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III/175 Optical spectroscopy of radio sources (Stickel+, 1989-94)
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Optical spectroscopy of 1Jy, S4 and S5 radio source identifications
STICKEL M., KUEHR H., FRIED J.W.
=1989A&AS...80..103S
=1993A&AS...97..483S
=1993A&AS..100..395S
=1993A&AS..101..521S
=1994A&AS..103..349S
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ADC_Keywords: Radio sources ; Active gal. nuclei ; QSOs ; Redshifts
Keywords: galaxies: active - quasars: emission lines - radio continuum: galaxies
radio continuum: general
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table1 126 114 Observed radio source identifications
table2 58 115 Journal of the observations
table3 68 510 Line data
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See also:
J/A+AS/98/393 (II-Observational data)
J/A+AS/105/67 (Optical identifications from 1Jy, S4, S5)
J/A+AS/105/211 (Optical identification of 1Jy)
J/A+AS/115/1 (Optical identifications from S5 catalog)
J/A+AS/115/11 (Optical identifications from 1Jy, S4, S5)
Byte-per-byte Description of file: table1
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Bytes Format Units Label Explanations
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2- 9 A8 --- Object Object name
12- 13 I2 h RAh Right Ascension 1950 (hours)
15- 16 I2 min RAm Right Ascension 1950 (minutes)
18- 22 F5.2 s RAs Right Ascension 1950 (seconds)
24 A1 --- DE- Declination 1950 (sign)
25- 26 I2 deg DEd Declination 1950 (degrees)
28- 29 I2 arcmin DEm Declination 1950 (minutes)
31- 34 F4.1 arcsec DEs Declination 1950 (seconds)
37- 40 F4.1 mag m Magnitude of the optical identification
42- 48 A7 --- Type Type of the optical identification
50- 54 F5.3 Jy S5GHz 5GHz flux
56- 60 F5.2 --- s(11-6) Two-point spectral index between 11 and 6 cm
64-126 A63 --- Names Entries in other radio sources catalogues
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Byte-per-byte Description of file: table2
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Bytes Format Units Label Explanations
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3- 10 A8 --- Object Object name
13- 18 A6 --- Tel Telescope (1)
21- 41 A21 --- Date Observation date
43- 47 I5 s IntTime Total integration time
50- 53 F4.1 0.1nm/pix Scale Scale of the wavelength calibrated spectra.
55- 58 F4.1 0.1nm/pix Scale2 []? Scale in in red channel for Twin
Spectrograph
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Note (1): Telescopes:
CA 3.5 = 3.5 m telescope on Calar Alto, Spain
CA 2.2 = 2.2 m telescope on Calar Alto, Spain
LS 2.2 = 2.2 m telescope on La Silla, Chile
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Byte-per-byte Description of file: table3
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Bytes Format Units Label Explanations
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3- 10 A8 --- Object Object name
13 A1 --- l_z ">" sign for lower redshift limit
14- 18 F5.3 --- z []? Redshift computed from unweighted zInd
20- 27 A8 --- Element Element identification
29- 32 I4 0.1nm Lam0 []? Rest wavelength
33 A1 --- u_Lam0 [?] ? when unknown
34- 37 I4 0.1nm LamObs Observed wavelength
39- 43 F5.3 --- zInd []? Individual redshift
44 A1 --- u_zInd [?] ? when unknown
45- 49 F5.1 0.1nm FWHM []? FWHM (for emission line)
52- 56 F5.1 0.1nm EW []? Equivalent width (for emission line)
57 A1 --- u_EW ":" sign indicating uncertain values
58- 63 F6.1 10-19W/m2 Flux []? Flux (10-16erg/s/cm2)
64 A1 --- u_Flux ":" sign indicating uncertain values
66- 68 A3 --- Rem Remarks (1)
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Note (1): gal = stellar absorption lines of host galaxy
abs = intervening absorption lines
cal = calibration uncertain due to second order contamination
atm = emission lines affected by atmospheric absorption
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Courtesy: Manfred Stickel
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(End) Patricia Bauer [CDS] 25-Nov-1994
J/A+AS/115/11 Optical identifications of radio sources (Stickel+, 1996)
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Optical identifications of radio sources from the 1 Jy, S4 and S5 catalogues
Stickel H., Kuehr M.
=1996A&AS..115...11S (SIMBAD/NED BibCode)
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ADC_Keywords: Radio sources ; Active gal. nuclei ; QSOs ; Redshifts
Keywords: catalogs - surveys - galaxies: active - quasars: general -
radio continuum: general
Description:
CCD images of the fields of 115 radio sources from the 1Jy, S4 and S5
catalogues are presented. New optical counterparts have been found for
a total of 34 sources, a large fraction of which had as yet only been
described as empty fields on Sky Survey Plates. Of the 54 radio
sources with previously published identifications, 50 optical
counterparts have been confirmed while for 4 sources new
identifications are proposed. R band magnitudes, derived from the CCD
images, are provided for all but a few identified optical
counterparts. The fields at the positions of 27 radio sources are
still empty down to a limiting magnitude of at least m_R_=22mag,
requiring much deeper optical as well as additional infrared images
for establishing their optical counterparts.
