Mel's home page
Research Interests
UNDERGRADUATE RESEARCH
Melvyn Wright UG Research 2022.pdf UG Research 2022
Black_Holes_and_Massive_Stars An Introduction 28Aug2020
Aperture Synthesis Telescopes An Introduction
The ALMA View of the OMC1 Explosion in Orion
Orion Source I Disk and Outflow Interface
Structure_of_the_Source_I_Disk in Orion-KL
Magnetic Field Structure of Orion Source I
Polarimetric Imaging of the Massive Black Hole, Bromley, Melia and Liu, 2001, ApJ 555, L83
The Event Horizon Telescope
The M87 Black Hole and Xray jet
The M87 Jet
Star orbits around the SgrA* black hole
CARMA Summer School 2014. CARMA Summer School 2014. pdf file.
Millimeter VLBI with ALMA Using the ALMA telescope as part of the millimeter VLBI network
CARMA_EHT_PRESENTATION. CARMA_EHT_PRESENTATION. pdf file.
Adaptive Real Time Synthesis Telescopes The International Journal of High Performance Computing Applications Volume 26 Issue 4, November 2012
The-role-of-magnetic-fields-in-the-formation-of-stars REVIEW: Front.Astron.Space Sci., 13 December 2018
PUBLICATIONS
publications
publications 2006-2011
Publications_2012-2020
Publications_Since_Retirement[2012-2020]
REAL TIME IMAGING
Adaptive Real Time Synthesis Telescopes The International Journal of High Performance Computing Applications Volume 26 Issue 4, November 2012
ICCS Workshop Jan2011 RealTime_ICCS_Jan2011.pdf
Berkeley DSP workshop Berkeley DSP workshop 16 Sept 2010
CARMA SUMMER SCHOOL
CARMA Summer School 2014. CARMA Summer School 2014. pdf file.
CARMA Summer School 2012. CARMA memo 60, 2012. pdf file.
CARMA Summer School 2011. CARMA memo 56, 2011. pdf file.
CARMA Summer School 2010. CARMA memo 55, 2010. pdf file.
CARMA Summer School 2009. CARMA memo 53, 2009. pdf file.
CARMA Summer School 2008. CARMA memo 48, 2008. pdf file.
CARMA Summer School 2007. CARMA memo 44, 2008. pdf file.
CARMA MEMOS
Bandpass Calibration and Stability. CARMA memo 55, July 2009. pdf file.
Aperture Efficiency, Pointing and Primary Beam Calibration. CARMA memo 52, June 2009. compressed ps file.
Deconvolving Primary Beam Patterns from Mosaic and Polarization Images. CARMA memo 43, 2008. pdf file.
Image Fidelity as a Function of Source Size and Calibration Errors. January 2007. pdf file.
CARMA memo 38 Image Fidelity as a Function of Source Size and Calibration Errors.
CARMA memo 27 Imaging Simulations with CARMA-23
CARMA memo 25 SZA location at CARMA site
CARMA memo 24 Antenna Configuration Evaluation
CARMA memo 14 CARMA Spectral Line Correlator Requirements
CARMA memo 5 Compact Configuration Evaluation for CARMA
VLBI
CARMA_EHT_PRESENTATION. CARMA_EHT_PRESENTATION. pdf file.
MEMORIALS
Don Backer memorial. Don Backer, Berkeley, July 2010.
John Baldwin memorial. Baldwin Day, Cambridge, May 2011.
SKA
SKA memo 103 Deconvolving Primary Beam Patterns from SKA Images. 2008. pdf file.
SKA Survey Optimization SKA memo 81. 2006.
SKA Surveys, Calibration and Imaging Paris 2006. pdf file.
Real Time Imaging SKA memo 60. 2005.
SKA memo 46 SKA Imaging. abstract - plain text.
SKA memo 46 SKA Imaging. 2004.
SKA memo 16
SKA model where individual antennas can be correlated to image the full field of view. 2002.
ALMA
Heterogeneous Array Imaging ALMA Single Dish and Array Combination Workshop, 2012
ALMA memo 465 Case for interoperability as an ALMA off-line model
ALMA memo 464 Comparison of the evaluations of the AIPS++ GILDAS and MIRIAD packages for ALMA off-line data processing
ALMA memo 463 ALMA Offline Data Processing Audit of the MIRIAD Package
BIMA memo 96 Evaluation of the GILDAS Package for ALMA Off-line Data Processing
BIMA memo 95 Evaluation of the MIRIAD Package for ALMA Off-line Data Processing
ALMA memo 450 Heterogeneous Imaging with the ALMA Compact Array. 2003
ALMA memo 430 Compact Configuration Evaluation - Mosaicing. 2002
ALMA memo 428 Compact Configuration Evaluation. 2002
ALMA memo 382 MM-VLBI with ALMA, 2001
ALMA memo 427 Antenna Position Calibration. 2002
ALMA memo 358 Observing Object. 2001.
