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Commit 2d128fe8 authored by Wei Shoulin's avatar Wei Shoulin
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parent 7eb699f1
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csst_dfs_api_cluster/common/catalog.py
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......@@ -28,7 +28,7 @@ class CatalogApi(object):
return: csst_dfs_common.models.Result
'''
try:
datas = bytearray()
datas = b''
totalCount = 0
for resp in self.stub.Gaia3Search(ephem_pb2.EphemSearchRequest(
ra = ra,
......@@ -41,8 +41,7 @@ class CatalogApi(object):
),metadata = get_auth_headers()):
if resp.success:
# data = from_proto_model_list(Gaia3Record, resp.records)
data = resp.records
datas.extend(data)
datas = datas + resp.records
totalCount = resp.totalCount
else:
return Result.error(message = str(resp.error.detail))
......@@ -50,164 +49,164 @@ class CatalogApi(object):
records = pickle.loads(datas)
ret_records2 = []
for r in records:
rec = Gaia3Record(
SolutionId = r[0],
Designation = r[1],
SourceId = r[2],
RandomIndex = r[3],
RefEpoch = r[4],
Ra = r[5],
RaError = r[6],
Dec = r[7],
DecError = r[8],
Parallax = r[9],
ParallaxError = r[10],
ParallaxOverError = r[11],
Pm = r[12],
Pmra = r[13],
PmraError = r[14],
Pmdec = r[15],
PmdecError = r[16],
RaDecCorr = r[17],
RaParallaxCorr = r[18],
RaPmraCorr = r[19],
RaPmdecCorr = r[20],
DecParallaxCorr = r[21],
DecPmraCorr = r[22],
DecPmdecCorr = r[23],
ParallaxPmraCorr = r[24],
ParallaxPmdecCorr = r[25],
PmraPmdecCorr = r[26],
AstrometricNObsAl = r[27],
AstrometricNObsAc = r[28],
AstrometricNGoodObsAl = r[29],
AstrometricNBadObsAl = r[30],
AstrometricGofAl = r[31],
AstrometricChi2Al = r[32],
AstrometricExcessNoise = r[33],
AstrometricExcessNoiseSig = r[34],
AstrometricParamsSolved = r[35],
AstrometricPrimaryFlag = r[36],
NuEffUsedInAstrometry = r[37],
Pseudocolour = r[38],
PseudocolourError = r[39],
RaPseudocolourCorr = r[40],
DecPseudocolourCorr = r[41],
ParallaxPseudocolourCorr = r[42],
PmraPseudocolourCorr = r[43],
PmdecPseudocolourCorr = r[44],
AstrometricMatchedTransits = r[45],
VisibilityPeriodsUsed = r[46],
AstrometricSigma5dMax = r[47],
MatchedTransits = r[48],
NewMatchedTransits = r[49],
MatchedTransitsRemoved = r[50],
IpdGofHarmonicAmplitude = r[51],
IpdGofHarmonicPhase = r[52],
IpdFracMultiPeak = r[53],
IpdFracOddWin = r[54],
Ruwe = r[55],
ScanDirectionStrengthK1 = r[56],
ScanDirectionStrengthK2 = r[57],
ScanDirectionStrengthK3 = r[58],
ScanDirectionStrengthK4 = r[59],
ScanDirectionMeanK1 = r[60],
ScanDirectionMeanK2 = r[61],
ScanDirectionMeanK3 = r[62],
ScanDirectionMeanK4 = r[63],
DuplicatedSource = r[64],
PhotGNObs = r[65],
PhotGMeanFlux = r[66],
PhotGMeanFluxError = r[67],
PhotGMeanFluxOverError = r[68],
PhotGMeanMag = r[69],
PhotBpNObs = r[70],
PhotBpMeanFlux = r[71],
PhotBpMeanFluxError = r[72],
PhotBpMeanFluxOverError = r[73],
PhotBpMeanMag = r[74],
PhotRpNObs = r[75],
PhotRpMeanFlux = r[76],
PhotRpMeanFluxError = r[77],
PhotRpMeanFluxOverError = r[78],
PhotRpMeanMag = r[79],
PhotBpRpExcessFactor = r[80],
PhotBpNContaminatedTransits = r[81],
PhotBpNBlendedTransits = r[82],
PhotRpNContaminatedTransits = r[83],
