The IPAC Image Subtraction and Discovery Pipeline for the Intermediate Palomar Transient Factory
暂无分享,去创建一个
Lin Yan | Mansi Kasliwal | Eran Ofek | Yi Cao | George Helou | Frank Masci | David Shupe | Jason Surace | Carl Grillmair | Lisa Storrie-Lombardi | Ed Jackson | Gary Doran | Russ Laher | S. Bradley Cenko | Eric Bellm | Umaa Rebbapragada | Adam Miller | Tom Barlow | Thomas Prince | Shrinivas Kulkarni | E. Ofek | M. Kasliwal | E. Bellm | C. Grillmair | S. Cenko | R. Laher | F. Masci | Yi Cao | L. Storrie-Lombardi | U. Rebbapragada | T. Prince | D. Shupe | J. Surace | G. Helou | T. Barlow | Lin Yan | E. Jackson | G. Doran | S. Kulkarni | Adam M Miller | S. Kulkarni | Yi Cao
[1] Peter E. Nugent,et al. SLOW-SPEED SUPERNOVAE FROM THE PALOMAR TRANSIENT FACTORY: TWO CHANNELS , 2014, 1405.7409.
[2] A. J. Connolly,et al. Regularization techniques for PSF-matching kernels - I. Choice of kernel basis , 2012, 1202.2902.
[3] E. O. Ofek,et al. Automating Discovery and Classification of Transients and Variable Stars in the Synoptic Survey Era , 2011, 1106.5491.
[4] K. Kafadar. John Tukey and robustness , 2003 .
[5] Ernest E. Croner,et al. The Palomar Transient Factory: System Overview, Performance, and First Results , 2009, 0906.5350.
[6] E. Ofek,et al. PROPER IMAGE SUBTRACTION—OPTIMAL TRANSIENT DETECTION, PHOTOMETRY, AND HYPOTHESIS TESTING , 2016, 1601.02655.
[7] R. Kotak,et al. Machine learning for transient discovery in Pan-STARRS1 difference imaging , 2015, 1501.05470.
[8] Adam D. Myers,et al. THE SLOAN DIGITAL SKY SURVEY STRIPE 82 IMAGING DATA: DEPTH-OPTIMIZED CO-ADDS OVER 300 deg2 IN FIVE FILTERS , 2014, 1405.7382.
[9] R. Lupton,et al. A Method for Optimal Image Subtraction , 1997, astro-ph/9712287.
[10] R. C. Wolf,et al. AUTOMATED TRANSIENT IDENTIFICATION IN THE DARK ENERGY SURVEY , 2015, 1504.02936.
[11] Carl J. Grillmair,et al. AUTOMATED CLASSIFICATION OF PERIODIC VARIABLE STARS DETECTED BY THE WIDE-FIELD INFRARED SURVEY EXPLORER , 2014, 1402.0125.
[12] M. Skrutskie,et al. The Two Micron All Sky Survey (2MASS) , 2006 .
[13] Leo Breiman,et al. Random Forests , 2001, Machine Learning.
[14] IoA,et al. OGLE-IV Real-Time Transient Search , 2014, 1409.1095.
[15] F. Yuan,et al. Astronomical Image Subtraction by Cross-Convolution , 2008, 0801.0336.
[16] Ashutosh Kumar Singh,et al. The Elements of Statistical Learning: Data Mining, Inference, and Prediction , 2010 .
[17] M. Sullivan,et al. The Palomar Transient Factory Photometric Calibration , 2011, 1112.4851.
[18] E. Rykoff,et al. The ROTSE‐III Robotic Telescope System , 2002, astro-ph/0210238.
[19] J. Munn,et al. The USNO-B Catalog , 2002, astro-ph/0210694.
[20] E. Greisen,et al. Representations of celestial coordinates in FITS , 2002, astro-ph/0207413.
[21] Kesheng Wu,et al. Implementing the Palomar Transient Factory Real-Time Detection Pipeline in GLADE: Results and Observations , 2014, DNIS.
[22] A. J. Drake,et al. FIRST RESULTS FROM THE CATALINA REAL-TIME TRANSIENT SURVEY , 2008, 0809.1394.
