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The Type Ia supernovae rate with Subaru/XMM-Newton Deep Survey

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The Type Ia supernovae rate with Subaru/XMM-Newton Deep Survey. / Okumura, Jun E.; Ihara, Yutaka; Doi, Mamoru et al.
In: Publications of the Astronomical Society of Japan, Vol. 66, No. 2, 49, 04.2014.

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

Harvard

Okumura, JE, Ihara, Y, Doi, M, Morokuma, T, Pain, R, Totani, T, Barbary, K, Takanashi, N, Yasuda, N, Aldering, G, Dawson, K, Goldhaber, G, Hook, I, Lidman, C, Perlmutter, S, Spadafora, A, Suzuki, N & Wang, L 2014, 'The Type Ia supernovae rate with Subaru/XMM-Newton Deep Survey', Publications of the Astronomical Society of Japan, vol. 66, no. 2, 49. https://doi.org/10.1093/pasj/psu024

APA

Okumura, J. E., Ihara, Y., Doi, M., Morokuma, T., Pain, R., Totani, T., Barbary, K., Takanashi, N., Yasuda, N., Aldering, G., Dawson, K., Goldhaber, G., Hook, I., Lidman, C., Perlmutter, S., Spadafora, A., Suzuki, N., & Wang, L. (2014). The Type Ia supernovae rate with Subaru/XMM-Newton Deep Survey. Publications of the Astronomical Society of Japan, 66(2), Article 49. https://doi.org/10.1093/pasj/psu024

Vancouver

Okumura JE, Ihara Y, Doi M, Morokuma T, Pain R, Totani T et al. The Type Ia supernovae rate with Subaru/XMM-Newton Deep Survey. Publications of the Astronomical Society of Japan. 2014 Apr;66(2):49. doi: 10.1093/pasj/psu024

Author

Okumura, Jun E. ; Ihara, Yutaka ; Doi, Mamoru et al. / The Type Ia supernovae rate with Subaru/XMM-Newton Deep Survey. In: Publications of the Astronomical Society of Japan. 2014 ; Vol. 66, No. 2.

Bibtex

@article{0106d3f6b39a43eb961a2a73b0196ec2,
title = "The Type Ia supernovae rate with Subaru/XMM-Newton Deep Survey",
abstract = "We present measurements of the rates of high-redshift Type Ia supernovae derived from the Subaru/XMM-Newton Deep Survey (SXDS). We carried out repeated deep imaging observations with Suprime-Cam on the Subaru Telescope, and detected 1040 variable objects over 0.918 deg(2) in the Subaru/XMM-Newton Deep Field. From the imaging observations, light curves in the observed i band are constructed for all objects, and we fit the observed light curves with template light curves. Out of the 1040 variable objects detected by the SXDS, 39 objects over the redshift range 0.2 ",
keywords = "galaxies: evolution, surveys, stars: evolution, stars: statistics, stars: supernovae: general, HUBBLE-SPACE-TELESCOPE, DIGITAL SKY SURVEY, HIGH-REDSHIFT SUPERNOVAE, DELAY-TIME DISTRIBUTION, ABSOLUTE MAGNITUDE DISTRIBUTIONS, CORE-COLLAPSE SUPERNOVAE, DARK-ENERGY CONSTRAINTS, STAR-FORMATION HISTORY, II-P SUPERNOVAE, LEGACY SURVEY",
author = "Okumura, {Jun E.} and Yutaka Ihara and Mamoru Doi and Tomoki Morokuma and Reynald Pain and Tomonori Totani and Kyle Barbary and Naohiro Takanashi and Naoki Yasuda and Greg Aldering and Kyle Dawson and Gerson Goldhaber and Isobel Hook and Chris Lidman and Saul Perlmutter and Anthony Spadafora and Nao Suzuki and Lifan Wang",
year = "2014",
month = apr,
doi = "10.1093/pasj/psu024",
language = "English",
volume = "66",
journal = "Publications of the Astronomical Society of Japan",
issn = "0004-6264",
publisher = "Astronomical Society of Japan",
number = "2",

}

RIS

TY - JOUR

T1 - The Type Ia supernovae rate with Subaru/XMM-Newton Deep Survey

AU - Okumura, Jun E.

AU - Ihara, Yutaka

AU - Doi, Mamoru

AU - Morokuma, Tomoki

AU - Pain, Reynald

AU - Totani, Tomonori

AU - Barbary, Kyle

AU - Takanashi, Naohiro

AU - Yasuda, Naoki

AU - Aldering, Greg

AU - Dawson, Kyle

AU - Goldhaber, Gerson

AU - Hook, Isobel

AU - Lidman, Chris

AU - Perlmutter, Saul

AU - Spadafora, Anthony

AU - Suzuki, Nao

AU - Wang, Lifan

PY - 2014/4

Y1 - 2014/4

N2 - We present measurements of the rates of high-redshift Type Ia supernovae derived from the Subaru/XMM-Newton Deep Survey (SXDS). We carried out repeated deep imaging observations with Suprime-Cam on the Subaru Telescope, and detected 1040 variable objects over 0.918 deg(2) in the Subaru/XMM-Newton Deep Field. From the imaging observations, light curves in the observed i band are constructed for all objects, and we fit the observed light curves with template light curves. Out of the 1040 variable objects detected by the SXDS, 39 objects over the redshift range 0.2

AB - We present measurements of the rates of high-redshift Type Ia supernovae derived from the Subaru/XMM-Newton Deep Survey (SXDS). We carried out repeated deep imaging observations with Suprime-Cam on the Subaru Telescope, and detected 1040 variable objects over 0.918 deg(2) in the Subaru/XMM-Newton Deep Field. From the imaging observations, light curves in the observed i band are constructed for all objects, and we fit the observed light curves with template light curves. Out of the 1040 variable objects detected by the SXDS, 39 objects over the redshift range 0.2

KW - galaxies: evolution

KW - surveys

KW - stars: evolution

KW - stars: statistics

KW - stars: supernovae: general

KW - HUBBLE-SPACE-TELESCOPE

KW - DIGITAL SKY SURVEY

KW - HIGH-REDSHIFT SUPERNOVAE

KW - DELAY-TIME DISTRIBUTION

KW - ABSOLUTE MAGNITUDE DISTRIBUTIONS

KW - CORE-COLLAPSE SUPERNOVAE

KW - DARK-ENERGY CONSTRAINTS

KW - STAR-FORMATION HISTORY

KW - II-P SUPERNOVAE

KW - LEGACY SURVEY

U2 - 10.1093/pasj/psu024

DO - 10.1093/pasj/psu024

M3 - Journal article

VL - 66

JO - Publications of the Astronomical Society of Japan

JF - Publications of the Astronomical Society of Japan

SN - 0004-6264

IS - 2

M1 - 49

ER -