コード例 #1
0
ファイル: ManualReduction.py プロジェクト: ytchenak/RMS
    def saveFTPdetectinfo(self):
        """ Saves the picks to a FTPdetectinfo file in the same folder where the first given file is. """

        # Compute the intensity sum done on the previous frame
        self.computeIntensitySum()

        # PNG mode
        if self.png_mode:
            dir_path = self.png_dir
            ff_name_ftp = "FF_" + self.frame0_time.strftime(
                "%Y%m%d_%H%M%S.%f") + '.bin'

        # FF mode
        else:
            # Extract the save directory
            if self.ff_file is not None:
                dir_path, ff_name_ftp = os.path.split(self.ff_file)

            elif self.fr_file is not None:
                dir_path, ff_name_ftp = os.path.split(self.fr_file)

        # Remove the file extension of the image file
        ff_name_ftp = ff_name_ftp.replace('.bin', '').replace('.fits', '')

        # Create the list of picks for saving
        centroids = []
        for pick in self.pick_list:
            centroids.append([
                pick.frame, pick.x_centroid, pick.y_centroid,
                pick.intensity_sum
            ])

        meteor_list = [[ff_name_ftp, 1, 0, 0, centroids]]

        # Create a name for the FTPdetectinfo
        ftpdetectinfo_name = "FTPdetectinfo_" + "_".join(
            ff_name_ftp.split('_')[1:]) + '_manual.txt'

        # Read the station code for the file name
        station_id = ff_name_ftp.split('_')[1]

        # Take the FPS from the FF file, if available
        if self.ff is not None:
            if hasattr(self.ff, 'fps'):
                self.fps = self.ff.fps

        if self.fps is None:
            self.fps = self.config.fps

        # Write the FTPdetect info
        writeFTPdetectinfo(meteor_list, dir_path, ftpdetectinfo_name, '',
                           station_id, self.fps)

        print('FTPdetecinfo written to:',
              os.path.join(dir_path, ftpdetectinfo_name))
コード例 #2
0
def applyAstrometryFTPdetectinfo(dir_path,
                                 ftp_detectinfo_file,
                                 platepar_file,
                                 UT_corr=0,
                                 platepar=None):
    """ Use the given platepar to calculate the celestial coordinates of detected meteors from a FTPdetectinfo
        file and save the updates values.
    Arguments:
        dir_path: [str] Path to the night.
        ftp_detectinfo_file: [str] Name of the FTPdetectinfo file.
        platepar_file: [str] Name of the platepar file.
    Keyword arguments:
        UT_corr: [float] Difference of time from UTC in hours.
        platepar: [Platepar obj] Loaded platepar. None by default. If given, the platepar file won't be read,
            but this platepar structure will be used instead.
    Return:
        None
    """

    # If the FTPdetectinfo file does not exist, skip everything
    if not os.path.isfile(os.path.join(dir_path, ftp_detectinfo_file)):
        print('The given FTPdetectinfo file does not exist:',
              os.path.join(dir_path, ftp_detectinfo_file))
        print('The astrometry was not computed!')
        return None

    # Save a copy of the uncalibrated FTPdetectinfo
    ftp_detectinfo_copy = "".join(
        ftp_detectinfo_file.split('.')[:-1]) + "_uncalibrated.txt"

    # Back up the original FTPdetectinfo, only if a backup does not exist already
    if not os.path.isfile(os.path.join(dir_path, ftp_detectinfo_copy)):
        shutil.copy2(os.path.join(dir_path, ftp_detectinfo_file),
                     os.path.join(dir_path, ftp_detectinfo_copy))

    # Load platepar from file if not given
    if platepar is None:

        # Load the platepar
        platepar = Platepar()
        platepar.read(os.path.join(dir_path, platepar_file), use_flat=None)

    # Load the FTPdetectinfo file
    meteor_data = readFTPdetectinfo(dir_path, ftp_detectinfo_file)

    # List for final meteor data
    meteor_list = []

    # Go through every meteor
    for meteor in meteor_data:

        ff_name, cam_code, meteor_No, n_segments, fps, hnr, mle, binn, px_fm, rho, phi, meteor_meas = meteor

        # Apply the platepar to the given centroids
        meteor_picks = applyPlateparToCentroids(ff_name, fps, meteor_meas,
                                                platepar)

