The Astrophysical Journal (Jan 2024)
Carnegie Supernova Project I and II: Measurements of H 0 Using Cepheid, Tip of the Red Giant Branch, and Surface Brightness Fluctuation Distance Calibration to Type Ia Supernovae
- Syed A. Uddin,
- Christopher R. Burns,
- M M. Phillips,
- Nicholas B. Suntzeff,
- Wendy L. Freedman,
- Peter J. Brown,
- Nidia Morrell,
- Mario Hamuy,
- Kevin Krisciunas,
- Lifan Wang,
- Eric Y. Hsiao,
- Ariel Goobar,
- Saul Perlmutter,
- Jing Lu,
- Maximilian Stritzinger,
- Joseph P. Anderson,
- Chris Ashall,
- Peter Hoeflich,
- Benjamin J. Shappee,
- S. E. Persson,
- Anthony L. Piro,
- E Baron,
- Carlos Contreras,
- Lluís Galbany,
- Sahana Kumar,
- Melissa Shahbandeh,
- Scott Davis,
- Jorge Anais,
- Luis Busta,
- Abdo Campillay,
- Sergio Castellón,
- Carlos Corco,
- Tiara Diamond,
- Christa Gall,
- Consuelo Gonzalez,
- Simon Holmbo,
- Miguel Roth,
- Jacqueline Serón,
- Francesco Taddia,
- Simón Torres,
- Charles Baltay,
- Gastón Folatelli,
- Ellie Hadjiyska,
- Mansi Kasliwal,
- Peter E. Nugent,
- David Rabinowitz,
- Stuart D. Ryder
Affiliations
- Syed A. Uddin
- ORCiD
- Observatories of the Carnegie Institution for Science , 813 Santa Barbara Street, Pasadena, CA 91101, USA ; [email protected]; George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University , Department of Physics and Astronomy, College Station, TX 77843, USA; US Naval Observatory , 3450 Massachusetts Avenue NW, Washington, DC 20392, USA; Center for Space Studies, American Public University System , 111 West Congress Street, Charles Town, WV 25414, USA
- Christopher R. Burns
- ORCiD
- Observatories of the Carnegie Institution for Science , 813 Santa Barbara Street, Pasadena, CA 91101, USA ; [email protected]
- M M. Phillips
- ORCiD
- Carnegie Observatories, Las Campanas Observatory , Casilla 601, La Serena, Chile
- Nicholas B. Suntzeff
- ORCiD
- George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University , Department of Physics and Astronomy, College Station, TX 77843, USA
- Wendy L. Freedman
- ORCiD
- Department of Astronomy and Astrophysics & Kavli Institute for Cosmological Physics, University of Chicago , 5640 South Ellis Avenue, Chicago, IL 60637, USA
- Peter J. Brown
- ORCiD
- George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University , Department of Physics and Astronomy, College Station, TX 77843, USA
- Nidia Morrell
- ORCiD
- Carnegie Observatories, Las Campanas Observatory , Casilla 601, La Serena, Chile
- Mario Hamuy
- ORCiD
- Hagler Institute for Advanced Studies, Texas A&M University , College Station, TX 77843, USA; Fundación Chilena de Astronomía , El Vergel 2252, Santiago, Chile
- Kevin Krisciunas
- ORCiD
- George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University , Department of Physics and Astronomy, College Station, TX 77843, USA
- Lifan Wang
- ORCiD
- George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University , Department of Physics and Astronomy, College Station, TX 77843, USA
- Eric Y. Hsiao
- ORCiD
- Department of Physics, Florida State University , 77 Chieftan Way, Tallahassee, FL 32306, USA
- Ariel Goobar
- ORCiD
- The Oskar Klein Centre, Department of Physics, Stockholm University , SE-106 91 Stockholm, Sweden
- Saul Perlmutter
- ORCiD
- Lawrence Berkeley National Laboratory, Department of Physics , 1 Cyclotron Road, Berkeley, CA 94720, USA; Astronomy Department, University of California at Berkeley , Berkeley, CA 94720, USA
