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FOBOS
With first-light in 2028, FOBOS will be the premier instrument for deep, high-target-density spectroscopy in the era of deep-imaging surveys, like the Vera C. Rubin Observatory Legacy Survey of Space and Time LSST, Euclid, and the Nancy Grace Roman Space Telescope. UC OBSERVATORIESSEE MORE ON UCOLICK.ORGUC OBSERVATORIES
Call for Proposals: UC time on the Keck telescopes. Semester 2021B (Aug 1, 2021 through Jan 31, 2022) Deadline: Proposals are due on Thursday, Mar 18 th, 2021 by 5:00 pm PDT * * Note this deadline is close to the Chandra proposal deadline so please plan accordinglyLICK OBSERVATORY
Volunteer. The Lick Observatory Volunteers are a dedicated collection of people interested in astronomy and eager to share their enthusiasm for Lick Observatory and the skies above.THE XIDL CODE
Installation: Installing the code: The code is now distributed via SVN (or you can try to grab a machine-built tarball from above).These notes decribe what do to. LECTURE 3 ATOMIC SPECTROSCOPY AND ABUNDANCES E m→E n+hν(or E n+hν→ E m)m>n hν= hc λ =E m−E n 1 λ = E m−E n hc = 2π2Z2e4m e h3c 1 n2 − 1 m2 1 λ mn =1.097×105Z2 1 n2 − 1 m2 cm−1 λ mn= 911.6 Z2 1 n2 − 1 m2 −1 Angstroms Radiation in the form of a single quantum (photon) is emitted MY INTERESTS BEYOND FAMILY AND WORK There was a time when I played all sorts of games as well: chess, bridge, xblast, intellivision, stratego, Mao-Mao. You name it. Maybe those days will return as the boys age.MY FAMILY TREE
Generated by Gramps 5.0.1 Last change was the 2014-10-12 23:45:11 ©2021 Steve Allen
HOW LONG WOULD IT TAKE US TO TRAVEL TO ALPHA CENTAURI [ASK If light travels at 186,000 miles per hour and a star is 75,000 light years away how long would it take for the light from the star to reachus.
STEVE ALLEN'S HOME PAGE Steve Allen I read my e-mail as MIME type text/plain If I receive e-mail as HTML or in proprietary (e.g., Microsoft) document formats, then that e-mail will not be read.FOBOS
With first-light in 2028, FOBOS will be the premier instrument for deep, high-target-density spectroscopy in the era of deep-imaging surveys, like the Vera C. Rubin Observatory Legacy Survey of Space and Time LSST, Euclid, and the Nancy Grace Roman Space Telescope. UC OBSERVATORIESSEE MORE ON UCOLICK.ORGUC OBSERVATORIES
Call for Proposals: UC time on the Keck telescopes. Semester 2021B (Aug 1, 2021 through Jan 31, 2022) Deadline: Proposals are due on Thursday, Mar 18 th, 2021 by 5:00 pm PDT * * Note this deadline is close to the Chandra proposal deadline so please plan accordinglyLICK OBSERVATORY
Volunteer. The Lick Observatory Volunteers are a dedicated collection of people interested in astronomy and eager to share their enthusiasm for Lick Observatory and the skies above.THE XIDL CODE
Installation: Installing the code: The code is now distributed via SVN (or you can try to grab a machine-built tarball from above).These notes decribe what do to. LECTURE 3 ATOMIC SPECTROSCOPY AND ABUNDANCES E m→E n+hν(or E n+hν→ E m)m>n hν= hc λ =E m−E n 1 λ = E m−E n hc = 2π2Z2e4m e h3c 1 n2 − 1 m2 1 λ mn =1.097×105Z2 1 n2 − 1 m2 cm−1 λ mn= 911.6 Z2 1 n2 − 1 m2 −1 Angstroms Radiation in the form of a single quantum (photon) is emitted MY INTERESTS BEYOND FAMILY AND WORK There was a time when I played all sorts of games as well: chess, bridge, xblast, intellivision, stratego, Mao-Mao. You name it. Maybe those days will return as the boys age.MY FAMILY TREE
Generated by Gramps 5.0.1 Last change was the 2014-10-12 23:45:11 ©2021 Steve Allen
HOW LONG WOULD IT TAKE US TO TRAVEL TO ALPHA CENTAURI [ASK If light travels at 186,000 miles per hour and a star is 75,000 light years away how long would it take for the light from the star to reachus.
