Simon Bonnefoy / gammalib

New Features and Important Changes in GammaLib 1.6.0

1 November 2018


1. Introduction
---------------
This document briefly summarizes module by module the most important changes
made since the last release of GammaLib.


2. Public interface modifications
---------------------------------
The following classes have been added:
- GModelSpectralExponential
- GWcsARC
- GCTAModelBackground
- GCTAModelSpatial
- GCTAModelSpatialMultiplicative
- GCTAModelSpatialRegistry

The following classes have been removed:
- none

The following classes have been renamed:
- none

The following methods have been added:
- gammalib::atan2()
- gammalib::plaw_integral()
- gammalib::gauss_integral()
- GApplication(std::string&, std::string&, GApplicationPars&)
- GApplicationPar::pickle()
- GApplicationPar::query()
- GApplicationPar::was_queried()
- GApplicationPars::pickle()
- GApplicationPars::syspfiles()
- GLog::buffer()
- operator==(GSkyPixel&, GSkyPixel&)
- operator!=(GSkyPixel&, GSkyPixel&)
- GArf::read(GFits&)
- GArf::header()
- GPha::read(GFits&)
- GPha::header()
- GPha::operator(int&, int&)
- GPha::operator[](std::string&)
- GPha::columns()
- GPha::at(int&, int&)
- GPha::append(std::string&, std::vector<double>&)
- GPha::emin_obs(GEnergy&)
- GPha::emin_obs()
- GPha::emax_obs(GEnergy&)
- GPha::emax_obs()
- GPha::backfile(std::string&)
- GPha::backfile()
- GPha::corrfile(std::string&)
- GPha::corrfile()
- GPha::respfile(std::string&)
- GPha::respfile()
- GPha::ancrfile(std::string&)
- GPha::ancrfile()
- GRmf::read(GFits&)
- GRmf::header()
- GFitsHDU::header(GFitsHeader&)
- GFitsHDU::card(std::string&, bool&, std::string&)
- GFitsHeaderCard(std::string&, std::string&, std::string&, std::string&)
- GFitsHeaderCard(std::string&, bool&, std::string&)
- GFitsTable::remove(int&)
- GFitsTable::remove(std::string&)
- GObservation::has_events()
- GModelSpatialPointSource::type(std::string&)
- GModelSpectralPlaw::type(std::string&)
- GModelSpatialRadialProfileGauss(GSkyDir&, double&)
- GModelSpatialRadialProfileGauss::sigma()
- GSkyDir::cos_dist()
- GSkyRegions::filename(GFilename&)
- GXml::GXml(GXmlDocument&)
- GXml::root()
- GXmlElement::attributes()
- GXmlElement::attribute(int&)
- GXmlDocument::GXmlDocument(GFilename&, std::string&, std::string&, std::string&)
- GCTAObservation::instrument(std::string&)
- GCTAObservation::lo_user_thres(double&)
- GCTAObservation::hi_user_thres(double&)
- GCTAOnOffObservation::has_response()
- GCTAInstDir::GCTAInstDir(double&, double&)
- GCTAInstDir::GCTAInstDir(GSkyDir&, double&, double&)
- GCTAInstDir::theta()
- GCTAInstDir::phi()
- GCTAInstDir::has_dir()
- GCTAInstDir::has_detx()
- GCTAInstDir::has_dety()
- GCTAEventAtom(GCTAInstDir&, GEnergy&, GTime&)
- GCTAEventAtom::index(int&)
- GCTABackground::rate_ebin()
- GCTABackgroundPerfTable::rate_ebin()
- GCTABackground3D::rate_ebin()
- GCTAEdisp::prob_erecobin()
- GCTAEdispPerfTable::prob_erecobin()
- GCTAEdispRmf::prob_erecobin()
- GCTAEdisp2D::prob_erecobin()
- GCTAAeff2D::rad_max()
- GCTAResponseTable::telescope()
- GCTAModelAeffBackground(GModelSpectral&, GModelTemporal&)
- GCTAModelAeffBackground::spectral(GModelSpectral*)
- GCTAModelAeffBackground::spectral(GModelTemporal*)
- GCTAModelCubeBackground(GModelSpectral&, GModelTemporal&)
- GCTAModelCubeBackground::spectral(GModelSpectral*)
- GCTAModelCubeBackground::spectral(GModelTemporal*)
- GCTAModelRadialAcceptance(GCTAModelRadial&, GModelSpectral&, GModelTemporal&)
- GCTAModelRadialAcceptance::radial(GCTAModelRadial*)
- GCTAModelRadialAcceptance::spectral(GModelSpectral*)
- GCTAModelRadialAcceptance::temporal(GModelTemporal*)
- GCTAModelIrfBackground::spectral(GModelSpectral*)
- GCTAModelIrfBackground::temporal(GModelTemporal*)
- GCOMD1Response::write(GFitsBinTable&)
- GCOMD2Response::write(GFitsBinTable&)
- GCOMEventBin::index(int&)
- GCOMEventBin::dir(GCOMInstDir&)
- GCOMEventBin::energy(GEnergy&)
- GCOMEventBin::time(GTime&)
- GCOMEventBin::counts(double&)
- GCOMEventBin::solidangle(double&)
- GCOMEventBin::ewidth(GEnergy&)
- GCOMEventBin::ontime(double&)
- GCOMResponse::write(GFitsImageFloat&)
- GCOMTim(GGti&)
- GLATObservation(GXmlElement&)
- GLATLtCube::read(GFits&)
- GLATLtCube::write(GFits&)
- GLATEfficiency::pars()
- GMWLDatum(GEnergy&, GEnergy&, double&, double&)
- GMWLDatum::energy(GEnergy&)
- GMWLDatum::energy_err(GEnergy&)