        # Add the calculated values to the final list
        meteor_list.append([ff_name, meteor_No, rho, phi, meteor_picks])

    # Calibration string to be written to the FTPdetectinfo file
    calib_str = 'Calibrated with RMS on: ' + str(
        datetime.datetime.utcnow()) + ' UTC'

    # If no meteors were detected, set dummpy parameters
    if len(meteor_list) == 0:
        cam_code = ''
        fps = 0

    # Save the updated FTPdetectinfo
    writeFTPdetectinfo(meteor_list,
                       dir_path,
                       ftp_detectinfo_file,
                       dir_path,
                       cam_code,
                       fps,
                       calibration=calib_str,
                       celestial_coords_given=True)
コード例 #3
0
def processNight(night_data_dir, config, detection_results=None, nodetect=False):
    """ Given the directory with FF files, run detection and archiving. 
    
    Arguments:
        night_data_dir: [str] Path to the directory with FF files.
        config: [Config obj]

    Keyword arguments:
        detection_results: [list] An optional list of detection. If None (default), detection will be done
            on the the files in the folder.
        nodetect: [bool] True if detection should be skipped. False by default.

    Return:
        night_archive_dir: [str] Path to the night directory in ArchivedFiles.
        archive_name: [str] Path to the archive.
        detector: [QueuedPool instance] Handle to the detector.
    """

    # Remove final slash in the night dir
    if night_data_dir.endswith(os.sep):
        night_data_dir = night_data_dir[:-1]

    # Extract the name of the night
    night_data_dir_name = os.path.basename(os.path.abspath(night_data_dir))

    platepar = None
    
    # If the detection should be run
    if (not nodetect):

        # If no detection was performed, run it
        if detection_results is None:

            # Run detection on the given directory
            calstars_name, ftpdetectinfo_name, ff_detected, \
                detector = detectStarsAndMeteorsDirectory(night_data_dir, config)

        # Otherwise, save detection results
        else:

            # Save CALSTARS and FTPdetectinfo to disk
            calstars_name, ftpdetectinfo_name, ff_detected = saveDetections(detection_results, \
                night_data_dir, config)

            # If the files were previously detected, there is no detector
            detector = None


        # Get the platepar file
        platepar, platepar_path, platepar_fmt = getPlatepar(config, night_data_dir)


        # Run calibration check and auto astrometry refinement
        if (platepar is not None) and (calstars_name is not None):

            # Read in the CALSTARS file
            calstars_list = CALSTARS.readCALSTARS(night_data_dir, calstars_name)

            # Run astrometry check and refinement
            platepar, fit_status = autoCheckFit(config, platepar, calstars_list)

            # If the fit was sucessful, apply the astrometry to detected meteors
            if fit_status:

                log.info('Astrometric calibration SUCCESSFUL!')

                # Save the refined platepar to the night directory and as default
                platepar.write(os.path.join(night_data_dir, config.platepar_name), fmt=platepar_fmt)
                platepar.write(platepar_path, fmt=platepar_fmt)

            else:
                log.info('Astrometric calibration FAILED!, Using old platepar for calibration...')


            # # Calculate astrometry for meteor detections
            # applyAstrometryFTPdetectinfo(night_data_dir, ftpdetectinfo_name, platepar_path)

            # If a flat is used, disable vignetting correction
            if config.use_flat:
                platepar.vignetting_coeff = 0.0

            log.info("Recalibrating astrometry on FF files with detections...")

            # Recalibrate astrometry on every FF file and apply the calibration to detections
            recalibrateIndividualFFsAndApplyAstrometry(night_data_dir, os.path.join(night_data_dir, \
                ftpdetectinfo_name), calstars_list, config, platepar)

            

            log.info("Converting RMS format to UFOOrbit format...")

            # Convert the FTPdetectinfo into UFOOrbit input file
            FTPdetectinfo2UFOOrbitInput(night_data_dir, ftpdetectinfo_name, platepar_path)



            # Generate a calibration report
            log.info("Generating a calibration report...")
            try:
                generateCalibrationReport(config, night_data_dir, platepar=platepar)

            except Exception as e:
                log.debug('Generating calibration report failed with the message:\n' + repr(e))
                log.debug(repr(traceback.format_exception(*sys.exc_info())))


            # Perform single station shower association
            log.info("Performing single station shower association...")
            try:
                showerAssociation(config, [os.path.join(night_data_dir, ftpdetectinfo_name)], \
                    save_plot=True, plot_activity=True)

            except Exception as e:
                log.debug('Shower association failed with the message:\n' + repr(e))
                log.debug(repr(traceback.format_exception(*sys.exc_info())))


    else:
        ff_detected = []
        detector = None



    log.info('Plotting field sums...')