See also:
Catalogue III/175 (gathers papers I-V)
J/A+AS/80/103 (I)
J/A+AS/97/483 (II)
J/A+AS/98/393 (II-Observational data)
J/A+AS/100/395 (III)
J/A+AS/101/521 (IV)
J/A+AS/103/349 (Update of optical identifications)
J/A+AS/105/67 (Optical identifications from 1Jy, S4, S5)
J/A+AS/105/211 (Optical identification of 1Jy)
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table1 68 27 Observed 1 Jy Radio Sources
table2 68 21 Observed S4 Radio Sources
table3 68 67 Observed S5 Radio Sources
table4 42 27 Journal of 1 Jy Observations
table5 42 21 Journal of S4 Observations
table6 42 67 Journal of S5 Observations
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Byte-by-byte Description of file: table1 table2 table3
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Bytes Format Units Label Explanations
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2- 9 A8 --- Name Source name
11- 12 I2 h RAh Right ascension of the radio source (1950)
14- 15 I2 min RAm Right ascension of the radio source (1950)
17- 21 F5.2 s RAs Right ascension of the radio source (1950)
23 A1 --- DE- Declination sign
24- 25 I2 deg DEd Declination of the radio source (1950)
27- 28 I2 arcmin DEm Declination of the radio source (1950)
30- 33 F4.1 arcsec DEs Declination of the radio source (1950)
35- 37 A3 --- RefPos Reference to the radio position (1)
39- 42 F4.1 mag Bright ? Brightness of the optical counterpart
44- 49 A6 --- SouType Source type
51- 56 F6.4 --- z ? Redshift
58- 62 F5.3 Jy S5GHz Radio flux density S_5GHz_
64- 68 F5.2 --- SpIndex Radio spectral index between 11 cm and 6 cm
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Note (1): AC White (1992)
BV Vigotti et al. (1989)
D Pearson and Readhead (1988)
EK Ekers et al. (1989)
FY1 Fey et al. (1992)
FY2 Fey et al. (1994)
J Kuehr et al. (1981)
K Kapahi (1981)
M1 Morabito et al. (1982)
M2 Morabito et al. (1983)
M3 Morabito et al. (1985)
M4 Morabito et al. (1986)
MK Morganti et al. (1993)
P Perley (1982)
PA Patnaik et al. (1992)
RO Robertson et al. (1993)
RU2 Russell et al. (1994)
S4 Pauliny-Toth et al. (1978)
S5 Kuehr et al. (1987)
U Ulvestad et al. (1981)
VLA VLA Calibrator position
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Byte-by-byte Description of file: table4 table5 table6
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Bytes Format Units Label Explanations
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2- 9 A8 --- Name Source name
11- 23 A13 --- Date Date of observation
25- 28 A4 --- Telescope Telescope used for the observation
30- 33 I4 s Time Total integration time
35- 37 F3.1 arcsec Seeing Estimate of the seeing during the
observation
39- 42 F4.2 arcsec/pix Scale Scale of the CCD image
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References:
Ekers R.D. et al. 1989, MNRAS 236, 737 =1989MNRAS.236..737E
Fey A.L. et al. 1992, AJ 104, 891 =1992AJ....104..891F
Fey A.L. et al. 1994, AJ 107, 385 =1994AJ....107..385F
Kapahi V.K. 1981, A&AS 43, 381 =1981A&AS...43..381K
Kuehr H. et al. 1981, A&AS 45, 367 =1981A&AS...45..367K
Kuehr H. et al. 1987, A&AS 71, 493 =1987A&AS...71..493K
Morabito D.D. et al. 1982, AJ 87, 517 =1982AJ.....87..517M
Morabito D.D. et al. 1983, AJ 88, 1138 =1982AJ.....87..517M
Morabito D.D. et al. 1985, AJ 90, 590 =1985AJ.....90..590M
Morabito D.D. et al. 1986, AJ 92, 546 =1986AJ.....92..546M
Morganti D.D. et al. 1993, MNRAS 263, 1023 =1993MNRAS.263.1023M
Patnaik A.R. et al. 1992, MNRAS 254, 655 =1992MNRAS.254..655P
Pauliny-Toth I.I.K. et al. 1978, AJ 83, 451 =1978AJ.....83..451P
Pearson T.J. and Readhead A.C.S. 1988, ApJ 328, 114 =1988ApJ...328..114P
Perley R.A. 1982, AJ 87, 859 =1982AJ.....87..859P
Robertson D.S. et al. 1993, AJ 105, 353 =1993AJ....105..353R
Russell J.L. et al. 1994, AJ 107, 379 =1994AJ....107..379R
Ulvestad J. et al. 1981, AJ 86, 1010 =1981AJ.....86.1010U
Vigotti M. et al. 1989, AJ 98, 419 =1989AJ.....98..419V
White G.L. 1992, Proc. Astron. Soc. Australia 10,140 =1992PASAu..10..140W
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(End) Simona Mei [CDS] 06-Sep-1995