(Spitzer Large
Area Survey with Hyper-Suprime-Cam)
- Hatfield, P. W.; Bowler, R. A. A.; et el. (2018) The
environment and host haloes of the brightest z ~ 6 Lyman-break
galaxies; Monthly Notices of the Royal Astronomical Society; Vol.
477; No. 3; 3760-3774; 10.1093/mnras/sty856
- Mehta, Vihang; Scarlata, Claudia; et el. (2018) SPLASH-SXDF
Multi-wavelength Photometric Catalog; Astrophysical Journal
Supplement Series; Vol. 235; No. 2; Art. No. 36; 10.3847/1538-4365/aab60c
- Gilbert, Karoline M.; Tollerud, Erik J.; et el. (2018) Global
Properties of M31’s Stellar Halo from the SPLASH Survey. III. Measuring
the Stellar Velocity Dispersion Profile; Astrophysical Journal; Vol.
852; No. 2; Art. No. 128; 10.3847/1538-4357/aa9f26
- Stefanon, Mauro; Labbé, Ivo; et el. (2017) HST
Imaging of the Brightest z ~ 8–9 Galaxies from UltraVISTA: The Extreme
Bright End of the UV Luminosity Function; Astrophysical Journal;
Vol. 851; No. 1; Art. No. 43; 10.3847/1538-4357/aa9a40
- Andrews, S. K.; Driver, S. P.; et el. (2017) G10/COSMOS:
38 band (far-UV to far-IR) panchromatic photometry using LAMBDAR;
Monthly Notices of the Royal Astronomical Society; Vol. 464; No. 2;
1569-1590; 10.1093/mnras/stw2395
- Davidzon, I.; Ilbert, O.; et el. (2017) The
COSMOS2015 galaxy stellar mass function: Thirteen billion years of
stellar mass assembly in ten snapshots; Astronomy and Astrophysics;
Vol. 605; Art. No. A70; 10.1051/0004-6361/201730419
- Stefanon, Mauro; Bouwens, Rychard J.; et el. (2017) The
rest-frame optical (900nm) galaxy luminosity function at z ~ 4-7:
abundance matching points to limited evolution in the M_(STAR)/M_(HALO)
ratio at z ⩾ 4; Astrophysical Journal; Vol. 843; No. 1; Art. No. 36;
10.3847/1538-4357/aa72d8
- Michałowski, Michał J.; Dunlop, J. S.; et el. (2017) The
SCUBA-2 Cosmology Legacy Survey: the nature of bright submm galaxies
from 2 deg² of 850-μm imaging; Monthly Notices of the Royal
Astronomical Society; Vol. 469; No. 1; 492-515; 10.1093/mnras/stx861
- Bowler, R. A. A.; McLure, R. J.; et el. (2017) No
evidence for Population III stars or a direct collapse black hole in the
z = 6.6 Lyman α emitter ‘CR7’; Monthly Notices of the Royal
Astronomical Society; Vol. 469; No. 1; 448-458; 10.1093/mnras/stx839
- Bowler, R. A. A.; Dunlop, J. S.; et el. (2017) Unveiling
the nature of bright z ≃ 7 galaxies with the Hubble Space Telescope;
Monthly Notices of the Royal Astronomical Society; Vol. 466; No. 3;
3612-3635; 10.1093/mnras/stw3296
- Pacucci, Fabio; Pallottini, Andrea; et el. (2017) The
nature of the Lyman α emitter CR7: a persisting puzzle; Monthly
Notices of the Royal Astronomical Society: Letters; Vol. 468; No. 1;
L77-L81; 10.1093/mnrasl/slx029
- Smolčić, V.; Miettinen, O.; et el. (2017) (Sub)millimetre
interferometric imaging of a sample of COSMOS/AzTEC submillimetre
galaxies. III. Environments; Astronomy and Astrophysics; Vol. 597;
Art. No. A4; 10.1051/0004-6361/201526989
- Miettinen, O.; Delvecchio, I.; et el. (2017) (Sub)millimetre
interferometric imaging of a sample of COSMOS/AzTEC submillimetre
galaxies. IV. Physical properties derived from spectral energy
distributions; Astronomy and Astrophysics; Vol. 597; Art. No. A5; 10.1051/0004-6361/201628128
- Mortlock, Alice; McLure, Ross J.; et el. (2017) Characterizing
the evolving K-band luminosity function using the UltraVISTA, CANDELS
and HUDF surveys; Monthly Notices of the Royal Astronomical Society;
Vol. 465; No. 1; 672-687; 10.1093/mnras/stw2728
- Schinnerer, E.; Groves, B.; et el. (2016) Gas
Fraction and depletion time of massive star-forming galaxies at z ∼ 3.2:
No change in global star formation process out to z > 3;
Astrophysical Journal; Vol. 833; No. 1; Art No 112; 10.3847/1538-4357/833/1/112
- Steinhardt, Charles. L.; Capak, Peter; et el. (2016) The
Impossibly Early Galaxy Problem; Astrophysical Journal; Vol. 824;
No. 1; Art. No. 21; 10.3847/0004-637X/824/1/21
- Roberts-Borsani, G. W.; Bouwens, R. J.; et el. (2016) z≳
7 galaxies with red Spitzer/IRAC [3.6]-[4.5] colors in the full CANDELS
data set: The brightest-known galaxies at z~ 7-9 and a probable
spectroscopic confirmation at z = 7.48; Astrophysical Journal; Vol.
