about
The most luminous galaxies discovered by WISEFirst NuSTAR Limits on Quiet Sun Hard X-Ray Transient EventsThe angular clustering of WISE-selected active galactic nuclei: different halos for obscured and unobscured active galactic nucleiStar formation in high-redshift cluster ellipticalsA UV to Mid-IR study of AGN selectionTwo local volume dwarf galaxies discovered in 21 cm emission: Pisces A and BThe NuSTAR Serendipitous Survey: Hunting for the Most Extreme Obscured AGN at >10 keVTHENuSTAREXTRAGALACTIC SURVEYS: THE NUMBER COUNTS OF ACTIVE GALACTIC NUCLEI AND THE RESOLVED FRACTION OF THE COSMIC X-RAY BACKGROUNDThe 2.4 μm Galaxy Luminosity Function as Measured Using WISE. II. Sample SelectionThe 2.4 μm Galaxy Luminosity Function as Measured Using WISE. III. Measurement ResultsEddington-limited Accretion in z ∼ 2 WISE-selected Hot, Dust-obscured GalaxiesInterferometric follow-up of WISE hyper-luminous hot, dust-obscured galaxiesInvestigating the Evolution of the Dual AGN System ESO 509-IG066The NuSTAR Extragalactic Survey: Average Broadband X-Ray Spectral Properties of the NuSTAR-detected AGNsThe Hunt for Red Quasars: Luminous Obscured Black Hole Growth Unveiled in the Stripe 82 X-Ray SurveyTheNuSTARSerendipitous Survey: The 40-month Catalog and the Properties of the Distant High-energy X-Ray Source PopulationNuSTAR OBSERVATIONS OF WISE J1036+0449, A GALAXY AT z ∼ 1 OBSCURED BY HOT DUSTANuSTARSURVEY OF NEARBY ULTRALUMINOUS INFRARED GALAXIESNuSTARSPECTROSCOPY OF MULTI-COMPONENT X-RAY REFLECTION FROM NGC 1068TheNuSTARHard X-Ray Survey of the Norma Arm RegionHard X-Ray-selected AGNs in Low-mass Galaxies from the NuSTAR Serendipitous SurveyThe geometry of the infrared and X-ray obscurer in a dusty hyperluminous quasarOptical spectroscopic observations of gamma-ray blazar candidates. IV. Results of the 2014 follow-up campaignDetermining the covering factor of compton-thick active galactic nuclei with NuSTARERRATUM: “NuSTARUNVEILS A COMPTON-THICK TYPE 2 QUASAR IN MrK 34” (2014, ApJ, 792, 117)Initial results from NuSTAR observations of the Norma armNuSTARUNVEILS A COMPTON-THICK TYPE 2 QUASAR IN MrK 34The variable hard X-ray emission of NGC 4945 as observed by NuSTARWeak hard X-ray emission from broad absorption line quasars: evidence for intrinsic X-ray weaknessThe NuSTAR Extragalactic Surveys: Unveiling Rare, Buried AGNs and Detecting the Contributors to the Peak of the Cosmic X-Ray BackgroundNew Spectral Model for Constraining Torus Covering Factors from Broadband X-Ray Spectra of Active Galactic NucleiEvidence for Pulsar-like Emission Components in the Broadband ULX SampleSpectral changes in the hyperluminous pulsar in NGC 5907 as a function of super-orbital phaseChandra X-Rays from the Redshift 7.54 Quasar ULAS J1342+0928Physical Properties of 15 Quasars at z ≳ 6.5The Pan-STARRS1 distant z > 5.6 quasar survey: more than 100 quasars within the first Gyr of the UniverseConstraining the radio-loud fraction of quasars at z > 5.5A Long Look at MCG-5-23-16 withNuSTAR. I. Relativistic Reflection and Coronal PropertiesAn Active Galactic Nucleus Caught in the Act of Turning Off and OnHST Grism Confirmation of 16 Structures at 1.4 < z < 2.8 from the Clusters Around Radio-Loud AGN (CARLA) Survey
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description
forsker
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researcher, ORCID id # 0000-0003-2686-9241
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wetenschapper
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name
D. Stern
@ast
D. Stern
@nl
Daniel Stern
@en
Daniel Stern
@es
Daniel Stern
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type
label
D. Stern
@ast
D. Stern
@nl
Daniel Stern
@en
Daniel Stern
@es
Daniel Stern
@nb
altLabel
D. Stern
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prefLabel
D. Stern
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D. Stern
@nl
Daniel Stern
@en
Daniel Stern
@es
Daniel Stern
@nb
P106
P31
P496
0000-0003-2686-9241