THE zCOSMOS 10k-BRIGHT SPECTROSCOPIC SAMPLE

By S. Lilly, V. Le Brun, C. Maier, V. Mainieri, M. Mignoli, M. Scodeggio, G. Zamorani, M. Carollo, Thierry Contini, Jean-Paul Kneib and 56 more. 2009

490 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/57bb8a933e8259f1fd49460ec09aec6ab7d2bd3c

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. P. Hopkins
2. L. Hernquist
3. D. M. Alexander
4. C. Conroy
5. R. Somerville
6. R. Dav'e
7. P. V. van Dokkum
8. A. Dekel

In Instrumentation

1. P. Hopkins
2. P. V. van Dokkum
3. L. Hernquist
4. C. Conroy
5. M. Franx
6. R. Dav'e
7. A. Dekel
8. D. M. Alexander

Citations in the corpus

• The Canadian Cluster Comparison Project: detailed study of systematics and updated weak lensing masses (2015, methodology): “The photometric redshifts were further refined by determining small offsets to the photometric zero-points using the ∼ 5000 spectroscopic redshifts available in the COSMOS field from the zCOSMOS-10k sample (Lilly et al. 2009).”
• KiDS+VIKING-450: Cosmic shear tomography with optical and infrared data (2018, methodology): “This is well documented for zCOSMOS-bright (Lilly et al. 2009), DEEP2 (Newman et al. 2013), and VVDS (Le Fèvre et al. 2013) showing an obvious trend with magnitude.”
• THE SINS/zC-SINF SURVEY of z ∼ 2 GALAXY KINEMATICS: OUTFLOW PROPERTIES (2012, background): “(1) Erb et al. (2006), (2) Steidel et al. (2004), (3) Erb et al. (2003), (4) Kurk et al. (2009), (5) Lilly et al. (2007), (6) Lilly et al. (2009), (7) McCracken et al. (2010). tation) in the narrow velocity component, and thus maximizes the contrast between the broad and narrow components.”
• PHIBSS: Unified Scaling Relations of Gas Depletion Time and Molecular Gas Fractions (2017, methodology): “…et al. 2007, Newman et al. 2013, Cooper et al. 2012), GOODS N/S (Giavalisco et al. 2004, Berta et al. 2010) and COSMOS fields (Scoville et al. 2007, Lilly et al. 2007, 2009), including the recent CANDELS J- and H-band HST imaging (Grogin et al. 2011, Koekemoer et al. 2011) and 3D-HST grism…”
• KiDS+VIKING-450 and DES-Y1 combined: Cosmology with cosmic shear (2019, methodology): “2 (inset), this overlap contains some 30,000 objects with spectroscopic redshifts from zCOSMOS (Lilly et al. 2009), the DEEP2 Redshift Survey (Newman et al. 2013), the VIMOS VLT Deep Survey (VVDS; Le Fèvre et al. 2013), and the Chandra Deep Field South (CDFS; Vanzella et al. 2008; Popesso et al.…”
• Identification of the brightest Lyα emitters at z = 6.6 : Implications for the evolution of the luminosity function in the reionization era (2015, background): “None of our LAE candidates are in the zCOSMOS (Lilly et al. 2009) or UDSz (Bradshaw et al. 2013; McLure et al. 2013) catalogues, which we also did not expect, since they would likely be interlopers in that case.”
• Galaxy Interactions Trigger Rapid Black Hole Growth: an unprecedented view from the Hyper Suprime-Cam Survey (2017, background): “In addition, the HSC Survey fields were carefully constructed to overlap with existing multi-wavelength survey fields, e.g., millimeter data from the Atacama Cosmology Telescope (ACT); X-ray data from multiple XMM-Newton and Chandra; near-/mid-infrared imaging surveys such as VIKING/VIDEO; UKIDSS; S”
• Second data release of the Hyper Suprime-Cam Subaru Strategic Program (2019, methodology): “The list includes redshifts from zCOSMOS DR3 (Lilly et al. 2009), UDSz (Bradshaw et al. 2013; McLure et al. 2013), 3DHST (Skelton et al. 2014; Momcheva et al. 2016), FMOSCOSMOS (Silverman et al. 2015; Kashino et al. 2019), VVDS (Le Fèvre et al. 2013), VIPERS PDR1 (Garilli et al. 2014), SDSS DR12 (A”
