Results 91 to 100 of about 30,270 (299)

Galaxy and Mass Assembly (GAMA): the GAMA galaxy group catalogue (G3Cv1) [PDF]

, 2011
Using the complete Galaxy and Mass Assembly I (GAMA-I) survey covering ∼142deg2 torAB= 19.4, of which ∼47deg2 is torAB= 19.8, we create the GAMA-I galaxy group catalogue (G3Cv1), generated using a friends-of-friends (FoF) based grouping algorithm ...
Frenk, C.S., Norberg, Peder, S. M. Croom, Baldry, I., Kampen, E. van, Pimbblet, K. A., Hopkins, A., Hill, D. T., Driver, S. P., Kelvin, L., R. J. Tuffs, Sutherland, W., Nichol, R., Frenk, Carlos S., Kuijken, K., Hopkins, Andrew M., Taylor, Edward N., Driver, S.P., S. P. Bamford, C. S. Frenk, S. P. Driver, J. Liske, Bamford, S.P., Hill, David T., Loveday, J., Brough, S., D. Thomas, E. van Kampen, Cameron, E., Sharp, Robert, Kuijken, K.H., Tuffs, R. J., D. H. Jones, Robotham, A. S. G., Jones, D. H., van Kampen, E., Sharp, R.G., Liske, Jochen, A. S. G. Robotham, Frenk, C., Robotham, A.S.G., Merson, A., C. J. Conselice, S. Phillipps, Bamford, S., D. T. Hill, Parkinson, Hannah R., Prescott, M., Sharp, R. G., Nichol, Robert C., Pimbblet, Kevin A., Peacock, J. A., C. C. Popescu, Baldry, Ivan K., Nichol, R. C., Thomas, Daniel, Taylor, E. N., Wijesinghe, D., Peacock, John A, J. A. Peacock, K. Kuijken, Popescu, C., Peacock, J.A., Kelvin, L.S., Conselice, C.J., Croom, S.M., Jones, D., W. J. Sutherland, Kelvin, Lee S., A. M. Hopkins, Jones, David Heath, Peacock, J., Thomas, D., Popescu, Cristina C., R. G. Sharp, Robotham, Aaron, Conselice, C., Kuijken, Konrad, Hill, D.T., Gunawardhana, M. L. P., Sharp, Robert G., Jones, D.H., Driver, Simon P., D. Wijesinghe, Robotham, A., H. R. Parkinson, Tuffs, R., Bamford, S. P., Norberg, P, Conselice, C. J., Taylor, E., Nichol, R.C., Baldry, I. K., I. K. Baldry, Sutherland, W. J., Tuffs, R.J., Baldry, I.K., Prescott, Matthew, Tuffs, Richard J., Hill, D., Sutherland, Will J., Phillipps, Steven, R. C. Nichol, Gunawardhana, M., Hopkins, A. M., M. Prescott, Croom, Scott M., Parkinson, H. R., Popescu, C. C., Croom, S. M., Liske, J., S. Brough, Peacock, John A., Conselice, Christopher J., Wijesinghe, D. B., Loveday, Jon, Driver, Simon P, Phillipps, S., Taylor, E.N., E. N. Taylor, Sutherland, W.J., Parkinson, H., M. Gunawardhana, A. Merson, Croom, S., P. Norberg, J. Loveday, E. Cameron, K. A. Pimbblet, Bamford, Steven P., Cameron, Ewan, Hopkins, A.M., Popescu, C.C., Frenk, C. S., Driver, S., L. S. Kelvin, Robotham, Aaron S. G., Norberg, P., Brough, Sarah, Kelvin, L. S., Parkinson, H.R., Van Kampen, Eelco, Baldry, Ivan, Pimbblet, K., Pimbblet, K.A., Sharp, R.   +145 more
core   +1 more source

Star Formation Histories with Gaia: The Galaxy and Beyond

Open Astronomy, 2003
ESA’s Gaia mission will provide accurate astrometric, photometric and spectroscopic data for millions of stars in the Galaxy and beyond. We discuss the prospects of using this vast amount of astrophysical information for understanding star formation ...
Kučinskas A., Lindegren L., Tanabé T., Vansevičius Savanorių   +3 more
doaj   +1 more source

