Abstract is: Ann Hornschemeier is an American astronomer specializing in X-ray emission from X-ray binary populations. She is the Chief Scientist for the Physics of the Cosmos program at NASA.
| human | Q5 |
| P2671 | Google Knowledge Graph ID | /g/11bzv3qnkj |
| P166 | award received | Annie Jump Cannon Award in Astronomy | Q566886 |
| P69 | educated at | Pennsylvania State University | Q739627 |
| P108 | employer | National Aeronautics and Space Administration | Q23548 |
| Johns Hopkins University | Q193727 | ||
| P735 | given name | Ann | Q558067 |
| Ann | Q558067 | ||
| P106 | occupation | astronomer | Q11063 |
| P21 | sex or gender | female | Q6581072 |
| Q59973406 | A new candidate Wolf–Rayet X-ray binary in NGC 253 |
| Q58907389 | Atmospheric gas dynamics in the Perseus cluster observed with Hitomi* |
| Q58907392 | Atomic data and spectral modeling constraints from high-resolution X-ray observations of the Perseus cluster with Hitomi* |
| Q58906979 | Concept of the X-ray Astronomy Recovery Mission |
| Q59785059 | Demonstrating the likely neutron star nature of five M31 globular cluster sources withSwift-NuSTAR spectroscopy |
| Q60366881 | Detection of polarized gamma-ray emission from the Crab nebula with the Hitomi Soft Gamma-ray Detector† |
| Q58474493 | Erratum: “The Hubble Higher z Supernova Search: Supernovae to z≈ 1.6 and Constraints on Type Ia Progenitor Models” (ApJ, 613, 200 [2004]) |
| Q58907396 | Glimpse of the highly obscured HMXB IGR J16318−4848 with Hitomi* |
| Q58907387 | Hitomi X-ray observation of the pulsar wind nebula G21.5−0.9 |
| Q58907398 | Hitomi X-ray studies of giant radio pulses from the Crab pulsar* |
| Q58907400 | Hitomi observation of radio galaxy NGC 1275: The first X-ray microcalorimeter spectroscopy of Fe-Kα line emission from an active galactic nucleus* |
| Q58907402 | Hitomi observations of the LMC SNR N 132 D: Highly redshifted X-ray emission from iron ejecta* |
| Q58907404 | Measurements of resonant scattering in the Perseus Cluster core with Hitomi SXS* |
| Q58907406 | Search for thermal X-ray features from the Crab nebula with the Hitomi soft X-ray spectrometer* |
| Q58914645 | Spectral and temporal properties of the ultraluminous X-ray pulsar in M82 from 15 years of Chandra observations and analysis of the pulsed emission using NuSTAR |
| Q58907408 | Temperature structure in the Perseus cluster core observed with Hitomi* |
| Q58907012 | The ASTRO-H (Hitomi) x-ray astronomy satellite |
| Q58357372 | The ASTRO-H Mission |
| Q58357352 | The ASTRO-H X-ray Observatory |
| Q55950372 | The ASTRO-H X-ray astronomy satellite |
| Q57651741 | The HST/ACS Coma cluster survey. II. Data description and source catalogs |
| Q58474523 | The Hubble Higher z Supernova Search: Supernovae to z≈ 1.6 and Constraints on Type Ia Progenitor Models |
| Q57651766 | The Hubble Space Telescope Advanced Camera for Surveys Coma Cluster Survey. I. Survey Objectives and Design |
| Q58912345 | The X‐Ray–derived Cosmological Star Formation History and the Galaxy X‐Ray Luminosity Functions in the Chandra Deep Fields North and South |
| Q58914692 | The ultraluminous X-ray sources NGC 1313 X-1 and X-2: a broadband study with NuSTAR and XMM-Newton |
| Q58909682 | X‐Ray Luminosity Functions of Normal Galaxies in the Great Observatories Origins Deep Survey |
| Q5334504 | 22414 Hornschemeier | named after | P138 |
| ast | Ann Hornschemeier | wikipedia |
| Ann Hornschemeier | wikipedia | |
| Ann Hornschemeier | wikipedia | |
| Basque language (eu / Q8752) | Ann Hornschemeier | wikipedia |
| ta | ஆன் ஆர்ன்சுகெமீயர் | wikipedia |
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