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J/AJ/136/181 Spectroscopy of PC 1643+4631A,B (Casey+, 2008)
PC 1643+4631A,B: the Lyman-α forest at the edge of coherence. Casey C.M., Impey C.D., Petry C.E., Marble A.R., Dave R. <Astron. J., 136, 181-196 (2008)> =2008AJ....136..181C
ADC_Keywords: QSOs ; Spectroscopy ; Equivalent widths ; Redshifts Keywords: cosmology: observations - intergalactic medium - quasars: absorption lines - quasars: individual (PC 1643+4631A, B) Abstract: This is the first measurement and detection of coherence in the intergalactic medium (IGM) at substantially high redshift (z∼3.8) and on large physical scales (∼2.5h-170Mpc). We perform the measurement by presenting new observations of the high-redshift quasar pair PC 1643+4631A, B and their Lyα-absorber coincidences. With data collected from Keck I Low Resolution Imaging Spectrometer (LRIS) in a 10200s integration, we have full coverage of the Lyα forest over the redshift range 2.6<z<3.8 at a resolution of 3.6Å (∼220km/s). Description: All data for this project were obtained with the Keck I Low Resolution Imaging Spectrometer (LRIS) on 2001 July 21 and were reduced using the standard IRAF longslit-spectra pipeline. To cover the wavelength range of scientific interest, only the red side of the spectrograph and the 900/5500 grating was used. Objects: ------------------------------------------------------- RA (2000) DE Designation(s) ------------------------------------------------------- 16 45 00.7 +46 26 13 PC 1643+4631A = QSO B1643+465A 16 45 19.6 +46 25 38 PC 1643+4631B = QSO B1643+465B ------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 28 4104 Flux and continuum of PC 1643+4631 A,B table2.dat 68 240 Absorption lines for PC 1643+4631A table3.dat 68 234 Absorption lines for PC 1643+4631B table4.dat 45 152 Symmetrically matched Lyα lines
Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1 A1 --- Comp [AB] Component of PC1643+4631 3- 8 F6.1 0.1nm lambda Wavelength in Angstroms (Å) 10- 15 F6.3 10-19W/m2/nm Flux Flux density (1) 17- 21 F5.3 10-19W/m2/nm e_Flux Error in Flux (1) 23- 28 F6.3 10-19W/m2/nm CFlux Continuum flux density (1)
Note (1): In units of 10-17ergs/s/cm2/Å.
Byte-by-byte Description of file: table[23].dat
Bytes Format Units Label Explanations
1- 3 I3 --- Line Line identification number 5- 11 F7.2 0.1nm lambda Central wavelength in Angstroms (Å) 13- 16 F4.2 0.1nm e_lambda Uncertainty in lambda in Angstroms (Å) 18- 21 F4.2 0.1nm Wobs Equivalent width in Angstroms (Å) 23- 26 F4.2 0.1nm e_Wobs Uncertainty in Wobs in Angstroms (Å) 28- 32 F5.2 --- chi Reduced χ^2^ value (1) 34- 38 F5.2 --- Sfit Equivalent width significance (2) 40- 45 F6.2 --- Sdet Detection limit significance (3) 47- 52 F6.4 --- z ? Redshift of absorber 54- 56 A3 --- f_z [a-f ,] Flag on line (4) 58- 68 A11 --- n_z Notes on line
Note (1): If this value is identical to that of an adjacent line, it indicates that the lines were fitted simultaneously. Note (2): Defined as Wobs/σfit, where σfit is the error in the equivalent width. Note (3): Defined as Wobs/σdet, where σdet is the detection limit of the data at λ (see text for further details). Note (4): Flags as follows: a = line included in the Lyα sample b = line associated with the opaque system at z=3.777 that is also labeled by its associated identification c = line redward of Lyα emission which is clearly excluded from the Lyα sample d = line fitted in the damped region at z=3.818 e = line associated with the opaque system at z=3.818 that is also labeled by its associated identification f = the blended line removed due to low significance
Byte-by-byte Description of file: table4.dat
Bytes Format Units Label Explanations
1- 3 I3 --- Match Symmetrically matched pair number 5- 11 F7.2 0.1nm Alambda Wavelength in spectrum A (in Å) 13- 19 F7.2 0.1nm Blambda Wavelength in spectrum B (in Å) 21- 24 F4.2 0.1nm Dlambda Wavelength separation of pair (in Å) 26- 30 F5.1 km/s dVel Velocity difference of pair 32- 35 F4.2 0.1nm W0A Rest equivalent width in spectrum A (in Å) 37- 40 F4.2 0.1nm W0B Rest equivalent width in spectrum B (in Å) 42- 45 F4.2 0.1nm dW0 Difference in rest equivalent widths (in Å)
History: From electronic version of the journal
(End) Greg Schwarz [AAS], Patricia Vannier [CDS] 21-Jan-2011
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