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[General Discussion]
1) Science Topics, sub-WGs, AIs and 1st year scientific projects
1.very high-z QSOs (z >6) : PI Kashikawa
[science]
-Survey strategy and "actual" discovery@z=7
-Discovery@z=6
#on the issue of faint end of AGN LF
-Galactic BD based on photometric sample

[A/I]
-probabllistic selection
-NIR(UKIDSS/VIKING):examinig actual data
-Identifying problems in images: software team
-Repeat/confirming photometry
-spectra:individual proposals? ex
-optical follow-up imaging ?
#If we obtain, we will propose to write optical(z-band) follow-up.
#20 min, 8m telescope for each targets
# how about 4m telescope ? probably ok
#Learn from SDSS
-preparation for ALMA &JVLA proposals: QSO@z=8
-Galactic BD sciences ? spatial distribution Y dwarfs ?
How we should do for faint candidatesin UD without spec

2. z=3-5 photometric selection (lower redshift too):PI Nagao
[A/I]
-multi-color selection (not 2color-based)
-stellarity criteria
-Effects of Baldwin effect 
-proper motion(SDSS-HSC; a few yr time separtion
only bright QSO(z=7) is useful (morokuma-san)
=>we should check this at lower-z

3. Clustering and environment: PI Strauss
[sicence]
-cross correlation
-z=4 g-drop LBGs with HSC (dep. on L)
-low z galaxies with photo-z (dep. gala properties)
(cluster of galaxies)

[A/I]
-Revising Mock catalog
-communication with galaxy people 

4. Lensed QSOs: PI Coupon
[science]
-mutiple-image lensed QSOs -> host galaxies studies
#quite rare, less than few
#SDSS QSOs

[A/I]
-spectra: individual
-other follow-up needed NIR? imaging?

5. QSO metallicity: PI Nagao
[science]
-z_BLR evolution, by product of the collected spectra

[A/I]
-NIR follow-up
-model predictions from theoretical works
=>Already build-in! (but TOTAL metallicity Z)
=>relative abundance can be also added (but though issue)

6. variability: PI Morokuma
[science]
-long-term year with HSC & previous data
=> structute func
if focus on Subaru data (SDSS) time sampling is so dense
saturation is worried on SDSS obs. 

[A/I]
-completeness
-incoprating variability in target selection, algorism

7. Mid : PI Silverman
[A/I]
-completness/contamination
-spectra
-SPLASH dataset(spa.resolution 3-4")
 what we should do ?
 Host galaxies of low-L AGN at z-1(rest K)=> Mstar
 extremely high-z (>20??)

8. X-ray: PI Terashima
[science]
-pecullar SED objects
-2color
-including obscured pop => f_abs z=4-5
-optical couterparts of opt-undetected cahndra obs @cosmos
 data coming soon within 1yr

[A/I]
-spectral
-X-ray follow-up of interesting AGN 

9. Radio/sub-mm: PI Nagao
[A/I]
-new members
-inviting radio people?
-JVLA new survey
-CCAT(timescale is too long)
-Japanese radio community meeting@mitaka
(->Imanishi-san)

10. Models: Wada
-AGN downsizing
-nexr SWANs theory meeting @ sendai
 LOC chair: Akiyama-san

2) HSC data
[Need some coordination?] through telecon
to maximize the multipllicity of spectrographs
to avoid submissions of multiple similar proposal

[which telescope?]
-subaru, gemini,keck
-subaru-VLT time-exchange 
-smaller telescope, APO, WHT, AAO?
 access from APO: end at summer 2014
 CFHT/MegaCaM/WIRCAM(Taiwan, but limited night)

-before HSC data we submit the proposal.
May not convincing ?

-approach from both JP and Princeton
dividing our target lists into two

-proposal for multi-wavelength dataset
 u-band in UD (next semestar SXDS done)
 6-7 night for each semestar(Taiwan)
 VISTA for HSC deep layer(40h) France and Brazil
 ALMA JVLA
-Instrumnetion issues
-Other surveys to watch
 VISTA
 JVLA: propo0.2mJyfor wide layer
      (TAC suspect survey)
 Euclid:  
 eROSITA:
 looking forward to TMT, JWST
#Survey parameters (HSC) on web page?? 
should be confirmed

3) Follow-up
4) software and database issues
5) PFS: Science opportunities and target selection
*target selection
-How will AGN be selected in wide survey
 deep survey
-How will AGN be recognised from specra of galaxy sample ?
 See Tanaka's simulations are useful
-working to prepare the SSP

*QSO photo-z
Tanaka, Coupon with photometric guys
[A/I]
adding MIR component
effects of variabillity
baldwin effect
cf. BOSS QSO catalog (Paris et al. 2012)
type-2 QSOs 

*HSC data and proposal
a)HSC commissioning

b)SSp 1st year obs
VIKING(GAMA), XXL(K22)
c)requirements for data under software
continuous interaction with software WG
-strengths and limitatios of HSC pipelines
-early data reveal problems and features
-features we identified we would like
contact with Furusawa-san

6) Fostering further collaborations
[Our activity]
- presentation file => HSC members in other sub-WGs
- each sub-group => continuing meeting (like Theory)
- encouraging younger PDs/students

-Next meeting?
--joint meeting with galaxy evolution WGs
--at where (NAOJ or IPMU would be convenient...)
  April/May? 
  coordination with Cosomos meeting in kyoto
  strauss-san will talk to takada-san
-other good ideas/suggestions
 Nothing