J/AN/333/706     Bochum survey of the southern Galactic disk       (Haas+, 2012)

The Bochum survey of the southern Galactic disk: I. Survey design and first results on 50 square degrees monitored in 2011. Haas M., Hackstein M., Ramolla M., Drass H., Watermann R., Lemke R., Chini R. <Astron. Nachrichten, 333, 706-716 (2012)> =2012AN....333..706H 2012AN....333..706H
ADC_Keywords: Surveys ; Stars, variable ; Photometry Keywords: surveys - stars: variables: general Abstract: We are monitoring a 6° wide stripe along the southern Galactic disk simultaneously in the r and i bands, using a robotic 15-cm twin telescope of the Universitatsternwarte Bochum near Cerro Armazones in Chile. Utilising the telescope's 2.7° field of view, the survey aims at observing a mosaic of 268 fields once per month and to monitor dedicated fields once per night. The survey reaches a sensitivity from 10m down to 18m (AB system), with a completeness limit of r∼15.5m and i∼14.5m which - due to the instrumental pixel size of 2.4" - refers to stars separated by >3". This brightness range is ideally suited to examine the intermediately bright stellar population supposed to be saturated in deep variability surveys with large telescopes. To connect to deep surveys or to explore faint long term variables, coadded images of several nights reach a depth of ∼20m. The astrometric accuracy is better than 1", as determined from the overlap of neighbouring fields. We describe the survey design, the data properties and our procedures to derive the light curves and to extract variable stars. We present a list of ∼2200 variable stars identified in 50 square degrees with 50-80 observations between May and October 2011. For bright stars the variability amplitude A reaches down to A∼0.05m, while at the faint end variations of A>1m are detected. About 200 stars were known to be variable, and their amplitudes and periods - as far as determinable from our six month monitoring - agree with literature values, demonstrating the performance of the Bochum Galactic Disk Survey. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 79 12 List of fields in Galactic Disk Survey (GDS) table2.dat 101 2288 List of variable stars -------------------------------------------------------------------------------- See also: B/gcvs : General Catalogue of Variable Stars (Samus+ 2007-2013) II/264 : ASAS Variable Stars in Southern hemisphere (Pojmanski+, 2002-2005) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 A3 --- --- [GDS] 5- 13 A9 --- Field GDS field name (NNNN-NNNN) 15- 16 I2 h RAh Right ascension (J2000) 18- 19 I2 min RAm Right ascension (J2000) 21- 24 F4.1 s RAs Right ascension (J2000) 26 A1 --- DE- Declination sign (J2000) 27- 28 I2 deg DEd Declination (J2000) 30- 31 I2 arcmin DEm Declination (J2000) 33- 34 I2 arcsec DEs Declination (J2000) 36- 37 I2 --- NObs Number of observations 39- 48 A10 "YYYY-MM-DD" Obs1 First night observation date 50- 59 A10 "YYYY-MM-DD" Obs2 Las2 night observation date 61- 65 I5 --- Nsr Number of stars used for the analysis in r-band 67- 69 I3 --- Nvr [70/238] Number of stars identified to be variable in r-band 71- 75 I5 --- Nsi Number of stars used for the analysis in i-band 77- 79 I3 --- Nvi [91/248] Number of stars identified to be variable in i-band -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Field Field name of the data set from which the light curve is created (NNNN-NNNN) 11- 20 F10.6 deg RAdeg Star right ascension (J2000) 22- 31 F10.6 deg DEdeg Star declination (J2000) 33- 34 I2 --- Nr [14/57]?=0 Number of data points of the light curve used in the r-band 36- 40 F5.2 mag ?=0 Mean brightness of the light curve in rmag (AB system) 42- 45 F4.2 mag e_ ?=0 Standard deviation on 47- 50 F4.2 mag Trs [0.02/0.5]?=0 Threshold at the brightness of the star to accept it as variable by means of the standard deviation in r-band 52- 55 F4.2 mag rAmp ?=0 Amplitude of the light curve in r-band 57- 60 F4.2 mag TrA [0.07/2.0]?=0 Threshold at the brightness of the star to accept it as variable by means of the amplitude in r-band 62- 66 F5.2 --- Jr ?=0 Stetson J-Index in r-band 68- 69 I2 --- Ni [14/42]?=0 Number of data points of the light curve used in the i-band 71- 75 F5.2 mag ?=0 Mean brightness of the light curve in imag (AB system) 77- 80 F4.2 mag e_ ?=0 Standard deviation on 82- 85 F4.2 mag Tis [0.02/0.5]?=0 Threshold at the brightness of the star to accept it as variable by means of the standard deviation in i-band 87- 90 F4.2 mag iAmp ?=0 Amplitude of the light curve in imag 92- 95 F4.2 mag TiA [0.07/2.0]?=0 Threshold at the brightness of the star to accept it as variable by means of the amplitude in i-band 97-101 F5.2 --- Ji ?=0 Stetson J-index in i-band -------------------------------------------------------------------------------- Acknowledgements: Martin Haas, haas(at)astro.rub.de
(End) Patricia Vannier [CDS] 27-Mar-2013
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