cosmos survey pi scoville hst 590 orbits i-band 2 deg.vla-cosmos: schinnerer (pi) 1.4 ghz continuum,...
TRANSCRIPT
![Page 1: Cosmos Survey PI Scoville HST 590 orbits I-band 2 deg.VLA-COSMOS: Schinnerer (PI) 1.4 GHz continuum, 1.5” res Large project (275hr): A+C array ~ 3,600 sources ~ 2(1) sqrdeg; rms](https://reader035.vdocuments.net/reader035/viewer/2022062605/5fdd894c54da571d3360045c/html5/thumbnails/1.jpg)
CosmosSurvey PI ScovilleHST 590 orbitsI-band 2 deg.2 !
![Page 2: Cosmos Survey PI Scoville HST 590 orbits I-band 2 deg.VLA-COSMOS: Schinnerer (PI) 1.4 GHz continuum, 1.5” res Large project (275hr): A+C array ~ 3,600 sources ~ 2(1) sqrdeg; rms](https://reader035.vdocuments.net/reader035/viewer/2022062605/5fdd894c54da571d3360045c/html5/thumbnails/2.jpg)
Major themes:
•Panchromatic studies of the coupled evolution of LSS, galaxies, star formation, AGN: environment and redshift
• Assembly of galaxies, clusters & dark matter (Coma supercluster)
• Area: mitigates cosmic variance
• Equitorial field
redshift slice from Λ CDM sim.
90 Mpc
![Page 3: Cosmos Survey PI Scoville HST 590 orbits I-band 2 deg.VLA-COSMOS: Schinnerer (PI) 1.4 GHz continuum, 1.5” res Large project (275hr): A+C array ~ 3,600 sources ~ 2(1) sqrdeg; rms](https://reader035.vdocuments.net/reader035/viewer/2022062605/5fdd894c54da571d3360045c/html5/thumbnails/3.jpg)
XMMHasinger et al.
GALEX FUV+NUVSchiminovich et al.
SUBARU BVr’i’z’SuprimeCam(Taniguchi et al.)
Xray -XMM
UV -Galex
Optical -UBVr’i’z’K + …HST/ACS F814W
Spectroscopy -VLT/VIMOSMagellan/IMACS
Infrared -Spitzer scheduled
mm -MAMBOBOLOCAM
cm -VLA
![Page 4: Cosmos Survey PI Scoville HST 590 orbits I-band 2 deg.VLA-COSMOS: Schinnerer (PI) 1.4 GHz continuum, 1.5” res Large project (275hr): A+C array ~ 3,600 sources ~ 2(1) sqrdeg; rms](https://reader035.vdocuments.net/reader035/viewer/2022062605/5fdd894c54da571d3360045c/html5/thumbnails/4.jpg)
VLA-COSMOS: Schinnerer (PI)1.4 GHz continuum, 1.5” res
Large project (275hr): A+C array ~ 3,600 sources ~ 2(1) sqrdeg; rms ~ 15(10) µJy/bm;
Deep project (60hr): A array~ 1 sqdeg; rms ~ 7 µJy/bm (central 30’)
Major science:• (dust-)obscured cosmic star formation history (Smolcic)• evolution of low luminosity radio AGN to high z (Jahnke)• evolution of the FIR-radio correlation (Schinnerer)• z=6 galaxies (Carilli)• absolute astrometry for COSMOS field (Aussel)
1.4d
![Page 5: Cosmos Survey PI Scoville HST 590 orbits I-band 2 deg.VLA-COSMOS: Schinnerer (PI) 1.4 GHz continuum, 1.5” res Large project (275hr): A+C array ~ 3,600 sources ~ 2(1) sqrdeg; rms](https://reader035.vdocuments.net/reader035/viewer/2022062605/5fdd894c54da571d3360045c/html5/thumbnails/5.jpg)
Hopkins et al. (2000)
AGN steep
flat
starbursts
spirals
SKA EVLA HDF/COSMOS++ 1st/NVSS Cambridge
