The Carnegie-Chicago Hubble Program. V. the Distances to NGC 1448 and NGC 1316 via the Tip of the Red Giant Branch

Dylan Hatt, Wendy L. Freedman, Barry F. Madore, In Sung Jang, Rachael L. Beaton, Taylor J. Hoyt, Myung Gyoon Lee, Andrew J. Monson, Jeffrey A. Rich, Victoria Scowcroft, Mark Seibert

Research output: Contribution to journalArticle

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Abstract

The Carnegie-Chicago Hubble Program (CCHP) is recalibrating the extragalactic SN Ia distance scale using exclusively Population II stars. This effort focuses on the Tip of the Red Giant Branch (TRGB) method, whose systematics are entirely independent of the Population I Cepheid-based determinations that have long served as calibrators for the SN Ia distance scale. We present deep Hubble Space Telescope imaging of the low surface density and low line-of-sight reddening halos of two galaxies, NGC 1448 and NGC 1316, each of which have been hosts to recent SN Ia events. Provisionally anchoring the TRGB zero-point to the geometric distance to the Large Magellanic Cloud derived from detached eclipsing binaries, we measure extinction-corrected distance moduli of 31.23 ± 0.04stat ± 0.06sys mag for NGC 1448 and 31.37 ± 0.04stat ± 0.06sys mag for NGC 1316, respectively, giving metric distances of 17.7 ± 0.3stat ± 0.5sys Mpc, and 18.8 ± 0.3stat ± 0.5sys Mpc. We find agreement between our result and the available Cepheid distance for NGC 1448; for NGC 1316, where there are relatively few published distances based on direct measurements, we find that our result is consistent with the published SN Ia distances whose absolute scales are set from other locally determined methods such as Cepheids. For NGC 1448 and NGC 1316, our distances are some of the most precise (and systematically accurate) measurements with errors at 1.7 (2.8)% and 1.6 (2.7)% levels, respectively.

Original languageEnglish (US)
Article number145
JournalAstrophysical Journal
Volume866
Issue number2
DOIs
StatePublished - Oct 20 2018

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extinction
Population II stars
programme
method
Magellanic clouds
Hubble Space Telescope
line of sight
halos
galaxies

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Hatt, D., Freedman, W. L., Madore, B. F., Jang, I. S., Beaton, R. L., Hoyt, T. J., ... Seibert, M. (2018). The Carnegie-Chicago Hubble Program. V. the Distances to NGC 1448 and NGC 1316 via the Tip of the Red Giant Branch. Astrophysical Journal, 866(2), [145]. https://doi.org/10.3847/1538-4357/aadfe8
Hatt, Dylan ; Freedman, Wendy L. ; Madore, Barry F. ; Jang, In Sung ; Beaton, Rachael L. ; Hoyt, Taylor J. ; Lee, Myung Gyoon ; Monson, Andrew J. ; Rich, Jeffrey A. ; Scowcroft, Victoria ; Seibert, Mark. / The Carnegie-Chicago Hubble Program. V. the Distances to NGC 1448 and NGC 1316 via the Tip of the Red Giant Branch. In: Astrophysical Journal. 2018 ; Vol. 866, No. 2.
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abstract = "The Carnegie-Chicago Hubble Program (CCHP) is recalibrating the extragalactic SN Ia distance scale using exclusively Population II stars. This effort focuses on the Tip of the Red Giant Branch (TRGB) method, whose systematics are entirely independent of the Population I Cepheid-based determinations that have long served as calibrators for the SN Ia distance scale. We present deep Hubble Space Telescope imaging of the low surface density and low line-of-sight reddening halos of two galaxies, NGC 1448 and NGC 1316, each of which have been hosts to recent SN Ia events. Provisionally anchoring the TRGB zero-point to the geometric distance to the Large Magellanic Cloud derived from detached eclipsing binaries, we measure extinction-corrected distance moduli of 31.23 ± 0.04stat ± 0.06sys mag for NGC 1448 and 31.37 ± 0.04stat ± 0.06sys mag for NGC 1316, respectively, giving metric distances of 17.7 ± 0.3stat ± 0.5sys Mpc, and 18.8 ± 0.3stat ± 0.5sys Mpc. We find agreement between our result and the available Cepheid distance for NGC 1448; for NGC 1316, where there are relatively few published distances based on direct measurements, we find that our result is consistent with the published SN Ia distances whose absolute scales are set from other locally determined methods such as Cepheids. For NGC 1448 and NGC 1316, our distances are some of the most precise (and systematically accurate) measurements with errors at 1.7 (2.8){\%} and 1.6 (2.7){\%} levels, respectively.",
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Hatt, D, Freedman, WL, Madore, BF, Jang, IS, Beaton, RL, Hoyt, TJ, Lee, MG, Monson, AJ, Rich, JA, Scowcroft, V & Seibert, M 2018, 'The Carnegie-Chicago Hubble Program. V. the Distances to NGC 1448 and NGC 1316 via the Tip of the Red Giant Branch', Astrophysical Journal, vol. 866, no. 2, 145. https://doi.org/10.3847/1538-4357/aadfe8

The Carnegie-Chicago Hubble Program. V. the Distances to NGC 1448 and NGC 1316 via the Tip of the Red Giant Branch. / Hatt, Dylan; Freedman, Wendy L.; Madore, Barry F.; Jang, In Sung; Beaton, Rachael L.; Hoyt, Taylor J.; Lee, Myung Gyoon; Monson, Andrew J.; Rich, Jeffrey A.; Scowcroft, Victoria; Seibert, Mark.

In: Astrophysical Journal, Vol. 866, No. 2, 145, 20.10.2018.

Research output: Contribution to journalArticle

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T1 - The Carnegie-Chicago Hubble Program. V. the Distances to NGC 1448 and NGC 1316 via the Tip of the Red Giant Branch

AU - Hatt, Dylan

AU - Freedman, Wendy L.

AU - Madore, Barry F.

AU - Jang, In Sung

AU - Beaton, Rachael L.

AU - Hoyt, Taylor J.

AU - Lee, Myung Gyoon

AU - Monson, Andrew J.

AU - Rich, Jeffrey A.

AU - Scowcroft, Victoria

AU - Seibert, Mark

PY - 2018/10/20

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