Home > Research > Publications & Outputs > ZTF SN Ia DR2

Research

Associated organisational unit

Links

Text available via DOI:

View graph of relations

ZTF SN Ia DR2: The diversity and relative rates of the thermonuclear supernova population

Research output: Contribution to Journal/Magazine › Journal article › peer-review

Published

Standard

ZTF SN Ia DR2: The diversity and relative rates of the thermonuclear supernova population. / Dimitriadis, G.; Burgaz, U.; Deckers, M. et al.
In: Astronomy and Astrophysics, Vol. 694, A10, 28.02.2025.

Research output: Contribution to Journal/Magazine › Journal article › peer-review

Harvard

Dimitriadis, G, Burgaz, U, Deckers, M, Maguire, K, Johansson, J, Smith, M, Rigault, M, Frohmaier, C, Sollerman, J, Galbany, L, Kim, Y-L, Liu, C, Miller, AA, Nugent, PE, Alburai, A, Chen, P, Dhawan, S, Ginolin, M, Goobar, A, Groom, SL, Harvey, L, Kenworthy, WD, Kulkarni, SR, Phan, K, Popovic, B, Riddle, RL, Rusholme, B, Müller-Bravo, TE, Nordin, J, Terwel, JH & Townsend, A 2025, 'ZTF SN Ia DR2: The diversity and relative rates of the thermonuclear supernova population', Astronomy and Astrophysics, vol. 694, A10. https://doi.org/10.1051/0004-6361/202451852

APA

Dimitriadis, G., Burgaz, U., Deckers, M., Maguire, K., Johansson, J., Smith, M., Rigault, M., Frohmaier, C., Sollerman, J., Galbany, L., Kim, Y.-L., Liu, C., Miller, A. A., Nugent, P. E., Alburai, A., Chen, P., Dhawan, S., Ginolin, M., Goobar, A., ... Townsend, A. (2025). ZTF SN Ia DR2: The diversity and relative rates of the thermonuclear supernova population. Astronomy and Astrophysics, 694, Article A10. https://doi.org/10.1051/0004-6361/202451852

Vancouver

Dimitriadis G, Burgaz U, Deckers M, Maguire K, Johansson J, Smith M et al. ZTF SN Ia DR2: The diversity and relative rates of the thermonuclear supernova population. Astronomy and Astrophysics. 2025 Feb 28;694:A10. Epub 2025 Feb 14. doi: 10.1051/0004-6361/202451852

Author

Dimitriadis, G. ; Burgaz, U. ; Deckers, M. et al. / ZTF SN Ia DR2 : The diversity and relative rates of the thermonuclear supernova population. In: Astronomy and Astrophysics. 2025 ; Vol. 694.

Bibtex

@article{6d8524cf4c044da1b780cefbff4ab09a,
title = "ZTF SN Ia DR2: The diversity and relative rates of the thermonuclear supernova population",
abstract = "The Zwicky Transient Facility SN Ia Data Release 2 (ZTF SN Ia DR2) contains more than 3000 Type Ia supernovae (SNe Ia), providing the largest homogeneous low-redshift sample of SNe Ia. Having at least one spectrum per event, this data collection is ideal for large-scale statistical studies of the photometric, spectroscopic and host-galaxy properties of SNe Ia, particularly of the rarer peculiar'sub-classes. In this paper we first present the method we developed to spectroscopically classify the SNe in the sample, and the techniques we used to model their multi-band light curves and explore their photometric properties. We then show a method to distinguish between the peculiar sub-types and the normal SNe Ia. We also explore the properties of their host galaxies and estimate their relative rates, focusing on the peculiar sub-types and their connection to the cosmologically useful SNe Ia. Finally, we discuss the implications of our study with respect to the progenitor systems of the peculiar SN Ia events.",
author = "G. Dimitriadis and U. Burgaz and M. Deckers and K. Maguire and J. Johansson and M. Smith and M. Rigault and C. Frohmaier and J. Sollerman and L. Galbany and Y.-L. Kim and C. Liu and A.A. Miller and P.E. Nugent and A. Alburai and P. Chen and S. Dhawan and M. Ginolin and A. Goobar and S.L. Groom and L. Harvey and W.D. Kenworthy and S.R. Kulkarni and K. Phan and B. Popovic and R.L. Riddle and B. Rusholme and T.E. M{\"u}ller-Bravo and J. Nordin and J.H. Terwel and A. Townsend",
year = "2025",
month = feb,
day = "28",
doi = "10.1051/0004-6361/202451852",
language = "English",
volume = "694",
journal = "Astronomy and Astrophysics",
issn = "1432-0746",
publisher = "EDP Sciences",

