1. 25 Nov 20091 Triggering radio galaxies at 0<z<1 Elaine M. Sadler  Luminosity functions and stellar populations  New spectroscopic samples at 0<z<1  High frequency: the AT20G survey [with Russell Cannon, Scott Croom, Tom Mauch, Tara Murphy, Helen Johnston, Paul Hancock & the AT20G, 6dFGS, 2SLAQ, WiggleZ and GAMA survey teams]

2. 25 Nov 20092 Radio-source populations at z~0 Local radio-source populations now mapped out in detail from large-area radio + optical surveys Good-quality optical spectra available for >20,000 local radio- emitting galaxies! (2dFGRS/SDSS/6dFGS +NVSS/SUMSS/FIRST)

3. 25 Nov 20093 Local (z~0) radio LFs for AGN and star- forming galaxies now accurately measured over six orders of magnitude. Sample is large enough to split by M K SF AGN (Mauch & Sadler 2007) NVSS+6dFGS

4. 25 Nov 20094 Fraction of galaxies hosting radio-loud AGN increases with galaxy stellar mass (Auriemma+ 77, Sadler+ 89, Best+ 05) BH duty cycle high in local massive galaxies (Mauch & Sadler 2007)

5. 25 Nov 20095 “Post-starburst” radio galaxies 2dFGRS radio galaxy: Balmer abs. lines imply a massive (~10 10 M sun ) starburst occurred ~0.15 Gyr ago. Compact, steep-spectrum radio source has P 1.4 ~ 10 25 W/Hz, M K ~ -25. Extremely rare locally! (<0.01% of radio AGN)

6. 25 Nov 20096 Stellar populations of radio galaxies at 0.4<z<0.8 Photometric selection from SDSS, sky area ~150 deg 2 Optical spectra and redshifts from AAT/2dF 15,000 spectra of luminous red galaxies (LRGs) at 0.4<z<0.8 10,000+ faint QSO spectra Survey paper: Cannon et al. (2006) MNRAS 372, 425

7. 25 Nov 20097 First detection of cosmic evolution for low-power radio galaxies. P<10 26 W/Hz radio AGN population well-fitted by luminosity evolution of the form (1+z) 2. More rapid evolution for powerful sources (Sadler+ 07, Donoso+ 09) z=0.5 z=0

8. 25 Nov 20098 z SF 2SLAQ radio galaxies redder (and more clustered: Wake+ 08) than the general LRG population, passively-evolving optical LF.

9. 25 Nov 20099 Composite LRG optical spectra 0.45<z<0.5 0.55<z<0.65 Analysed matched composite spectra to test for differences between the stellar populations of radio-loud and radio-quiet 2SLAQ galaxies (Johnston+ 08). 0.65<z<0.85

10. 25 Nov 200910 Binned in redshiftBinned in radio power (Johnston+08)

11. 25 Nov 200911 Fitted composite spectra with two single-age stellar populations, old (~7 Gyr) plus younger (10 Myr to 5 Gyr). In general, no difference between stellar populations of radio-detected galaxies and full 2SLAQ LRG sample. Around 30-40% of the light at 4000A comes from intermediate-age stars (~1 Gyr old, <1% by mass). The most powerful radio galaxies (>10 26 W/Hz) have strong emission lines, AND a younger (100 Myr) stellar population. Stellar populations at z~0.5

12. 25 Nov 200912 L* Recent mergers? Rapid evolution like ULIRGS, QSOs. “Optically-quiet” radio galaxies Evolution as (1+z) 2, similar to cosmic SF density. Not yet observed beyond z~0.7. FRI FRII Represent ~ 0.5% of 2SLAQ galaxies at z~0.6 Cold mode? Hot mode

13. 25 Nov 200913 Blue radio galaxies at 0<z<1? What about the effects of colour selection in LRG samples? Are we missing a population of blue radio galaxies? How are are radio galaxies and radio-loud QSOs related? Work in progress: New spectroscopic survey, piggy- backed on AAT large-area WiggleZ and GAMA surveys

14. 25 Nov 200914 Piggyback spectroscopy: Spare fibres from AAT WiggleZ survey. FIRST radio sources with i<20.5 mag, no colour selection. ~3000 spectra so far

15. 25 Nov 200915 Wigglez radio galaxies LRGs QSOs

16. 25 Nov 200916 Wigglez radio galaxies

17. 25 Nov 200917 Wigglez radio galaxies

18. 25 Nov 200918 Wigglez radio galaxies

19. 25 Nov 200919 Currently ~3000 radio-loud AGN spectra from WiggleZ/GAMA, redshift range 0<z<1. Goal is to map out hot/cold accretion systems vs redshift and clustering environment to z~1.

20. 25 Nov 200920 Image Credit: D.Smyth The Australia Telescope 20 GHz Survey 2004-2009: Wide-band correlator on ATCA, 2.4 arcmin FoV, fast scanning at 15 deg/minute, 54ms sampling AT20G team: PI Ron Ekers and 25 astronomers/engineers/students

21. 25 Nov 200921 VLSS WENSS SUMSS NVSS AT20G PMN WMAP Most work on radio galaxy populations/demographics has been at frequencies near 1.4 GHz - where the deepest radio surveys are. Can we learn something new at higher frequencies?

22. 25 Nov 200922 Full AT20G source catalogue just released (Murphy et al. 2009) Almost 6000 sources above 40 mJy limit, optical positions to ~1 arcsec. Also simultaneous 5 and 8 GHz meas, polarization www.atnf.csiro.au/re search/AT20G/

23. 25 Nov 200923 AT20G, radio two-colour diagram: 65% QSOs & BL Lacs, 25% galaxies, 10% faint/blank.

24. 25 Nov 200924 O’Dea (1998)AT20G Sample Typical Peak Freq1 GHz8-15 GHz Number of sources31688 Galaxy/QSO fraction50% / 50%23% / 77% Median z0.5 / 1.60.2 / 1.2 Median Log(P 5 )27 / 28 W/Hz25 / 27 W/Hz AT20G `extreme GPS’ sources Paul Hancock (2009 PhD thesis): Complete sample of 688 GigaHertz Peaked Spectrum (GPS) sources with spectral peaks above 5GHz - the youngest nearby radio sources?

25. 25 Nov 200925 SUMSS 843 MHz AT20G AT20G J074618-570258: z=0.13, passive early-type galaxy. FRI Giant radio galaxy at 843 MHz (Saripalli+ 05), extreme GPS source with peak above 20 GHz (Hancock+ 09) A nearby recently- retriggered radio galaxy?

26. 25 Nov 200926 Local AT20G sources: the 6dFS sample Complete spectroscopic sample, 195 sources with K<12.6 mag, median z~0.05. ~25% extended at 20GHz Many `old friends’ from the 2Jy sample Work in progress! First measurement of the local (z<0.1) RLF at 20 GHz

27. 25 Nov 200927 Summary Luminosity functions are important - they tell us what’s common and what’s rare. High-frequency radio surveys are becoming easier, and can provide a new perspective on the demographics and triggering of young radio sources.

28. 25 Nov 200928