Measuring galaxy environment with the synergy of future photometric and spectroscopic surveys
Cucciati, O.; Marulli, F.; Cimatti, A.; Merson, A.I.; Norberg, P.; Pozzetti, L.; Baugh, C.M.; Branchini, E.
Professor Peder Norberg email@example.com
Professor Carlton Baugh firstname.lastname@example.org
We exploit the synergy between low-resolution spectroscopy and photometric redshifts to study environmental effects on galaxy evolution in slitless spectroscopic surveys from space. As a test case, we consider the future Euclid Deep survey (∼40 deg2), which combines a slitless spectroscopic survey limited at Hα flux ≥5 × 10−17 erg cm−2 s−1 and a photometric survey limited in H band (H ≤ 26). We use Euclid-like galaxy mock catalogues, in which we anchor the photometric redshifts to the 3D galaxy distribution of the available spectroscopic redshifts. We then estimate the local density contrast by counting objects in cylindrical cells with radius from 1 to 10 h−1Mpc, over the redshift range 0.9 < z < 1.8. We compare this density field with the one computed in a mock catalogue with the same depth as the Euclid Deep survey (H = 26) but without redshift measurement errors. We find that our method successfully separates high- from low-density environments (the last from the first quintile of the density distribution), with higher efficiency at low redshift and large cells: the fraction of low-density regions mistaken by high-density peaks is <1 per cent for all scales and redshifts explored, but for scales of 1 h−1Mpc for which is a few per cent. These results show that we can efficiently study environment in photometric samples if spectroscopic information is available for a smaller sample of objects that sparsely samples the same volume. We demonstrate that these studies are possible in the Euclid Deep survey, i.e. in a redshift range in which environmental effects are different from those observed in the local Universe, hence providing new constraints for galaxy evolution models.
Cucciati, O., Marulli, F., Cimatti, A., Merson, A., Norberg, P., Pozzetti, L., …Branchini, E. (2016). Measuring galaxy environment with the synergy of future photometric and spectroscopic surveys. Monthly Notices of the Royal Astronomical Society, 462(2), 1786-1801. https://doi.org/10.1093/mnras/stw1729
|Journal Article Type||Article|
|Acceptance Date||Jul 14, 2016|
|Online Publication Date||Jul 19, 2016|
|Publication Date||Oct 21, 2016|
|Deposit Date||Sep 28, 2016|
|Publicly Available Date||Oct 6, 2016|
|Journal||Monthly Notices of the Royal Astronomical Society|
|Publisher||Royal Astronomical Society|
|Peer Reviewed||Peer Reviewed|
Published Journal Article
This article has been published in Monthly Notices of the Royal Astronomical Society ©: 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
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