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J/MNRAS/266/317      Quasars in ESO/SERC field 927               (Clowes+, 1994)

Observations of quasars in ESO/SERC field 927 CLOWES R.G., CAMPUSANO L.E. <Mon. Not. R. Astron. Soc. 266, 317 (1994)> =1994MNRAS.266..317C (SIMBAD/NED Reference)
ADC_Keywords: Regional catalog; QSOs; Spectroscopy; Positional data; Magnitudes; Redshifts; Equivalent widths Keywords: galaxies: clustering - quasars: absorption lines - quasars: emission lines - quasars: general - large-scale structure of Universe. Abstract: We present the spectroscopic observations of 56 quasars that were discovered by AQD (Automated Quasar Detection) in a field of ∼25.3deg2, centred at (1950) RA l0h40m00s, Dec. 05deg00'00". These observations, with the CTIO 4-m telescope, led to the discovery by Clowes & Campusano of a large group of quasars with size ∼100-200h-1Mpc at z∼1.3. Quasars of particular interest are noted, including one that is a BAL quasar with z∼1.78. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1 113 56 A summary of the observations of the 56 candidates that were confirmed as quasars.
Byte-by-byte Description of file: table1
Bytes Format Units Label Explanations
2- 3 I2 h RAh Right ascension (1950) 5- 6 I2 min RAm Right ascension (1950) 8- 11 F4.1 s RAs Right ascension (1950) 13- 14 I2 deg DEd Declination (1950) 16- 17 I2 arcmin DEm Declination (1950) 19- 20 I2 arcsec DEs Declination (1950) 22- 23 I2 h RA2000h Right ascension (2000) 25- 26 I2 min RA2000m Right ascension (2000) 28- 31 F4.1 s RA2000s Right ascension (2000) 32 A1 --- DE2000- Declination sign 33- 34 I2 deg DE2000d Declination (2000) 36- 37 I2 arcmin DE2000m Declination (2000) 39- 40 I2 arcsec DE2000s Declination (2000) 42- 55 A14 --- Date Date of observation 57- 60 I4 s Int Integration time 62 A1 --- Band [SW] Band (1) 64- 68 F5.2 mag Bj []? Bj magnitude 70- 74 F5.3 --- z redshift 76- 78 I3 0.1nm EW Equivalent width 81 I1 --- n_EW Note on equivalent width (2) 84-113 A30 --- Com Comments
Note (1): 'S' for strong-lined, 'W' for weak-lined Note (2): Identification of strongest emission lines: (1) Ly-alpha lambda 1216 +Nv lambda 1240; (2) C IV lambda 1549; (3) C III lambda 1909; (4) Mg II lambda 2798.
References: Clowes R.G., Campusano L.E., 1991, MNRAS, 249, 218 Historical Notes: Keypunched at CDS
(End) James Marcout, Patricia Bauer [CDS] 14-Feb-1995
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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