- Jing Lu
- ORCiD
- Department of Physics, Florida State University , 77 Chieftan Way, Tallahassee, FL 32306, USA; Department of Physics and Astronomy, Michigan State University , East Lansing, MI 48824, USA
- Maximilian Stritzinger
- ORCiD
- Department of Physics and Astronomy, Aarhus University , Ny Munkegade 120, DK-8000 Aarhus C, Denmark
- Joseph P. Anderson
- ORCiD
- European Southern Observatory , Alonso de Córdova 3107, Casilla 19, Santiago, Chile
- Chris Ashall
- ORCiD
- Department of Physics, Virginia Tech , Blacksburg, VA 24061, USA
- Peter Hoeflich
- ORCiD
- Department of Physics, Florida State University , 77 Chieftan Way, Tallahassee, FL 32306, USA
- Benjamin J. Shappee
- ORCiD
- Institute for Astronomy, University of Hawaii , 2680 Woodlawn Drive, Honolulu, HI 96822, USA
- S. E. Persson
- ORCiD
- Observatories of the Carnegie Institution for Science , 813 Santa Barbara Street, Pasadena, CA 91101, USA ; [email protected]
- Anthony L. Piro
- ORCiD
- Observatories of the Carnegie Institution for Science , 813 Santa Barbara Street, Pasadena, CA 91101, USA ; [email protected]
- E Baron
- ORCiD
- Planetary Science Institute , 1700 East Fort Lowell Road, Suite 106, Tucson, AZ 85719-2395, USA; Hamburger Sternwarte , Gojenbergsweg 112, D-21029 Hamburg, Germany; Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma , 440 West Brooks Street, Room 100, Norman, OK 73019-2061, USA
- Carlos Contreras
- ORCiD
- Carnegie Observatories, Las Campanas Observatory , Casilla 601, La Serena, Chile
- Lluís Galbany
- ORCiD
- Institute of Space Sciences (ICE, CSIC) , Campus UAB, Carrer de Can Magrans, s/n, E-08193 Barcelona, Spain; Institut d’Estudis Espacials de Catalunya (IEEC) , E-08034 Barcelona, Spain
- Sahana Kumar
- ORCiD
- Department of Physics, Florida State University , 77 Chieftan Way, Tallahassee, FL 32306, USA; Department of Astronomy, University of Virginia , 350 McCormic Road, Charlottesville, VA 22904, USA
- Melissa Shahbandeh
- ORCiD
- Physics and Astronomy Department, Johns Hopkins University , Baltimore, MD 21218, USA; Space Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218, USA
- Scott Davis
- ORCiD
- Department of Physics, University of California , 1 Shields Avenue, Davis, CA 95616-5270, USA
- Jorge Anais
- ORCiD
- Centro de Astronomía (CITEVA), Universidad de Antofagasta , Av. Angamos 601, Antofagasta, Chile
- Luis Busta
- ORCiD
- Carnegie Observatories, Las Campanas Observatory , Casilla 601, La Serena, Chile
- Abdo Campillay
- ORCiD
- Carnegie Observatories, Las Campanas Observatory , Casilla 601, La Serena, Chile; Departamento de Física, Universidad de La Serena , Cisternas 1200, La Serena, Chile
- Sergio Castellón
- Carnegie Observatories, Las Campanas Observatory , Casilla 601, La Serena, Chile
- Carlos Corco
- Carnegie Observatories, Las Campanas Observatory , Casilla 601, La Serena, Chile; SOAR Telescope , Casilla 603, La Serena, Chile
- Tiara Diamond
- ORCiD
- Department of Physics, Florida State University , 77 Chieftan Way, Tallahassee, FL 32306, USA; Laboratory of Observational Cosmology, Code 665, NASA Goddard Space Flight Center , Greenbelt, MD 20771, USA
- Christa Gall
- ORCiD
- DARK, Niels Bohr Institute, University of Copenhagen , Jagtvej 128, 2200 Copenhagen, Denmark
- Consuelo Gonzalez
- Carnegie Observatories, Las Campanas Observatory , Casilla 601, La Serena, Chile
- Simon Holmbo
- ORCiD