    # Plot field sums
    try:
        plotFieldsums(night_data_dir, config)

    except Exception as e:
        log.debug('Plotting field sums failed with message:\n' + repr(e))
        log.debug(repr(traceback.format_exception(*sys.exc_info())))



    # Archive all fieldsums to one archive
    archiveFieldsums(night_data_dir)


    # List for any extra files which will be copied to the night archive directory. Full paths have to be 
    #   given
    extra_files = []


    log.info('Making a flat...')

    # Make a new flat field image
    try:
        flat_img = makeFlat(night_data_dir, config)

    except Exception as e:
        log.debug('Making a flat failed with message:\n' + repr(e))
        log.debug(repr(traceback.format_exception(*sys.exc_info())))
        flat_img = None
        

    # If making flat was sucessfull, save it
    if flat_img is not None:

        # Save the flat in the night directory, to keep the operational flat updated
        flat_path = os.path.join(night_data_dir, os.path.basename(config.flat_file))
        saveImage(flat_path, flat_img)
        log.info('Flat saved to: ' + flat_path)

        # Copy the flat to the night's directory as well
        extra_files.append(flat_path)

    else:
        log.info('Making flat image FAILED!')


    ### Add extra files to archive

    # Add the config file to the archive too
    extra_files.append(os.path.join(os.getcwd(), '.config'))

    # Add the mask
    if (not nodetect):
        if os.path.exists(config.mask_file):
            mask_path = os.path.abspath(config.mask_file)
            extra_files.append(mask_path)


    # Add the platepar to the archive if it exists
    if (not nodetect):
        if os.path.exists(platepar_path):
            extra_files.append(platepar_path)


    # Add the json file with recalibrated platepars to the archive
    if (not nodetect):
        recalibrated_platepars_path = os.path.join(night_data_dir, config.platepars_recalibrated_name)
        if os.path.exists(recalibrated_platepars_path):
            extra_files.append(recalibrated_platepars_path)

    ### ###



    # If the detection should be run
    if (not nodetect):

        # Make a CAL file and a special CAMS FTPdetectinfo if full CAMS compatibility is desired
        if (config.cams_code > 0) and (platepar is not None):

            log.info('Generating a CAMS FTPdetectinfo file...')

            # Write the CAL file to disk
            cal_file_name = writeCAL(night_data_dir, config, platepar)

            # Check if the CAL file was successfully generated
            if cal_file_name is not None:

                cams_code_formatted = "{:06d}".format(int(config.cams_code))

                # Load the FTPdetectinfo
                _, fps, meteor_list = readFTPdetectinfo(night_data_dir, ftpdetectinfo_name, \
                    ret_input_format=True)

                # Replace the camera code with the CAMS code
                for met in meteor_list:

                    # Replace the station name and the FF file format
                    ff_name = met[0]
                    ff_name = ff_name.replace('.fits', '.bin')
                    ff_name = ff_name.replace(config.stationID, cams_code_formatted)
                    met[0] = ff_name


                # Write the CAMS compatible FTPdetectinfo file
                writeFTPdetectinfo(meteor_list, night_data_dir, \
                    ftpdetectinfo_name.replace(config.stationID, cams_code_formatted),\
                    night_data_dir, cams_code_formatted, fps, calibration=cal_file_name, \
                    celestial_coords_given=(platepar is not None))



    night_archive_dir = os.path.join(os.path.abspath(config.data_dir), config.archived_dir, 
        night_data_dir_name)


    log.info('Archiving detections to ' + night_archive_dir)
    
    # Archive the detections
    archive_name = archiveDetections(night_data_dir, night_archive_dir, ff_detected, config, \
        extra_files=extra_files)


    return night_archive_dir, archive_name, detector
コード例 #4
0
                print("{:5.1f}, {:7.2f}, {:8.2f}, {:10.1f}".format(
                    frame_n, mag, unsaturated_mag, bg_val))

