CERES: A Set of Automated Routines for Echelle Spectra

We present the Collection of Elemental Routines for Echelle Spectra (CERES). These routines were developed for the construction of automated pipelines for the reduction, extraction and analysis of spectra acquired with different instruments, allowing the obtention of homogeneous and standardised results. This modular code includes tools for handling the different steps of the processing: CCD image reductions, identification and tracing of the echelle orders, optimal and rectangular extraction, computation of the wavelength solution, estimation of radial velocities, and rough and fast estimation of the atmospheric parameters. Currently, CERES has been used to develop automated pipelines for thirteen different spectrographs, namely CORALIE, FEROS, HARPS, ESPaDOnS, FIES, PUCHEROS, FIDEOS, CAFE, DuPont/Echelle, Magellan/Mike, Keck/HIRES, Magellan/PFS and APO/ARCES, but the routines can be easily used in order to deal with data coming from other spectrographs. We show the high precision in radial velocity that CERES achieves for some of these instruments and we briefly summarize some results that have already been obtained using the CERES pipelines.

[1]  Rebecca A. Bernstein,et al.  MASE: A New Data-Reduction Pipeline for the Magellan Echellette Spectrograph , 2009, 0910.1834.

[2]  O. Toloza,et al.  The first pre-supersoft X-ray binary , 2015, 1503.07151.

[3]  Edward W. Dunham,et al.  Instrumentation for Astronomy with large optical telescopes: Astrophysics and Space Science Library; V. 92. Proceedings of IAU Colloquium No. 67. Edited by Colin M. Humphries. Reidel, Dordrecht/Boston/ London, 1982. 321 pp., $48.00 , 1983 .

[4]  Didier Queloz,et al.  Echelle Spectroscopy with a CCD at Low Signal-to-Noise Ratio , 1995 .

[5]  Constance M. Rockosi,et al.  ARCES: an echelle spectrograph for the Astrophysical Research Consortium (ARC) 3.5m telescope , 2003, SPIE Astronomical Telescopes + Instrumentation.

[6]  K. G. Helminiak,et al.  Orbital and physical parameters of eclipsing binaries from the All-Sky Automated Survey catalogue - VI. AK Fornacis: a rare, bright K-type eclipsing binary , 2014, 1405.2887.

[7]  Jean-Luis Lizon,et al.  Setting New Standards with HARPS , 2003 .

[8]  R. Brahm,et al.  Search for associations containing young stars (SACY). VII. New stellar and substellar candidate members in the young associations , 2016, 1604.03550.

[9]  S. Dreizler,et al.  CAFE: Calar Alto Fiber-fed Echelle spectrograph , 2013, 1301.2066.

[10]  Miguel de Val-Borro,et al.  HATS9-b AND HATS10-b: TWO COMPACT HOT JUPITERS IN FIELD 7 OF THE K2 MISSION , 2015, 1503.00062.

[11]  H. C. Stempels,et al.  FIES: The high-resolution Fiber-fed Echelle Spectrograph at the Nordic Optical Telescope , 2014 .

[12]  M. Mayor,et al.  A Jupiter-mass companion to a solar-type star , 1995, Nature.

[13]  K. Horne,et al.  AN OPTIMAL EXTRACTION ALGORITHM FOR CCD SPECTROSCOPY. , 1986 .

[14]  S. Baliunas,et al.  No Planet for Hd 166435 , 2022 .

[15]  Xavier Bonfils,et al.  Disentangling between stellar activity and planetary signals , 2010 .

[16]  Carlos Guirao,et al.  PUCHEROS: a cost-effective solution for high-resolution spectroscopy with small telescopes , 2012 .

[17]  K. G. Helminiak,et al.  Orbital and physical parameters of eclipsing binaries from the ASAS catalogue – VII. V1200 Centauri: a bright triple in the Hyades moving group , 2015, 1501.01033.