LICK OBSERVATORY
Lick Observatory has been at the forefront of astronomy since 1888. Lick Observatory was founded thanks to James Lick, an eccentric California millionaire who dreamed of building a "telescope superior to and more powerful than any telescope yet made." STEVE ALLEN'S HOME PAGE Steve Allen I read my e-mail as MIME type text/plain If I receive e-mail as HTML or in proprietary (e.g., Microsoft) document formats, then that e-mail will not be read.UC OBSERVATORIES
Call for Proposals: UC time on the Keck telescopes. Semester 2021B (Aug 1, 2021 through Jan 31, 2022) Deadline: Proposals are due on Thursday, Mar 18 th, 2021 by 5:00 pm PDT * * Note this deadline is close to the Chandra proposal deadline so please plan accordingly DAVID KOO'S HOME PAGE David Koo's Home Page UCO/Lick Observatory University of California, Santa Cruz 1156 High Street Santa Cruz, CA 95064 koo@ucolick.org. Latest Modification: TARGET - 2017 May 1 Background (Under Construction): I was faculty (Astronomer and Professor) at the University of California, Santa Cruz from 1988 until summer 2014 whenI retired.
GARTH D. ILLINGWORTH Garth Illingworth is a Professor at the University of California, Santa Cruz. He was a Miller Fellow at UC Berkeley, the Deputy-Director of the Space Telescope Science Institute, and in 2010 was awarded an honorary Doctor of Science degree at the University of WesternAustralia.
MY INTERESTS BEYOND FAMILY AND WORK There was a time when I played all sorts of games as well: chess, bridge, xblast, intellivision, stratego, Mao-Mao. You name it. Maybe those days will return as the boys age. THE W. M. KECK OBSERVATORY SCIENTIFIC STRATEGIC PLAN W. M. Keck Observatory Scientific Strategic Plan July, 2016. 3. C. Prepare for increasing opportunities in Time Domain Astronomy (TDA). We are entering a new age; that of TDA, made possible by advances in digital electronics and computing. KECK HIRES SPECTROGRAPH The xhires control room simulator The xhires program is the user interface which is used at the summit to control the HIRES spectrograph. It can be run in a standalone mode without being atMauna Kea.
MY FAMILY TREE
This page contains an index of all the surnames in the database. Selecting a link will lead to a list of individuals in the database with this same surname. ABERRATIONS OF THE HUMAN EYE: STRUCTURE Spatial frequency (c/deg) 1 10 100 Modulation transfer 10 20 30 40 50 60 70 80 90 0 10 20 30 40 50 60 70 80 90 0.0 0.2 0.4 0.6 0.8 1.0 RatioAberration-free
UC OBSERVATORIES
Proposals for UC observing time on the Keck Telescopes for Semester 2021B are due by 5:00 pm PDT on Thursday, Mar 18th, 2021. There will be 62.5 nights available on K1 and 57 nights available on K2 spread evenly across the semester and lunar phase. There are 7 one-hour Partnership ToO interrupts available. NOTE: There is a new requirementbased
STEVE ALLEN'S HOME PAGE The MOS project is nearly complete. A few docs are seen here. IRAF cl scripts for Lick images. These help astronomers with images from Lick use them in IRAF. The HIRES Spectrograph. I constructed the X11 user interface for the HIRES instrument simulator.LICK OBSERVATORY
Volunteer. The Lick Observatory Volunteers are a dedicated collection of people interested in astronomy and eager to share their enthusiasm for Lick Observatory and the skies above. UC OBSERVATORIESSEE MORE ON UCOLICK.ORGFOBOS
With first-light in 2028, FOBOS will be the premier instrument for deep, high-target-density spectroscopy in the era of deep-imaging surveys, like the Vera C. Rubin Observatory Legacy Survey of Space and Time LSST, Euclid, and the Nancy Grace Roman Space Telescope.MY FAMILY TREE
Pedigree. Charles Thomas Maddox Lois Nelle Christen Thomas Michael “Mike” Maddox Susan Lucille Maddox. unknownM Garrity Emily Louise Maddox Anne ElizabethMaddox
THE XIDL CODE
Installation: Installing the code: The code is now distributed via SVN (or you can try to grab a machine-built tarball from above).These notes decribe what do to. MY INTERESTS BEYOND FAMILY AND WORK My interests beyond family and work. In the few minutes a day that I have for myself, they are dominated by athletics (what Europeans refer to as Sport). It used to be I spent all of my time chasing after a ball. These days my body isn’t so up for all of that contact so I find myself climbing on the tops of mountains instead. There was atime