An HI-selected galaxy group at redshift z=0.45 [PDF]

, 2020
The cosmic star-formation history has now been mapped in detail over a wide range in redshift, but our knowledge about the amount and distribution of neutral hydrogen (HI) gas in galaxies beyond the local (z 2 x 10^20 cm-2.
Simon Weng
core   +1 more source

The Draco Dwarf Spheroidal Galaxy in the First Year of Dark Energy Spectroscopic Instrument Data

The Astrophysical Journal
We investigate the spatial distribution, kinematics, and metallicity of stars in the Draco dwarf spheroidal galaxy using data from the Dark Energy Spectroscopic Instrument (DESI).
J. Ding, C. Rockosi, Ting S. Li, S. E. Koposov, A. H. Riley, W. Wang, A. P. Cooper, N. Kizhuprakkat, M. Lambert, G. E. Medina, N. Sandford, J. Aguilar, S. Ahlen, D. Bianchi, D. Brooks, T. Claybaugh, A. de la Macorra, P. Doel, J. E. Forero-Romero, E. Gaztañaga, S. Gontcho A Gontcho, G. Gutierrez, J. Guy, M. Ishak, R. Kehoe, T. Kisner, A. Kremin, O. Lahav, M. Landriau, L. Le Guillou, A. Meisner, R. Miquel, J. Moustakas, F. Prada, I. Pérez-Ràfols, G. Rossi, E. Sanchez, M. Schubnell, J. Silber, D. Sprayberry, G. Tarlé, B. A. Weaver, R. Zhou   +42 more
doaj   +1 more source

Human Sustainability Leadership and Employee Wellbeing (Flourishing) in Organizations

Sustainable Development, EarlyView.
ABSTRACT This qualitative case study research examines how designing for human sustainability leadership (HSL) affects employee wellbeing (flourishing) (HWBF) in organizations. It is undertaken at a university in the United Kingdom including academics and administrators.
Elli Meleti
wiley   +1 more source

The Clustering of Dark Matter, Haloes & Galaxies [PDF]

, 2008
In this thesis I study the spatial distribution of galaxies, haloes and dark matter particlesin the Universe. The subjects investigated are conceptually divided into three areas.One line of research, which is made up of Chapters 2 and 3， is to explore ...
Raúl Esteban Angulo de la Puente,
core  

Connecting clustering and the cosmic web

Astronomy & Astrophysics
Context. Cosmological simulations predict significant secondary dependences of halo clustering on a variety of internal halo properties, and on environmental factors.
Rodriguez Facundo, Montero-Dorta Antonio D.   +1 more
doaj   +1 more source

Mechanically Durable Intrinsically Stretchable Neuromorphic Devices via Molecular Microstructure Design

Small, EarlyView.
This study reports intrinsically stretchable neuromorphic devices that exhibit outstanding mechanical stability while fully preserving their electrical characteristics over 105 repeated deformation cycles under 50% tensile strain. Such robustness is achieved through a rational molecular design strategy that systematically modulates the chain packing of
Kwan‐Nyeong Kim, Ho‐Eon Baek, Min‐Jun Choi, Min‐Jun Sung, Seung‐Woo Lee, Chae‐Yun Song, Hyun‐Haeng Lee, Sangjun Ma, Karina Ayu Larasati, Jeong‐Yun Sun, Hea‐Lim Park, Yun‐Hi Kim, Tae‐Woo Lee   +12 more
wiley   +1 more source

Dwarf spheroidals in the M81 galaxy group [PDF]

, 2010
The M81 group consists of a few large galaxies and about 40 dwarf galaxies. It is a highly interacting group which makes it an important nearby laboratory to study the role of the environment and interactions in the dwarf galaxy formation and evolution ...
Lianou, S., Koch, Andreas, Grebel, E. K.
core  

Investigating the impact of group environment on galaxy properties [PDF]

, 2017
The properties of galaxies, such as their shape and star formation rate (SFR), correlate strongly with the galaxy number density in the surrounding Universe. This is well known for cluster galaxies, which show a suppression of the star formation activity
Stefania Barsanti (16793734)
core   +1 more source