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1. Full Text Inferring the dark matter power spectrum from the Lyman α forest in high‐resolution QSO absorption spectra
by Viel, Matteo and Haehnelt, Martin G and Springel, Volker
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 11/2004, Volume 354, Issue 3, pp. 684 - 694
ABSTRACT We use the LUQAS sample, a set of 27 high‐resolution and high signal‐to‐noise ratio quasi‐stellar object (QSO) absorption spectra at a median redshift... 
quasars: absorption lines | intergalactic medium | large‐scale structure of Universe | Intergalactic medium | Quasars: absorption lines | Large-scale structure of Universe | GALACTIC WINDS | LARGE-SCALE STRUCTURE | large-scale structure of Universe | PROBE WMAP OBSERVATIONS | MASS FLUCTUATIONS | COSMOLOGICAL SIMULATIONS | LARGE-SAMPLE | ASTRONOMY & ASTROPHYSICS | UNIVERSE | EQUATION | quasars : absorption lines | PARTICLE HYDRODYNAMICS SIMULATIONS | Physics - Cosmology and Nongalactic Astrophysics | Physics - Earth and Planetary Astrophysics | Physics - Instrumentation and Methods for Astrophysics | Physics - High Energy Astrophysical Phenomena | Physics - Solar and Stellar Astrophysics | Physics - Astrophysics of Galaxies
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2. Full Text Signatures of the non-Maxwellian kappa-distributions in optically thin line spectra II. Synthetic Fe XVII-XVIII X-ray coronal spectra and predictions for the Marshall Grazing-Incidence X-ray Spectrometer (MaGIXS)
by Dudik, J and Dzifcakova, E and Del Zanna, G and Mason, HE and Golub, LL and Winebarger, AR and Savage, SL
ASTRONOMY & ASTROPHYSICS, ISSN 1432-0746, 06/2019, Volume 626, p. A88
Aims. We investigated the possibility of diagnosing the degree of departure from the Maxwellian distribution using the Fe XVII-Fe XVIII spectra originating in... 
radiation mechanisms: non-thermal | gamma rays | TELESCOPE | Sun: corona | CHIANTI | EMISSION-LINES | Sun: UV radiation | Sun: X-rays | ELEMENTS HYDROGEN | HOT PLASMA | SPECTROSCOPY | ATOMIC DATABASE | QUIET-SUN | ASTRONOMY & ASTROPHYSICS | SOLAR-WIND | ELECTRON DISTRIBUTIONS
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3. Full Text Mid-infrared atomic fine-structure emission-line spectra of luminous infrared galaxies: Spitzer/IRS spectra of the goals sample
by Inami, H and Armus, L and Charmandaris, V and Groves, B and Kewley, L and Petric, A and Stierwalt, S and Díaz-Santos, T and Surace, J and Rich, J and Haan, S and Howell, J and Evans, A.S and Mazzarella, J and Marshall, J and Appleton, P and Lord, S and Spoon, H and Frayer, D and Matsuhara, H and Veilleux, S
Astrophysical Journal, ISSN 0004-637X, 11/2013, Volume 777, Issue 2, pp. 156 - 16
We present the data and our analysis of mid-infrared atomic fine-structure emission lines detected in Spitzer/Infrared Spectrograph high-resolution spectra of... 
