/*
*  Copyright (C) 2007 Thomas Essinger-Hileman, Jolien Creighton, Ian Jones, Benjamin Owen, Reinhard Prix, Karl Wette
*
*  This program is free software; you can redistribute it and/or modify
*  it under the terms of the GNU General Public License as published by
*  the Free Software Foundation; either version 2 of the License, or
*  (at your option) any later version.
*
*  This program is distributed in the hope that it will be useful,
*  but WITHOUT ANY WARRANTY; without even the implied warranty of
*  MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE.  See the
*  GNU General Public License for more details.
*
*  You should have received a copy of the GNU General Public License
*  along with with program; see the file COPYING. If not, write to the
*  Free Software Foundation, Inc., 59 Temple Place, Suite 330, Boston,
*  MA  02111-1307  USA
*/

#ifndef _PTOLEMETRIC_H
#define _PTOLEMETRIC_H

#ifdef  __cplusplus
extern "C" {
#endif

#include <gsl/gsl_matrix.h>
#include <lal/DetectorSite.h>
#include <lal/LALConstants.h>
#include <lal/LALStdlib.h>
#include <lal/SkyCoordinates.h>
#include <lal/LALBarycenter.h>

/**
 * \defgroup PtoleMetric_h Header PtoleMetric.h
 * \author Jones, D. I.  Owen, B. J.
 * \date 2001 -- 2006
 * \ingroup lalpulsar_metric
 * \brief Provides routines to compute pulsar parameter-space metrics using the
 * ``Ptolemaic'' approximation.
 *
 * ### Synopsis ###
 *
 * \code
 * #include <lal/PtoleMetric.h>
 * \endcode
 *
 * This module covers routines for using a ``Ptolemaic'' (epicyclic)
 * approximation to the detector motion to compute the parameter-space metric
 * for a pulsar search. (At the moment, the search is assumed to be a single
 * coherent integration.) The results should be very similar to those under
 * StackMetric.h, and reading that documention is a good
 * background for this documentation.
 *
 * Why this extra module? Two words: simplicity and speed. The metric
 * components can be expressed analytically in terms of trig functions,
 * allowing one to get a feel for what the parameter space will look like
 * before using a single CPU cycle. In addition, CPU usage is much reduced
 * (compared to the routines in StackMetric.h) in numerical
 * explorations such as testing the suitability of various tiling codes. Thus,
 * the functions in this header can be very useful in the current stage of
 * exploring parameter space and wondering how we can practically take
 * advantage of correlations. It's also good at catching bugs and errors in the
 * numerical routines under StackMetric.h. The effectiveness of the
 * tiling at catching signals should be very little reduced by the
 * approximation. Jones, Owen, and Whitbeck will write a short paper on this
 * and other details.
 *
 */
/*@{*/

#define PMETRIC_MIN(x,y) ((x) < (y) ? (x) : (y))
#define PMETRIC_MAX(x,y) ((x) > (y) ? (x) : (y))

/** Translate metrix matrix-indices (a,b) into vector-index l */
#define PMETRIC_INDEX(a,b) (PMETRIC_MIN((a),(b))+PMETRIC_MAX((a),(b))*(PMETRIC_MAX((a),(b)) + 1 ) / 2 )

/** \name Error conditions */
/*@{*/
#define PTOLEMETRICH_ENULL   1
#define PTOLEMETRICH_EPARM   2
#define PTOLEMETRICH_EDIM    3
#define PTOLEMETRICH_ENONULL 4
#define PTOLEMETRICH_EMETRIC 5

#define PTOLEMETRICH_MSGENULL   "unexpected null pointer"
#define PTOLEMETRICH_MSGEPARM   "bad parameter value"
#define PTOLEMETRICH_MSGEDIM    "bad array length"
#define PTOLEMETRICH_MSGENONULL "unexpected non-null pointer"
#define PTOLEMETRICH_MSGEMETRIC "unknown metric type"
/* @} */


/** Constants defining different types of pulsar-metrics. */
typedef enum tagLALPulsarMetricType
{
  LAL_PMETRIC_NONE = 0,
  LAL_PMETRIC_COH_PTOLE_ANALYTIC,
  LAL_PMETRIC_LAST
} LALPulsarMetricType;


/**
 * This structure will likely be changed to match up better with
 * those under StackMetric.h; it contains the bare
 * necessities, not needing function pointers etc.
 */
#ifdef SWIG /* SWIG interface directives */
SWIGLAL(IMMUTABLE_MEMBERS(tagPtoleMetricIn, site, ephemeris));
#endif /* SWIG */
typedef struct
tagPtoleMetricIn
{
  SkyPosition    position;	/**< The equatorial coordinates at which the metric components are evaluated. */
  REAL4Vector   *spindown;	/**< The (dimensionless) spindown parameters for which the metric components are evaluated. */
  LIGOTimeGPS    epoch;		/**< When the coherent integration begins */
  REAL4          duration;	/**< Duration of integration, in seconds. */
  REAL4          maxFreq;	/**< The maximum frequency to be searched, in Hz. */
  const LALDetector    *site;	/**< The detector site, used only for its latitude and longitude. */
  const EphemerisData  *ephemeris;	/**< Not used for the Ptolemaic approximation, this is for compatibility with other metrics. */
  LALPulsarMetricType metricType; /**< The type of metric to use: analytic, Ptolemaic or fully ephemeris-based. */
} PtoleMetricIn;

/* ----- prototypes ----- */
void
LALPtoleMetric( LALStatus      *status,
                REAL8Vector    *metric,
                PtoleMetricIn  *input );

void
LALPulsarMetric( LALStatus      *status,
                 REAL8Vector    **metric,
                 PtoleMetricIn  *input );

void
LALProjectMetric( LALStatus *, REAL8Vector *metric, BOOLEAN errors );

int XLALFindMetricDim ( const REAL8Vector *metric );

int XLALSpindownMetric(
  gsl_matrix* metric,
  double Tspan
  );

/*@}*/

#ifdef  __cplusplus
}
#endif

#endif