LECTURE 3 ATOMIC SPECTROSCOPY AND ABUNDANCES E m→E n+hν(or E n+hν→ E m)m>n hν= hc λ =E m−E n 1 λ = E m−E n hc = 2π2Z2e4m e h3c 1 n2 − 1 m2 1 λ mn =1.097×105Z2 1 n2 − 1 m2 cm−1 λ mn= 911.6 Z2 1 n2 − 1 m2 −1 Angstroms Radiation in the form of a single quantum (photon) is emittedMY FAMILY TREE
Birth Name: Guy Leslie Leveck Gramps ID: I0605: Gender: male: Age at Death: 23 years, 1 month, 1 dayUC OBSERVATORIES
Proposals for UC observing time on the Keck Telescopes for Semester 2021B are due by 5:00 pm PDT on Thursday, Mar 18th, 2021. There will be 62.5 nights available on K1 and 57 nights available on K2 spread evenly across the semester and lunar phase. There are 7 one-hour Partnership ToO interrupts available. NOTE: There is a new requirementbased
STEVE ALLEN'S HOME PAGE The MOS project is nearly complete. A few docs are seen here. IRAF cl scripts for Lick images. These help astronomers with images from Lick use them in IRAF. The HIRES Spectrograph. I constructed the X11 user interface for the HIRES instrument simulator.LICK OBSERVATORY
Volunteer. The Lick Observatory Volunteers are a dedicated collection of people interested in astronomy and eager to share their enthusiasm for Lick Observatory and the skies above. UC OBSERVATORIESSEE MORE ON UCOLICK.ORGFOBOS
With first-light in 2028, FOBOS will be the premier instrument for deep, high-target-density spectroscopy in the era of deep-imaging surveys, like the Vera C. Rubin Observatory Legacy Survey of Space and Time LSST, Euclid, and the Nancy Grace Roman Space Telescope.MY FAMILY TREE
Pedigree. Charles Thomas Maddox Lois Nelle Christen Thomas Michael “Mike” Maddox Susan Lucille Maddox. unknownM Garrity Emily Louise Maddox Anne ElizabethMaddox
THE XIDL CODE
Installation: Installing the code: The code is now distributed via SVN (or you can try to grab a machine-built tarball from above).These notes decribe what do to. MY INTERESTS BEYOND FAMILY AND WORK My interests beyond family and work. In the few minutes a day that I have for myself, they are dominated by athletics (what Europeans refer to as Sport). It used to be I spent all of my time chasing after a ball. These days my body isn’t so up for all of that contact so I find myself climbing on the tops of mountains instead. There was atime
LECTURE 3 ATOMIC SPECTROSCOPY AND ABUNDANCES E m→E n+hν(or E n+hν→ E m)m>n hν= hc λ =E m−E n 1 λ = E m−E n hc = 2π2Z2e4m e h3c 1 n2 − 1 m2 1 λ mn =1.097×105Z2 1 n2 − 1 m2 cm−1 λ mn= 911.6 Z2 1 n2 − 1 m2 −1 Angstroms Radiation in the form of a single quantum (photon) is emittedMY FAMILY TREE
Birth Name: Guy Leslie Leveck Gramps ID: I0605: Gender: male: Age at Death: 23 years, 1 month, 1 dayLICK OBSERVATORY
Lick Observatory has been at the forefront of astronomy since 1888. Lick Observatory was founded thanks to James Lick, an eccentric California millionaire who dreamed of building a "telescope superior to and more powerful than any telescope yet made."UC OBSERVATORIES
Proposals for UC observing time on the Keck Telescopes for Semester 2021B are due by 5:00 pm PDT on Thursday, Mar 18th, 2021. There will be 62.5 nights available on K1 and 57 nights available on K2 spread evenly across the semester and lunar phase. There are 7 one-hour Partnership ToO interrupts available. NOTE: There is a new requirementbased
STEVE ALLEN'S HOME PAGE The MOS project is nearly complete. A few docs are seen here. IRAF cl scripts for Lick images. These help astronomers with images from Lick use them in IRAF. The HIRES Spectrograph. I constructed the X11 user interface for the HIRES instrument simulator. DAVID KOO'S HOME PAGE David Koo's Home Page UCO/Lick Observatory University of California, Santa Cruz 1156 High Street Santa Cruz, CA 95064 koo@ucolick.org. Latest Modification: TARGET - 2017 May 1 Background (Under Construction): I was faculty (Astronomer and Professor) at the University of California, Santa Cruz from 1988 until summer 2014 whenI retired.
