2.9k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Centre National de la Recherche ScientifiqueFR147 papers
- University of OxfordGB114 papers
- University of CambridgeGB88 papers
- Max Planck Institute for Extraterrestrial PhysicsDE84 papers
- University of BristolGB80 papers
- University College LondonGB78 papers
- Center for Astrophysics Harvard & SmithsonianUS72 papers
- Space Telescope Science InstituteUS72 papers
- National Institute for AstrophysicsIT71 papers
- University of EdinburghGB69 papers
- University of WarwickGB69 papers
- University of CopenhagenDK63 papers
23 papers · 2 filters
Probing black hole accretion tracks, scaling relations and radiative efficiencies from stacked X-ray active galactic nuclei
Francesco Shankar, David H. Weinberg, Christopher Marsden +25
The masses of supermassive black holes at the centres of local galaxies appear to be tightly correlated with the mass and velocity dispersions of their galactic hosts. However, the…
The Subaru HSC Galaxy Clustering with Photometric Redshift I: Dark Halo Masses Versus Baryonic Properties of Galaxies at 0.3<z<1.4
Shogo Ishikawa, Nobunari Kashikawa, Masayuki Tanaka +8
We present the clustering properties of low- galaxies selected by the Hyper Suprime-Cam Subaru Strategic Program Wide layer over deg. The wide-field and…
Discovery of Protoclusters at z~3.7 & 4.9: Embedded in Primordial Superclusters
Jun Toshikawa, Matthew A. Malkan, Nobunari Kashikawa +5
We have carried out follow-up spectroscopy on three overdense regions of - and -dropout galaxies in the Canada-France-Hawaii Telescope Legacy Survey Deep Fields, finding two…
Planck far-infrared detection of Hyper Suprime-Cam protoclusters at : hidden AGN and star formation activity
Mariko Kubo, Jun Toshikawa, Nobunari Kashikawa +11
We perform a stacking analysis of {\it Planck}, {\it AKARI}, Infrared Astronomical Satellite (), Wide-field Infrared Survey Eplorer (), and {\it Herschel} images of the…
A BCG with offset cooling: is the AGN feedback cycle broken in A2495?
Thomas Pasini, Myriam Gitti, Fabrizio Brighenti +6
We present a combined radio/X-ray analysis of the poorly studied galaxy cluster Abell 2495 (z=0.07923) based on new EVLA and Chandra data. We also analyze and discuss Halpha emissi…
Searching for Super-Eddington Quasars using a Photon Trapping Accretion Disc Model
Quentin Pognan, Benny Trakhtenbrot, Tullia Sbarrato +2
Accretion onto black holes at rates above the Eddington limit has long been discussed in the context of supermassive black hole (SMBH) formation and evolution, providing a possible…
The KMOS^3D Survey: data release and final survey paper
E. Wisnioski, N. M. Förster Schreiber, M. Fossati +28
We present the completed KMOS survey an integral field spectroscopic survey of 739, , galaxies at using the K-band Multi…
Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback
R. S. Beckmann, Y. Dubois, P. Guillard +8
Extended filamentary H emission nebulae are a striking feature of nearby galaxy clusters but the formation mechanism of the filaments, and the processes which shape their morpho…
Stellar mass -- halo mass relation for the brightest central galaxies of X-ray clusters since z~0.65
G. Erfanianfar, A. Finoguenov, K. Furnell +25
We present the brightest cluster galaxies (BCGs) catalog for SPectroscoic IDentification of eROSITA Sources (SPIDERS) DR14 cluster program value-added catalog. We list the 416 BCGs…
The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method
Rachael L. Beaton, Mark Seibert, Dylan Hatt +9
The Carnegie-Chicago Hubble Program (CCHP) is building a direct path to the Hubble constant (H0) using Population II stars as the calibrator of the SN Ia-based distance scale. This…
Understanding the Discrepancy between IRX and Balmer Decrement in Tracing Galaxy Dust Attenuation
Jianbo Qin, Xian Zhong Zheng, Stijn Wuyts +2
We compare the infrared excess (IRX) and Balmer decrement () as dust attenuation indicators in relation to other galaxy parameters using a sample of 32 000 local…