The following methods have been removed:
- GSkyRegionMap::filename()

The following methods have been renamed:
- GPhoton::mc_id() from GPhoton::mcid()
- GCTAEdisp::ereco_bounds() from GCTAEdisp::ebounds_obs()
- GCTAEdisp::etrue_bounds() from GCTAEdisp::ebounds_src()

The arguments for the following methods have been changed:
- GCTAOnOffObservation(GCTAObservation&, GModelSpatial&, GEbounds&, GEbounds&, GSkyRegions&, GSkyRegions&, bool&)
- GCTAModelRadial::mc(GRan&)
- GCTAEdisp::operator(GEnergy&, GEnergy&, double&, double&, double&, double&)
- GCTAEdisp::mc(GRan&, GEnergy&, double&, double&, double&, double&)
- GCTAResponseIrf::edisp(GEnergy&, GEnergy&, double&, double&, double&, double&)
- GLATAeff(GFits&, std::string&)
- GLATEdisp(GFits&, std::string&)
- GLATPsf(GFits&, std::string&)


The return value of the following methods has been changed:
- none

All at() methods were removed from the Python interface.


3. Configuration
-----------------
Keep existing library path in installation script on Mac OS X (#2420).

GammaLib classes can now be pickled from Python (#1938).


4. Application module
---------------------
Add GLog::buffer() method that returns the content of the logger buffer.

A GApplicationPars::syspfiles() setter and getter method was added to allow the
specification of an application specific system parameter file path. If such a
file path is specified, the loading of the application parameters needs to be
redone by the client. The GApplicationPars::load() methods now gives priority
to a parameter file found in the syspfiles folder and updates parameter values
using the parameter file found in the user's pfiles folder. In that way, any
changes in the parameter file structure should be handled transparently (#2513).

The GApplicationPar::query() method was made public.

Add GApplicationPar::was_queried() method and do no longer change the mode
of queried parameters to hidden. This makes sure that the correct mode will
be written to the parfile, also for q-mode parameters (#2495).


5. Base module
--------------
None


6. FITS I/O Interface
---------------------
Add GFitsTable::remove() methods that allow the removal of table columns from
a GFitsTable object. A protected GFitsTable::update_header() method was also
added to update the header after FITS table row or column manipulations (#2339).

None


7. Linear algebra module
------------------------
None


8. Model module
---------------
The GModelSpectralExponential class was added that implements an exponential
function that can be used for EBL studies (#2454).