ALMA memo 289 Atmospheric Noise in Single Dish Observations. 2000
ALMA memo 282 DYNAMIC SCHEDULING. 1999.
ALMA memo 272 IMAGE FIDELITY: IMPLICATIONS FOR ALMA, 1999
MM-VLBI ARRAYS memo FUTURE MM-VLBI ARRAYS, 1997
ALMA memo fig 1 uv-tracks for 3C273
ALMA memo fig 2 uv-tracks for SGRA*
FIRST IMAGES WITH NEW TELESCOPES
M33 HI (Cambridge 1970) M33 HI, Cambridge 1970
Circum Nuclear HCN Circum Nuclear Disk, Hat Creek 1987
HCN(1-0) [contours] and HCO+ Hat Creek, 2000
H42-HCN-OH-NH3 H42 alpha, HCN, NH3 and OH masers.
20cm-HCN-OH-NH3 SgrA East interacting with molecular gas.
6cm-HCN-OH-NH3 SgrA East interacting with molecular gas.
dust-HCN-NH3 Circum nuclear disk: Dust, HCN and NH3
NH3-HCN-OH-6cm Circum nuclear disk: NH3 and HCN in same velocity range.
Hot Spots A&B Cygnus A at 230, 15 and 5 GHz. Hat Creek, 2002
Hot Spots D&E Cygnus A at 230, 15 and 5 GHz. Hat Creek, 2002
SOFTWARE
Calculate theoretical rms noise for radio telescopes python script
ALMA memo 463 Censored ALMA Offline Data Processing Audit of the MIRIAD Package
Introduction to MIRIAD Introduction to MIRIAD
ATNF version of the Miriad User's Guide
A retrospective view of MIRIAD Sault, R.J., Teuben, P.J., & Wright,M.C.H., 1995, in Astronomical Data Analysis Software and Systems IV, ed. R. Shaw, H.E. Payne, & J.J.E.Hayes, ASP Conf. Ser., 77, 433
MIRIAD Timings for 250x250x100 channel Imaging Simulated ALMA data with 60 antennas in configuration 12
MIRIAD Timings for 1573x1573x10 channel Imaging Simulated ALMA data with 60 antennas in configuration 29
ALLEN TELESCOPE ARRAY
ATA memo 84 Extended ATA telescope with outrigger stationa. 2009.
ATA memo 83 Antenna Gain, Pointing, Primary Beam and Bandpass Calibration. 2009.
ATA memo 59 Comparison of imaging performance ATA and VLA. 2003.
ATA memo 52 Allen Telescope Array Imaging. 2002.
ALLEN TELESCOPE ARRAY IMAGES
M31 continuum emission at 1.4 GHz HII regions and background continuum sources.
M31 HI emission at 1.4 GHz integrated HI emission.
M31 HI velocity HI velocity.
M33 continuum emission at 1.4 GHz HII regions and background continuum sources.
M33 HI emission at 1.4 GHz integrated HI emission.
M33 HI velocity HI velocity.
ALLEN TELESCOPE ARRAY SIMULATED IMAGES
CASA at x-band with the ATA Model Image of CASA at 11.2 GHz in 1 minute and 100 MHz. Peak 3.19 Jy/beam, Total Flux 729 Jy.
CASA convolved to ATA x-band resolution VLA image of CASA convolved to ATA resolution at 11.2 GHz. Peak 3.20 Jy/beam, Total Flux 732 Jy.
CASA ATA - VLA residual at x-band Difference between ATA & VLA images at 11.2 GHz. Max,Min,Rms = 2.5, -3.2, 0.35 mJy
CASA 1.5 x real size with the ATA Model Image of CASA scaled up 1.5 x real size. Peak 1.62 Jy/beam, Total Flux 718 Jy
CASA 1.5 x real size with the VLA Model Image of CASA scaled up 1.5 x real size. Peak 1.63 Jy/beam, Total Flux 732 Jy
CASA 1.5 x residual Shows bowl from missing short spacings. MFS over 400 MHz. Max,Min,Rms = 7.8, -4.1, 1.2 mJy/beam.