galaxies: starburst | galaxies: ISM | infrared: galaxies | NEARBY GALAXIES | OXYGEN ABUNDANCES | STAR-FORMING GALAXIES | HUBBLE-SPACE-TELESCOPE | HIGH-RESOLUTION SPECTROSCOPY | STARBURST GALAXIES | ACTIVE GALACTIC NUCLEI | SUPERNOVA-REMNANTS | ASTRONOMY & ASTROPHYSICS | STELLAR POPULATIONS | SKY LIRG SURVEY | Spectral emissivity | Neon | Infrared | Galaxies | Emission analysis | Emission | Mathematical models | Fluxes | Physics - Cosmology and Nongalactic Astrophysics | SULFUR IONS | NEON IONS | FINE STRUCTURE | RESOLUTION | CORRELATIONS | COMPARATIVE EVALUATIONS | IRON IONS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | ASTRONOMY | ASTROPHYSICS | OXYGEN IONS | EMISSION SPECTRA | ELECTRON DENSITY | STARS | LINE WIDTHS | GALAXIES | POLYCYCLIC AROMATIC HYDROCARBONS | GALAXY NUCLEI
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4. Full Text The metal content of bulge field stars from FLAMES-GIRAFFE spectra: I. Stellar parameters and iron abundances
by Zoccali, M and Hill, V and Lecureur, A and Barbuy, B and Renzini, A and Minniti, D and Gómez, A and Ortolani, S
Astronomy and Astrophysics, ISSN 0004-6361, 2008, Volume 486, Issue 1, pp. 177 - 189
Aims. We determine the iron distribution function (IDF) for bulge field stars, in three different fields along the Galactic minor axis and at latitudes b = -4... 
Stars: atmospheres | Stars: abundances | Galaxy: bulge | stars : atmospheres | BAADES WINDOW GIANTS | KECK HIRES SPECTRA | MICROLENSING OPTICAL DEPTH | galaxy : bulge | 1ST DETAILED ABUNDANCES | GRAVITATIONAL LENSING EXPERIMENT | INFRARED-SPECTROSCOPY | GALACTIC BULGE | GLOBULAR-CLUSTER | ASTRONOMY & ASTROPHYSICS | MILKY-WAY | EFFECTIVE TEMPERATURE SCALE | stars : abundances | Physics - Cosmology and Nongalactic Astrophysics | Physics - Earth and Planetary Astrophysics | Physics - Instrumentation and Methods for Astrophysics | Physics - High Energy Astrophysical Phenomena | Physics - Solar and Stellar Astrophysics | Physics - Astrophysics of Galaxies
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5. Full Text Hubble Space Telescope spectra of the Type Ia supernova SN 2011fe: A tail of low-density, high-velocity material with Z ≤ Z
by Mazzali, P.A and Mazzali, P.A and Sullivan, M and Hachinger, S and Ellis, R.S and Nugent, P.E and Nugent, P.E and Howell, D.A and Gal-Yam, A and Gal-Yam, A and Maguire, K and Cooke, J and Thomas, R and Nomoto, K and Nomoto, K and Walker, E.S
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2014, Volume 439, Issue 2, pp. 1959 - 1979
Hubble Space Telescope spectroscopic observations of the nearby Type Ia supernova (SN Ia) SN 2011fe, taken on 10 epochs from -13.1 to +40.8 d relative to... 
Supernovae: general | Radiative transfer | Techniques: spectroscopic | Supernovae: individual: SN 2011fe | radiative transfer | supernovae: individual: SN 2011fe | WHITE-DWARFS | LIGHT CURVES | ULTRAVIOLET-SPECTRA | supernovae: general | NEBULAR SPECTRA | LUMINOSITY INDICATORS | LOW-REDSHIFT | DARK-ENERGY | techniques: spectroscopic | ASTRONOMY & ASTROPHYSICS | ABUNDANCE STRATIFICATION | LEGACY SURVEY | CHANDRASEKHAR-MASS MODELS
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6. Full Text CRIRES-POP: A library of high resolution spectra in the near-infrared: II. Data reduction and the spectrum of the K giant 10 Leonis
by Nicholls, C.P and Lebzelter, T and Smette, A and Wolff, B and Hartman, H and Kaüfl, H.-U and Przybilla, N and Ramsay, S and Uttenthaler, S and Wahlgren, G.M and Bagnulo, S and Hussain, G.A.J and Nieva, M.-F and Seemann, U and Seifahrt, A and Lund Observatory and Astronomi and Lund University and Lunds universitet
Astronomy and Astrophysics, ISSN 0004-6361, 02/2017, Volume 598, p. A79
Context. High resolution stellar spectral atlases are valuable resources to astronomy. They are rare in the 1-5 mu m region for historical reasons, but once... 
