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相关论文: MEGARA-GTC Stellar Spectral Library (I)

200 篇论文

The Galactic Archaeology with HERMES (GALAH) Survey is a massive observational project to trace the Milky Way's history of star formation, chemical enrichment, stellar migration and minor mergers. Using high-resolution (R$\simeq$28,000)…

We present a multi-band photometric catalog of $\approx$ 1.7 million cluster members for a field of view of $\approx$ 2x2 degree across $\omega$ Cen. Photometry is based on images collected with the Dark Energy Camera on the 4m Blanco…

星系天体物理 · 物理学 2017-04-05 A. Calamida , G. Strampelli , A. Rest , G. Bono , I. Ferraro , A. Saha , G. Iannicola , D. Scolnic , D. James , C. Smith , A. Zenteno

Both the quality and amount of astrophysical data are steadily increasing over time owing to the improvement of telescopes and their instruments. This requires corresponding evolution of the techniques used for obtaining and analyzing the…

太阳与恒星天体物理 · 物理学 2021-04-14 J. C. Trelles Arjona , B. Ruiz Cobo , M. J. Martínez González

We present systematic spectral analyses of GRBs detected by the Fermi Gamma-Ray Burst Monitor (GBM) during its first two years of operation. This catalog contains two types of spectra extracted from 487 GRBs, and by fitting four different…

We present a catalog of Galactic star clusters, associations and candidates with 10978 entries. This multi-band catalog was constructed over 20 years, starting with visual inspections on the Digital Sky Survey and incremented with the…

星系天体物理 · 物理学 2019-01-02 Eduardo Bica , Daniela B. Pavani , Charles J. Bonatto , Eliade F. Lima

[ABRIDGED] $\omega$ Centauri (NGC 5139) contains large numbers of variable stars of different types and, in particular, more than a hundred RR Lyrae stars. We have conducted a variability survey of $\omega$ Cen in the NIR, using ESO's 4.1m…

太阳与恒星天体物理 · 物理学 2015-05-13 C. Navarrete , R. Contreras Ramos , M. Catelan , C. M. Clement , F. Gran , J. Alonso-García , R. Angeloni , M. Hempel , I. Dékány , D. Minniti

We present the main-sequence binary (MSMS) Catalog derived from Gaia Data Release 3 BP/RP (XP) spectra. Leveraging the vast sample of low-resolution Gaia XP spectra, we develop a forward modeling approach that maps stellar mass and…

Globular clusters produce many exotic stars due to a much higher frequency of dynamical interactions in their dense stellar environments. Some of these objects were observed together with several hundred thousands other stars in our MUSE…

The occurrence of multiple stars, dominantly binaries, is studied using the \textit{Gaia}-ESA DR2 catalogue. We apply the optimized statistical method that we previously developed for the analysis of 2D patterns. The field of stars is…

星系天体物理 · 物理学 2022-01-05 Petr Zavada , Karel Píška

In the era of vast spectroscopic surveys focusing on Galactic stellar populations, astronomers want to exploit the large quantity and good quality of data to derive their atmospheric parameters without losing precision from automatic…

太阳与恒星天体物理 · 物理学 2017-12-13 M. Tsantaki , D. T. Andreasen , G. D. C. Teixeira , S. G. Sousa , N. C. Santos , E. Delgado-Mena , G. Bruzual

We report an independent spectral classification of a sample of poorly studied M-dwarf candidate stars observed with the OSIRIS instrument at GTC. Our project was carried out as an independent test of the spectral classification. It is…

太阳与恒星天体物理 · 物理学 2019-12-24 Cristina Cabello , Géza Csörnyei , Jaroslav Merc , Verónica Ferreirós Lopez , Peter Pessev

This work makes available a further 2,860deg$^2$ of the GLEAM survey, covering half of the accessible Galactic Plane, across twenty frequency bands sampling $72-231$MHz, with resolution $4'-2'$. Unlike previous GLEAM data releases, we used…

A standard library of theoretical stellar spectra intended for multiple synthetic photometry applications including spectral evolutionary synthesis is presented. The grid includes M dwarf model spectra, hence complementing the first library…

天体物理学 · 物理学 2009-07-28 T. Lejeune , F. Cuisinier , R. Buser

We present ALMA observations at 233, 678, and 870 GHz of the Galactic Center black hole, Sagittarius A*. These observations reveal a flat spectrum over this frequency range with spectral index $\alpha \approx -0.3$, where the flux density…

We present a library of Utrecht echelle spectrograph (UES) observations of a sample of F, G, K and M field dwarf stars covering the spectral range from 4800 AA to 10600 AA with a resolution of 55000. These spectra include some of the…

天体物理学 · 物理学 2016-08-15 D. Montes , E. L. Martin

We present a new library of semi-empirical stellar spectra that is based on the empirical MILES library. A new, high resolution library of theoretical stellar spectra is generated that is specifically designed for use in stellar population…

太阳与恒星天体物理 · 物理学 2021-04-15 Adam T. Knowles , Anne E. Sansom , Carlos Allende Prieto , Alex Vazdekis

This paper reports on the application of the supervised machine-learning algorithm to the stellar effective temperature regression for the second $Gaia$ data release, based on the combination of the stars in four spectroscopic surveys:…

太阳与恒星天体物理 · 物理学 2019-08-14 Yu Bai , JiFeng Liu , ZhongRui Bai , Song Wang , DongWei Fan

Globular clusters (GCs) play an important role in the formation and evolution of the Milky Way. New candidates are continuously found, particularly in the high-extinction low-latitude regions of the bulge, although their existence and…

星系天体物理 · 物理学 2022-10-12 Dongwook Lim , Andreas J. Koch-Hansen , Sang-Hyun Chun , Seungsoo Hong , Young-Wook Lee

Spectral indices are useful tools for quantifying the strengths of features in moderate-resolution spectra and relating them to intrinsic stellar parameters. This paper focuses on the 4300AA CH G-band, a classic example of a feature…

天体物理学 · 物理学 2009-11-13 Sarah L. Martell , Graeme H. Smith , Michael M. Briley

Globular clusters with their large populations of millisecond pulsars (MSPs) are believed to be potential emitters of high-energy gamma-ray emission. Our goal is to constrain the millisecond pulsar populations in globular clusters from…

星系天体物理 · 物理学 2015-05-18 The Fermi LAT collaboration