(put together by Bianca)
DATA STATUS:
HI: done.
Radio continuum. Done! Continuum sources in A2192 are restored with a circular instead of an elliptical beam. Is this also the case for A963? Are the continuum fluxes and positions in Dwaraka's map consistent with what Boris has derived? (Dwaraka)
BR imaging:
spectra: reduced + catalogs (Yara)
Spitzer: reduced + catalogs (Ryan)
Galex: reduced + catalogs (Maria)
morphologies available (Yara, Bia, Jac, and some Maria and Marc)
stellar masses available (Yara)
TO COME:
Herschel outcome?
Near-IR all allocated
CO (Aeree)
wide-field VLBI (Arpad)
Marc proposes: Deeper optical spectroscopy of HI detections? WHT service proposals for spring 2011?
Yara proposes: other kind of spectroscopy: not fiber, but perhaps long slit or even better IFU
THINGS DISCUSSED AND DONE IN PADOVA
identified structures and substructures in the two fields by looking at the 3D distribution (RA, DEC and z) of galaxies in the spectroscopic catalog (including WHT, HI and literature redshifts)
GALAXY STELLAR MASSES (solved!!) Zibetti, DR7 and Bell & de Jong masses for our
spec sample are in agreement We will use Zibetti's masses, for Kroupa IMF (Zibetti in agreement with dynamical estimate of stellar masses)
decided how to compute spectroscopic completeness (color, magnitude, position)
based on Herschel + HI overlays received by Bianca, discussed the necessity to use the Egami Herschel data asap - If we use these data, should we offer the PI of this Herschel program co-authorship? Bianca to check this out.
telecons with Boris and Aeree/Ryan/Min
Marc classified the morphologies of HI galaxies
papers (see below)
TENTATIVE AUTHORSHIP POLICY (suggested - to be approved by everybody)
Each paper includes everybody who has contributed to the acquisition,
reduction, analysis, interpretation of any of the data contained in that paper.
Before submission, every draft is anyway circulated to anybody, giving
anyone the possibility to be included if they feel they should be.
ACTION ITEMS:
Yara/Bia to compute spectroscopic completeness
Yara to put galaxy stellar masses and absolute magnitudes (SDSS + Johnson) on the WIKI (DONE)
Yara to put final morphologies on the WIKI, including Maria's and Marc's (DONE)
Boris to clean HI catalog from few spurious detections (provided by Yara)
Bianca to check for Egami policy
Dwaraka to compute SFRs from radio continuum using Yara's
spec tables
Jacqueline to look into X-ray data of the two fields
Jacqueline + student: mergers and interactions
Boris and Dwaraka to check radio continuum fluxes
Ryan to produce Spitzer SFR catalog
Maria to produce Galex SFR catalog
Min to get SPIRE archive data, and do catalogs
AGN - star formation discrimination: Ryan/Min to attempt from Spitzer data
Marc to solve optical photometry zero point issue
Bia to see if we can access CFHT calibrated images
Marc to produce UV + opt + Spit * HI postage stamps. Boris already made overlays of HI contours on B,R,UV images for the HI atlas. Overlays on Spitzer images requires final Spitzer maps, not yet on wiki. Ryan?
Arpad to write wide-field VLBI proposal
Everybody !! to put everything they have done on the wiki
Everybody !! to check these minutes and answer to questions regarding them
Papers we propose for now:
HI paper + M_HI/L at z=0.2 –> BORIS. Use absolute mags from Yara, compare to Ursa Major + “old field” (no ALPHAALPHA)
Optical imaging paper + blue fraction BORIS
Omega_HI MARC
Spectroscopy data and products (cluster vel. dispersions, emission lines, environments, HI) YARA
Also, (Yara) to extract a letter/short paper on A2192 four structures
M_HI + M* + Ttypes + environment YARA
Radio Butcher-Oemler effect or/and SFRs at all z's DWARAKA
SFR Spitzer RYAN
GALEX (analysis a la Geach et al.) MARIA
Dust (CO Herschel) AEREE
Mergers and interactions JACQUELINE
Egami Herschel + HI + redshifts + … ??
Tully Fisher relation ? (TO DO galaxy inclination)
Ideas/suggestions for these or other papers welcome
Other comments/things to keep in mind or discuss:
Cosmological parameters: decide them now, used by everybody Bia suggests: use Omega_M=0.3, Omega_L=0.7, H_0=70 - if anyone disagrees, please shout
K-corrections: Yara uses interRest to compute rest frame magnitudes - if other people needs to compute other rest frame quantities, check consistency
SFRs: different estimates to be consistent, when consistency needed