}

RIS

TY - JOUR

T1 - ZTF SN Ia DR2

T2 - The diversity and relative rates of the thermonuclear supernova population

AU - Dimitriadis, G.

AU - Burgaz, U.

AU - Deckers, M.

AU - Maguire, K.

AU - Johansson, J.

AU - Smith, M.

AU - Rigault, M.

AU - Frohmaier, C.

AU - Sollerman, J.

AU - Galbany, L.

AU - Kim, Y.-L.

AU - Liu, C.

AU - Miller, A.A.

AU - Nugent, P.E.

AU - Alburai, A.

AU - Chen, P.

AU - Dhawan, S.

AU - Ginolin, M.

AU - Goobar, A.

AU - Groom, S.L.

AU - Harvey, L.

AU - Kenworthy, W.D.

AU - Kulkarni, S.R.

AU - Phan, K.

AU - Popovic, B.

AU - Riddle, R.L.

AU - Rusholme, B.

AU - Müller-Bravo, T.E.

AU - Nordin, J.

AU - Terwel, J.H.

AU - Townsend, A.

PY - 2025/2/28

Y1 - 2025/2/28

N2 - The Zwicky Transient Facility SN Ia Data Release 2 (ZTF SN Ia DR2) contains more than 3000 Type Ia supernovae (SNe Ia), providing the largest homogeneous low-redshift sample of SNe Ia. Having at least one spectrum per event, this data collection is ideal for large-scale statistical studies of the photometric, spectroscopic and host-galaxy properties of SNe Ia, particularly of the rarer peculiar'sub-classes. In this paper we first present the method we developed to spectroscopically classify the SNe in the sample, and the techniques we used to model their multi-band light curves and explore their photometric properties. We then show a method to distinguish between the peculiar sub-types and the normal SNe Ia. We also explore the properties of their host galaxies and estimate their relative rates, focusing on the peculiar sub-types and their connection to the cosmologically useful SNe Ia. Finally, we discuss the implications of our study with respect to the progenitor systems of the peculiar SN Ia events.

AB - The Zwicky Transient Facility SN Ia Data Release 2 (ZTF SN Ia DR2) contains more than 3000 Type Ia supernovae (SNe Ia), providing the largest homogeneous low-redshift sample of SNe Ia. Having at least one spectrum per event, this data collection is ideal for large-scale statistical studies of the photometric, spectroscopic and host-galaxy properties of SNe Ia, particularly of the rarer peculiar'sub-classes. In this paper we first present the method we developed to spectroscopically classify the SNe in the sample, and the techniques we used to model their multi-band light curves and explore their photometric properties. We then show a method to distinguish between the peculiar sub-types and the normal SNe Ia. We also explore the properties of their host galaxies and estimate their relative rates, focusing on the peculiar sub-types and their connection to the cosmologically useful SNe Ia. Finally, we discuss the implications of our study with respect to the progenitor systems of the peculiar SN Ia events.

U2 - 10.1051/0004-6361/202451852

DO - 10.1051/0004-6361/202451852

M3 - Journal article

VL - 694

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

SN - 1432-0746

M1 - A10

ER -