CASA 2 x real size with the ATA Model Image of CASA scaled up 2 x real size. Peak 0.99 Jy/beam, Total Flux 679 Jy
CASA 2 x real size with the VLA Model Image of CASA scaled up 2 x real size. Peak 1.01 Jy/beam, Total Flux 732 Jy
CASA 2 x residual Shows bowl from missing short spacings. MFS over 400 MHz. Max,Min,Rms = 25, -14, 4.2 mJy/beam.
CASA 2.5 x real size with the ATA Model Image of CASA scaled up 2.5 x real size. Peak 0.66 Jy/beam, Total Flux 561 Jy.
CASA 2.5 x real size with the VLA Model Image of CASA scaled up 2.5 x real size. Peak 0.69 Jy/beam, Total Flux 732 Jy.
CASA 2.5 x residual Shows bowl from missing short spacings. MFS over 400 MHz. Max,Min,Rms = 96, -60, 14 mJy/beam.
CASA 20 x real size with the ATA Mosaic Image of CASA scaled up 20 x real size.
CASA 40 x pointing 1 CASA Image illuminated by ATA Primary beam at 1.4 GHz
CASA 40 x pointing 7 CASA Image illuminated by ATA Primary beam at 1.4 GHz
CASA 40 x real size at declination 30 with the ATA Mosaic MFS Image of CASA scaled up 40 x real size. Peak 0.187 Jy/beam, Total Flux 486 Jy
CASA 40 x real size at declination 30 with the VLA Mosaic Image of CASA scaled up 40 x real size. Peak 0.201 Jy/beam, Total Flux 732 Jy
CASA 40 x residual at declination 30 ATA - VLA Residual Image of CASA. Max,Min,Rms = 61, -23, 4.8 mJy
ATA point source response at declination 30 Point source response with Natural weighting
Point source response with 30deg_phase_noise Point source response with 30deg_phase_noise
uvplot with 30deg_phase_noise uv-plot with 30deg_phase_noise
Point source response after selfcal with 30deg_phase_noise Point source response after selfcal with 30deg_phase_noise
NVSS model Point sources convolved with clean response; Max=1.12 Jy/beam; Total Flux = 30.66 Jy
BIMA MEMO's
memo 44 A RECIPE FOR PHASE PREDICTION FROM TOTAL POWER MEASUREMENTS
memo 45 BIMA ARRAY RESPONSE TO EXTENDED STRUCTURE, 1996
memo 53 DYNAMIC SCHEDULING FOR THE BIMA ARRAY, 1997
memo 55 FUTURE MM-VLBI ARRAYS, Wright & Bower, 1997
memo 58 DYNAMIC SCHEDULING: Selection criteria & evaluation, Wright & Akeson, 1997
memo 59 IMAGING WITH HETEROGENEOUS ARRAYS, 1997
memo 60 DYNAMIC SCHEDULING: Implementation at Hat Creek, 1997
memo 66 COMMENTS ON ARRAY CONFIGURATIONS, 1998
memo 69 NEW ARRAY CONFIGURATIONS FOR HAT CREEK, 1998
memo 73 IMAGE FIDELITY, 1999
memo 75 Astronomical Imaging with the One Hectare Telescope, 1998
memo 78 Atmospheric Phase Correction using Water Vapor Radiometers. 2000
BIMA memo 84 CARMA Sensitivity and Correlator Requirements
BIMA memo 85 CARMA Calibration Requirements
BIMA memo 91 Compact Configuration Evaluation for CARMA
BIMA memo 92 Allen Telescope Array Imaging.
BIMA memo 93 Characterizing BIMA proposals 2000-2003
BIMA memo 95 Evaluation of the MIRIAD Package for ALMA Off-line Data Processing
Real Time Imaging - URSI talk URSI, Boulder 2006 pdf file.
PAPERS
230 GHz cygnus paper Images of the hot spots in Cygnus A at 230 GHz
87 GHz cygnus paper Images of the hot spots in Cygnus A at 87 GHz
atmos paper ATMOSPHERIC PHASE NOISE AND APERTURE SYNTHESIS IMAGING AT MILLIMETER WAVELENGTHS
orion paper A Multi-line aperture synthesis study of Orion-KL
MISC
Kyesa in the garden at Euclid. Kyesa in the garden at Euclid April 2001, 5.5 yrs old.
Fuel Energy Conversion Factors. Fuel Energy Conversion Factors.
Email: wright@astro.berkeley.edu