Add a GModelSpatialRadialProfileGauss() position and width constructor, add
GModelSpatialRadialProfileGauss::sigma() getter and setter methods, and avoid
recomputations if the position of the Gaussian changed (#2463). 


9. Numerics module
------------------
The gammalib::gauss_integral() function was added to compute the area under a
Gaussian between two boundaries (#2422).

The gammalib::atan2() function was added to compute the arc tangens of a ratio
in radians (#2308).

The gammalib::plaw_integral() function was added to compute the area under a
power law between two boundaries (#2308).


10. Observation module
----------------------
Add "parallel" to the OpenMP pragma in GObservations::likelihood::eval() to avoid
freezing of the code (#2678).


11. Optimization module
-----------------------
None


12. Sky module
--------------
The class GWcsARC was added to handle ARC WCS projections (#2541). In addition
the private GWcs::prj_bchk() method was added to implement boundary checking
similar to the checking done in WCS.

A precomputation cache was added to the GWcs::dir2pix() and GWcs::pix2dir()
methods so that results are not recomputed for the same arguments. This should
provide some speed-up as it avoids unnecessary coordinate transformations.

Add GSkyDir::cos_dist() method that computes the cosine of the angular distance
between two sky directions. Using this method avoids computation of the arc
cosine (#2309).


13. Support module
------------------
The gammalib::replace_segment() function was added that replaces string segments
by replacement strings.


14. XML module
--------------
None


15. VO module
-------------
None


16. Xspec module
----------------
The GPha::write() method wrote the correct header keywords in the PHA files,
but those were overwritten by the initial header keywords that were actually
found in the PHA file before. This led to a problem when stacking CTA On/Off
observations (#2683).

Add setter and getter methods to access the attributes backfile, corrfile,
respfile and ancrfile that inform about related files, and that are needed
for OGIP/XSPEC compliance. The attributes are written and read from FITS
files (#2404).

Add methods and operators to GPha to store additional columns in the data
structure, similar to what exists for GArf. In addition, GPha::emin_obs()
and GPha::emax_obs() setter and getter methods were added that allow storing
and retrieving the minimum and maximum energy of the observation that was
used to fill the spectrum. This allows to define an ROI for On/Off analysis. 

The output files of the GPha, GArf and GRmf files are now compliant with the
OGIP format that is needed for a XSPEC analysis (#2404).


17. Test module
---------------
None


18. Multi-wavelength interface
------------------------------
None


19. Fermi-LAT interface
----------------------
None


20. CTA interface
-----------------
GCTABackground3D::init_mc_cache now pre-computes the Monte Carlo cache at energy
nodes of the background cube, and in addition, inserts 8 logarithmically spaced
nodes between each pair of nodes. This assures that the energy variations of the
background rate are precisely captured and reproduced in the Monte Carlo
simulations (#2708).

The GCTAEdisp::operator() now returns energy dispersion values per MeV. The
units are now consistent with the expectation in GResponse, and this changes
assurance the coherence between the various classes. In particular, no re-
normalization is needed anymore to digest the H.E.S.S. energy dispersion, and
also the CTA energy dispersion is handled correctly (#2704).

The GCTAEdisp class now uses GEnergy objects instead of log10(E) to deal with
true and reconstructed energies. This avoids computational overhead when going
from one unit to another (#2704).

The GCTAInstDir class now assures that only valid information can be accessed.
Since the class can hold a sky direction and detector coordinates, flags were
added that signal what information actually exists in the class. If a non-
existing information is accessed an exception is thrown (#2694).

Add the GCTAModelBackground class that implements a general factorised CTA
background model. The spatial component of the model is implemented by the
abstract GCTAModelSpatial based class, the GCTAModelSpatialRegistry class
registers all possible spatial model component. GCTAModelRadial now derives
from GCTAModelSpatial and is a special instance of the spatial model component.
The GCTAModelSpatialMultiplicative class was added to implement an arbitrary
multiplicative spatial model (#2694).

Correct the handling of stacked On/Off observations in the absence of a
background IRF template (#2683).

The GCTACubeBackground class is now defined for energy boundaries instead of
nodes so that the background cube can have the same dimensions as the counts
cube and no interpolation is needed anymore. The GCTACubeBackground::fill()
method now computes the integral of the background rate over a energy bin
assuming a power law dependence throughout the bin (#2677).