[18]  Nuno C. Santos,et al.  SOAP 2.0: A TOOL TO ESTIMATE THE PHOTOMETRIC AND RADIAL VELOCITY VARIATIONS INDUCED BY STELLAR SPOTS AND PLAGES , 2014, 1409.3594.

[19]  Stephen A. Shectman,et al.  MIKE: A Double Echelle Spectrograph for the Magellan Telescopes at Las Campanas Observatory , 2003, SPIE Astronomical Telescopes + Instrumentation.

[20]  J. Southworth,et al.  An optical transmission spectrum of the transiting hot Jupiter in the metal-poor WASP-98 planetary system , 2016, 1606.00432.

[21]  Michel Mayor,et al.  ELODIE: A spectrograph for accurate radial velocity measurements , 1996 .

[22]  Dan Lubin,et al.  Relative Flux Calibration of Keck HIRES Echelle Spectra , 2003 .

[23]  Suvrath Mahadevan,et al.  Development of Fiber Fabry-Perot Interferometers as Stable Near-infrared Calibration Sources for High Resolution Spectrographs , 2014, 1403.6841.

[24]  L. Pasquini,et al.  EARLY OPTICAL SPECTRA OF NOVA V1369 CEN SHOW THE PRESENCE OF LITHIUM , 2015, 1506.08048.

[25]  Michitoshi Yoshida,et al.  High Dispersion Spectrograph (HDS) for the Subaru Telescope , 2002 .

[26]  R. Griffin A Photoelectric Radial-Velocity Spectrometer , 1967 .

[27]  P. Rojo,et al.  Four new planets around giant stars and the mass-metallicity correlation of planet-hosting stars , 2016, 1603.03738.

[28]  T. Marsh THE EXTRACTION OF HIGHLY DISTORTED SPECTRA , 1989 .

[29]  Debra A. Fischer,et al.  NEWLY DISCOVERED PLANETS ORBITING HD 5319, HD 11506, HD 75784 AND HD 10442 FROM THE N2K CONSORTIUM , 2014, 1411.5374.

[30]  J. Southworth,et al.  Physical properties of the planetary systems WASP-45 and WASP-46 from simultaneous multiband photometry , 2015, 1511.05171.

[31]  C. Moutou,et al.  Transiting exoplanets from the CoRoT space mission XIII. CoRoT-13b: a dense hot Jupiter in transit around a star with solar metallicity and super-solar lithium content , 2010, 1007.5481.

[32]  R. Schiavon,et al.  A library of high resolution synthetic stellar spectra from 300 nm to 1.8 μm with solar and α-enhanced composition , 2005, astro-ph/0505511.

[33]  Preben Grosbol,et al.  MIDAS - ESO's new image processing system , 1983 .

[34]  Miguel de Val-Borro,et al.  HATS-17b: A TRANSITING COMPACT WARM JUPITER IN A 16.3 DAY CIRCULAR ORBIT , 2015, 1510.05758.

[35]  Miguel de Val-Borro,et al.  HATS-13b and HATS-14b: two transiting hot Jupiters from the HATSouth survey , 2015, 1503.03469.

[36]  Miguel de Val-Borro,et al.  HATS-4b: A DENSE HOT JUPITER TRANSITING A SUPER METAL-RICH G STAR , 2014, The Astronomical Journal.

[37]  A. Reiners,et al.  A laser-lock concept to reach cm s 1 -precision in Doppler experiments with Fabry-Pérot wavelength calibrators , 2014, 1408.6111.

[38]  Michel Mayor,et al.  Search for exoplanets with the radial-velocity technique : quantitative diagnostics of stellar activity , 2007, 0708.4338.

[39]  Andrew Szentgyorgyi,et al.  A laser frequency comb that enables radial velocity measurements with a precision of 1 cm s-1 , 2008, Nature.

[40]  John Asher Johnson,et al.  THE PAN-PACIFIC PLANET SEARCH. IV. TWO SUPER-JUPITERS IN A 3:5 RESONANCE ORBITING THE GIANT STAR HD 33844 , 2015, 1512.07316.