Contents 1. Ia? 2. Ia 3. WISH Ia cosmology 4. WISH Ia + rate 5.
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1 Type Ia Supernova Survey w/ WISH
2 Contents 1. Ia? 2. Ia 3. WISH Ia cosmology 4. WISH Ia + rate 5.
3 Contents 1. Ia? 2. Ia 3. WISH Ia cosmology 4. WISH Ia + rate 5.
4 Type Ia Supernova + +?? (single degenerate)? (double degenerate) +?? + + standard(izable) candle
5 Type Ia Supernova + MB=-19.3mag - (z>1) + - Δm15, stretch, Δ ".,+"8)+9::9
6 Contents 1. Ia? 2. Ia 3. WISH Ia cosmology 4. WISH Ia + rate 5.
7 Type Ia Supernova Cosmology!" Supernova Cosmology Project (SCP) High-Z Team #$%& '()"*+),--. /0'11 '()"*+),--2 31(0'4 '()"*+),--5 ESSENCE Supernova Survey 6%%789"1': '()"*+),--; #'11*'4)'()"*+),--< Supernova Legacy Survey (SNLS) SDSS-II Supernova Survey
8 Type Ia Supernova Cosmology + advantage - (=luminosity distance) - ( ) - luminosity distance - redshift relation - - 0<z<1.5 redshift + disadvantage - dust extinction - evolution, metallicity - - Malmquist - K-correction -
9 statistical/systematic errors # z omega-m omega-l w Knop+03 (SCP) +11 ~50 (total) /-0.04 ( 1) /-0.04 ( 1) /-0.09 ( 2) riess+04 (High-Z Team) +16 ~157 (total) ( 3) ( 3) ( 4) Astier+06 (SNLS) nearby / / ( 5) +/ / ( 5) +/ / ( 6) Wood-Vasey+07 (ESSENCE) ( 7) /-0.13 ( 8) Kowalski+08 (Union Sample) +~10 nearby 307 (total) ( 9) ( 10) Kessler+09 (SDSS-II SN) (total) / / ( 9) +/ /-0.11 ( 9) ( 1): flat universe, w=-1 ( 2): w=constant, +CMB+galaxy redshift distortion ( 3): flat universe, w=constant ( 4): +CMB+LSS ( 5): flat ΛCDM ( 6): flat universe, w=constant, +BAO ( 7): +BAO ( 8): +SNLS SNe Ia ( 9): flat, ΛCDM universe ( 10): +BAO+CMB
10 Type Ia Supernova Cosmology + advantage - (=luminosity distance) - ( ) - - 0<z<1.5 redshift + disadvantage - dust extinction - evolution, metallicity - - Malmquist - K-correction - systematic error universal SN Ia color? dust extinction Av = Rv x E(B-V) universal extinction law?
11 XMMU J z=0.98 dust extinction correction + 最大のsystematic error + 統計errorとコンパラ RCS z= 超新星固有の色 と dustによるreddening が縮退 1. dustの影響が小さい静止系でなるべく長い波長で観測したい NIRでの超新星サーベイ RDCS J z= dustの影響が小さい環境の超新星を観測したい 楕円銀河超新星サーベイ HST/ACSでのz>1銀河団サーベイ(Dawson+2009) W
12 Carnegie Supernova Project (CSP) + low-z (z<0.1) Ia, 100 II - Swope 1-m: - Dupont 2.5-m: + high-z (0.2<z<0.7) - 75 Ia I-band lightcurve template I-band - Magellan 6.5-m: - : SDSS, SNLS, ESSENCE I-band Hubble diagram - rest-frame UBV - systematic error : dust extinction, K-correction