                # Compute the intensity from unsaturated magnitude
                unsaturated_inten = round(10**((photom_offset - mag) / 2.5), 0)

                corrected_meteor_meas.append([
                    frame_n, x, y, ra, dec, azim, elev, unsaturated_inten,
                    unsaturated_mag
                ])

            if not corrected_meteor_meas:
                corrected_meteor_meas = meteor_meas

        corrected_meteor_list.append(
            [ftp_ff_name, meteor_No, rho, phi, corrected_meteor_meas])

    # Calibration string to be written to the FTPdetectinfo file
    calib_str = "RMS - Saturation corrected on {:s} UTC".format(
        str(datetime.datetime.utcnow()))

    # Write a corrected FTPdetectinfo file
    corrected_ftpdetectinfo_name = ftpdetectinfo_name.strip(
        '.txt') + '_saturation_corrected.txt'

    print('Saving to:', os.path.join(dir_path, corrected_ftpdetectinfo_name))

    writeFTPdetectinfo(corrected_meteor_list, dir_path, corrected_ftpdetectinfo_name, dir_path, cam_code, \
        fps, calibration=calib_str, celestial_coords_given=True)
コード例 #5
0
def applyAstrometryFTPdetectinfo(dir_path,
                                 ftp_detectinfo_file,
                                 platepar_file,
                                 UT_corr=0):
    """ Use the given platepar to calculate the celestial coordinates of detected meteors from a FTPdetectinfo
        file and save the updates values.

    Arguments:
        dir_path: [str] Path to the night.
        ftp_detectinfo_file: [str] Name of the FTPdetectinfo file.
        platepar_file: [str] Name of the platepar file.

    Keyword arguments:
        UT_corr: [float] Difference of time from UTC in hours.

    Return:
        None
    """

    # Save a copy of the uncalibrated FTPdetectinfo
    ftp_detectinfo_copy = "".join(
        ftp_detectinfo_file.split('.')[:-1]) + "_uncalibrated.txt"

    # Back up the original FTPdetectinfo, only if a backup does not exist already
    if not os.path.isfile(os.path.join(dir_path, ftp_detectinfo_copy)):
        shutil.copy2(os.path.join(dir_path, ftp_detectinfo_file),
                     os.path.join(dir_path, ftp_detectinfo_copy))

    # Load the platepar
    platepar = Platepar()
    platepar.read(os.path.join(dir_path, platepar_file))

    # Load the FTPdetectinfo file
    meteor_data = readFTPdetectinfo(dir_path, ftp_detectinfo_file)

    # List for final meteor data
    meteor_list = []

    # Go through every meteor
    for meteor in meteor_data:

        ff_name, cam_code, meteor_No, n_segments, fps, hnr, mle, binn, px_fm, rho, phi, meteor_meas = meteor

        meteor_meas = np.array(meteor_meas)

        # Extract frame number, x, y, intensity
        frames = meteor_meas[:, 1]
        X_data = meteor_meas[:, 2]
        Y_data = meteor_meas[:, 3]
        level_data = meteor_meas[:, 8]

        # Get the beginning time of the FF file
        time_beg = filenameToDatetime(ff_name)

        # Calculate time data of every point
        time_data = []
        for frame_n in frames:
            t = time_beg + datetime.timedelta(seconds=frame_n / fps)
            time_data.append([
                t.year, t.month, t.day, t.hour, t.minute, t.second,
                int(t.microsecond / 1000)
            ])

        # Convert image cooredinates to RA and Dec, and do the photometry
        JD_data, RA_data, dec_data, magnitudes = XY2CorrectedRADecPP(np.array(time_data), X_data, Y_data, \
            level_data, platepar)

        # Compute azimuth and altitude of centroids
        az_data = np.zeros_like(RA_data)
        alt_data = np.zeros_like(RA_data)

        for i in range(len(az_data)):

            jd = JD_data[i]
            ra_tmp = RA_data[i]
            dec_tmp = dec_data[i]

            az_tmp, alt_tmp = raDec2AltAz(jd, platepar.lon, platepar.lat,
                                          ra_tmp, dec_tmp)

            az_data[i] = az_tmp
            alt_data[i] = alt_tmp

        # print(ff_name, cam_code, meteor_No, fps)
        # print(X_data, Y_data)
        # print(RA_data, dec_data)
        # print('------------------------------------------')

        # Construct the meteor measurements array
        meteor_picks = np.c_[frames, X_data, Y_data, RA_data, dec_data, az_data, alt_data, level_data, \
            magnitudes]