Faint Radio Sources - Number Counts
(uncorrected)
![Page 6: Cosmos Survey PI Scoville HST 590 orbits I-band 2 deg.VLA-COSMOS: Schinnerer (PI) 1.4 GHz continuum, 1.5” res Large project (275hr): A+C array ~ 3,600 sources ~ 2(1) sqrdeg; rms](https://reader035.vdocuments.net/reader035/viewer/2022062605/5fdd894c54da571d3360045c/html5/thumbnails/6.jpg)
Low z examples
22””
z=0.2
22”” z=1.0
Higher z
22””
z=1.3
![Page 7: Cosmos Survey PI Scoville HST 590 orbits I-band 2 deg.VLA-COSMOS: Schinnerer (PI) 1.4 GHz continuum, 1.5” res Large project (275hr): A+C array ~ 3,600 sources ~ 2(1) sqrdeg; rms](https://reader035.vdocuments.net/reader035/viewer/2022062605/5fdd894c54da571d3360045c/html5/thumbnails/7.jpg)
VLAVLA--COSMOS COSMOS –– Optical IDs and Optical IDs and redshiftsredshifts
• within 1.0” – 2886 radio-optical associations (79%) for I < 23.5• Photo-z ~ 75%• Spectroscopic z’s ~ 50% (so far ~ 300 observed)
radio sources
allAGN
Redshift
all galaxies
![Page 8: Cosmos Survey PI Scoville HST 590 orbits I-band 2 deg.VLA-COSMOS: Schinnerer (PI) 1.4 GHz continuum, 1.5” res Large project (275hr): A+C array ~ 3,600 sources ~ 2(1) sqrdeg; rms](https://reader035.vdocuments.net/reader035/viewer/2022062605/5fdd894c54da571d3360045c/html5/thumbnails/8.jpg)
CWAT-01 at z~0.2:Merging of 4+ sub-clusters of galaxies Individual sub-clusters = 5e13 M_sun
z ~ 0.2
Wide Angle Tail Radio Galaxy (Smolcic et al. 2006)
20cm
Xray: rainbowOptical: RGBRadio: red
200kpc
![Page 9: Cosmos Survey PI Scoville HST 590 orbits I-band 2 deg.VLA-COSMOS: Schinnerer (PI) 1.4 GHz continuum, 1.5” res Large project (275hr): A+C array ~ 3,600 sources ~ 2(1) sqrdeg; rms](https://reader035.vdocuments.net/reader035/viewer/2022062605/5fdd894c54da571d3360045c/html5/thumbnails/9.jpg)
(Sub)mm Galaxies: formation of large elliptical galaxies(Bertoldi et al. 2006)
• 23 MAMBO (250 GHZ) sources (3.5< σ < 7; σ = 0.9 mJy)• 50% radio counterparts > 30 µJy• >50% (?) IRAC and/or 24um counterparts
Opt/rad/mamboIRAC/24um/mambo/rad
20”
10”
![Page 10: Cosmos Survey PI Scoville HST 590 orbits I-band 2 deg.VLA-COSMOS: Schinnerer (PI) 1.4 GHz continuum, 1.5” res Large project (275hr): A+C array ~ 3,600 sources ~ 2(1) sqrdeg; rms](https://reader035.vdocuments.net/reader035/viewer/2022062605/5fdd894c54da571d3360045c/html5/thumbnails/10.jpg)
Ly alpha emitting galaxies at z=5.7 (Ajiki et al)
LBG’s ==>
LAE’s ==>
100 candidates –double known samples
![Page 11: Cosmos Survey PI Scoville HST 590 orbits I-band 2 deg.VLA-COSMOS: Schinnerer (PI) 1.4 GHz continuum, 1.5” res Large project (275hr): A+C array ~ 3,600 sources ~ 2(1) sqrdeg; rms](https://reader035.vdocuments.net/reader035/viewer/2022062605/5fdd894c54da571d3360045c/html5/thumbnails/11.jpg)
Radio Properties of LAEs(Carilli et al. 2006)
2”
