Experimental Study of an Advanced Concept of Moderate-resolution Holographic Spectrographs
暂无分享,去创建一个
Eduard Muslimov | Nadezhda Pavlycheva | Gennady Valyavin | S. Fabrika | G. Valyavin | N. Pavlycheva | E. Muslimov | Sergei Fabrika | F. Musaev | Faig Musaev | Gazinur Galazutdinov | Eduard Emelyanov | G. Galazutdinov | E. Emelianov
[1] D. Bizyaev,et al. New luminous blue variables in the Andromeda galaxy , 2014, 1412.5319.
[2] L. Fossati,et al. On the incidence of weak magnetic fields in DA white dwarfs , 2012, 1208.3650.
[3] P. Massey,et al. The Wolf-Rayet Content of M31 , 2012, 1209.1177.
[5] R. Hunstead,et al. Optical spectroscopy of GX 339-4 during the high—soft and low—hard states — II. Line ionization and emission region , 1999, astro-ph/0008016.
[6] S. Fabrika,et al. Advanced modeling of a moderate-resolution holographic spectrograph. , 2017, Applied optics.
[7] Andrea Bianco,et al. Spectral multiplexing using stacked volume-phase holographic gratings – I , 2017 .
[8] Olivier Schnurr,et al. The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150 M⊙ stellar mass limit , 2010, 1007.3284.
[9] Eduard R. Muslimov,et al. Design and optimization of a dispersive unit based on cascaded volume phase holographic gratings , 2017, Optics + Optoelectronics.
[10] A. F. Valeev,et al. Search for and study of photometric variability in magnetic white dwarfs , 2017 .
[11] C. Baltay,et al. Atmospheric extinction properties above Mauna Kea from the Nearby SuperNova Factory spectro-photometric data set , 2012, 1210.2619.
[12] Maximilian Fabricius,et al. Prime Focus Spectrograph (PFS) for the Subaru telescope: overview, recent progress, and future perspectives , 2016, Astronomical Telescopes + Instrumentation.
[13] Kashiko Kodate,et al. Grisms Developed for FOCAS , 2011, 1105.0997.
[14] D. Walton,et al. The nova-like nebular optical spectrum of V404 Cygni at the beginning of the 2015 outburst decay , 2016, 1611.02278.
[15] G. G. Valyavin,et al. Magnetic survey of bright northern main sequence stars , 2002 .
[16] V. Afanasiev,et al. The SCORPIO focal reducer , 2005, astro-ph/0502095.
[17] Christian Knigge,et al. MEASURING THE ROTATIONAL PERIODS OF ISOLATED MAGNETIC WHITE DWARFS , 2013 .
[18] S. Fabrika,et al. Supercritical accretion disks in ultraluminous X-ray sources and SS 433 , 2015, Nature Physics.
[19] Jan Swevers,et al. Ground-based and airborne instrumentation for astronomy , 2010 .
[20] Andrea Bianco,et al. Photopolymers for holographic optical elements in astronomy , 2017, Optics + Optoelectronics.
[21] Robert H. Anderson,et al. The Goodman spectrograph , 2004, SPIE Astronomical Telescopes + Instrumentation.
[22] Xin Liu,et al. A comparison of spectroscopic methods for detecting the starlight scattered by transiting hot Jupiters, with an application to Subaru data for HD 209458b and HD 189733b , 2010, 1006.5492.
[23] H. G. Jerrard. Handbook of optical holography: Edited by H.J. Caulfield Academic Press, 1979, pp 637 + xiv, $55 , 1980 .
[24] H. Fahr,et al. GENERALIZED MULTI-POLYTROPIC RANKINE–HUGONIOT RELATIONS AND THE ENTROPY CONDITION , 2016, 1610.04381.
[25] T. Becker,et al. Crowded field 3D spectroscopy of LBV candidates in M 33 , 2005, astro-ph/0503586.
[26] M. Couture,et al. HIRES: the high-resolution echelle spectrometer on the Keck 10-m Telescope , 1994, Astronomical Telescopes and Instrumentation.
[27] S. Fabrika. The Supercritical Accretion Disk of SS 433 , 1997 .
[28] D. Shulyak,et al. Detection of regular low-amplitude photometric variability of the magnetic dwarf WD0009+501. on the possibility of photometric investigation of exoplanets on the basis of 1-meter class telescopes of the special and crimean astrophysical observatories , 2015 .
[29] Eduard R. Muslimov,et al. Design and modeling of a moderate-resolution astronomic spectrograph with volume-phase holographic gratings , 2016, Astronomical Telescopes + Instrumentation.
[30] S. Fabrika,et al. Spectral variability of LBV star V 532 (Romano’s star) , 2011 .
[31] Friedrich-Karl Bruder,et al. Reaction-diffusion model applied to high resolution Bayfol HX photopolymer , 2010, OPTO.
[32] C. Motch,et al. A 300-parsec-long jet-inflated bubble around a powerful microquasar in the galaxy NGC 7793 , 2010, Nature.
[33] N. Gehrels,et al. M31N 2008-12a—THE REMARKABLE RECURRENT NOVA IN M31: PANCHROMATIC OBSERVATIONS OF THE 2015 ERUPTION , 2016, 1607.08082.
[34] G. G. Valyavin,et al. Moderate-resolution holographic spectrograph , 2016 .
[35] Kris Davidson,et al. THE LUMINOUS BLUE VARIABLES: ASTROPHYSICAL GEYSERS , 1994 .
[36] S. Fabrika,et al. Possible variability of the magnetic field of T Tau , 2004 .
[37] J. Newell,et al. Optical holography in dichromated gelatin , 1987 .
[38] G. A. Wade,et al. A search for kilogauss magnetic fields in white dwarfs and hot subdwarf stars , 2006 .
[39] Peter G. Nelson,et al. The Visible Spectro-Polarimeter (ViSP) for the Advanced Technology Solar Telescope , 2010, Astronomical Telescopes + Instrumentation.
[40] V. Afanasiev,et al. The SCORPIO universal focal reducer of the 6-m telescope , 2005 .
[41] S. Fabrika,et al. A search for unique objects in nearby galaxies , 1995 .
[42] A. F. Valeev,et al. Spectroscopic observations of the exoplanet WASP-32b transit , 2017 .
[43] R. Manuputy,et al. X-shooter, the new wide band intermediate resolution spectrograph at the ESO Very Large Telescope , 2011, 1110.1944.
[44] S. Fabrika,et al. Fast line-profile variability in the spectra of O stars , 2003 .
[45] H. Falcke,et al. Towards a dynamical mass of the ultraluminous X-ray source NGC 5408 X-1 , 2013, 1308.1251.