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Record W7049030091

Mira and Cepheid Variables as Extragalactic Distance Indicators in the Optical and the Near-Infrared

2023· dissertation· en· W7049030091 on OpenAlexaboutno aff

Bibliographic record

VenueOakTrust (Texas A&M University Libraries) · 2023
Typedissertation
Languageen
FieldEngineering
TopicAdvanced Electrical Measurement Techniques
Canadian institutionsnot available
Fundersnot available
KeywordsCepheid variableMilky WayLight curveVariable starLarge Magellanic CloudGalaxyAstrometryGravitational lensPhotometry (optics)Stars
DOInot available

Abstract

fetched live from OpenAlex

Local measurements of the Hubble constant rely on extragalactic distance measurements, which are made using observations of Type Ia supernovae and certain variable stars. This dissertation focuses on two classes of variable star that are used to make distance measurements: Classical Cepheids and Mira variables.\n\nThe Legacy Survey of Space and Time (LSST), which will be conducted at the Vera C. Rubin Observatory, will return time-series data that have an ideal cadence for Mira studies. In anticipation of these data, we perform a search for Miras in the LSST photometric bands. We use archival optical and near-infrared observations of the galaxy M33 taken with the Canada-France-Hawaii Telescope’s MegaCam and WIRCam instruments. We use machine learning classifiers to efficiently identify strong Mira candidates, which are visually confirmed. We also use period-luminosity relations for Miras in the Large Magellanic Cloud to identify Mira candidates in M33. We present the first empirical characterization of Miras in the LSST bands. We also recover approximately 70 percent of a sample of previously identified Miras and identify 2,916 new Mira candidates. For the first time, we find evidence for a first-overtone pulsation sequence in M33’s Miras.\n\nWe also present H-band Milky Way Cepheid light curves extracted via difference imaging from observations taken with the United Kingdom InfraRed Telecope’s Wide-Field Infrared Camera. The crowded nature of the Cepheid fields renders traditional photometric methods less effective, so we adapt and deploy a difference imaging pipeline originally written for data from the Transiting Exoplanet Survey Satellite. The light curves are used to derive corrections to “mean light” for random-phase Hubble Space Telescope observations. The phase corrections obtained from the H-band light curves are in good agreement with similar corrections obtained from VI light curves from the literature.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.002
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.003
Threshold uncertainty score0.007

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.002
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0020.002
Science and technology studies0.0000.000
Scholarly communication0.0020.001
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0020.001

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.006
GPT teacher head0.192
Teacher spread0.185 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designObservational
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations0
Published2023
Admission routes1
Has abstractyes

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