13 Rest-frame NIR observation --> 0+.)1.2%$) *-'$34'5667' 8//&"9$)*: *-'$34'566;
14 Rest-frame NIR observation --> rest-frame rest-frame Altavilla )1.2%$) *-'$34'5667' 8//&"9$)*: *-'$34'566;
15 Contents 1. Ia? 2. Ia 3. WISH 4. 5.
16 Space-based observations for SNe 1 HST
17 SN Ia light curves -21 SN Ia light curves (Hsiao template) peak u g ri -20 z absolute magnitude [mag] mag days (rest-frame) t [days]
18 Riess+2007 (HST/ACS) WISH SN Survey Strategies + Ultra-Deep Survey (UDS) mag AB -? - N=5-5days@rest x (1+z) ~10days@z~1 - rolling search N~20 - N - visibility - multi-band ( 3 ) N 1 mag margin
19 WISH SN Survey Strategies N 1 mag margin band (main) band (color) z_max set3-f0,f1,f2,f3 set4-f0.f1,f2,f3 set3-f4,f5 set4-f4,f set3-f0,f1,f2 set4-f0,f1,f2,f3 set3-f3,f4,f5 set4-f4,f set3-f0,f1,f2 set4-f0,f1,f2,f3 set3-f3,f4,f5 set4-f4,f5 2.0 peak magnitude as a function of redshift N=20 visibility? rest-frame the higher-z, the better apparent magnitude [mag] peak magnitude set3-f0 set3-f1 set4-f4 set4-f5 set3-f2 set3-f3 set3-f4 set3-f5 set4-f0 set4-f1 set4-f2 set4-f observed-frame epoch [days]
20 WISH SN Survey Strategies + rest-frame B-band ( as high-z as possible ): color(b-r) - ID: WISH/ AO(8m, TMT) - N=5 1.0<z<3.0 (set3-f0,f1,f2,f3, set4-f0,f1,f2,f3) - ~3 SNe Ia [day^-1 deg^-2] (z>1.5 2 ) <-- --> peak 15 days 44 deg^ SNe Ia (~1200 SNe
21 WISH SN Survey Strategies + rest-frame I/i-band - ID: OK, highest-z NIR(WISH or AO) - N=5 0.2<z<2.2 (set3-f0,f1,f2,f3 or set4-f0,f1,f2,f3) - ~2.5 SNe Ia [day^-1 deg^-2] --> peak 10 days 80 deg^ SNe Ia - N=10 0.2<z<1.6 (set3-f0,f1,f2,f3 or set4-f0,f1,f2,f3) - ~1.5 SNe Ia [day^-1 deg^-2] --> peak 10 days x 6 22 deg^ SNe Ia + rest-frame H-band - ID: OK, highest-z NIR(WISH or AO) - N=5 0<z<1.4 (set3-f2,3,f4,f5 or set4-f3,f4,f5) - ~1.2 SNe Ia [day^-1 deg^-2] --> peak 10 days 167 deg^ SNe Ia - N=10 0<z<1.0 (set3-f2,3,f4,f5 or set4-f3,f4,f5) - ~0.5 SNe Ia [day^-1 deg^-2] --> peak 10 days x 6 67 deg^ SNe Ia
22 Riess+2007 HST/ACS grism, ~15000? sec z=1.36, 1.39 Morokuma+2010 Subaru/FOCAS, sec z=1.35 HST/ACS images
23 WISH grism spectroscopy for SNe 1.2e-08 1e-08 z= µm f-lambda (arbitary) 8e-09 6e-09 4e-09 SiII: Ia feature - z<1 OK - 1<z<1.5 (Riess+2004, Morokuma+2010) - z>1 2e-09 (+ AO ) wavelength [um] wavelength [µm] + R~ OK +? + background? wavelength [µm] wavelength [um] redshift
24 Contents 1. Ia? 2. Ia 3. WISH Ia cosmology 4. WISH Ia + rate 5.
25 SN rate (Ia & Core-Collapse) + Ia - (progenitor system) - single degenerate and/or double degenerate - [SN Ia rate] = [ ] + [ ] - SN Ia : metallicity, (Sullivan+2006) - delay time distribution: Ia (Totani+2008 ) - (Ihara+2007), (SPY; Napiwotzki+2001) - metallicity effect: high-z Ia rate (Kobayashi & Nomoto 2008), z>1.5?? - dusty (missing) fraction + core-collapse - IIn (very bright) SN at z>2 (Cooke+2009) - dusty SN search? - (z>2; Stanishev+2009)
26 Contents 1. Ia? 2. Ia 3. WISH Ia cosmology 4. WISH Ia + rate 5.
27 + Ia cosmology systematic error ~ statistical error + dust extinction NIR + + WISH UDS ~2000 Ia + WISH + strategy 3 3 cosmology rest-frame I- band redshift (?) - rest-frame B-band: systematic error 1.0<z<3.0 - rest-frame I-band: systematic error 0.2<z<2.2 - rest-frame H-band: z< µm grism z<1 OK + SN rate (z>1.5 SN Ia rate, IIn rate, dusty fraction) + Subaru/HSC photo-z ( )
Contents 1. Ia cosmology 2. Ia / rate 3.
WISH ( ) Contents 1. Ia cosmology 2. Ia / rate 3. supernova (CC SN) Ia (SN Ia) supernova classification supernova Ia (SN Ia) - : redshift z~1.5 - progenitor system: Single Degenerate? Double Degenerate?
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Independent discoveries of a tidally disrupting dwarf galaxy around NGC 253! A Tidally Disrupting Dwarf Galaxy in the Halo of NGC 253 Toloba, E. et al. 2016, ApJL, 816, L5 (hereafter T16, accepted 2015.12.07)
SN 2007bi Yoshida, T. & Umeda, H., MNRAS 412, L78-L82 (2011)
SN 2007bi Yoshida, T. & Umeda, H., MNRAS 412, L78-L82 (2011) SN 2007bi SN 2007bi (Gal-Yam et al. 2009) 2007 4 6.5 Type Ic subluminous dwarf galaxy Z ~ (0.2-0.4) Z (Young et al. 2010) 36 (Young et al. 2010)
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Summary of WISH Filter Set and Sensitivity: Filters suitable for various scientific case Filters cover wavelength range of 1-5µm without any gaps Narr
Summary of WISH Survey Plan Kiyoto Yabe (NAOJ) Summary of WISH Filter Set and Sensitivity: Filters suitable for various scientific case Filters cover wavelength range of 1-5µm without any gaps Narrower
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