Distances to PHANGS galaxies: New tip of the red giant branch measurements and adopted distances

GS Anand, JC Lee, SD Van Dyk… - Monthly Notices of …, 2021 - academic.oup.com
ABSTRACT PHANGS-HST is an ultraviolet-optical imaging survey of 38 spiral galaxies
within∼ 20 Mpc. Combined with the PHANGS-ALMA, PHANGS-MUSE surveys and other …

The low-luminosity end of the radius–luminosity relationship for active galactic nuclei

MC Bentz, KD Denney, CJ Grier, AJ Barth… - The Astrophysical …, 2013 - iopscience.iop.org
We present an updated and revised analysis of the relationship between the Hβ broad-line
region (BLR) radius and the luminosity of the active galactic nucleus (AGN). Specifically, we …

The discovery of the first “changing look” quasar: new insights into the physics and phenomenology of active galactic nuclei

SM LaMassa, S Cales, EC Moran… - The Astrophysical …, 2015 - iopscience.iop.org
ABSTRACT SDSS J015957. 64+ 003310.5 is an X-ray selected, z= 0.31 active galactic
nucleus (AGN) from the Stripe 82X survey that transitioned from a Type 1 quasar to a Type …

The rest-frame extreme-ultraviolet spectral properties of quasi-stellar objects

RC Telfer, W Zheng, GA Kriss… - The Astrophysical …, 2002 - iopscience.iop.org
We use a sample of 332 Hubble Space Telescope spectra of 184 quasi-stellar objects
(QSOs) with z> 0.33 to study the typical ultraviolet spectral properties of QSOs, with …

Infrared radiation from an extrasolar planet

D Deming, S Seager, LJ Richardson, J Harrington - Nature, 2005 - nature.com
A class of extrasolar giant planets—the so-called 'hot Jupiters'(ref.)—orbit within 0.05 au of
their primary stars (1 au is the Sun–Earth distance). These planets should be hot and so emit …

A composite HST spectrum of quasars

W Zheng, GA Kriss, RC Telfer, JP Grimes… - The Astrophysical …, 1997 - iopscience.iop.org
We construct a composite quasar spectrum from 284 HST FOS spectra of 101 quasars with
redshifts z> 0.33. The spectrum covers the wavelengths between 350 and 3000 Å in the rest …

Radio-loud narrow-line type 1 quasars

S Komossa, W Voges, D Xu, S Mathur… - The Astronomical …, 2006 - iopscience.iop.org
We present the first systematic study of (non-radio-selected) radio-loud narrow-line Seyfert 1
(NLS1) galaxies. Cross-correlation of the Catalogue of Quasars and Active Nuclei with …

Now you see it, now you don't: the disappearing central engine of the quasar J1011+ 5442

JC Runnoe, S Cales, JJ Ruan… - Monthly Notices of …, 2016 - academic.oup.com
We report the discovery of a new 'changing-look'quasar, SDSS J101152. 98+ 544206.4,
through repeat spectroscopy from the Time Domain Spectroscopic Survey. This is an …

Origins of weak lensing systematics, and requirements on future instrumentation (or knowledge of instrumentation)

R Massey, H Hoekstra, T Kitching… - Monthly Notices of …, 2013 - academic.oup.com
The first half of this paper explores the origin of systematic biases in the measurement of
weak gravitational lensing. Compared to previous work, we expand the investigation of point …

[HTML][HTML] Evidence for a massive black hole in the active galaxy NGC 4261 from Hubble Space Telescope images and spectra

L Ferrarese, HC Ford, W Jaffe - Astrophysical Journal v. 470, p …, 1996 - adsabs.harvard.edu
Evidence for a Massive Black Hole in the Active Galaxy NGC 4261 from Hubble Spac ADS
Classic is now deprecated. It will be completely retired in October 2019. This page will …