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Journal Article

The SINS/zC-SINF Survey of z ̃ 2 Galaxy Kinematics: SINFONI Adaptive Optics-assisted Data and Kiloparsec-scale Emission-line Properties

MPS-Authors

Förster Schreiber,  N. M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Renzini,  A.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Mancini,  C.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Genzel,  R.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Bouché,  N.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Cresci,  G.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Hicks,  E. K. S.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Lilly,  S. J.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Peng,  Y.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Burkert,  A.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Carollo,  C. M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Cimatti,  A.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Daddi,  E.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Davies,  R. I.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Genel,  S.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Kurk,  J. D.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Lang,  P.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Lutz,  D.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Mainieri,  V.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

McCracken,  H. J.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Mignoli,  M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Naab,  T.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Oesch,  P.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Pozzetti,  L.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Scodeggio,  M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Shapiro Griffin,  K.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Shapley,  A. E.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Sternberg,  A.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Tacchella,  S.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Tacconi,  L. J.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Wuyts,  S.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Zamorani,  G.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

External Resource

https://ui.adsabs.harvard.edu/abs/2018ApJS..238...21F
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Citation

Förster Schreiber, N. M., Renzini, A., Mancini, C., Genzel, R., Bouché, N., Cresci, G., et al. (2018). The SINS/zC-SINF Survey of z ̃ 2 Galaxy Kinematics: SINFONI Adaptive Optics-assisted Data and Kiloparsec-scale Emission-line Properties. The Astrophysical Journal Supplement Series, 238.


Cite as: https://hdl.handle.net/21.11116/0000-0005-CDBC-1
Abstract
We present the “SINS/zC-SINF AO survey” of 35 star-forming galaxies, the largest sample with deep adaptive optics (AO)-assisted near-infrared integral field spectroscopy at z ̃ 2. The observations, taken with SINFONI at the Very Large Telescope, resolve the Hα and [N II] emission and kinematics on scales of ̃1.5 kpc. The sample probes the massive (M ⋆ ̃ 2 × 109 - 3 × 1011 M ☉), actively star-forming (SFR ̃ 10-600 M ☉ yr-1) part of the z ̃ 2 galaxy population over a wide range of colors ((U - V)rest ̃ 0.15-1.5 mag) and half-light radii (R e,H ̃ 1-8.5 kpc). The sample overlaps largely with the “main sequence” of star-forming galaxies in the same redshift range to a similar K AB = 23 mag limit; it has ̃0.3 dex higher median specific SFR, ̃0.1 mag bluer median (U - V)rest color, and ̃10% larger median rest-optical size. We describe the observations, data reduction, and extraction of basic flux and kinematic properties. With typically 3-4 times higher resolution and 4-5 times longer integrations (up to 23 hr) than the seeing-limited data sets of the same objects, the