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CLASH Prediction and Discovery

CLASH Prediction and Discovery. Survey Limit. Postman et al. 2011. Candidates of z ~10 in CANDLES. Oesch et al. 2013. Candidate of z ~12 in UDF. Bouwens et al. 2011. UDF-JD. Ellis et al. 2013. Star Formation Rate Density. Oesch et al. 2013. Extreme Emission Line Galaxies.

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CLASH Prediction and Discovery

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  1. CLASH Prediction and Discovery Survey Limit Postman et al. 2011 London

  2. Candidates of z~10 in CANDLES Oesch et al. 2013 London

  3. Candidate of z~12 in UDF Bouwens et al. 2011 London

  4. UDF-JD Ellis et al. 2013 London

  5. Star Formation Rate Density Oesch et al. 2013 London

  6. Extreme Emission Line Galaxies Brammer et al. 2013 London

  7. Potential Contamination London

  8. Emission Lines in Broad Bands London

  9. Color Selection Coe et al. 2013 London

  10. Emission Line Galaxies in CLASH Database • 58 candidates in J sample (F125W) • 21 candidates in Y sample (F105W) • Continuum magnitude 24-30 • Largest EW >3000 Å in restframe • Source density ~3× CANDELS London

  11. Equivalent Width vs. Magnitude London

  12. Distribution of Magnification London

  13. Broad Band Property in Y Sample London

  14. Broad Band Property in J Sample London

  15. Candidates with Extreme High EW London

  16. Summary • Emission line galaxies of z~1.5 are common at the faint end • Some of them exhibit very large equivalent widths • Potential misidentification as z~7 galaxies with very blue continuum • Potential misidentification with z~11 galaxies London

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