        # Add the calculated values to the final list
        meteor_list.append([ff_name, meteor_No, rho, phi, meteor_picks])

    # Calibration string to be written to the FTPdetectinfo file
    calib_str = 'Calibrated with RMS on: ' + str(
        datetime.datetime.utcnow()) + ' UTC'

    # If no meteors were detected, set dummpy parameters
    if len(meteor_list) == 0:
        cam_code = ''
        fps = 0

    # Save the updated FTPdetectinfo
    writeFTPdetectinfo(meteor_list,
                       dir_path,
                       ftp_detectinfo_file,
                       dir_path,
                       cam_code,
                       fps,
                       calibration=calib_str,
                       celestial_coords_given=True)
コード例 #6
0
                # Compute the intensity from unsaturated magnitude
                unsaturated_inten = round(10**((photom_offset - mag)/2.5), 0)

                corrected_meteor_meas.append([frame_n, x, y, ra, dec, azim, elev, unsaturated_inten, 
                    unsaturated_mag])



            if not corrected_meteor_meas:
                corrected_meteor_meas = meteor_meas


        corrected_meteor_list.append([ftp_ff_name, meteor_No, rho, phi, corrected_meteor_meas])


    # Calibration string to be written to the FTPdetectinfo file
    calib_str = "RMS - Saturation corrected on {:s} UTC".format(str(datetime.datetime.utcnow()))

    # Write a corrected FTPdetectinfo file
    corrected_ftpdetectinfo_name = ftpdetectinfo_name.strip('.txt') + '_saturation_corrected.txt'

    print('Saving to:', os.path.join(dir_path, corrected_ftpdetectinfo_name))

    writeFTPdetectinfo(corrected_meteor_list, dir_path, corrected_ftpdetectinfo_name, dir_path, cam_code, \
        fps, calibration=calib_str, celestial_coords_given=True)




コード例 #7
0
def processNight(night_data_dir, config, detection_results=None, nodetect=False):
    """ Given the directory with FF files, run detection and archiving. 
    
    Arguments:
        night_data_dir: [str] Path to the directory with FF files.
        config: [Config obj]

    Keyword arguments:
        detection_results: [list] An optional list of detection. If None (default), detection will be done
            on the the files in the folder.
        nodetect: [bool] True if detection should be skipped. False by default.

    Return:
        night_archive_dir: [str] Path to the night directory in ArchivedFiles.
        archive_name: [str] Path to the archive.
        detector: [QueuedPool instance] Handle to the detector.
    """

    # Remove final slash in the night dir
    if night_data_dir.endswith(os.sep):
        night_data_dir = night_data_dir[:-1]

    # Extract the name of the night
    night_data_dir_name = os.path.basename(night_data_dir)
    
    # If the detection should be run
    if (not nodetect):

        # If no detection was performed, run it
        if detection_results is None:

            # Run detection on the given directory
            calstars_name, ftpdetectinfo_name, ff_detected, \
                detector = detectStarsAndMeteorsDirectory(night_data_dir, config)

        # Otherwise, save detection results
        else:

            # Save CALSTARS and FTPdetectinfo to disk
            calstars_name, ftpdetectinfo_name, ff_detected = saveDetections(detection_results, \
                night_data_dir, config)

            # If the files were previously detected, there is no detector
            detector = None


        # Get the platepar file
        platepar, platepar_path, platepar_fmt = getPlatepar(config, night_data_dir)


        # Run calibration check and auto astrometry refinement
        if platepar is not None:

            # Read in the CALSTARS file
            calstars_list = CALSTARS.readCALSTARS(night_data_dir, calstars_name)

            # Run astrometry check and refinement
            platepar, fit_status = autoCheckFit(config, platepar, calstars_list)

            # If the fit was sucessful, apply the astrometry to detected meteors
            if fit_status:

                log.info('Astrometric calibration SUCCESSFUL!')

                # Save the refined platepar to the night directory and as default
                platepar.write(os.path.join(night_data_dir, config.platepar_name), fmt=platepar_fmt)
                platepar.write(platepar_path, fmt=platepar_fmt)

            else:
                log.info('Astrometric calibration FAILED!, Using old platepar for calibration...')


            # # Calculate astrometry for meteor detections
            # applyAstrometryFTPdetectinfo(night_data_dir, ftpdetectinfo_name, platepar_path)

            

            log.info("Recalibrating astrometry on FF files with detections...")

