The interstellar dust properties of nearby galaxies

F Galliano, M Galametz, AP Jones - Annual Review of …, 2018 - annualreviews.org
This article gives an overview of the constitution, physical conditions, and observables of
dust in the interstellar medium of nearby galaxies. We first review the macroscopic, spatial …

Hubble tension or a transition of the Cepheid SnIa calibrator parameters?

L Perivolaropoulos, F Skara - Physical Review D, 2021 - APS
We reanalyze the Cepheid data used to infer the value of the Hubble constant H 0 by
calibrating type Ia supernovae. We do not enforce a universal value of the empirical …

The HDUV Survey: a revised assessment of the relationship between UV slope and dust attenuation for high-redshift galaxies

NA Reddy, PA Oesch, RJ Bouwens… - The Astrophysical …, 2018 - iopscience.iop.org
We use a newly assembled sample of 3545 star-forming galaxies with secure spectroscopic,
grism, and photometric redshifts at z= 1.5–2.5 to constrain the relationship between UV …

[图书][B] Supernova explosions

D Branch, JC Wheeler - 2017 - Springer
JCW had long wanted to write a new monograph on supernovae. Despite an immense
explosion in the literature and many review articles, there had not been one since that of …

Sensitivity of the Hubble constant determination to Cepheid calibration

E Mörtsell, A Goobar, J Johansson… - The Astrophysical …, 2022 - iopscience.iop.org
Motivated by the large observed diversity in the properties of extragalactic extinction by dust,
we reanalyze the Cepheid calibration used to infer the Hubble constant, H 0, from Type Ia …

A JWST near-and mid-infrared nebular spectrum of the type Ia supernova 2021aefx

LA Kwok, SW Jha, T Temim, OD Fox… - The Astrophysical …, 2023 - iopscience.iop.org
We present JWST near-infrared (NIR) and mid-infrared (MIR) spectroscopic observations of
the nearby normal Type Ia supernova (SN) SN 2021aefx in the nebular phase at+ 255 days …

Cobalt-56 γ-ray emission lines from the type Ia supernova 2014J

E Churazov, R Sunyaev, J Isern, J Knödlseder, P Jean… - Nature, 2014 - nature.com
A type Ia supernova is thought to be a thermonuclear explosion of either a single carbon–
oxygen white dwarf or a pair of merging white dwarfs. The explosion fuses a large amount of …

A hierarchical Bayesian SED model for Type Ia supernovae in the optical to near-infrared

KS Mandel, S Thorp, G Narayan… - Monthly Notices of …, 2022 - academic.oup.com
ABSTRACT While conventional Type Ia supernova (SN Ia) cosmology analyses rely
primarily on rest-frame optical light curves to determine distances, SNe Ia are excellent …

Astronomical Distance Determination in the Space Age: Secondary Distance Indicators

B Czerny, R Beaton, M Bejger, E Cackett… - Space Science …, 2018 - Springer
The formal division of the distance indicators into primary and secondary leads to difficulties
in description of methods which can actually be used in two ways: with, and without the …

Near-infrared supernova Ia distances: host galaxy extinction and mass-step corrections revisited

J Johansson, SB Cenko, OD Fox… - The Astrophysical …, 2021 - iopscience.iop.org
We present optical and near-infrared (NIR, Y-, J-, H-band) observations of 42 Type Ia
supernovae (SNe Ia) discovered by the untargeted intermediate Palomar Transient Factory …