Timothy Faerber
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View article: Expansion Signatures in 35 HII Regions traced by SOFIA [CII] Emission
Expansion Signatures in 35 HII Regions traced by SOFIA [CII] Emission Open
We analyze the expansion signatures of 35 HII regions mapped in [CII] 158 micron emission by the Stratospheric Observatory for Infrared Astronomy (SOFIA). The [CII] emission primarily traces photodissociation regions (PDRs) at the transiti…
View article: Supernova remnant candidates discovered by the SARAO MeerKAT Galactic Plane Survey
Supernova remnant candidates discovered by the SARAO MeerKAT Galactic Plane Survey Open
Context . Sensitive radio continuum data could bring the number of known supernova remnants (SNRs) in the Galaxy more in line with what is expected. Due to confusion in the Galactic plane, however, faint SNRs can be challenging to distingu…
View article: Supernova Remnant Candidates Discovered by the SARAO MeerKAT Galactic Plane Survey
Supernova Remnant Candidates Discovered by the SARAO MeerKAT Galactic Plane Survey Open
Context. Sensitive radio continuum data could remove the difference between the number of known supernova remnants (SNRs) in the Galaxy compared to that expected, but due to confusion in the Galactic plane, faint SNRs can be challenging to…
View article: In-Situ Field Massive Star Formation in the Small Magellanic Cloud
In-Situ Field Massive Star Formation in the Small Magellanic Cloud Open
A fundamental question for theories of massive star formation is whether OB stars can form in isolation. We assess the contribution of any in-situ OB star formation by using 210 field OB stars in the Small Magellanic Cloud (SMC) from the R…
View article: A Chi-Squared Analysis of the Measurements of Two Cosmological Parameters Over Time
A Chi-Squared Analysis of the Measurements of Two Cosmological Parameters Over Time Open
The aim of this analysis was to determine whether or not the given error bars truly represented the dispersion of values in a historical compilation of two cosmological parameters: the amplitude of mass fluctuations ($σ_8$) and Hubble's co…
View article: A Chi-Squared Analysis of the Measurements of Two Cosmological\n Parameters Over Time
A Chi-Squared Analysis of the Measurements of Two Cosmological\n Parameters Over Time Open
The aim of this analysis was to determine whether or not the given error bars\ntruly represented the dispersion of values in a historical compilation of two\ncosmological parameters: the amplitude of mass fluctuations ($\\sigma_8$) and\nHu…
View article: A Chi-Squared Analysis of the Measurements of Two Cosmological Parameters over Time
A Chi-Squared Analysis of the Measurements of Two Cosmological Parameters over Time Open
The aim of this analysis was to determine whether or not the given error bars truly represented the dispersion of values in a historical compilation of two cosmological parameters: the amplitude of mass fluctuations (σ8) and Hubble’s const…
View article: Properties of Near-Infrared Type Ia Supernovae Light Curves
Properties of Near-Infrared Type Ia Supernovae Light Curves Open
As a result of the standardizability of SNe Ia light curves over a wide range of photometric bands, they are used as standard candles to accurately measure distances in the cosmos up to z ≈ 1 [22]. As dust extinction is smaller in the NIR …
View article: Large-Scale Structure under Λ-CDM Paradigm
Large-Scale Structure under Λ-CDM Paradigm Open