GARTH D. ILLINGWORTH Garth Illingworth is a Professor at the University of California, Santa Cruz. He was a Miller Fellow at UC Berkeley, the Deputy-Director of the Space Telescope Science Institute, and in 2010 was awarded an honorary Doctor of Science degree at the University of WesternAustralia.
MY INTERESTS BEYOND FAMILY AND WORK My interests beyond family and work. In the few minutes a day that I have for myself, they are dominated by athletics (what Europeans refer to as Sport). It used to be I spent all of my time chasing after a ball. These days my body isn’t so up for all of that contact so I find myself climbing on the tops of mountains instead. There was atime
MY FAMILY TREE
This page contains an index of all the surnames in the database. Selecting a link will lead to a list of individuals in the database with this same surname. KECK HIRES SPECTROGRAPH The xhires control room simulator The xhires program is the user interface which is used at the summit to control the HIRES spectrograph. It can be run in a standalone mode without being atMauna Kea.
ABERRATIONS OF THE HUMAN EYE: STRUCTURE Spatial frequency (c/deg) 1 10 100 Modulation transfer 10 20 30 40 50 60 70 80 90 0 10 20 30 40 50 60 70 80 90 0.0 0.2 0.4 0.6 0.8 1.0 RatioAberration-free
3-METER ALUMINIZING: FEBRUARY 2000 A. 3-M. M. F. 2000. The delicate metalic surface of the mirror at the heart of an astronomical telescope must be renewed periodically. When a telescope is pointed to the sky, its mirror is necessarily exposed to the elements. Oxidation and airborn particles such as dust and pollen gradually reduce the mirror's reflectivity, making thetelescope
UC OBSERVATORIES
Proposals for UC observing time on the Keck Telescopes for Semester 2021B are due by 5:00 pm PDT on Thursday, Mar 18th, 2021. There will be 62.5 nights available on K1 and 57 nights available on K2 spread evenly across the semester and lunar phase. There are 7 one-hour Partnership ToO interrupts available. NOTE: There is a new requirementbased
STEVE ALLEN'S HOME PAGE The MOS project is nearly complete. A few docs are seen here. IRAF cl scripts for Lick images. These help astronomers with images from Lick use them in IRAF. The HIRES Spectrograph. I constructed the X11 user interface for the HIRES instrument simulator.LICK OBSERVATORY
Volunteer. The Lick Observatory Volunteers are a dedicated collection of people interested in astronomy and eager to share their enthusiasm for Lick Observatory and the skies above. UC OBSERVATORIESSEE MORE ON UCOLICK.ORGFOBOS
With first-light in 2028, FOBOS will be the premier instrument for deep, high-target-density spectroscopy in the era of deep-imaging surveys, like the Vera C. Rubin Observatory Legacy Survey of Space and Time LSST, Euclid, and the Nancy Grace Roman Space Telescope.MY FAMILY TREE
Pedigree. Charles Thomas Maddox Lois Nelle Christen Thomas Michael “Mike” Maddox Susan Lucille Maddox. unknownM Garrity Emily Louise Maddox Anne ElizabethMaddox
THE XIDL CODE
Installation: Installing the code: The code is now distributed via SVN (or you can try to grab a machine-built tarball from above).These notes decribe what do to. MY INTERESTS BEYOND FAMILY AND WORK My interests beyond family and work. In the few minutes a day that I have for myself, they are dominated by athletics (what Europeans refer to as Sport). It used to be I spent all of my time chasing after a ball. These days my body isn’t so up for all of that contact so I find myself climbing on the tops of mountains instead. There was atime
LECTURE 3 ATOMIC SPECTROSCOPY AND ABUNDANCES E m→E n+hν(or E n+hν→ E m)m>n hν= hc λ =E m−E n 1 λ = E m−E n hc = 2π2Z2e4m e h3c 1 n2 − 1 m2 1 λ mn =1.097×105Z2 1 n2 − 1 m2 cm−1 λ mn= 911.6 Z2 1 n2 − 1 m2 −1 Angstroms Radiation in the form of a single quantum (photon) is emittedMY FAMILY TREE
