiachen | Jiang | Institute of Astronomy, University of Cambridge | Modelling the Multiwavelength Variability of Mrk 335 using Machine Learning | ||||||||||||||||||||
77 | 174 | Jiachen | Jiang | Institute of Astronomy, University of Cambridge | The Awakening Beast in the Seyfert 1 Galaxy KUG 1141+371 | ||||||||||||||||||||
78 | 176 | Aysegul | Tumer | MIT Kavli Institute for Astrophysics and Space Research | From BCGs to cosmic filaments, from AGNi to merger shocks: multi-scale and multi-phase galaxy cluster evolution in X-rays | ||||||||||||||||||||
79 | 177 | Amy | Gall | Smithsonian Astrophysical Observatory | Calibration of the Line Emission Mapper (LEM) Observatory | ||||||||||||||||||||
80 | 178 | Sylvain | Guiriec | GW/NASA GSFC | Broadband modeling of the GRB prompt emission from optical to gamma-rays | ||||||||||||||||||||
81 | 179 | Brendan | O'Connor | George Washington University | The Transient Universe: Compact Objects Near and Far | ||||||||||||||||||||
82 | 181 | Jennifer | Rodriguez | The Ohio State University | Assessing Stellar Wind Feedback in 30 Doradus using Deep Chandra and JWST Observations | ||||||||||||||||||||
83 | 183 | Nicholas | Kirschner | George Washington University | GRB Prompt Emission Spectral Curvature in the MeV Regime | ||||||||||||||||||||
84 | 185 | Kevin | France | University of Colorado | The Extreme-UV Radiation Environment of Extrasolar Planets: the ESCAPE Small Explorer Mission | ||||||||||||||||||||
85 | 186 | Thomas | Wevers | ESO | Live to die another day: the rebrightening of AT2018fyk as a repeating partial tidal disruption event | ||||||||||||||||||||
86 | 187 | Edmund | Hodges-Kluck | NASA/GSFC | Superbubble Growth, Energetics, and Breakout with the Line Emission Mapper | ||||||||||||||||||||
87 | 188 | Ralf | Ballhausen | UMCP and NASA GSFC | The NuSTAR view of the 2021 giant X-ray outburst of EXO 2030+375 | ||||||||||||||||||||
88 | 189 | Brian | Fleming | University of Colorado, Boulder | Transient Imaging with the STAR-X Ultraviolet Telescope (UVT) | ||||||||||||||||||||
89 | 190 | Steven | Boggs | University of California, San Diego | Uncovering the origin of Galactic positrons with the Compton Spectrometer and Imager | ||||||||||||||||||||
90 | 191 | James | Tutt | Pennsylvania State University | Silicon-carbide grids for microcalorimeter thermal baffles | ||||||||||||||||||||
91 | 192 | Laurel | White | Massachusetts Institute of Technology | What's for LUNCH?: Population statistics of the Low-z UNbiased Chandra galaxy cluster sample | ||||||||||||||||||||
92 | 193 | Sophie | Koudmani | CCA, Flatiron Institute | Next-generation AGN models in galaxy formation: from dwarf galaxies to massive black hole binaries | ||||||||||||||||||||
93 | 194 | Peter | Jenke | MSFC | The Moon Burst Energetics All-sky Monitor (MoonBEAM) | ||||||||||||||||||||
94 | 195 | Peter | Jenke | MSFC | The Gamma Ray Burst Monitor Accreting Pulsar Program. Fifteen years of monitoring the pulsed sky. | ||||||||||||||||||||
95 | 196 | Dustin | Swarm | University of Iowa | Spectral Analysis of Intermediate Polar Candidates in the Galactic Center | ||||||||||||||||||||
96 | 197 | Matthew | Baring | Rice University | Opacity Diagnostics for Magnetar Giant Flare Emission Regions | ||||||||||||||||||||
97 | 198 | Stefan | Wagner | LSW, ZAH, U Heidelberg | The population of VHE Gamma-Ray sources | ||||||||||||||||||||
98 | 199 | Maxim | Markevitch | NASA GSFC | Mapping the IGM in the Cosmic Web in emission and absorption with LEM | ||||||||||||||||||||
99 | 201 | Paarmita | Pandey | The Ohio State University | Evaluating Stellar Winds from Young Massive Star Clusters as Cosmic-ray Acceleration Sites using Fermi Gamma-ray Observations | ||||||||||||||||||||
100 | 202 | Dany | Atallah | Northwestern University | Growing Black Holes through Successive Mergers in Galactic Nuclei |