Forward modeling of galaxy kinematics in slitless spectroscopy [PDF]
Astronomy & Astrophysics, 2019 Context. Slitless spectroscopy has long been considered a complicated and confused technique. Nonetheless, with the advent of Hubble Space Telescope (HST) instruments, characterized by a low sky background level and a high spatial resolution (most ...
Mehdi Outini, Y. Copin
semanticscholar +1 more source
Searching for environmental effects on galaxy kinematics in groups and clusters atz∼ 1 from the ORELSE survey [PDF]
Monthly notices of the Royal Astronomical Society, 2018 We present an investigation of the dependence of galaxy kinematics on the environment for a sample of 94 star-forming galaxies at $z\sim0.9$ from the ORELSE survey.
D. Pelliccia +11 more
semanticscholar +1 more source
Point-spread Function Deconvolution of the IFU Data and Restoration of Galaxy Stellar Kinematics [PDF]
Astrophysical Journal Supplement Series, 2020 We present a performance test of the point-spread function (PSF) deconvolution algorithm applied to astronomical integral field unit (IFU) spectroscopy data for restoration of galaxy kinematics.
Haeun Chung +2 more
semanticscholar +1 more source
Galaxy kinematics and mass calibration in massive SZE-selected galaxy clusters toz = 1.3 [PDF]
Monthly notices of the Royal Astronomical Society, 2017 The galaxy phase-space distribution in galaxy clusters provides insights into the formation and evolution of cluster galaxies, and it can also be used to measure cluster mass profiles.
R. Capasso +38 more
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Spatially Resolved Stellar Kinematics of the Ultra-diffuse Galaxy Dragonfly 44. I. Observations, Kinematics, and Cold Dark Matter Halo Fits [PDF]
Astrophysical Journal, 2019 We present spatially resolved stellar kinematics of the well-studied ultra-diffuse galaxy (UDG) Dragonfly 44, as determined from 25.3 hr of observations with the Keck Cosmic Web Imager.
P. V. van Dokkum +10 more
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THE KMOS3D SURVEY: DESIGN, FIRST RESULTS, AND THE EVOLUTION OF GALAXY KINEMATICS FROM 0.7 ⩽ z ⩽ 2.7 [PDF]
, 2014 We present the KMOS3D survey, a new integral field survey of over 600 galaxies at 0.7 < z < 2.7 using KMOS at the Very Large Telescope. The KMOS3D survey utilizes synergies with multi-wavelength ground- and space-based surveys to trace the evolution of ...
E. Wisnioski +26 more
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The kinematic centre of the Galaxy [PDF]
Monthly Notices of the Royal Astronomical Society, 1985 La decouverte d'un anneau d'hydrogene moleculaire chaud, optiquement mince autour du noyau galactique permet d'etudier si le champ des vitesses dans la region centrale de la Galaxie est approximativement a symetrie ...
S. V. M. Clube, R. Pan
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LINKING THE SPIN EVOLUTION OF MASSIVE BLACK HOLES TO GALAXY KINEMATICS [PDF]
, 2014 We present the results of a semianalytical model that evolves the masses and spins of massive black holes together with the properties of their host galaxies across the cosmic history.
A. Sesana +3 more
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THE SINS/zC-SINF SURVEY OF z ∼ 2 GALAXY KINEMATICS: REST-FRAME MORPHOLOGY, STRUCTURE, AND COLORS FROM NEAR-INFRARED HUBBLE SPACE TELESCOPE IMAGING [PDF]
, 2014 We present the analysis of Hubble Space Telescope (HST) J- and H-band imaging for 29 galaxies on the star-forming main sequence at z ∼ 2, which have adaptive optics Very Large Telescope SINFONI integral field spectroscopy from our SINS/zC-SINF program ...
S. Tacchella +17 more
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The SAMI Galaxy Survey: first detection of a transition in spin orientation with respect to cosmic filaments in the stellar kinematics of galaxies [PDF]
Monthly notices of the Royal Astronomical Society, 2019 We present the first detection of mass-dependent galactic spin alignments with local cosmic filaments with >2σ confidence using IFS kinematics. The 3D network of cosmic filaments is reconstructed on Mpc scales across GAlaxy and Mass Assembly fields ...
C. Welker +19 more
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