PhotRpNBlendedTransits = r[84],
PhotProcMode = r[85],
BpRp = r[86],
BpG = r[87],
GRp = r[88],
RadialVelocity = r[89],
RadialVelocityError = r[90],
RvMethodUsed = r[91],
RvNbTransits = r[92],
RvNbDeblendedTransits = r[93],
RvVisibilityPeriodsUsed = r[94],
RvExpectedSigToNoise = r[95],
RvRenormalisedGof = r[96],
RvChisqPvalue = r[97],
RvTimeDuration = r[98],
RvAmplitudeRobust = r[99],
RvTemplateTeff = r[100],
RvTemplateLogg = r[101],
RvTemplateFeH = r[102],
RvAtmParamOrigin = r[103],
Vbroad = r[104],
VbroadError = r[105],
VbroadNbTransits = r[106],
GrvsMag = r[107],
GrvsMagError = r[108],
GrvsMagNbTransits = r[109],
RvsSpecSigToNoise = r[110],
PhotVariableFlag = r[111],
L = r[112],
B = r[113],
EclLon = r[114],
EclLat = r[115],
InQsoCandidates = r[116],
InGalaxyCandidates = r[117],
NonSingleStar = r[118],
HasXpContinuous = r[119],
HasXpSampled = r[120],
HasRvs = r[121],
HasEpochPhotometry = r[122],
HasEpochRv = r[123],
HasMcmcGspphot = r[124],
HasMcmcMsc = r[125],
InAndromedaSurvey = r[126],
ClassprobDscCombmodQuasar = r[127],
ClassprobDscCombmodGalaxy = r[128],
ClassprobDscCombmodStar = r[129],
TeffGspphot = r[130],
TeffGspphotLower = r[131],
TeffGspphotUpper = r[132],
LoggGspphot = r[133],
LoggGspphotLower = r[134],
LoggGspphotUpper = r[135],
MhGspphot = r[136],
MhGspphotLower = r[137],
MhGspphotUpper = r[138],
DistanceGspphot = r[139],
DistanceGspphotLower = r[140],
DistanceGspphotUpper = r[141],
AzeroGspphot = r[142],
AzeroGspphotLower = r[143],
AzeroGspphotUpper = r[144],
AgGspphot = r[145],
AgGspphotLower = r[146],
AgGspphotUpper = r[147],
EbpminrpGspphot = r[148],
EbpminrpGspphotLower = r[149],
EbpminrpGspphotUpper = r[150],
LibnameGspphot = r[151],
NS8HIdx = r[152],
NS16HIdx = r[153],
NS32HIdx = r[154],
NS64HIdx = r[155],
FileIdx = r[156])
rec = Gaia3Record()
rec.SolutionId = r[0]
rec.Designation = r[1]
rec.SourceId = r[2]
rec.RandomIndex = r[3]
rec.RefEpoch = r[4]
rec.Ra = r[5]
rec.RaError = r[6]
rec.Dec = r[7]
rec.DecError = r[8]
rec.Parallax = r[9]
rec.ParallaxError = r[10]
rec.ParallaxOverError = r[11]
rec.Pm = r[12]
rec.Pmra = r[13]
rec.PmraError = r[14]
rec.Pmdec = r[15]
rec.PmdecError = r[16]
rec.RaDecCorr = r[17]
rec.RaParallaxCorr = r[18]
rec.RaPmraCorr = r[19]
rec.RaPmdecCorr = r[20]
rec.DecParallaxCorr = r[21]
rec.DecPmraCorr = r[22]
rec.DecPmdecCorr = r[23]
rec.ParallaxPmraCorr = r[24]
rec.ParallaxPmdecCorr = r[25]
rec.PmraPmdecCorr = r[26]
rec.AstrometricNObsAl = r[27]
rec.AstrometricNObsAc = r[28]
rec.AstrometricNGoodObsAl = r[29]
rec.AstrometricNBadObsAl = r[30]
rec.AstrometricGofAl = r[31]
rec.AstrometricChi2Al = r[32]
rec.AstrometricExcessNoise = r[33]
rec.AstrometricExcessNoiseSig = r[34]
rec.AstrometricParamsSolved = r[35]
rec.AstrometricPrimaryFlag = r[36]
rec.NuEffUsedInAstrometry = r[37]
rec.Pseudocolour = r[38]
rec.PseudocolourError = r[39]
rec.RaPseudocolourCorr = r[40]
rec.DecPseudocolourCorr = r[41]
rec.ParallaxPseudocolourCorr = r[42]
rec.PmraPseudocolourCorr = r[43]
rec.PmdecPseudocolourCorr = r[44]
rec.AstrometricMatchedTransits = r[45]
rec.VisibilityPeriodsUsed = r[46]
rec.AstrometricSigma5dMax = r[47]
rec.MatchedTransits = r[48]
rec.NewMatchedTransits = r[49]
rec.MatchedTransitsRemoved = r[50]