Stars: late-type | Atmospheric effects | Infrared: stars | Stars: atmospheres | Techniques: spectroscopic | Atlases | stars: atmospheres | infrared: stars | COOL STARS | BAND | M DWARFS | stars: late-type | atmospheric effects | STELLAR SPECTRA | techniques: spectroscopic | PHOTOMETRY | ASTRONOMY & ASTROPHYSICS | atlases | FUNDAMENTAL PARAMETERS | Fysik | Astronomi, astrofysik och kosmologi | Physical Sciences | Naturvetenskap | Natural Sciences | Astronomy, Astrophysics and Cosmology
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7. Stars and their spectra
: an introduction to the spectral sequence
by Kaler, James B
2011, 2nd ed., ISBN 0521899540, xviii, 394
"Stellar spectroscopy is the fundamental tool for investigating the natures of stars and is central to our understanding of modern astronomy and astrophysics.... 
Stars | Spectra
Book
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8. Stars and their spectra
: an introduction to the spectral sequence
by Kaler, James B
1989, ISBN 0521304946, xvi, 300
Stars | Spectra
Book
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9. Full Text PEPSI deep spectra: I. the Sun-as-a-star
by Strassmeier, K.G and Ilyin, I and Steffen, M
Astronomy and Astrophysics, ISSN 0004-6361, 04/2018, Volume 612, p. A44
Context. Full-disk solar flux spectra can be directly compared to stellar spectra and thereby serve as our most important reference source for, for example... 
Methods: observational | Sun: photosphere | Sun: abundances | Techniques: spectroscopic | Atlases | PLANETS | SYSTEM | CALIBRATION | methods: observational | LAMBDA 6707.8A | HARPS | techniques: spectroscopic | ASTRONOMY & ASTROPHYSICS | atlases | CHEMICAL-COMPOSITION | LI-7/LI-6 RATIO | SPECTROGRAPH | SOLAR LITHIUM ABUNDANCE
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10. Full Text Strong nebular line ratios in the spectra of z ∼ 2-3 star forming galaxies: First results from KBSS-mosfire
by Steidel, Charles C and Rudie, Gwen C and Strom, Allison L and Pettini, Max and Reddy, Naveen A and Shapley, Alice E and Trainor, Ryan F and Erb, Dawn K and Turner, Monica L and Konidaris, Nicholas P and Kulas, Kristin R and Mace, Gregory and Matthews, Keith and McLean, Ian S
Astrophysical Journal, ISSN 0004-637X, 11/2014, Volume 795, Issue 2, pp. 1 - 40
We present initial results of a deep near-IR spectroscopic survey covering the 15 fields of the Keck Baryonic Structure Survey using the recently commissioned... 
galaxies: formation | galaxies: starburst | galaxies: evolution | galaxies: fundamental parameters | cosmology: observations | instrumentation: spectrographs | galaxies: abundances | galaxies: high-redshift | Star formation | Galaxies | Metallicity | Asymptotic properties | Ionization | Spectrometers | Astronomical models | Estimating | TELESCOPES | RED SHIFT | EXCITATION | ELEMENT ABUNDANCE | METALLICITY | OXYGEN | NEAR INFRARED RADIATION | PHOTOIONIZATION | COSMOLOGY | EVOLUTION | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | SPECTROMETERS | MASS | STARS | MILKY WAY | EMISSION | SPECTRA
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11. Full Text The nature and evolution of the highly ionized near-zones in the absorption spectra of z≃ 6 quasars
by Bolton, James S and Haehnelt, Martin G
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2007, Volume 374, Issue 2, pp. 493 - 514
We use state-of-the-art hydrodynamical simulations combined with a one-dimensional radiative transfer code to assess the extent to which the highly ionized... 
