Commit 9b146a2e authored by Wei Shoulin's avatar Wei Shoulin
Browse files

add columns

parent 7ca3a10e
......@@ -18,12 +18,13 @@ class CatalogApi(object):
def __init__(self):
self.stub = ephem_pb2_grpc.EphemSearchSrvStub(ServiceProxy().channel())
def gaia3_query(self, ra: float, dec: float, radius: float, min_mag: float, max_mag: float, obstime: int, limit: int):
def gaia3_query(self, ra: float, dec: float, radius: float, columns: tuple, min_mag: float, max_mag: float, obstime: int, limit: int):
''' retrieval GAIA DR 3
args:
ra: in deg
dec: in deg
radius: in deg
tuple of str, like ('ra','dec','phot_g_mean_mag')
min_mag: minimal magnitude
max_mag: maximal magnitude
obstime: seconds
......@@ -38,6 +39,7 @@ class CatalogApi(object):
ra = ra,
dec = dec,
radius = radius,
columns = ",".join(columns),
minMag = min_mag,
maxMag = max_mag,
obstime = obstime,
......@@ -55,169 +57,7 @@ class CatalogApi(object):
t_start = time.time()
records = pickle.loads(datas.getvalue())
log.info("unserialization used: %.6f's" %(time.time() - t_start,))
t_start = time.time()
ret_records2 = []
for r in records:
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)
log.info("to object list used: %.6f's" %(time.time() - t_start,))
return Result.ok_data(data = ret_records2).append("totalCount", totalCount)
return Result.ok_data(data = records).append("totalCount", totalCount).append("columns", columns)
except grpc.RpcError as e:
return Result.error(message="%s:%s" % (e.code().value, e.details()))
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