- Department of Physics and Astronomy, Aarhus University , Ny Munkegade 120, DK-8000 Aarhus C, Denmark
- Miguel Roth
- ORCiD
- Carnegie Observatories, Las Campanas Observatory , Casilla 601, La Serena, Chile; GMTO Corporation , Presidente Riesco 5335, Of. 501, Nueva Las Condes, Santiago, Chile
- Jacqueline Serón
- ORCiD
- Cerro Tololo Inter-American Observatory/NSF’s NOIRLab , Casilla 603, La Serena, Chile
- Francesco Taddia
- ORCiD
- The Oskar Klein Centre, Department of Physics, Stockholm University , SE-106 91 Stockholm, Sweden
- Simón Torres
- SOAR Telescope , Casilla 603, La Serena, Chile
- Charles Baltay
- ORCiD
- Department of Physics, Yale University , 217 Prospect Street, New Haven, CT 06511, USA
- Gastón Folatelli
- ORCiD
- Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de La Plata , Instituto de Astrofísica de La Plata (IALP), CONICET, Paseo del Bosque S/N, B1900FWA La Plata, Argentina
- Ellie Hadjiyska
- Department of Physics, Yale University , 217 Prospect Street, New Haven, CT 06511, USA
- Mansi Kasliwal
- ORCiD
- Division of Physics, Mathematics, and Astronomy, California Institute of Technology , 1200 East California Boulevard, MC 249-17, Pasadena, CA 91125, USA
- Peter E. Nugent
- ORCiD
- Lawrence Berkeley National Laboratory, Department of Physics , 1 Cyclotron Road, Berkeley, CA 94720, USA; Astronomy Department, University of California at Berkeley , Berkeley, CA 94720, USA
- David Rabinowitz
- ORCiD
- Department of Physics, Yale University , 217 Prospect Street, New Haven, CT 06511, USA
- Stuart D. Ryder
- ORCiD
- School of Mathematical and Physical Sciences, Macquarie University , NSW 2109, Australia; Astronomy, Astrophysics and Astrophotonics Research Centre, Macquarie University , Sydney, NSW 2109, Australia
- DOI
- https://doi.org/10.3847/1538-4357/ad3e63
- Journal volume & issue
-
Vol. 970,
no. 1
p. 72
Abstract
We present an analysis of Type Ia supernovae (SNe Ia) from the Carnegie Supernova Project I and II and extend the Hubble diagram from optical to near-infrared wavelengths ( uBgVriYJH ). We calculate the Hubble constant, H _0 , using various distance calibrators: Cepheids, the tip of the red giant branch (TRGB), and surface brightness fluctuations (SBFs). Combining all methods of calibration, we derive H _0 = 71.76 ± 0.58 (stat) ± 1.19 (sys) km s ^−1 Mpc ^−1 from the B band and H _0 = 73.22 ± 0.68 (stat) ± 1.28 (sys) km s ^−1 Mpc ^−1 from the H band. By assigning equal weight to the Cepheid, TRGB, and SBF calibrators, we derive the systematic errors required for consistency in the first rung of the distance ladder, resulting in a systematic error of 1.2 ∼ 1.3 km s ^−1 Mpc ^−1 in H _0 . As a result, relative to the statistics-only uncertainty, the tension between the late-time H _0 we derive by combining the various distance calibrators and the early-time H _0 from the cosmic microwave background is reduced. The highest precision in SN Ia luminosity is found in the Y band (0.12 ± 0.01 mag), as defined by the intrinsic scatter ( σ _int ). We revisit SN Ia Hubble residual-host mass correlations and recover previous results that these correlations do not change significantly between the optical and near-infrared wavelengths. Finally, SNe Ia that explode beyond 10 kpc from their host centers exhibit smaller dispersion in their luminosity, confirming our earlier findings. A reduced effect of dust in the outskirts of hosts may be responsible for this effect.
Keywords
