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FIELD: Automated emission line detection software for Subaru/FMOS near-infrared spectroscopy

Publications of the Astronomical Society of Japan Oxford University Press (OUP) 67:3 (2015) 31

Authors:

Motonari Tonegawa, Tomonori Totani, Fumihide Iwamuro, Masayuki Akiyama, Gavin Dalton, Karl Glazebrook, Kouji Ohta, Hiroyuki Okada, Kiyoto Yabe
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A multiwavelength exploration of the [C ii]/IR ratio in H-ATLAS/GAMA galaxies out to z = 0.2

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 449:3 (2015) 2498-2513

Authors:

E Ibar, MA Lara-López, R Herrera-Camus, R Hopwood, A Bauer, RJ Ivison, MJ Michałowski, H Dannerbauer, P van der Werf, D Riechers, N Bourne, M Baes, I Valtchanov, L Dunne, A Verma, S Brough, A Cooray, G De Zotti, S Dye, S Eales, C Furlanetto, S Maddox, M Smith, O Steele, D Thomas, E Valiante
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The Subaru-XMM-Newton Deep Survey (SXDS) VIII.: Multi-wavelength Identification, Optical/NIR Spectroscopic Properties, and Photometric Redshifts of X-ray Sources

(2015)

Authors:

Masayuki Akiyama, Yoshihiro Ueda, Mike G Watson, Hisanori Furusawa, Tadafumi Takata, Chris Simpson, Tomoki Morokuma, Toru Yamada, Kouji Ohta, Fumihide Iwamuro, Kiyoto Yabe, Naoyuki Tamura, Yuuki Moritani, Naruhisa Takato, Masahiko Kimura, Toshinori Maihara, Gavin Dalton, Ian Lewis, Hanshin Lee, Emma Curtis Lake, Edward Macaulay, Frazer Clarke, John D Silverman, Scott Croom, Masami Ouchi, Hitoshi Hanami, J Diaz Tello, Tomohiro Yoshikawa, Naofumi Fujishiro, Kazuhiro Sekiguchi
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Characterizing gravitational instability in turbulent multicomponent galactic discs

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 449:2 (2015) 2156-2166

Authors:

Oscar Agertz, Alessandro B Romeo, Kearn Grisdale
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General spherical anisotropic Jeans models of stellar kinematics: including proper motions and radial velocities

(2015)

Abstract:

Cappellari (2008) presented a flexible and efficient method to model the stellar kinematics of anisotropic axisymmetric and spherical stellar systems. The spherical formalism could be used to model the line-of-sight velocity second moments allowing for essentially arbitrary radial variations in the anisotropy and general luminous and total density profiles. Here we generalize the spherical formalism by providing the expressions for all three components of the projected second moments, including the two proper motion components. A reference implementation is now included in the public JAM package available at http://purl.org/cappellari/software.
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