2009ApJ...694..924M


Query : 2009ApJ...694..924M

2009ApJ...694..924M - Astrophys. J., 694, 924-942 (2009/April-1)

Automated detection of galaxy-scale gravitational lenses in high-resolution imaging data.

MARSHALL P.J., HOGG D.W., MOUSTAKAS L.A., FASSNACHT C.D., BRADAC M., SCHRABBACK T. and BLANDFORD R.D.

Abstract (from CDS):

We expect direct lens modeling to be the key to successful and meaningful automated strong galaxy-scale gravitational lens detection. We have implemented a lens-modeling "robot" that treats every bright red galaxy (BRG) in a large imaging survey as a potential gravitational lens system. Having optimized a simple model for "typical" galaxy-scale gravitational lenses, we generate four assessments of model quality that are then used in an automated classification. The robot infers from these four data the lens classification parameter H that a human would have assigned; the inference is performed using a probability distribution generated from a human-classified training set of candidates, including realistic simulated lenses and known false positives drawn from the Hubble Space Telescope (HST) Extended Groth Strip (EGS) survey. We compute the expected purity, completeness, and rejection rate, and find that these statistics can be optimized for a particular application by changing the prior probability distribution for H; this is equivalent to defining the robot's "character." Adopting a realistic prior based on expectations for the abundance of lenses, we find that a lens sample may be generated that is ∼100% pure, but only ∼20% complete. This shortfall is due primarily to the oversimplicity of the model of both the lens light and mass. With a more optimistic robot, ∼90% completeness can be achieved while rejecting ∼90% of the candidate objects. The remaining candidates must be classified by human inspectors. Displaying the images used and produced by the robot on a custom "one-click" web interface, we are able to inspect and classify lens candidates at a rate of a few seconds per system, suggesting that a future 1000 deg2 imaging survey containing 107 BRGs, and some 104 lenses, could be successfully, and reproducibly, searched in a modest amount of time. We have verified our projected survey statistics, albeit at low significance, using the HST EGS data, discovering four new lens candidates in the process.

Abstract Copyright:

Journal keyword(s): galaxies: elliptical and lenticular, cD - gravitational lensing - methods: data analysis - methods: statistical - surveys - techniques: miscellaneous

Nomenclature: Tables 1, 6: [MHM2009] HST JHHMMSS.ss+DDMMSS.s N=3+10.

Simbad objects: 17

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Number of rows : 17
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 8C 0958+561 QSO 10 01 20.6918953728 +55 53 55.593949272   17.16 16.95     ~ 735 3
2 DEEP2-GRS 12008260 G 14 17 19.80 +52 28 23.9   23.56   20.878 20.062 ~ 8 0
3 [MHM2009] HST J141731.17+522636.2 Le? 14 17 31.17 +52 26 36.2           ~ 1 0
4 CFRS 14.1311 G 14 17 35.70 +52 26 45.9   24.04 21.53 21.38 19.971 ~ 62 1
5 [MMN2007] A1 gLS 14 17 35.9 +52 26 46     21.53   19.69 ~ 71 0
6 [TCB2007] 12016415 G 14 17 59.01092 +52 35 14.5069   24.21   21.50 20.338 ~ 5 0
7 [MHM2009] HST J141807.31+523030.0 G 14 18 07.22 +52 30 29.0           ~ 5 0
8 [MMN2007] A2 G 14 18 20.834 +52 36 10.98           ~ 5 0
9 [TCB2007] 12016031 G 14 18 20.85943 +52 36 10.9886           ~ 6 1
10 EGSIRAC J141828.03+523646.0 G 14 18 28.03432 +52 36 46.0621   22.41   21.77 20.92 ~ 4 0
11 DEEP2-GRS 12024284 G 14 18 33.12 +52 43 52.2   22.98   20.447 19.680 ~ 9 1
12 [MMN2007] A3 G 14 18 33.131 +52 43 52.30           ~ 6 0
13 EGSIRAC J141856.18+523843.1 G 14 18 56.16550 +52 38 43.4288   23.46   22.38 21.35 ~ 5 0
14 EGSIRAC J141857.15+523823.9 G 14 18 57.12691 +52 38 24.4644   25.3   22.87 21.58 ~ 6 0
15 NAME Extended Groth Strip reg 14 19 +52.8           ~ 828 0
16 SDSS J141958.51+530124.1 EmG 14 19 58.515 +53 01 24.11           ~ 3 0
17 [MHM2009] HST J142053.90+530608.1 Le? 14 20 53.90 +53 06 08.1           ~ 1 0

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