NLS1-2018
9-13 April 2018
Padova Botanical Garden, Italy
published December 21, 2018
Padova Botanical Garden, Italy
published December 21, 2018
Although more than 30 years have passed since their discovery, narrow-line Seyfert 1 galaxies (NLS1s) still present challenges for unified models of active galactic nuclei (AGN). Sources of electromagnetic emission at all frequencies, their physical properties and role in galaxy evolution remain poorly understood. The aim of this workshop is to present and to discuss developments in the field over the seven years since the most recent NLS1 conference (Milano 2011). The main topics of the workshop will include the multiwavelength properties of these objects from radio wavelengths to gamma rays, their role in AGN evolution, their relationship to other classes of AGN, and their place in the framework of AGN unified models. The workshop will be held at the Orto Botanico di Padova (Italy), the world's oldest academic botanical garden. During the event, a one-hour session will be devoted to the topic of gender balance in astrophysics. This session will be dedicated to Lucrezia Cornaro of the University of Padova, the first woman in the world to obtain a Ph.D. degree. We will commemorate the 340th anniversary of this event.
Editorial Board
- Sonia Antón
CIDMA, University of Aveiro, Portugal - Marco Berton
Università Padova - Luigi Foschini
INAF-Osservatorio Astronomoco di Brera in Merate, Merate, Italy - Dragana Ilic
Department of Astronomy - Faculty of Mathematics - Unviversity of Belgrade - Preeti Kharb
National Centre for Radio Astrophysics - Tata Institute of Fundamental Research - Wolfram Kollatschny
Institute for Astrophysics, Göttingen University, Germany - Anne Lähteenmäki
Aalto University Metsähovi Radio Observatory - Bradley Peterson
Department of Astronomy, The Ohio State University, USA - Luka Popovic
Astronomical Observatory of Belgrade, Republic of Serbia - Piero Rafanelli
Department of Astronomy - University of Padua - Eleonora Sani
European Southern Observatory, Chile
| Sessions |
|---|
| Optical properties of NLS1 galaxies |
| Jetted NLS1s |
| The central engine |
| Black hole and host galaxy |
| Poster |
| Optical properties of NLS1 galaxies |
|---|
|
Polarization in the broad lines of NLSy1 and BLSy1 galaxies
|
|
Narrow-line Seyfert 1s: what is wrong in a name?
|
|
Narrow Line Seyfert 1 galaxies in the era of large surveys
|
|
A catalog of narrow-line Seyfert 1 galaxies in the southern hemisphere
|
|
Models of optical emission lines to investigate Narrow-Line Seyfert 1 galaxies in spectroscopic databases
|
|
Fe II reverberation in narrow-line Seyfert 1 galaxies
|
|
Fe II velocity shifts in optical spectra of type 1 AGN
|
|
Reverberation Mapping and Implications for Narrow-Line Seyfert 1 Galaxies
|
|
Reverberation mapping of narrow-line Seyfert 1 galaxies: shortened Hbeta lags
|
|
Modeling time-dependence of continuum and polarized optical-UV emission in AGN
|
|
Saturated luminosity of slim accretion disks in narrow line Seyfert 1 galaxies
|
|
Changing-look Narrow-Line Seyfert 1s?
|
|
Interrogating narrow-line regions: Spatially probing metallicity and the radiation field
|
|
Narrow Line Seyfert 1 galaxies in the context of Quasar Main Sequence
|
|
Long-term spectral optical monitoring of Ark 564
|
| Jetted NLS1s |
|
Multi-wavelength properties of radio-loud Narrow-line Seyfert 1 galaxies
|
|
On the multiwavelength properties of several γ-ray detected narrow-line Seyfert 1 galaxies
|
|
A close look at the gamma-ray emitting NLSy1 FBQS J1644+2619
|
|
The gamma-ray emitting NLS1 1H 0323+342 and the disc-jet connection
|
|
Optical polarisation variability of narrow line Seyfert 1 galaxies
|
|
GeV gamma-ray narrow-line Seyfert 1 galaxies and the Fermi LAT Flare Advocate service
|
|
Simulations of gamma-ray narrow-line Seyfert 1 galaxies with the Cherenkov Telescope Array
|
|
Radio Properties of Narrow-Line Seyfert 1 Galaxies
|
|
Parsec-scale Nuclear Radio Structures in Seyfert Galaxies
|
|
High-frequency radio properties of NLS1 galaxies
|
|
VLBI study of the jets in radio-loud narrow-line Seyfert 1 galaxies
|
|
An updated view on the parent population of $\gamma$-ray emitting narrow-line Seyfert 1 galaxies
|
|
The nature of the gamma-ray emitting PKS 2004-447: CSS or NLS1?
|
|
Kpc-scale radio-jets in narrow-line Seyfert 1 galaxies
|
| The central engine |
|
Relativistic spectroscopy of the extreme NLS1 IRAS 13224-3809
|
|
Radio and X-ray variability of the NLSy1 Mkn 110
|
|
Soft X-ray excess emission in NLS1 galaxies
|
|
X-ray perspective of Narrow-line Seyfert 1 galaxies
|
|
Ionized outflows in the NLSy1 IZw1: departing from the classical picture
|
|
Narrow Line Seyfert 1s in the IBISCO Sample
|
|
Testing General Relativity with X-ray Reflection Spectroscopy of a ’Bare’ Active Galactic Nucleus
|
|
The nature of X-ray spectral variability in MCG-6-30-15
|
|
On the underlying physics of NLS1
|
| Black hole and host galaxy |
|
The Warm Polar Dust in the NLS1 ESO 323-G77
|
|
Infrared variability of radio-loud narrow-line Seyfert 1 galaxies
|
|
X-ray variability plane using NLSy1 and Sy1: Importance of obscuration
|
|
The mass of NLS1 black holes: reconciling accretion disk and virial estimates
|
|
The host galaxies of radio-loud vs. gamma-loud Narrow-Line Seyfert 1s
|
|
Host galaxies of jetted narrow-line Seyfert 1 galaxies
|
|
What is in a radio loud NLS1?
|
| Poster |
|
The link between X-ray complexity and optical lines in NLS1s
|
|
Comparison of the rich optical Fe II line spectra of selected I Zw 1 type objects from two epochs
|
|
Chemi-ionization processes in Narrow-Line Seyfert 1 Galaxies
|
|
Using vo tools to investigate Quasar Spectra (UNIQS)
|
|
Kinematic differences between NLS1 and BLAGN sources
|
|
FAQS: Fitting Automatic Quasar Spectra
|
|
The intrinsic Baldwin effect in NLSy1 galaxies
|
|
FSRQs, BL Lacs, and NLS1s: all that jets
|
|
A Dynamical Modeling for Broad-Line Regions in Narrow-Line Seyfert Galaxies
|
|
Accretion disk reverberation mapping of Active Galactic Nuclei at Wise Observatory
|
|
The broad line region and dust torus structure of the Seyfert 1 WPVS48
|
|
NLS1 vs BLS1: Polarization observations and modeling
|
