1/15 are photoz bao surveys competitive? · are photoz bao surveys competitive? 1.what do we lose...
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Are photoz BAO surveys competitive?
1. What do we lose cf specz?
2. What photo-z accuracy can we expect?
3. How well will this detect the wiggles?
4. How much more area is reqd cf spec-z ?
5. How well can the BAO scale be measured?
6. Errors on w?
7. Requirements?
Sarah Bridle, UCL & Chris Blake, UBC
1/15
2015
CMB WMAP 2/3 WMAP 6 yr
Planck Planck 4yr
Clusters AMI
SZA
APEX
AMIBA
SPT
ACT
DES
Supernovae
Pan-STARRS
DES LSST
JDEM/SNAP
CFHTLS
CSP
Spectroscopy
ATLAS
SKAFMOS
SDSS
Imaging CFHTLS
ATLAS KIDS JDEM
LSST SKA
SDSS
SUBARU
Surveys to measure Dark Energy
2005
20152005
ESSENCE
XCS
DUNE
2010
2010
WFMOS
DLS
LAMOST
DES, VISTA
Pan-STARRSHyper suprime
2/15
2015
CMB WMAP 2/3 WMAP 6 yr
Planck Planck 4yr
Clusters AMI
SZA
APEX
AMIBA
SPT
ACT
DES
Supernovae
Pan-STARRS
DES LSST
JDEM/SNAP
CFHTLS
CSP
Spectroscopy
ATLAS
SKAFMOS
SDSS
Imaging CFHTLS
ATLAS KIDS JDEM
LSST SKA
SDSS
SUBARU
Surveys to measure Dark Energy
2005
20152005
ESSENCE
XCS
DUNE
2010
2010
WFMOS
DLS
LAMOST
DES, VISTA
Pan-STARRSHyper suprime
2/15
1. What do we lose cf specz?
2. What photo-z accuracy can we expect?
3. How well will this detect the wiggles?
4. How much more area is reqd cf spec-z ?
5. How well can the BAO scale be measured?
6. Errors on w?
7. Requirements?
Are photoz BAO surveys competitive?
1/15
Gla
zeb
roo
k &
Bla
ke a
stro
-ph
/050
5608
3/15
4/15
Non-linear theory
4/15
Non-linear theoryPhoto-zs only
4/15
See Zhan & Knox 2005 for use of red lines to measure H/σz
Non-linear theoryPhoto-zs only
Glazebrook & Blake 2005
5/15
Bla
ke &
Bri
dle
ast
ro-p
h/0
4117
13
Increasingphoto-z accuracy
6/15
1. Is any BAO information available?
2. What photo-z accuracy can we expect?
3. How well will this detect the wiggles?
4. How much more area is reqd cf spec-z ?
5. How well can the BAO scale be measured?
6. Errors on w?
7. Requirements?
Are photoz BAO surveys competitive?
1/15
DE
S W
hit
epap
er a
stro
-ph
/051
0346
7/15
griz
DE
S W
hit
epap
er a
stro
-ph
/051
0346
7/15
σz = σ68/(1+z) ~ 0.03
+ VISTAgriz
1. Is any BAO information available?
2. What photo-z accuracy can we expect?
3. How well will this detect the wiggles?
4. How much more area is reqd cf spec-z ?
5. How well can the BAO scale be measured?
6. Errors on w?
7. Requirements?
Are photoz BAO surveys competitive?
1/15
Bla
ke &
Bri
dle
ast
ro-p
h/0
4117
13
Fit a sin wave instead:Model independent.
-amplitude >0?
Following Blake & Glazebrookand Seo & Eisenstein
6/15
Bla
ke &
Bri
dle
ast
ro-p
h/0
4117
13
8/15
1. Is any BAO information available?
2. What photo-z accuracy can we expect?
3. How well will this detect the wiggles?
4. How much more area is reqd cf spec-z ?
5. How well can the BAO scale be measured?
6. Errors on w?
7. Requirements?
Are photoz BAO surveys competitive?
1/15
Bla
ke &
Bri
dle
ast
ro-p
h/0
4117
13
9/15
1. Is any BAO information available?
2. What photo-z accuracy can we expect?
3. How well will this detect the wiggles?
4. How much more area is reqd cf spec-z ?
5. How well can the BAO scale be measured?
6. Errors on w?
7. Requirements?
Are photoz BAO surveys competitive?
1/15
Bla
ke &
Bri
dle
ast
ro-p
h/0
4117
13
Fit a sin wave instead:Model independent.
- amplitude >0?- k position = ?
Following Blake & Glazebrookand Seo & Eisenstein
6/15
Bla
ke &
Bri
dle
ast
ro-p
h/0
4117
13
10/15
1. Is any BAO information available?
2. What photo-z accuracy can we expect?
3. How well will this detect the wiggles?
4. How much more area is reqd cf spec-z ?
5. How well can the BAO scale be measured?
6. Errors on w?
7. Requirements?
Are photoz BAO surveys competitive?
1/15
by Chris Blake
11/15
Glazebrook & Blake 2005
5/15
by Chris Blake
12/15
Gla
zeb
roo
k &
Bla
ke a
stro
-ph
/050
5608
Constraints on w(z)
See also Dolney, Jain, Takada 2005
13/15
Predictions for LSST
Zh
an, K
no
x, T
yso
n, M
arg
on
iner
200
5
14/15
1. Is any BAO information available?
2. What photo-z accuracy can we expect?
3. How well will this detect the wiggles?
4. How much more area is reqd cf spec-z ?
5. How well can the BAO scale be measured?
6. Errors on w?
7. Requirements?
Are photoz BAO surveys competitive?
1/15
Requirements
• Homogeneous photometric calibration– Galactic extinction
– Cirrus
• Representative spectroscopic calibrationsample– VVDS IAB <24 50,000 zs
– WFMOS?!
15/15
2015
CMB WMAP 2/3 WMAP 6 yr
Planck Planck 4yr
Clusters AMI
SZA
APEX
AMIBA
SPT
ACT
DES
Supernovae
Pan-STARRS
DES LSST
JDEM/SNAP
CFHTLS
CSP
Spectroscopy
ATLAS
SKAFMOS
SDSS
Imaging CFHTLS
ATLAS KIDS
LSST SKA
SDSS
SUBARU
Surveys to measure Dark Energy
2005
20152005
ESSENCE
XCS
DUNE
2010
2010
WFMOS
DLS
LAMOST
DES, VISTA
Pan-STARRSHyper suprime
2/15
JDEM
2015
CMB WMAP 2/3 WMAP 6 yr
Planck Planck 4yr
Clusters AMI
SZA
APEX
AMIBA
SPT
ACT
DES
Supernovae
Pan-STARRS
DES LSST
JDEM/SNAP
CFHTLS
CSP
ATLAS
SKAFMOS WFMOS
SDSS
Imaging CFHTLS
ATLAS KIDS
DES, VISTA
JDEM
LSST SKA
Pan-STARRS
SUBARU
Surveys to measure Dark Energy
2005
20152005
ESSENCE
XCS
DUNE
2010
2010
Wiggles LSST
SDSSDLS
LAMOST
Hyper suprime
DES, VISTA
Pan-STARRSHyper suprime JDEM
2/15
4/15
4/15
See Zhan & Knox 2005 for use of red lines to measure H/σz