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Tully-Fisher Distance Measurements of Spiral Galaxies with Well-Observed Type Ia Supernovae

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Tully-Fisher Distance Measurements of Spiral Galaxies with Well-Observed Type Ia Supernovae ResearchOnline@JCU This file is part of the following reference: Seibel, Daryl Lee (2016) Tully-Fisher distance measurements of spiral galaxies with well-observed type Ia supernovae. PhD thesis, James Cook University. Access to this file is available from: http://researchonline.jcu.edu.au/49763/ The author has certified to JCU that they have made a reasonable effort to gain permission and acknowledge the owner of any third party copyright material included in this document. If you believe that this is not the case, please contact [email protected] and quote http://researchonline.jcu.edu.au/49763/ TULLY-FISHER DISTANCE MEASUREMENTS OF SPIRAL GALAXIES WITH WELL-OBSERVED TYPE Ia SUPERNOVAE Thesis submitted by Daryl Lee SEIBEL BPA MBA MSc 07 November 2016 For the degree of Doctor of Philosophy in Astronomy in the Centre for Astronomy James Cook University Townsville QLD, Australia STATEMENT OF ACCESS I, Daryl L. Seibel, author of this work, understand that James Cook University will make this thesis available for use within the University Library and, via the Australian Digital Thesis network, for use elsewhere. I understand that, as an unpublished work, a thesis has significant protection under the Copyright Act and I do not wish to place any further restriction on access to this work. Daryl L. SEIBEL 07 November 2016 Signature Date ii STATEMENT OF SOURCES I, Daryl L. Seibel, declare that this thesis is my own work and has not been submitted in any form for another degree or diploma at any university or other institution of tertiary education. Information derived from the published or unpublished work of others has been acknowledged in the text and a list of references is given. Daryl L. SEIBEL 07 November 2016 Signature Date iii STATEMENT OF ELECTRONIC COPY I, Daryl L. Seibel, the author of this work, declare that the electronic copy of this thesis provided to the James Cook University Library is an accurate copy of the print thesis submitted, within the limits of the technology available. Daryl L. SEIBEL 07 November 2016 Signature Date iv STATEMENT OF CONTRIBUTION OF OTHERS I, Daryl L. Seibel, author of this thesis acknowledge the contribution of John Danziger of Observatorio Astronomico di Trieste, as supervisor for this project, and David Blank of JCU as initial co-supervisor, for the editorial assistance of this paper. I acknowledge the contribution of Ray Cooke, Université Bordeaux for the editorial comments for the preliminary version of this paper. I acknowledge Lister Staveley-Smith, of the University of Western Australia for the contributory analysis and suggestions for the finalization of the thesis. I acknowledge the contribution of Lister Staveley-Smith, of the University of Western Australia, and John Danziger for the observational supervision at the Parkes 64 m Radio Telescope and data reduction at CSIRO ATNF at Sydney, Australia for the Parkes sample. I acknowledge the contribution of John Danziger for the initial collection of the Literature, Parkes, and the Parkes / NTT samples. I acknowledge the contribution of Preben Grosbøl for the NIR observations at ESO La Silla, Chile for the Parkes / NTT sample. I acknowledge the contribution of Lister Staveley-Smith and John Danziger for the 21 cm line width velocity measurements at the Parkes 64 m Radio Telescope and data reduction at CSIRO ATNF at Sydney, Australia for the 51-galaxy sub-sample of the Parkes / NTT sample set. I acknowledge the contributions of Christina Magoulas for the assistance in using the Erdoğdu predictive peculiar velocity algorithm. I declare that I made use of the advice of Lister Staveley-Smith of the University of Western Australia for the finalisation of this thesis. I declare I did use the infrastructure of CSIRO ATNF for the use of the Parkes 64 m Radio Telescope for the observations in the course of the research for this thesis. I declare I did use the infrastructure of ESO for the use of SOFI on the 3.5 m NTT, and TAROT at the La Silla Observatory, for the observations in the course of the research for this thesis. v I declare there were no other infrastructures external to JCU or external to an organisational unit within JCU used for this thesis. I declare there were no other fees, stipend support, other supervision or collaborations, statistical support, editorial assistance, research assistance or other assistance. Daryl L. SEIBEL 07 November 2016 Signature Date vi CONTENTS ACKNOWLEDGMENT ............................................................................................. xvi ABSTRACT .................................................................................................................... 1 1 INTRODUCTION 1.1 Aim ................................................................................................................. 3 1.2 Lambda-CDM ................................................................................................ 3 1.3 The Distance Ladder ...................................................................................... 4 1.4 The Tully-Fisher (TF) Relation: discovery .................................................... 5 1.5 The Tully-Fisher Relation: refinement ........................................................... 6 1.6 Malmquist Bias ............................................................................................ 10 1.7 Type Ia Supernovae ...................................................................................... 11 1.8 The Hubble Constant .................................................................................... 13 1.9 Peculiar Velocities ........................................................................................ 16 References .......................................................................................................... 18 2 TULLY-FISHER AND SNe Ia TEMPLATES 2.1 Tully-Fisher Relation ................................................................................... 22 2.2 SNe Ia Distance Scale .................................................................................. 27 References .......................................................................................................... 30 3 DATA FOR A LITERATURE-SAMPLE WITH WELL-OBSERVED SNe Ia 3.1 Sample Overview ......................................................................................... 32 3.2 Detailed Data ................................................................................................ 32 3.2.1 Apparent Magnitudes .................................................................... 34 3.2.2 Distance Moduli ............................................................................ 36 3.3 Summary ...................................................................................................... 37 References .......................................................................................................... 64 vii 4 PARKES OBSERVATIONS OF HOST GALAXIES WITH WELL-OBSERVED SNe Ia 4.1 The Joint Parkes and SNe Ia Sample (the Parkes Sample) .......................... 67 4.2 The Parkes Multibeam Receiver .................................................................. 67 4.2.1 Observations and Reduction .......................................................... 69 4.3 Parameterisation ........................................................................................... 70 4.4 Tabulation of the Parkes Data ...................................................................... 79 4.5 Results .......................................................................................................... 81 4.6 Summary ...................................................................................................... 85 References ........................................................................................................ 105 5 PARKES / NTT SAMPLE NEW NIR AND 21 CM LINE WIDTH VELOCITY MEASUREMENTS 5.1 The Parkes / NTT Sample .......................................................................... 107 5.2 Light Curve of SN Ia 2012fr ...................................................................... 108 5.3 The Tully-Fisher Relation Measurements .................................................. 109 5.4 Calculations for the SNe Ia ........................................................................ 111 5.5 Summary .................................................................................................... 112 References ........................................................................................................ 142 6 DISCUSSION FOR THE THREE SAMPLE SETS 6.1 The Combined Data ................................................................................... 143 6.2 The Hubble Constant .................................................................................. 155 6.3 Galaxy Morphology and Bars .................................................................... 157 6.4 Malmquist Bias .......................................................................................... 157 6.5 Peculiar Velocities ...................................................................................... 161 6.5.1 Bulk Flow .................................................................................... 161 6.5.2 Matter Density ............................................................................. 165 References ........................................................................................................ 171 7 CONCLUSION FOR THE THREE SAMPLE SETS Conclusions .....................................................................................................
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