The distribution of dark matter in galaxies

P Salucci - The Astronomy and Astrophysics Review, 2019 - Springer
The distribution of the non-luminous matter in galaxies of different luminosity and Hubble
type is much more than a proof of the existence of dark particles governing the structures of …

Modeling the panchromatic spectral energy distributions of galaxies

C Conroy - Annual Review of Astronomy and Astrophysics, 2013 - annualreviews.org
The spectral energy distributions (SEDs) of galaxies are shaped by nearly every physical
property of the system, including the star-formation history, metal content, abundance …

The near-infrared spectrograph (nirspec) on the james webb space telescope-iii. integral-field spectroscopy

T Böker, S Arribas, N Lützgendorf… - Astronomy & …, 2022 - aanda.org
The near-infrared spectrograph (NIRSpec) on the James Webb Space Telescope (JWST)
offers the first opportunity to use integral-field spectroscopy from space at near-infrared …

The data processing pipeline for the MUSE instrument

PM Weilbacher, R Palsa, O Streicher, R Bacon… - Astronomy & …, 2020 - aanda.org
The processing of raw data from modern astronomical instruments is often carried out
nowadays using dedicated software, known as pipelines, largely run in automated …

Overview of the sdss-iv manga survey: mapping nearby galaxies at apache point observatory

K Bundy, MA Bershady, DR Law, R Yan… - The Astrophysical …, 2014 - iopscience.iop.org
We present an overview of a new integral field spectroscopic survey called MaNGA
(Mapping Nearby Galaxies at Apache Point Observatory), one of three core programs in the …

How to constrain your M dwarf: measuring effective temperature, bolometric luminosity, mass, and radius

AW Mann, GA Feiden, E Gaidos… - The Astrophysical …, 2015 - iopscience.iop.org
Precise and accurate parameters for late-type (late K and M) dwarf stars are important for
characterization of any orbiting planets, but such determinations have been hampered by …

The data reduction pipeline for the SDSS-IV MaNGA IFU galaxy survey

DR Law, B Cherinka, R Yan, BH Andrews… - The Astronomical …, 2016 - iopscience.iop.org
ABSTRACT Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) is an optical
fiber-bundle integral-field unit (IFU) spectroscopic survey that is one of three core programs …

Review of snapshot spectral imaging technologies

N Hagen, MW Kudenov - Optical Engineering, 2013 - spiedigitallibrary.org
Within the field of spectral imaging, the vast majority of instruments used are scanning
devices. Recently, several snapshot spectral imaging systems have become commercially …

BAT AGN spectroscopic survey. I. Spectral measurements, derived quantities, and AGN demographics

M Koss, B Trakhtenbrot, C Ricci, I Lamperti… - The Astrophysical …, 2017 - iopscience.iop.org
We present the first catalog and data release of the Swift-BAT AGN Spectroscopic Survey.
We analyze optical spectra of the majority of the detected AGNs (77%, 642/836) based on …

Structure and kinematics of early-type galaxies from integral field spectroscopy

M Cappellari - Annual review of astronomy and astrophysics, 2016 - annualreviews.org
Observations of galaxy isophotes, long-slit kinematics, and high-resolution photometry
suggested a possible dichotomy between two distinct classes of elliptical galaxies. But these …