The rate of Type Ia supernovae at high redshift

被引：64

作者：

Barris, BJ ^{[1
]}

Tonry, JL ^{[1
]}

机构：

[1] Univ Hawaii, Astron Inst, Honolulu, HI 96822 USA

来源：

ASTROPHYSICAL JOURNAL | 2006年 / 637卷 / 01期

关键词：

supernovae : general; surveys;

D O I：

10.1086/498292

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We derive the rates of Type Ia supernovae (SNe Ia) over a wide range of redshifts using a complete sample from the IfA Deep Survey. This sample of more than 100 SNe Ia is the largest set ever collected from a single survey and therefore uniquely powerful for a detailed supernova rate (SNR) calculation. Measurements of the SNR as a function of cosmological time offer a glimpse into the relationship between the star formation rate (SFR) and Type Ia SNR and may provide evidence for the progenitor pathway. We observe a progressively increasing Type Ia SNR between redshifts z approximate to 0.3 and 0.8. The Type Ia SNR measurements are consistent with a short time delay (t approximate to 1 Gyr) with respect to the SFR, indicating a fairly prompt evolution of SN Ia progenitor systems. We derive a best-fit value of SFR/SNR approximate to 580 h(70)(-2) 70 M-circle dot per SN Ia for the conversion factor between the star formation and the SN Ia rates, as determined for a delay time of t approximate to 1 Gyr between the SFR and the Type Ia SNR. More complete measurements of the Type Ia SNR at z > 1 are necessary to conclusively determine the SFR-SNR relationship and constrain SN Ia evolutionary pathways.

引用

页码：427 / 438

页数：12

共 52 条

[41]

RIESS AG, 2002, BAAS, V34, P1164

[42] The binary progenitor of Tycho Brahe's 1572 supernova [J].

Ruiz-Lapuente, P ;

Comeron, F ;

Méndez, J ;

Canal, R ;

Smartt, SJ ;

Filippenko, AV ;

Kurucz, RL ;

Chornock, R ;

Foley, RJ ;

Stanishev, V ;

Ibata, R .

NATURE, 2004, 431 (7012) :1069-1072

[43]

RUIZLAPUENTE P, 2000, TYPE SUPERNOVAE THEO, P49

[44]

RUZLAPUENTE P, 1995, APJ, V447, pL69

[45] THE LUMINOSITY FUNCTION AND STELLAR EVOLUTION [J].

SALPETER, EE .

ASTROPHYSICAL JOURNAL, 1955, 121 (01) :161-167

[46] The Type Ia supernova rate [J].

Scannapieco, E ;

Bildsten, L .

ASTROPHYSICAL JOURNAL, 2005, 629 (02) :L85-L88

[47] The High-Z Supernova Search: Measuring cosmic deceleration and global curvature of the universe using Type IA supernovae [J].

Schmidt, BP ;

Suntzeff, NB ;

Phillips, MM ;

Schommer, RA ;

Clocchiatti, A ;

Kirshner, RP ;

Garnavich, P ;

Challis, P ;

Leibundgut, B ;

Spyromilio, J ;

Riess, AG ;

Filippenko, AV ;

Hamuy, M ;

Smith, RC ;

Hogan, C ;

Stubbs, C ;

Diercks, A ;

Reiss, D ;

Gilliland, R ;

Tonry, J ;

Maza, J ;

Dressler, A ;

Walsh, J ;

Ciardullo, R .

ASTROPHYSICAL JOURNAL, 1998, 507 (01) :46-63

[48] Lyman-break galaxies at z≥4 and the evolution of the ultraviolet luminosity density at high redshift [J].

Steidel, CC ;

Adelberger, KL ;

Giavalisco, M ;

Dickinson, M ;

Pettini, M .

ASTROPHYSICAL JOURNAL, 1999, 519 (01) :1-17

[49] The Hubble Higher z supernova search:: Supernovae to z ≈ 1.6 and constraints on type Ia progenitor models [J].

Strolger, LG ;

Riess, AG ;

Dahlen, T ;

Livio, M ;

Panagia, N ;

Challis, P ;

Tonry, JL ;

Filippenko, AV ;

Chornock, R ;

Ferguson, H ;

Koekemoer, A ;

Mobasher, B ;

Dickinson, M ;

Giavalisco, M ;

Casertano, S ;

Hook, R ;

Bondin, S ;

Leibundgut, B ;

Nonino, M ;

Rosati, P ;

Spinrad, H ;

Steidel, CC ;

Stern, D ;

Garnavich, PM ;

Matheson, T ;

Grogin, N ;

Hornschemeier, A ;

Kretchmer, C ;

Laidler, VG ;

Lee, K ;

Lucas, R ;

de Mello, D ;

Moustakas, LA ;

Ravindranath, S ;

Richardson, M ;

Taylor, E .

ASTROPHYSICAL JOURNAL, 2004, 613 (01) :200-223

[50] Cosmological results from high-z supernovae [J].

Tonry, JL ;

Schmidt, BP ;

Barris, B ;

Candia, P ;

Challis, P ;

Clocchiatti, A ;

Coil, AL ;

Filippenko, AV ;

Garnavich, P ;

Hogan, C ;

Holland, ST ;

Jha, S ;

Kirshner, RP ;

Krisciunas, K ;

Leibundgut, B ;

Li, WD ;

Matheson, T ;

Phillips, MM ;

Riess, AG ;

Schommer, R ;

Smith, RC ;

Sollerman, J ;

Spyromilio, J ;

Stubbs, CW ;

Suntzeff, NB .

ASTROPHYSICAL JOURNAL, 2003, 594 (01) :1-24

← 1 2 3 4 5 6 →