[23] Peter E. Nugent,et al. AN ACCRETING WHITE DWARF NEAR THE CHANDRASEKHAR LIMIT IN THE ANDROMEDA GALAXY , 2014, 1401.2426.
[24] M. Wainwright,et al. Using machine learning for discovery in synoptic survey imaging data , 2012, 1209.3775.
[25] C. Alard. Image subtraction using a space-varying kernel , 2000 .
[26] Peter E. Nugent,et al. Exploring the spectral diversity of low-redshift Type Ia supernovae using the Palomar Transient Factory , 2014, 1408.1430.
[27] Parameter Estimation in Astronomy with Poisson-distributed Data. I. The χγ2 Statistic , 1999, astro-ph/9903093.
[28] Stuart E. Sale,et al. Reference image selection for difference imaging analysis , 2014, 1404.6948.
[29] P. Stetson. DAOPHOT: A COMPUTER PROGRAM FOR CROWDED-FIELD STELLAR PHOTOMETRY , 1987 .
[30] E. Bertin,et al. SExtractor: Software for source extraction , 1996 .
[31] Christopher Bebek,et al. The Zwicky Transient Facility: Observing System , 2014, Astronomical Telescopes and Instrumentation.
[32] Carl J. Grillmair,et al. TRACING THE ORPHAN STREAM TO 55 kpc WITH RR LYRAE STARS , 2013, 1308.0857.
[33] Adam A. Miller,et al. ACTIVE LEARNING TO OVERCOME SAMPLE SELECTION BIAS: APPLICATION TO PHOTOMETRIC VARIABLE STAR CLASSIFICATION , 2011, 1106.2832.
[34] R. Lupton,et al. Astrometric Calibration of the Sloan Digital Sky Survey , 2002, astro-ph/0211375.
[35] S. Roweis,et al. ASTROMETRY.NET: BLIND ASTROMETRIC CALIBRATION OF ARBITRARY ASTRONOMICAL IMAGES , 2009, 0910.2233.
[36] Eduardo Serrano,et al. LSST: From Science Drivers to Reference Design and Anticipated Data Products , 2008, The Astrophysical Journal.
[37] David Polishook,et al. Main-belt comets in the Palomar Transient Factory survey – I. The search for extendedness , 2013, 1305.7176.
[38] Brian D. Bue,et al. THE NEEDLE IN THE 100 deg2 HAYSTACK: UNCOVERING AFTERGLOWS OF FERMI GRBs WITH THE PALOMAR TRANSIENT FACTORY , 2015, 1501.00495.
[39] D. M. Bramich,et al. A new algorithm for difference image analysis , 2008, 0802.1273.
[40] Oxford,et al. Exploring the Optical Transient Sky with the Palomar Transient Factory , 2009, 0906.5355.
[41] Yi Cao,et al. Intermediate Palomar Transient Factory: Realtime Image Subtraction Pipeline , 2016, 1608.01006.
[42] J. Prieto,et al. THE SLOAN DIGITAL SKY SURVEY-II SUPERNOVA SURVEY: SEARCH ALGORITHM AND FOLLOW-UP OBSERVATIONS , 2007, 0708.2750.
[43] E. Bachelet,et al. Difference image analysis: automatic kernel design using information criteria , 2015, 1512.04655.
[44] Umaa Rebbapragada,et al. iPTF SEARCH FOR AN OPTICAL COUNTERPART TO GRAVITATIONAL-WAVE TRANSIENT GW150914 , 2016, 1602.08764.
[45] Richard Walters,et al. EVIDENCE FOR AN FU ORIONIS-LIKE OUTBURST FROM A CLASSICAL T TAURI STAR , 2010, 1011.2063.
[46] W. M. Wood-Vasey,et al. THE NINTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY: FIRST SPECTROSCOPIC DATA FROM THE SDSS-III BARYON OSCILLATION SPECTROSCOPIC SURVEY , 2012, 1207.7137.
[47] Holger Israel,et al. Optimising optimal image subtraction , 2007 .