Mira Mechtley
biphenyl.org
0000-0001-6462-6190
Arizona State University
25 papers found
Refreshing results…
Major Mergers Are Not the Dominant Trigger for High-accretion AGNs at z ∼ 2
DO THE MOST MASSIVE BLACK HOLES ATz= 2 GROW VIA MAJOR MERGERS?
PHYSICAL PROPERTIES OF SPECTROSCOPICALLY CONFIRMED GALAXIES ATz≥ 6. III. STELLAR POPULATIONS FROM SED MODELING WITH SECURE LyαEMISSION AND REDSHIFTS
Do the Most Massive Black Holes at $z=2$ Grow via Major Mergers?
Searching the Sky for the Brightest Galaxies in the Distant Universe
Markov Chain Monte Carlo Modeling of High-Redshift Quasar Host Galaxies in Hubble Space Telescope Imaging
Deep Spitzer/IRAC Imaging of the Subaru Deep Field
PHYSICAL PROPERTIES OF SPECTROSCOPICALLY CONFIRMED GALAXIES ATz⩾ 6. II. MORPHOLOGY OF THE REST-FRAME UV CONTINUUM AND Lyα EMISSION
PHYSICAL PROPERTIES OF SPECTROSCOPICALLY CONFIRMED GALAXIES ATz⩾ 6. I. BASIC CHARACTERISTICS OF THE REST-FRAME UV CONTINUUM AND Lyα EMISSION
Emission-Line Galaxies From Thehubble Space Telescopeprobing Evolution and Reionization Spectroscopically (Pears) Grism Survey. Ii. The Complete Sample
Quasar Host Galaxies at z=2 and z=6: Point Source Subtraction With MCMC
WFC3IR Imaging of UV-Faint z=6 Quasars: Star-Forming Host Galaxies of AGN in the Early Universe
The Size Evolution of Passive Galaxies: Observations From the Wide-Field Camera 3 Early Release Science Program
Multi-component SED Fitting Of AGN Host Galaxies
WFC3 Imaging Of z=6 Quasars: Examining The Host Galaxies Of AGN In The Early Universe
Hubble Space Telescopeobservations of Field Ultracool Dwarfs at High Galactic Latitude
The surficial nature of lunar swirls as revealed by the Mini-RF instrument
WFC3 Imaging Of z=6 QSO Hosts: A Method For PSF Characterization And Subtraction
The Surficial Nature of Lunar Swirls as Revealed by Mini-RF on LRO
Coordinated Mini-RF and LROC Observations of the Lunar Surface
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