In this section, the obtained RC sample is cross-matched with other RC star catalogues available in the literature to verify the completeness and distance determination. 4.1. Sample completeness layout = spotlight. layouts. debug_classification( label = 'gender', prediction = 'm1_gender_prediction', embedding = 'm1_embedding', features =[ 'age', 'emotion']) APOGEE and Gaia distances can only be used to compare nearby distances (< 3–5 kpc). On the other hand, The L20 catalogue provides the distances of 2.4 million stars with ∼75 000 stars at distances > 10 kpc by correcting for the extinction in the W1 WISE band. A comparison of the L20 distances with ours (bottom right panel of Fig. 4) shows that the vast majority of the stars are on a one-to-one correlation. The distance to the fainter stars seems to be overestimated in the L20 catalogue, which may result from an uncertain extinction in the W1 band. 5. Results To change the game's resolution, open your "SFC.INI" file and edit the entries below to one of the values above. The 1992-built (as "Royal Viking Queen") and acquired in 2015 from Seabourn (as "Seabourn Legend"), the Star Legend cruise ship is the third and last of all three identical superyachts in the Windstar fleet - together with Star Pride (Seabourn Pride) and Star Breeze (Seabourn Spirit).

Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, Laboratoire Lagrange, Bd de l’Observatoire, CS 34229, 06304 Nice Cedex 4, France APOGEE has another value-added catalogue named ‘StarHorse’. It is dedicated to finding the distance, extinction, and astrophysical parameters of the stars by combining the high-resolution spectroscopic data from APOGEE with broadband photometric data (Pan-STARRS, 2MASS, and ALLWISE) and parallax ( Gaia EDR3) using Bayesian statistics ( Santiago et al. 2016; Queiroz et al. 2020). The StarHorse DR17 catalogues list 562 424 (RC as well as non-RC) APOGEE sources with distance uncertainties of ∼5%. The region 39.5°< ℓ≤320° and −10°≤ b≤10° contains 111 438 StarHorse stars. A cross-match of these stars with our catalogue in a 1″ sky region results in 45 580 stars in common. The distance comparison of the cross-matched stars obtained from our method ( x-axis) with the StarHorse median distance is shown in the bottom left panel of Fig. 4. Most of the stars lie close to the 1:1 line, with some scattering of the outliers. Methods. We developed a method for systematically extracting the RC stars from a 2MASS ( J− K s, J) colour-magnitude diagram of 1°×1° bins in ℓ× b, covering the range 40°≤ ℓ≤320° and −10°≤ b≤10°. 2MASS data continue to be important because we are able to identify and trace the RC stars to much farther distances than in any optical survey of the Galactic disc. The foreground star contamination in the selected sample was removed using the accurate astrometric data from Gaia EDR3. We analysed the spiral arms and asymmetry in the Galaxy above and below the Galactic plane in galactocentric coordinates.import datasets from renumics import spotlight ds = datasets. load_dataset( 'renumics/emodb-enriched', split = 'all') Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system). In this section, we present the distribution of selected RC stars in the Galactic disc with the aim to find an over-density in the spiral arms and to explore the asymmetry above and below the Galactic plane. 5.1. Distribution in the Galactic plane Yusifov, I. 2004, in The Magnetized Interstellar Medium, eds. B. Uyaniker, W. Reich, & R. Wielebinski, 165

Windstar's "Star Plus" project increased the fleet's capacity by 24%. The project (completed in 2021 October) resulted in bigger capacity (254 to 320 passengers, 140 to 190 crew), increased GT tonnage/volume (9975 to 12995 tons), increased length (134 to 159 m), more staterooms (106 to 156), adding new venues and public spaces, machinery upgrades (new Wartsila marine diesel engines). The project was scheduled for the period October 2019 through November 2020, at Fincantieri's shipyards in Palermo (Sicily Island, Italy) and Trieste (Italy). The details are spread around this forum under topics associated with hex editing, the sfc launcher, q3_editor and other tools.In addition to the spiral features, the asymmetry in the disc structure due to the warping of the disc is also observed in various tracers (e.g., Kerr 1957; Henderson 1979; Drimmel & Spergel 2001; Nakanishi & Sofue 2003; López-Corredoira et al. 2002; Yusifov 2004; Marshall et al. 2006; Levine et al. 2006; Poggio et al. 2018; Chen et al. 2019; Chrobáková et al. 2022). However, the asymmetries in the spiral arms due to disc warping have not been studied so far. We also used data from the Gaia space-based telescope. Gaia early data release 3 (EDR3), ( Gaia Collaboration 2021) includes data for the first 34 months of its operational phase. Gaia EDR3 contains information about 1.8 billion sources ranging from 3 to 21 G-band magnitude. This data release contains the full astrometric data ( Lindegren et al. 2021) of 1.4 billion sources. We make use of the distance information of Gaia EDR3 stars ( Bailer-Jones et al. 2021), and astrophysical parameters from Gaia data release 3 (DR3), ( Andrae et al. 2023) to remove contamination by foreground and evolved stars. 3. RC sample selection Here, m J and m K s represent the apparent magnitude in J and K s bands. We assumed a Dirac delta luminosity function for K giant stars with an absolute magnitude M J and M K s of −0.945±0.01 and −1.606±0.009 ( Ruiz-Dern et al. 2018). The effect of metallicity on the absolute magnitude and intrinsic colours of RC stars observed in the SDSS Apache Point Observatory Galactic Evolution Experiment (APOGEE) and the GALactic Archaeology with HERMES (GALAH) was calculated in Plevne et al. (2020) by using the Bayesian-based distance from Bailer-Jones et al. (2018). The median colours of RC stars in the NIR bands J− K s=0.62±0.05 mag are the same for low- and high-metallicity RC stars. However, the median value of absolute magnitude in the J band shows a slight difference, M J=−1.05±0.21 for low- α RC stars, and M J=0.89±0.27 mag for high- α sources. The distance derived using these values of absolute magnitude and colours for the low and high metallicity in APOGEE RC sample ( Bovy et al. 2014) shows an offset of only ∼200 pc. Hence, it is safe to assume solar neighbourhood values of absolute magnitude and intrinsic colour in the NIR bands to calculate the distance.

Machine learning and engineering teams use Spotlight to understand and communicate on complex unstructured data problems. Here are some examples on publicly available datasets along with code snippets (👨‍💻), interactive demos (🕹️) and blog articles (📝): Modality While NASA did not directly say how this imagery will assist Webb, of note is the newer telescope's efforts to understand how galaxies were formed and evolved, particularly in the early universe. AmphorA Restaurant (ship's dining room, open-seating; offers 5-course gourmet dinner menu which is changed daily; along with onboard-made bread, in all ports of call the executive chef goes to the local markets to shop for fresh ingredients)

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