How to find the dependencies of a table in redshift?
Answers from top 8 papers
More filters
| Papers (8) | Insight |
|---|---|
| However, we find that for the data used the inclusion of morphological information does not have a statistically significant benefit for photometric redshift estimation with the techniques employed here. | |
| These results have strong implications for the analysis of redshift surveys at intermediate redshift. | |
| We present a simple and powerful empirical method to constrain photometric redshift uncertainties in the absence of spectroscopic redshifts. | |
| The methods that we develop are applicable to general photometric redshift surveys. | |
| We show that the redshift distribution of our sample is in excellent agreement with smaller and much deeper photometric and spectroscopic redshift surveys. | |
28 Citations | Finally, reconstruction can improve the determination of Ω and b from joint analyses of redshift and peculiar velocity surveys because it provides a fully nonlinear prediction of the peculiar velocity distribution at each point in redshift space. |
116 Citations | The new high signal-to-noise ratio spectra therefore allow us to measure the redshift of 18 sources. |
75 Citations | Our analysis proves that photometric redshift techniques can and must be used to extend the range of applicability of the spectroscopic redshift measurements. |