823; No. 2; Art. No. 143; 10.3847/0004-637X/823/2/143
- Laigle, C.; Capak, P.; et el. (2016) The
COSMOS2015 Catalog: Exploring the 1 < z < 6 Universe with Half a
Million Galaxies; Astrophysical Journal Supplement Series; Vol. 224;
No. 2; Art. No. 24; 10.3847/0067-0049/224/2/24
- Faisst, A. L.; Capak, P. L.; et el. (2016) Rest-UV
Absorption Lines as Metallicity Estimator: the Metal Content of
Star-Forming Galaxies at z ~ 5; Astrophysical Journal; Vol. 822;
No. 1; Art. No. 29; 10.3847/0004-637X/822/1/29
- Faisst, A. L.; Capak, P.; et el. (2016) A
Coherent Study of Emission Lines from Broadband Photometry: Specific
Star Formation Rates and [O III]/Hβ Ratio at 3 < z < 6;
Astrophysical Journal; Vol. 821; No. 2; Art. No. 122; 10.3847/0004-637X/821/2/122
- Parsa, Shaghayegh; Dunlop, James S.; et el. (2016) The
galaxy UV luminosity function at z≃ 2–4; new results on faint-end slope
and the evolution of luminosity density; Monthly Notices of the
Royal Astronomical Society; Vol. 456; No. 3; 3194-3211; 10.1093/mnras/stv2857
- Civano, F.; Capak, P.; et el. (2016) The
Chandra COSMOS Legacy survey: overview and point source catalog;
Astrophysical Journal; Vol. 819; No. 1; Art. No. 62; 10.3847/0004-637X/819/1/62
- Lin, Lihwai; Capak, P. L.; et el. (2016) The
SPLASH Survey: Quiescent Galaxies Are More Strongly Clustered but Are
Not Necessarily Located in High-density Environments; Astrophysical
Journal; Vol. 817; No. 2; Art. No. 97; 10.3847/0004-637X/817/2/97
- Marchesi, S.; Civano, F.; et el. (2016) The
CHANDRA COSMOS Legacy Survey: Optical / IR Identifications;
Astrophysical Journal; Vol. 817; No. 1; Art No 34; 10.3847/0004-637X/817/1/34
- Ilbert, O.; Arnouts, S.; et el. (2015) Evolution
of the specific star formation rate function at z < 1.4 Dissecting
the mass-SFR plane in COSMOS and GOODS; Astronomy and Astrophysics;
Vol. 579; Art. No. A2; 10.1051/0004-6361/201425176
- Coupon, J.; Arnouts, S.; et el. (2015) The
galaxy-halo connection from a joint lensing, clustering and abundance
analysis in the CFHTLenS/VIPERS field; Monthly Notices of the Royal
Astronomical Society; Vol. 449; No. 2; 1352-1379; 10.1093/mnras/stv276
- Miettinen, O.; Smolčić, V.; et el. (2015) (Sub)millimetre
interferometric imaging of a sample of COSMOS/AzTEC submillimetre
galaxies. I. Multiwavelength identifications and redshift
distribution; Astronomy and Astrophysics; Vol. 577; Art. No. A29; 10.1051/0004-6361/201425032
- Lee, Nicholas; Sanders, D. B.; et el. (2015) A
Turnover in the Galaxy Main Sequence of Star Formation at M_* ~ 10^(10)
M_☉ for Redshifts z < 1.3; Astrophysical Journal; Vol. 801;
No. 2; Art. No. 80; 10.1088/0004-637X/801/2/80
- Scoville, Nick; Faisst, Andreas; et el. (2015) Dust
Attenuation in High Redshift Galaxies: “Diamonds in the Sky”;
Astrophysical Journal; Vol. 800; No. 2; Art. No. 108; 10.1088/0004-637X/800/2/108
- Gilbert, Karoline M.; Kalirai, Jason S.; et el. (2014) Global
Properties of M31’s Stellar Halo from the SPLASH Survey. II. Metallicity
Profile; Astrophysical Journal; Vol. 796; No. 2; Art. No. 76; 10.1088/0004-637X/796/2/76
- Steinhardt, Charles L.; Speagle, Josh S.; et el. (2014) Star
Formation at 4 < z < 6 from the Spitzer Large Area Survey with
Hyper-Suprime-Cam (SPLASH); Astrophysical Journal Letters; Vol. 791;
No. 2; Art. No. L25; 10.1088/2041-8205/791/2/L25
- Bowler, R. A. A.; Dunlop, J. S.; et el. (2014) The
bright end of the galaxy luminosity function at z =7: before the onset
of mass quenching?; Monthly Notices of the Royal Astronomical
Society; Vol. 440; No. 3; 2810-2842; 10.1093/mnras/stu449
- Kalirai, Jason S.; Beaton, Rachael L.; et el. (2010) The
SPLASH Survey: Internal Kinematics, Chemical Abundances, and Masses of
the Andromeda I, II, III, VII, X, and XIV Dwarf Spheroidal Galaxies;
Astrophysical Journal; Vol. 711; No. 2; 671-692; 10.1088/0004-637X/711/2/671
- Gilbert, Karoline M.; Guhathakurta, Puragra; et el. (2009) The
Splash Survey: A Spectroscopic Portrait of Andromeda’s Giant Southern
Stream; Astrophysical Journal; Vol. 705; No. 2; 1275-1297; 10.1088/0004-637X/705/2/1275