AGN obscuration and the Unified Model
Unification Models of Active Galactic Nuclei postulate that all the observed differences
between type 1 and type 2 objects are due to orientation effects with respect to the line of …
between type 1 and type 2 objects are due to orientation effects with respect to the line of …
High-z galaxies with JWST and local analogues–it is not only star formation
J Brinchmann - Monthly Notices of the Royal Astronomical …, 2023 - academic.oup.com
ABSTRACT I present an analysis of the JWST NIRSpec data of SMACS 0723 released as
Early Release Observations. As part of this three new redshifts are provided, bringing the …
Early Release Observations. As part of this three new redshifts are provided, bringing the …
Star formation inside a galactic outflow
Recent observations have revealed massive galactic molecular outflows,, that may have the
physical conditions (high gas densities,,) required to form stars. Indeed, several recent …
physical conditions (high gas densities,,) required to form stars. Indeed, several recent …
Determining star formation rates for infrared galaxies
We show that measures of star formation rates (SFRs) for infrared galaxies using either
single-band 24 μm or extinction-corrected Paα luminosities are consistent in the total …
single-band 24 μm or extinction-corrected Paα luminosities are consistent in the total …
PS16dtm: a tidal disruption event in a narrow-line Seyfert 1 galaxy
We present observations of PS16dtm (also known as SN 2016ezh), a luminous transient that
occurred at the nucleus of a narrow-line Seyfert 1 galaxy hosting a 10 6 M⊙ black hole. The …
occurred at the nucleus of a narrow-line Seyfert 1 galaxy hosting a 10 6 M⊙ black hole. The …
BASS. XXV. DR2 Broad-line-based Black Hole Mass Estimates and Biases from Obscuration
JE Mejía-Restrepo, B Trakhtenbrot… - The Astrophysical …, 2022 - iopscience.iop.org
We present measurements of broad emission lines and virial estimates of supermassive
black hole masses (M BH) for a large sample of ultrahard X-ray-selected active galactic …
black hole masses (M BH) for a large sample of ultrahard X-ray-selected active galactic …
A sample of massive black holes in dwarf galaxies detected via [Fe X] coronal line emission: active galactic nuclei and/or tidal disruption events
M Molina, AE Reines, L Latimer… - The Astrophysical …, 2021 - iopscience.iop.org
The massive black hole (BH) population in dwarf galaxies (M BH≲ 10 5 M⊙) can provide
strong constraints on the origin of BH seeds. However, traditional optical searches for active …
strong constraints on the origin of BH seeds. However, traditional optical searches for active …
Torus and active galactic nucleus properties of nearby seyfert galaxies: Results from fitting infrared spectral energy distributions and spectroscopy
We used the CLUMPY torus models and a Bayesian approach to fit the infrared spectral
energy distributions and ground-based high angular resolution mid-infrared spectroscopy of …
energy distributions and ground-based high angular resolution mid-infrared spectroscopy of …
The AGNIFS survey: spatially resolved observations of hot molecular and ionized outflows in nearby active galaxies
We present the hot molecular and warm ionized gas kinematics for 33 nearby (0.001≲ z≲
0.056) X-ray selected active galaxies using the H m and Br γ emission lines observed in the …
0.056) X-ray selected active galaxies using the H m and Br γ emission lines observed in the …
BASS. XXIX. The near-infrared view of the broad-line region (BLR): the effects of obscuration in BLR characterization
F Ricci, E Treister, FE Bauer… - The Astrophysical …, 2022 - iopscience.iop.org
Virial black hole (BH) mass (M BH) determination directly involves knowing the broad-line
region (BLR) clouds' velocity distribution, their distance from the central supermassive BH (R …
region (BLR) clouds' velocity distribution, their distance from the central supermassive BH (R …