            # Recalibrate astrometry on every FF file and apply the calibration to detections
            recalibrateIndividualFFsAndApplyAstrometry(night_data_dir, os.path.join(night_data_dir, \
                ftpdetectinfo_name), calstars_list, config, platepar)

            

            log.info("Converting RMS format to UFOOrbit format...")

            # Convert the FTPdetectinfo into UFOOrbit input file
            FTPdetectinfo2UFOOrbitInput(night_data_dir, ftpdetectinfo_name, platepar_path)



            # Generate a calibration report
            log.info("Generating a calibration report...")
            try:
                generateCalibrationReport(config, night_data_dir, platepar=platepar)

            except Exception as e:
                log.debug('Generating calibration report failed with message:\n' + repr(e))
                log.debug(repr(traceback.format_exception(*sys.exc_info())))


    else:
        ff_detected = []
        detector = None



    log.info('Plotting field sums...')

    # Plot field sums
    try:
        plotFieldsums(night_data_dir, config)

    except Exception as e:
        log.debug('Plotting field sums failed with message:\n' + repr(e))
        log.debug(repr(traceback.format_exception(*sys.exc_info())))



    # Archive all fieldsums to one archive
    archiveFieldsums(night_data_dir)


    # List for any extra files which will be copied to the night archive directory. Full paths have to be 
    #   given
    extra_files = []


    log.info('Making a flat...')

    # Make a new flat field image
    try:
        flat_img = makeFlat(night_data_dir, config)

    except Exception as e:
        log.debug('Making a flat failed with message:\n' + repr(e))
        log.debug(repr(traceback.format_exception(*sys.exc_info())))
        flat_img = None
        

    # If making flat was sucessfull, save it
    if flat_img is not None:

        # Save the flat in the night directory, to keep the operational flat updated
        flat_path = os.path.join(night_data_dir, os.path.basename(config.flat_file))
        scipy.misc.imsave(flat_path, flat_img)
        log.info('Flat saved to: ' + flat_path)

        # Copy the flat to the night's directory as well
        extra_files.append(flat_path)

    else:
        log.info('Making flat image FAILED!')


    ### Add extra files to archive

    # Add the config file to the archive too
    extra_files.append(os.path.join(os.getcwd(), '.config'))

    # Add the platepar to the archive if it exists
    if (not nodetect):

        if os.path.exists(platepar_path):
            extra_files.append(platepar_path)


    # Add the json file with recalibrated platepars to the archive
    if (not nodetect):

        recalibrated_platepars_path = os.path.join(night_data_dir, config.platepars_recalibrated_name)
        if os.path.exists(recalibrated_platepars_path):
            extra_files.append(recalibrated_platepars_path)

    ### ###



    # If the detection should be run
    if (not nodetect):

        # Make a CAL file and a special CAMS FTpdetectinfo if full CAMS compatibility is desired
        if config.cams_code > 0:

            log.info('Generating a CAMS FTPdetectinfo file...')

            # Write the CAL file to disk
            cal_file_name = writeCAL(night_data_dir, config, platepar)


            cams_code_formatted = "{:06d}".format(int(config.cams_code))

            # Load the FTPdetectinfo
            _, fps, meteor_list = readFTPdetectinfo(night_data_dir, ftpdetectinfo_name, \
                ret_input_format=True)

            # Replace the camera code with the CAMS code
            for met in meteor_list:

                # Replace the station name and the FF file format
                ff_name = met[0]
                ff_name = ff_name.replace('.fits', '.bin')
                ff_name = ff_name.replace(config.stationID, cams_code_formatted)
                met[0] = ff_name

                # Replace the station name
                met[1] = cams_code_formatted


            # Write the CAMS compatible FTPdetectinfo file
            writeFTPdetectinfo(meteor_list, night_data_dir, \
                ftpdetectinfo_name.replace(config.stationID, cams_code_formatted),\
                night_data_dir, cams_code_formatted, fps, calibration=cal_file_name, \
                celestial_coords_given=(platepar is not None))



    night_archive_dir = os.path.join(os.path.abspath(config.data_dir), config.archived_dir, 
        night_data_dir_name)


    log.info('Archiving detections to ' + night_archive_dir)
    
    # Archive the detections
    archive_name = archiveDetections(night_data_dir, night_archive_dir, ff_detected, config, \
        extra_files=extra_files)


    return night_archive_dir, archive_name, detector