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Marinucci, A.Arévalo, Patricia.Bauer, Franz Erik.[The Seyfert 2 galaxy NGC 2110: hard X-ray emission observed by NuSTAR and variability of the iron K alpha line]The Seyfert 2 galaxy NGC 2110: hard X-ray emission observed by NuSTAR and variability of the iron K alpha line

Bauer, Franz Erik.[THE NuSTAR EXTRAGALACTIC SURVEY: A FIRST SENSITIVE LOOK AT THE HIGH-ENERGY COSMIC X-RAY BACKGROUND POPULATION]THE NuSTAR EXTRAGALACTIC SURVEY: A FIRST SENSITIVE LOOK AT THE HIGH-ENERGY COSMIC X-RAY BACKGROUND POPULATION

Guaita, Lucía.Francke Henríquez, Harold Johanns Phillippe.Bauer, Franz Erik.Padilla, Nelson.[Magellan/MMIRS near-infrared multi-object spectroscopy of nebular emission from star-forming galaxies at 2 < z < 3]Magellan/MMIRS near-infrared multi-object spectroscopy of nebular emission from star-forming galaxies at 2 < z < 3

Plionis MBauer, Franz Erik.[Luminosity-dependent X-Ray Active Galactic Nucleus Clustering]Luminosity-dependent X-Ray Active Galactic Nucleus Clustering

Ptak, AndrewBauer, Franz Erik.[X-Ray Luminosity Functions of Normal Galaxies in the Great Observatories Origins Deep Survey]X-Ray Luminosity Functions of Normal Galaxies in the Great Observatories Origins Deep Survey

Geach, JE.Bauer, Franz Erik.[The chandra deep protocluster survey : Ly-alpha blobs are powered by heating, not cooling.]The chandra deep protocluster survey : Ly-alpha blobs are powered by heating, not cooling.

Harrison, F.Bauer, Franz Erik.[THE NUCLEAR SPECTROSCOPIC TELESCOPE ARRAY (NuSTAR) HIGH-ENERGY X-RAY MISSION]THE NUCLEAR SPECTROSCOPIC TELESCOPE ARRAY (NuSTAR) HIGH-ENERGY X-RAY MISSION

Rafferty, D.Bauer, Franz Erik.[Supermassive black hole growth in starburst galaxies over cosmic time: constraints from the deepest chandra fields]Supermassive black hole growth in starburst galaxies over cosmic time: constraints from the deepest chandra fields

Lehmer, B.Bauer, Franz Erik.[The 4 Ms Chandra deep field-south number counts apportioned by source class: pervasive active galactic nuclei and the ascent of normal galaxies]The 4 Ms Chandra deep field-south number counts apportioned by source class: pervasive active galactic nuclei and the ascent of normal galaxies

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