Lyα emitters (z~5.7):(Ajiki et al. 2006)
No radio counterparts < 30 µJy⇒ No AGN (FRI ~ M87)⇒ no (sub)mm galaxy w/
SFR > 1500 Msun
Stacked limit (2σ): 4.4 µJy⇒ mean SFR < 250 Msun
⇒ consistent w/ LAEs being moderate luminosity star forming galaxies(no beastly outliers)
![Page 12: Cosmos Survey PI Scoville HST 590 orbits I-band 2 deg.VLA-COSMOS: Schinnerer (PI) 1.4 GHz continuum, 1.5” res Large project (275hr): A+C array ~ 3,600 sources ~ 2(1) sqrdeg; rms](https://reader035.vdocuments.net/reader035/viewer/2022062605/5fdd894c54da571d3360045c/html5/thumbnails/12.jpg)
VLA-COSMOS -
- Status - 3,644 sources (> 4.5σ) in 2 sqrdeg (rms ~ 10 µJy)- central 30’ down to rms ~ 7 µJy (underway)- ~ 80% optical counterparts (--> spectroscopy)
- Science- 20cm emission: SF/AGN contribution - single targets: e.g. WAT radio galaxy- identification: (sub)mm sources - stacking analysis: LAE, …
- Products- 1.4 GHz image - source catalog - public release @ IRSA archive: ~ June ‘06
![Page 13: Cosmos Survey PI Scoville HST 590 orbits I-band 2 deg.VLA-COSMOS: Schinnerer (PI) 1.4 GHz continuum, 1.5” res Large project (275hr): A+C array ~ 3,600 sources ~ 2(1) sqrdeg; rms](https://reader035.vdocuments.net/reader035/viewer/2022062605/5fdd894c54da571d3360045c/html5/thumbnails/13.jpg)
END
![Page 14: Cosmos Survey PI Scoville HST 590 orbits I-band 2 deg.VLA-COSMOS: Schinnerer (PI) 1.4 GHz continuum, 1.5” res Large project (275hr): A+C array ~ 3,600 sources ~ 2(1) sqrdeg; rms](https://reader035.vdocuments.net/reader035/viewer/2022062605/5fdd894c54da571d3360045c/html5/thumbnails/14.jpg)
20cm continuum surveys:
VLA-COSMOS survey:unique phase spaceX-ray - mm complementary data~ 70% optical counterpartsphotometric redshifts (~ 900,000) spectroscopy (> 210 available; expected: 50%)
![Page 15: Cosmos Survey PI Scoville HST 590 orbits I-band 2 deg.VLA-COSMOS: Schinnerer (PI) 1.4 GHz continuum, 1.5” res Large project (275hr): A+C array ~ 3,600 sources ~ 2(1) sqrdeg; rms](https://reader035.vdocuments.net/reader035/viewer/2022062605/5fdd894c54da571d3360045c/html5/thumbnails/15.jpg)
9
10
11
12
13
14
Log
(FIR
Lum
inos
ity)
ULIRGs
LIRGs
AGN - SF
Sadler et al. (2002), Chapman et al. (2003) Radio Surveys Radio Surveys -- LimitsLimits
Milky Way
![Page 16: Cosmos Survey PI Scoville HST 590 orbits I-band 2 deg.VLA-COSMOS: Schinnerer (PI) 1.4 GHz continuum, 1.5” res Large project (275hr): A+C array ~ 3,600 sources ~ 2(1) sqrdeg; rms](https://reader035.vdocuments.net/reader035/viewer/2022062605/5fdd894c54da571d3360045c/html5/thumbnails/16.jpg)
•Ages around 0.1 Gyr
•Masses around 1010 M
•Ages and Masses consistent with z~6 LBG galaxies (Yan et. al. 2005)
•All LBGS known at z~6 have strong Lyman Alpha Emission
•Very compact morphology in ACS and NICMOS. No clear mergers