rec.IpdGofHarmonicAmplitude = r[51]
rec.IpdGofHarmonicPhase = r[52]
rec.IpdFracMultiPeak = r[53]
rec.IpdFracOddWin = r[54]
rec.Ruwe = r[55]
rec.ScanDirectionStrengthK1 = r[56]
rec.ScanDirectionStrengthK2 = r[57]
rec.ScanDirectionStrengthK3 = r[58]
rec.ScanDirectionStrengthK4 = r[59]
rec.ScanDirectionMeanK1 = r[60]
rec.ScanDirectionMeanK2 = r[61]
rec.ScanDirectionMeanK3 = r[62]
rec.ScanDirectionMeanK4 = r[63]
rec.DuplicatedSource = r[64]
rec.PhotGNObs = r[65]
rec.PhotGMeanFlux = r[66]
rec.PhotGMeanFluxError = r[67]
rec.PhotGMeanFluxOverError = r[68]
rec.PhotGMeanMag = r[69]
rec.PhotBpNObs = r[70]
rec.PhotBpMeanFlux = r[71]
rec.PhotBpMeanFluxError = r[72]
rec.PhotBpMeanFluxOverError = r[73]
rec.PhotBpMeanMag = r[74]
rec.PhotRpNObs = r[75]
rec.PhotRpMeanFlux = r[76]
rec.PhotRpMeanFluxError = r[77]
rec.PhotRpMeanFluxOverError = r[78]
rec.PhotRpMeanMag = r[79]
rec.PhotBpRpExcessFactor = r[80]
rec.PhotBpNContaminatedTransits = r[81]
rec.PhotBpNBlendedTransits = r[82]
rec.PhotRpNContaminatedTransits = r[83]
rec.PhotRpNBlendedTransits = r[84]
rec.PhotProcMode = r[85]
rec.BpRp = r[86]
rec.BpG = r[87]
rec.GRp = r[88]
rec.RadialVelocity = r[89]
rec.RadialVelocityError = r[90]
rec.RvMethodUsed = r[91]
rec.RvNbTransits = r[92]
rec.RvNbDeblendedTransits = r[93]
rec.RvVisibilityPeriodsUsed = r[94]
rec.RvExpectedSigToNoise = r[95]
rec.RvRenormalisedGof = r[96]
rec.RvChisqPvalue = r[97]
rec.RvTimeDuration = r[98]
rec.RvAmplitudeRobust = r[99]
rec.RvTemplateTeff = r[100]
rec.RvTemplateLogg = r[101]
rec.RvTemplateFeH = r[102]
rec.RvAtmParamOrigin = r[103]
rec.Vbroad = r[104]
rec.VbroadError = r[105]
rec.VbroadNbTransits = r[106]
rec.GrvsMag = r[107]
rec.GrvsMagError = r[108]
rec.GrvsMagNbTransits = r[109]
rec.RvsSpecSigToNoise = r[110]
rec.PhotVariableFlag = r[111]
rec.L = r[112]
rec.B = r[113]
rec.EclLon = r[114]
rec.EclLat = r[115]
rec.InQsoCandidates = r[116]
rec.InGalaxyCandidates = r[117]
rec.NonSingleStar = r[118]
rec.HasXpContinuous = r[119]
rec.HasXpSampled = r[120]
rec.HasRvs = r[121]
rec.HasEpochPhotometry = r[122]
rec.HasEpochRv = r[123]
rec.HasMcmcGspphot = r[124]
rec.HasMcmcMsc = r[125]
rec.InAndromedaSurvey = r[126]
rec.ClassprobDscCombmodQuasar = r[127]
rec.ClassprobDscCombmodGalaxy = r[128]
rec.ClassprobDscCombmodStar = r[129]
rec.TeffGspphot = r[130]
rec.TeffGspphotLower = r[131]
rec.TeffGspphotUpper = r[132]
rec.LoggGspphot = r[133]
rec.LoggGspphotLower = r[134]
rec.LoggGspphotUpper = r[135]
rec.MhGspphot = r[136]
rec.MhGspphotLower = r[137]
rec.MhGspphotUpper = r[138]
rec.DistanceGspphot = r[139]
rec.DistanceGspphotLower = r[140]
rec.DistanceGspphotUpper = r[141]
rec.AzeroGspphot = r[142]
rec.AzeroGspphotLower = r[143]
rec.AzeroGspphotUpper = r[144]
rec.AgGspphot = r[145]
rec.AgGspphotLower = r[146]
rec.AgGspphotUpper = r[147]
rec.EbpminrpGspphot = r[148]
rec.EbpminrpGspphotLower = r[149]
rec.EbpminrpGspphotUpper = r[150]
rec.LibnameGspphot = r[151]
rec.NS8HIdx = r[152]
rec.NS16HIdx = r[153]
rec.NS32HIdx = r[154]
rec.NS64HIdx = r[155]
rec.FileIdx = r[156]
ret_records2.append(rec)
return Result.ok_data(data = ret_records2).append("totalCount", totalCount)
......
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