J/ApJS/199/3           The quasars MMT-BOSS pilot survey           (Ross+, 2012)

The SDSS-III Baryon Oscillation Spectroscopic Survey: quasar target selection for data release nine. Ross N.P., Myers A.D., Sheldon E.S., Yeche C., Strauss M.A., Bovy J., Kirkpatrick J.A., Richards G.T., Aubourg E., Blanton M.R., Brandt W.N., Carithers W.C., Croft R.A.C., da Silva R., Dawson K., Eisenstein D.J., Hennawi J.F., Ho S., Hogg D.W., Lee K.-G., Lundgren B., McMahon R.G., Miralda-Escude J., Palanque-Delabrouille N., Paris I., Petitjean P., Pieri M.M., Rich J., Roe N.A., Schiminovich D., Schlegel D.J., Schneider D.P., Slosar A.Z., Suzuki N., Tinker J.L., Weinberg D.H., Weyant A., White M., Wood-Vasey W.M. <Astrophys. J. Suppl. Ser., 199, 3 (2012)> =2012ApJS..199....3R 2012ApJS..199....3R
ADC_Keywords: Photometry, SDSS ; Redshifts ; QSOs ; Surveys Keywords: cosmology: observations - intergalactic medium - surveys - quasars: absorption lines - quasars: general - techniques: miscellaneous Abstract: The SDSS-III Baryon Oscillation Spectroscopic Survey (BOSS), a five-year spectroscopic survey of 10000deg2, achieved first light in late 2009. One of the key goals of BOSS is to measure the signature of baryon acoustic oscillations (BAOs) in the distribution of Lyα absorption from the spectra of a sample of ∼150000 z>2.2 quasars. Along with measuring the angular diameter distance at z∼2.5, BOSS will provide the first direct measurement of the expansion rate of the universe at z>2. One of the biggest challenges in achieving this goal is an efficient target selection algorithm for quasars in the redshift range 2.2<z<3.5, where their colors tend to overlap those of the far more numerous stars. During the first year of the BOSS survey, quasar target selection (QTS) methods were developed and tested to meet the requirement of delivering at least 15 quasars/deg2 in this redshift range, with a goal of 20 out of 40 targets/deg2 allocated to the quasar survey. To achieve these surface densities, the magnitude limit of the quasar targets was set at g≤22.0 or r≤21.85. We have defined a uniformly selected subsample of 20 targets/deg2, for which the selection efficiency is just over 50% (∼10 z>2.20 quasars/deg2). This "CORE" subsample will be fixed for Years Two through Five of the survey. In this paper, we describe the evolution and implementation of the BOSS QTS algorithms during the first two years of BOSS operations (through 2011 July), in support of the science investigations based on these data, and we analyze the spectra obtained during the first year. During this year, 11263 new z>2.20 quasars were spectroscopically confirmed by BOSS, roughly double the number of previously known quasars with z>2.20. Our current algorithms select an average of 15 z>2.20 quasars/deg2 from 40 targets/deg2 using single-epoch SDSS imaging. Description: The Sloan Digital Sky Survey is now in its third phase (SDSS-III; Eisenstein et al. 2011AJ....142...72E 2011AJ....142...72E) and is carrying out a combination of four interleaved surveys that will continue until the summer of 2014. One of those surveys, the Baryon Oscillation Spectroscopic Survey (BOSS), commenced operations in late 2009 and is using essentially all the dark time for SDSS-III. BOSS uses the same 2.5m Sloan Foundation telescope that was used in SDSS-I/II, but since BOSS will observe fainter targets, the fiber-fed spectrographs have been significantly upgraded. These upgrades include: new CCDs with improved blue and red response; 1000 2" instead of 640 3" optical diameter fibers; higher throughput gratings over a spectral range of 3600-10000Å at a resolution of about 2000, and improved optics. Prior to the commencement of BOSS spectroscopy, we carried out spectroscopy of quasar candidates selected from co-added photometry in SDSS Stripe 82. Observations of these candidates were carried out in queue mode between 2008 September and 2009 January using the Hectospec multi-fiber spectrograph on the 6.5m Multiple Mirror Telescope (MMT). In Tables 14 and 15, we provide positions, PSF photometry (as observed, uncorrected for Galactic extinction), and redshifts for confirmed quasars from the MMT survey. Objects that are not flagged Primary in the CAS are listed separately (table 15). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table14.dat 94 437 Quasars discovered in the MMT survey table15.dat 94 7 Quasars discovered in the MMT survey that are non-primary in SDSS DR8 imaging -------------------------------------------------------------------------------- See also: II/306 : The SDSS Photometric Catalog, Release 8 (Adelman-McCarthy+, 2011) VII/241 : The 2dF QSO Redshift Survey (Croom+ 2004) J/A+A/525/A37 : Variability indexes of QSOs in SDSS Stripe 82 (Meusinger+, 2011) J/MNRAS/392/19 : The 2dF-SDSS QSO survey (Croom+, 2009) J/AJ/131/2766 : Quasar luminosity function from SDSS-DR3 (Richards+, 2006) J/AJ/131/2788 : Redshifts in the SFQS survey (Jiang+, 2006) http://www.sdss3.org/surveys/boss.php : BOSS home page http://www.sdss.org/ : SDSS home page Byte-by-byte Description of file: table1[45].dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 h RAh Hour of Right Ascension (J2000) 4- 5 I2 min RAm Minute of Right Ascension (J2000) 7- 11 F5.2 s RAs Second of Right Ascension (J2000) 13 A1 --- DE- Sign of the Declination (J2000) 14- 15 I2 deg DEd Degree of Declination (J2000) 17- 18 I2 arcmin DEm Arcminute of Declination (J2000) 20- 23 F4.1 arcsec DEs Arcsecond of Declination (J2000) 25- 30 F6.3 mag umag SDSS-DR8 u band magnitude (1) 32- 36 F5.3 mag e_umag Error in umag 38- 43 F6.3 mag gmag SDSS-DR8 g band magnitude (1) 45- 49 F5.3 mag e_gmag Error in umag 51- 56 F6.3 mag rmag SDSS-DR8 r band magnitude (1) 58- 62 F5.3 mag e_rmag Error in umag 64- 69 F6.3 mag imag SDSS-DR8 i band magnitude (1) 71- 75 F5.3 mag e_imag Error in umag 77- 82 F6.3 mag zmag SDSS-DR8 z band magnitude (1) 84- 88 F5.3 mag e_zmag Error in umag 90- 94 F5.3 --- z Redshift -------------------------------------------------------------------------------- Note (1): Many of these objects were subsequently confirmed in the SDSS DR7 quasar catalog (Cat. VII/260) or in the BOSS (SDSS-III Baryon Oscillation Spectroscopic Survey). Imaging information is taken from the SDSS DR8 Catalog Archive Server (http://www.sdss3.org/dr8/). -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Emmanuelle Perret [CDS] 21-Mar-2012
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