• zCOSMOS – 10k-bright spectroscopic sample - The bimodality in the galaxy stellar mass function: exploring its evolution with redshift (2009, methodology): “Compared to previous spectroscopic surveys, the larger area and number of spectroscopic redshifts of zCOSMOS allows higher precision, higher quality statistics, and lower cosmic variance (Lilly et al. 2009) to be achieved in our analysis, in particular for the massive end of the GSMF s.”
• THE COS-DWARFS SURVEY: THE CARBON RESERVOIR AROUND SUB-L* GALAXIES (2014, methodology): “The advent of large galaxy surveys (York et al. 2000; Lilly et al. 2009), and the introduc- 1 Based on observations made with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc.,…”
• A large Hα survey at z = 2.23, 1.47, 0.84 and 0.40: the 11 Gyr evolution of star-forming galaxies from HiZELS (2012, background): “Spectroscopic redshift are also available for a fraction of the selected lineemitters (Lilly et al. 2009; Yamada et al. 2005; Simpson et al. 2006; Geach et al. 2008; van Breukelen et al. 2007; Ouchi et al. 2008; Smail et al. 2008; Ono et al. 2010)6.”
• THE CHANDRA COSMOS LEGACY SURVEY: OVERVIEW AND POINT SOURCE CATALOG (2016, methodology): “, over 300 nights of large ground-based telescopes VLT, Keck, Subaru, VISTA for both imaging and spectroscopy (Lilly et al. 2009, Hasinger et al. in prep., Taniguchi et al. 2007, McCraken et al. 2014) has been made in this field.”
• The Herschel* PEP/HerMES luminosity function - I. Probing the evolution of PACS selected Galaxies to z ≃ 4 (2013, methodology): “Finally, in COSMOS we could use a collection of ∼3000 spectroscopic redshifts from either the public zCOSMOS bright database or the non-public zCOSMOS deep database (Lilly, S.J. et al. 2007; Lilly et al. 2009).”
• THE XMM-NEWTON WIDE-FIELD SURVEY IN THE COSMOS FIELD (XMM-COSMOS): DEMOGRAPHY AND MULTIWAVELENGTH PROPERTIES OF OBSCURED AND UNOBSCURED LUMINOUS ACTIVE GALACTIC NUCLEI (2010, background): “…from Magellan/IMACS and MMT observation campaigns (∼ 530 objects, Trump et al. 2007, 2009), from the VIMOS/zCOSMOS bright project (∼ 500 objects, Lilly et al. 2009), from the VIMOS/zCOSMOS faint project (∼ 80 objects, Lilly et al. 2007) or were already present either in the SDSS survey…”
• Improved constraints on the expansion rate of the Universe up to z ∼ 1.1 from the spectroscopic evolution of cosmic chronometers (2012, methodology): “This sample has been extracted from the zCOSMOS 20k bright sample [38].”
• THE SFR–M* RELATION AND EMPIRICAL STAR FORMATION HISTORIES FROM ZFOURGE AT 0.5 < z < 4 (2015, background): “For COSMOS spectroscopic redshifts come from Lilly et al. (2009) and Trump et al. (2009).”
• Photometric redshift analysis in the Dark Energy Survey Science Verification data (2014, methodology): “…was likewise obtained during DES SV. Deep dithered imaging data for the COSMOS field, centered on the Cosmological Evolution Survey (COSMOS) area (Lilly et al. 2007, 2009) were obtained during February 2013 by a DECam community program.2 Each one of the four fields covers about the area of a…”
• The WIRCam Deep Survey I. Counts, colours, and mass-functions derived from near-infrared imaging in the CFHTLS deep fields (2011, methodology): “In the D2/COSMOS field we use the zCOSMOS “10K” spectroscopic sample (Lilly et al. 2009).”
• Tracking the impact of environment on the galaxy stellar mass function up to z ~ 1 in the 10 k zCOSMOS sample (2009, methodology): “The data used in this paper belong to the so-called 10k sample (Lilly et al. 2009), consisting of the first 10644 observed objects of the “bright” survey, over an area of 1.402 deg2 with a mean sampling rate of∼ 33%.”