Remove setting of effective area energy boundaries in GCTAAeff2D::read() method
from "LO_THRES" and "HI_THRES" keywords, since the values are reconstructued
energies but the effective area is given in true energies. The keywords are also
read in GCTAResponseIrf::load_aeff() and it is not required to apply the values
in GCTAAeff2D (#2674).

The maximum energy in GCTAAeff2D was not computed correctly due to a bug in the
indexing. This was corrected now (#2674).

GCTAEdisp2D now supports "ENERG" as column name instead of "ETRUE" in an energy
dispersion FITS file (#2670).

Change PSF table default extension name in GCTAPsfTable.hpp to "PSF_2D_TABLE".
Allow also "EDISP_2D" as extension name for the energy dispersion and pickle
GCTAResponseIrf class via XML interface. Drop the storing of component filenames
and use instead directly the filenames stored with the IRF components (#2660).

The GCTAOnOffObservation now supports IRFs where the effective area is given
for an applied theta-cut. In that case, the "RAD_MAX" keyword is set, and
GCTAOnOffObservation will detect this and will not compute the PSF containment
since it is already included in the IRF. The class will check whether the radial
cut is consistent with the size of the On region, so that inconsistent computations
are avoided (#2657).

The optional argument "use_irf_bkg" was assed to the GCTAOnOffObservation
constructor to turn off the usage of the IRF background template in the
computation of the On/Off observation and to assume an identical background
rate in the On and Off regions instead. This is the classical analysis method
for IACT data using reflected regions. If use_irf_bkg=false the alpha parameter
that is stored in the "BACKSCAL" column of the On spectrum will become energy
independent, and reflect the solid angle between On and Off regions. The
"BACKRESP" column, stored in the Off spectrum, will be set to zero. Fitting
using the "cstat" statistic will not be possible, the usage of the "wstat"
statistic is mandatory (#2659).

Non-mandatory column names are now ignored in GCTABackground3D::read() to
make the code compatible with the current H.E.S.S. data structure (#2339).

The 3D background model now supports "BKG" column names instead of the "BGD"
column names. Since "BKG" should be the default, all "BGD" keywords in the
calibration files were changed to "BKG" (#2343). 

The likelihood value is now also computed in GObservations::likelihood::eval(),
CTAOnOffObservation::likelihood_wstat() and CTAOnOffObservation::likelihood_cstat()
for the case that the model has no parameters. This is particularily needed for
the TS computation with the "wstat" statistic which is meaningful without any
model (#2312).

The GCTAOnOffObservation observation constructor now takes a spatial model
component of type GModelSpatial instead of a sky direction as argument, and the
ARF computation is performed by computing the IRF for the spatial model over the
On region. In that way also extended source can be properly handled (#2292).

The energy bounds of a CTA observations are now taken into account when setting
up a GCTAOnOffObservation so that observation-specific energy thresholds are
correctly handled (#2429).

The computation of diffuse map models was sped-up by including some value caching
and avoiding allocation and de-allocation of variables during response computation
(#2466).

The integration precision of the diffuse model response was increase to cope with
sky maps that have a higher spatial resolution than the size of the PSF (#2458).

A GCTAEdisp::prob_erecobin() method has been defined and implemented in the
derived energy dispersion classes that returns the probability that a photon with
a given true energy is reconstructed with a energy comprised in a given energy
interval. The method makes use of the internal structure of the response information
and avoids a numerical integration over reconstructed energy (#2422).

A GCTAInstDir::theta() and GCTAInstDir::phi() methods were added that return the
distance to the camera centre in radians and the azimuth angle, respectively (#2308).

A rate_ebin() method was added to the interface of the GCTABackground class and
implemented for the GCTABackgroundPerfTable and GCTABackground3D classes. The method
computes for a given instrument direction the background rate integrated over an
energy bin (#2308).

The GTIs a preserved when copying a GCTAEventList or GCTAEventCube object. In addition,
the MJD reference of the first observation is used when building an exposure cube
(#2054).


21. COMPTEL interface
---------------------
None