Esempio n. 1
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def loadMultipleDetrendings(epic, campaign, dataStorePath, detrendTypes):
    #Definition of the different kinds of detrendings and how to
    #parse the output of their archive class
    dTypeDict = dict()
    dTypeDict['PDC'] = (mastio.K2Archive(), pdcParser, "PDC")
    dTypeDict['AGP'] = (mastio.K2SCArchive(), agpParser, "K2SC")
    dTypeDict['EVEREST'] = (mastio.EverestArchive(), everestParser, "Everest")
    dTypeDict['SFF'] = (mastio.VanderburgArchive(), sffParser,
                        "Vanderburg SFF")

    out = dpc.Clipboard()

    #Load the TPF data cube
    ar = mastio.K2Archive(dataStorePath)
    fits, hdr = ar.getLongTpf(epic, campaign, header=True, mmap=False)
    hdr0 = ar.getLongTpf(epic, campaign, ext=0, mmap=False)
    cube = tpf.getTargetPixelArrayFromFits(fits, hdr)

    out['time'] = fits['TIME']
    out['cube'] = cube
    out['tpfHeader'] = hdr
    out['tpfHeader0'] = hdr0

    #Load PA data
    fits = ar.getLongCadence(epic, campaign)
    out['rawFlux'] = fits['SAP_FLUX']

    #Load lightcurves from a specific detrending, and replace
    #the pdc time series with the new detrending
    nDetrend = 0
    for i, dType in enumerate(detrendTypes):
        key = dType.upper()
        if key not in dTypeDict:
            raise IOError("Unrecognised detrended %s" % (key))

        ar, parser, label = dTypeDict[key]

        data = ar.getLongCadence(epic, campaign)
        flux = parser(out['time'], data)

        typeName = "type%i" % (i + 1)
        out[typeName] = key
        fluxName = "flux%i" % (i + 1)
        out[fluxName] = flux
        labelName = "label%i" % (i + 1)
        out[labelName] = label

        nDetrend += 1

    out['numDetrendings'] = nDetrend

    #Enforce contract
    out['flux1']
    out['label1']
    out['cube']

    return out
Esempio n. 2
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def getData(epic, campaign):
    ar = mastio.K2Archive()
    fits, hdr = ar.getLongTpf(epic, campaign, header=True)
    cube = tpf.getTargetPixelArrayFromFits(fits, hdr)

    # get the thruster firing indeces
    q = fits['QUALITY'].astype(np.uint32)
    idx1 = q & kplrfits.SapQuality['DefiniteRollTweak']
    idx2 = q & kplrfits.SapQuality['MomDump']
    idx3 = idx1 + idx2

    return cube, idx3
Esempio n. 3
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def serveTask(clip):
    k2id = clip['value']
    campaign = clip['config.campaign']
    storeDir = clip['config.dataStorePath']
    detrendType = clip.get('config.detrendType', 'PDC')

    ar = mastio.K2Archive(storeDir)
    clip['serve'] = loadTpfAndLc(k2id, campaign, ar, detrendType)

    #Enforce contract. (Make sure expected keys are in place)
    clip['serve.time']
    clip['serve.cube']
    clip['serve.socData']
    clip['serve.tpfHeader']
    return clip
Esempio n. 4
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def exampleDiffImgCentroiding():
    k2id = 206103150
    campaign = 3

    ar = mastio.K2Archive()
    fits, hdr = ar.getLongTpf(k2id, campaign, header=True)
    hdr0 = ar.getLongTpf(k2id, campaign, ext=0)
    cube = tpf.getTargetPixelArrayFromFits(fits, hdr)
    idx = np.isfinite(cube)
    cube[~idx] = 0  #Remove Nans

    flags = fits['QUALITY']
    ccdMod = hdr0['module']
    ccdOut = hdr0['output']

    #Compute roll phase
    llc = ar.getLongCadence(k2id, campaign)
    time = llc['TIME']
    cent1 = llc['MOM_CENTR1']
    cent2 = llc['MOM_CENTR2']
    centColRow = np.vstack((cent1, cent2)).transpose()
    rot = arclen.computeArcLength(centColRow, flags > 0)
    rollPhase = rot[:, 0]
    rollPhase[flags > 0] = -9999  #A bad value

    prfObj = prf.KeplerPrf("/home/fergal/data/keplerprf")
    bbox = getBoundingBoxForImage(cube[0], hdr)

    period = 4.1591409
    epoch = fits['time'][491]
    dur = 3.0

    out, log = measureDiffOffset(period, epoch, dur, time, prfObj, \
        ccdMod, ccdOut, cube, bbox, rollPhase, flags)

    idx = out[:, 1] > 0
    mp.clf()
    mp.plot(out[:, 3] - out[:, 1], out[:, 4] - out[:, 2], 'ro')
    return out
Esempio n. 5
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def getData(epic, campaign):
    """Obtains the data for the star

    For a particular star, this obtains its pixel time series data cube as well
    as time points which may be bad due to thruster firings.


    Inputs:
    ----------
    epic
        (int) The k2 epic number for the desired star
    campaign
        (int) The k2 campaign for the desired star

    Returns:
    ------------
    cube
        (3d numpy array) The k2 pixel time series data for the star with 
        dimensions (time, number of rows per cadence, number of columns per 
        cadence)
    badIdx
        (1d boolean numpy array) Boolean array with true corresponding to a bad
        time point due to thruster firings
    """

    ar = mastio.K2Archive()
    fits, hdr = ar.getLongTpf(epic, campaign, header=True)
    cube = tpf.getTargetPixelArrayFromFits(fits, hdr)

    # get the thruster firing indeces
    q = fits['QUALITY'].astype(np.uint32)
    rollTweakIdx = q & kplrfits.SapQuality['DefiniteRollTweak']
    momDumpIdx = q & kplrfits.SapQuality['MomDump']
    badIdx = rollTweakIdx | momDumpIdx
    badIdx = badIdx.astype(bool)
    return cube, badIdx
Esempio n. 6
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def example():
    ar = mastio.K2Archive()

    kepid = 206103150  #A wasp planet

    fits = ar.getLongCadence(kepid, 3)
    flags = fits['SAP_QUALITY']
    cent1 = fits['MOM_CENTR1']
    cent2 = fits['MOM_CENTR2']

    fits, hdr = ar.getLongTpf(kepid, 3, header=True)
    cube = tpf.getTargetPixelArrayFromFits(fits, hdr)
    #    cube *= gain

    #Compute roll phase
    centColRow = np.vstack((cent1, cent2)).transpose()
    rot = arclen.computeArcLength(centColRow, flags > 0)
    rollPhase = rot[:, 0]
    rollPhase[flags > 0] = -9999  #A bad value

    cadenceInTransit = 490
    diff, oot = constructK2DifferenceImage(cube, cadenceInTransit, rollPhase,
                                           flags)
    return diff, oot