New constraints on the physical conditions in H-bearing GRB-host damped Lyman- absorbers
K. E. Heintz, J. Bolmer, C. Ledoux +25
We report the detections of molecular hydrogen (H), vibrationally-excited H (H), and neutral atomic carbon (CI), in two new afterglow spectra of GRBs\,181020A ($z=2.9…
The first spectroscopic dust reverberation programme on active galactic nuclei: the torus in NGC 5548
H. Landt, M. J. Ward, D. Kynoch +16
We have recently initiated the first spectroscopic dust reverberation programme on active galactic nuclei (AGN) in the near-infrared. Spectroscopy enables measurement of dust prope…
The CANDELS/SHARDS multi-wavelength catalog in GOODS-N: Photometry, Photometric Redshifts, Stellar Masses, Emission line fluxes and Star Formation Rates
Guillermo Barro, Pablo G. Perez-Gonzalez, Antonio Cava +52
We present a WFC3 F160W (-band) selected catalog in the CANDELS/GOODS-N field containing photometry from the ultraviolet (UV) to the far-infrared (IR), photometric redshifts and…
Constraining cold accretion onto supermassive black holes: molecular gas in the cores of eight brightest cluster galaxies revealed by joint CO and CN absorption
Tom Rose, A. C. Edge, F. Combes +18
To advance our understanding of the fuelling and feedback processes which power the Universe's most massive black holes, we require a significant increase in our knowledge of the m…
Space Telescope and Optical Reverberation Mapping Project. VIII. Time Variability of Emission and Absorption in NGC 5548 Based on Modeling the Ultraviolet Spectrum
G. A. Kriss, G. De Rosa, J. Ely +164
We model the ultraviolet spectra of the Seyfert 1 galaxy NGC~5548 obtained with the Hubble Space Telescope during the 6-month reverberation-mapping campaign in 2014. Our model of t…
The Evolution and Origin of Ionized Gas Velocity Dispersion from to with KMOS
Hannah D. N. Übler, Reinhard Genzel, Emily Wisnioski +27
We present the evolution of the ionized gas velocity dispersion in 175 star-forming disk galaxies based on data from the full KMOS integral field spectroscop…
Nuclear kinematics in nearby AGN. I. An ALMA perspective on the Morphology and Kinematics of the molecular CO(2-1) emission
V. Ramakrishnan, N. M. Nagar, C. Finlez +6
We present the molecular gas morphology and kinematics of seven nearby Seyfert galaxies obtained from our 230~GHz ALMA observations. The CO J=2-1 kinematics within the inner $\sim3…
Major mergers are not the dominant trigger for high-accretion AGNs at z = 2
V. Marian, K. Jahnke, M. Mechtley +8
Research over the past decade has shown diminishing empirical evidence for major galaxy mergers being a dominating or even important mechanism for the growth of supermassive black…
A Universal Relation of Dust Obscuration Across Cosmic Time
Jianbo Qin, X. Z. Zheng, Stijn Wuyts +2
We investigate dust obscuration as parameterised by the infrared excess IRX in relation to global galaxy properties, using a sample of 3200…
PHIBSS2: survey design and z=0.5-0.8 results. Molecular gas reservoirs during the winding-down of star formation
J. Freundlich, F. Combes, L. J. Tacconi +29
Following the success of the Plateau de Bure high-z Blue Sequence Survey (PHIBSS), we present the PHIBSS2 legacy program, a survey of the molecular gas properties of star-forming g…
Interpreting the star formation - extinction relation with MaNGA
Huan Li, Stijn Wuyts, Lei Hao +5
We investigate the resolved relation between local extinction and star formation surface density within nearby star-forming galaxies selected from the MaNGA survey. Balmer decremen…
Present-day mass-metallicity relation for galaxies using a new electron-temperature method
Robert M. Yates, Patricia Schady, Ting-Wan Chen +2
We investigate electron temperature (Te) and gas-phase oxygen abundance (Z_Te) measurements for galaxies in the local Universe (z < 0.25). Our sample comprises spectra from a total…