Experimental Study of an Advanced Concept of Moderate-resolution Holographic Spectrographs

We present the results of an experimental study of an advanced moderate-resolution spectrograph based on a cascade of narrow-band holographic gratings. The main goal of the project is to achieve a moderately high spectral resolutionwith R up to 5000 simultaneously in the 4300-6800 A visible spectral range on a single standard CCD, together with an increased throughput. The experimental study consisted of (1) resolution and image quality tests performed using the solar spectrum; and (2) a total throughput test performed for a number of wavelengths using a calibrated lab monochromator. The measured spectral resolving power reaches values over R>4000 while the experimental throughput is as high as 55%, which is in good agreement with the modeling results. Comparing the obtained characteristics of the spectrograph under consideration with the best existing spectrographs, we conclude that the used concept can be considered a very competitive and cheap alternative to the existing spectrographs of the given class. We propose several astrophysical applications for the instrument and discuss the prospect of creating its full-scale version.

[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.