intergalactic medium | methods: numerical | H ii regions | quasars: absorption lines | radiative transfer | cosmology: theory | Radiative transfer | Cosmology: theory | H II regions | Intergalactic medium | Quasars: absorption lines | Methods: numerical | Quasars | Red shift | Adsorption | Spectrum analysis | Physics - Cosmology and Nongalactic Astrophysics | Physics - Earth and Planetary Astrophysics | Physics - Instrumentation and Methods for Astrophysics | Physics - High Energy Astrophysical Phenomena | Physics - Solar and Stellar Astrophysics | Physics - Astrophysics of Galaxies
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12. Interpreting astronomical spectra
by Emerson, David
1996, ISBN 047194176X, vii, 461
Astronomical spectroscopy
Book
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13. Full Text Spectral calibration of K-M giants from medium-resolution near-infrared HK-band spectra
by Ghosh, S and Mondal, S and Das, R and Khata, D
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 04/2019, Volume 484, Issue 4, pp. 4619 - 4634
We present here new medium resolution spectra (lambda/Delta lambda similar to 1200) of K-M giants covering wavelength ranges 1.50-1.80 and 1.95-2.45 mu m. The... 
methods: observational | infrared: stars | CLASSIFICATION | COOL STARS | METALLICITY | EFFECTIVE TEMPERATURES | SUPERGIANTS | NEWTON-TELESCOPE LIBRARY | STELLAR SPECTRA | techniques: spectroscopic | ASTRONOMY & ASTROPHYSICS | stars: fundamental parameters | RADIAL-VELOCITIES | FUNDAMENTAL PARAMETERS | SPECTROSCOPIC SURVEY
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14. Full Text Non-LTE models for synthetic spectra of Type Ia supernovae: IV. A modified Feautrier scheme for opacity-sampled pseudo-continua at high expansion velocities and application to synthetic SN Ia spectra
by Hoffmann, T.L and Sauer, D.N and Pauldrach, A.W.A and Hultzsch, P.J.N
Astronomy and Astrophysics, ISSN 0004-6361, 09/2014, Volume 569, p. A62
Context. Type Ia supernovae (SN Ia) have become an invaluable cosmological tool because their exceptional brightness makes them observable even at very large... 
Supernovae: general | Radiative transfer | Supernovae: individual: SN 1992A | MASSIVE STARS | BOUNDARY-CONDITIONS | radiative transfer | EXPANDING ATMOSPHERES | supernovae: general | CURVES | MAXIMUM LIGHT | HOT LUMINOUS STARS | EVOLUTION | RADIATION-DRIVEN WINDS | supernovae: individual: SN 1992A | ASTRONOMY & ASTROPHYSICS | IONIZED-GAS | LINE BLOCKING | Physics - Solar and Stellar Astrophysics
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15. Full Text THE MUSCLES TREASURY SURVEY. II. INTRINSIC LYα and EXTREME ULTRAVIOLET SPECTRA of K and M DWARFS with EXOPLANETS
by Youngblood, Allison and France, Kevin and Loyd, R. O. Parke and Linsky, Jeffrey L and Redfield, Seth and Schneider, P. Christian and Wood, Brian E and Brown, Alexander and Froning, Cynthia and Miguel, Yamila and Rugheimer, Sarah and Walkowicz, Lucianne
Astrophysical Journal, ISSN 0004-637X, 06/2016, Volume 824, Issue 2, p. 101
The ultraviolet (UV) spectral energy distributions (SEDs) of low-mass (K- and M-type) stars play a critical role in the heating and chemistry of exoplanet... 
ISM: clouds | stars: low-mass | POTENTIALLY HABITABLE PLANETS | LOW-MASS STARS | LYMAN-ALPHA | EMISSION-LINES | COOL STARS | UV-RADIATION | ATOMIC DATABASE | ASTRONOMY & ASTROPHYSICS | X-RAY | LOCAL INTERSTELLAR-MEDIUM | MAGNETIC-STRUCTURE | ROTATION | TELESCOPES | MARKOV PROCESS | MONTE CARLO METHOD | PHOTONS | HEATING | ENERGY SPECTRA | CORRELATIONS | EXTREME ULTRAVIOLET RADIATION | ATMOSPHERES | LYMAN LINES | EXTREME ULTRAVIOLET SPECTRA | COMPUTERIZED SIMULATION | DENSITY | SPACE | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | MASS | STARS | ABSORPTION | DWARF STARS | SURFACES
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16. Full Text The Indo-US Library of Coudé Feed Stellar Spectra
by Valdes, Francisco and Gupta, Ranjan and Rose, James A and Singh, Harinder P and