Birth Name: Guy Leslie Leveck Gramps ID: I0605: Gender: male: Age at Death: 23 years, 1 month, 1 dayUC OBSERVATORIES
Proposals for UC observing time on the Keck Telescopes for Semester 2021B are due by 5:00 pm PDT on Thursday, Mar 18th, 2021. There will be 62.5 nights available on K1 and 57 nights available on K2 spread evenly across the semester and lunar phase. There are 7 one-hour Partnership ToO interrupts available. NOTE: There is a new requirementbased
STEVE ALLEN'S HOME PAGE The MOS project is nearly complete. A few docs are seen here. IRAF cl scripts for Lick images. These help astronomers with images from Lick use them in IRAF. The HIRES Spectrograph. I constructed the X11 user interface for the HIRES instrument simulator.LICK OBSERVATORY
Volunteer. The Lick Observatory Volunteers are a dedicated collection of people interested in astronomy and eager to share their enthusiasm for Lick Observatory and the skies above. UC OBSERVATORIESSEE MORE ON UCOLICK.ORGFOBOS
With first-light in 2028, FOBOS will be the premier instrument for deep, high-target-density spectroscopy in the era of deep-imaging surveys, like the Vera C. Rubin Observatory Legacy Survey of Space and Time LSST, Euclid, and the Nancy Grace Roman Space Telescope.MY FAMILY TREE
Pedigree. Charles Thomas Maddox Lois Nelle Christen Thomas Michael “Mike” Maddox Susan Lucille Maddox. unknownM Garrity Emily Louise Maddox Anne ElizabethMaddox
THE XIDL CODE
Installation: Installing the code: The code is now distributed via SVN (or you can try to grab a machine-built tarball from above).These notes decribe what do to. MY INTERESTS BEYOND FAMILY AND WORK My interests beyond family and work. In the few minutes a day that I have for myself, they are dominated by athletics (what Europeans refer to as Sport). It used to be I spent all of my time chasing after a ball. These days my body isn’t so up for all of that contact so I find myself climbing on the tops of mountains instead. There was atime
LECTURE 3 ATOMIC SPECTROSCOPY AND ABUNDANCES E m→E n+hν(or E n+hν→ E m)m>n hν= hc λ =E m−E n 1 λ = E m−E n hc = 2π2Z2e4m e h3c 1 n2 − 1 m2 1 λ mn =1.097×105Z2 1 n2 − 1 m2 cm−1 λ mn= 911.6 Z2 1 n2 − 1 m2 −1 Angstroms Radiation in the form of a single quantum (photon) is emittedMY FAMILY TREE
Birth Name: Guy Leslie Leveck Gramps ID: I0605: Gender: male: Age at Death: 23 years, 1 month, 1 dayLICK OBSERVATORY
Lick Observatory has been at the forefront of astronomy since 1888. Lick Observatory was founded thanks to James Lick, an eccentric California millionaire who dreamed of building a "telescope superior to and more powerful than any telescope yet made."UC OBSERVATORIES
Proposals for UC observing time on the Keck Telescopes for Semester 2021B are due by 5:00 pm PDT on Thursday, Mar 18th, 2021. There will be 62.5 nights available on K1 and 57 nights available on K2 spread evenly across the semester and lunar phase. There are 7 one-hour Partnership ToO interrupts available. NOTE: There is a new requirementbased
STEVE ALLEN'S HOME PAGE The MOS project is nearly complete. A few docs are seen here. IRAF cl scripts for Lick images. These help astronomers with images from Lick use them in IRAF. The HIRES Spectrograph. I constructed the X11 user interface for the HIRES instrument simulator. DAVID KOO'S HOME PAGE David Koo's Home Page UCO/Lick Observatory University of California, Santa Cruz 1156 High Street Santa Cruz, CA 95064 koo@ucolick.org. Latest Modification: TARGET - 2017 May 1 Background (Under Construction): I was faculty (Astronomer and Professor) at the University of California, Santa Cruz from 1988 until summer 2014 whenI retired.
GARTH D. ILLINGWORTH Garth Illingworth is a Professor at the University of California, Santa Cruz. He was a Miller Fellow at UC Berkeley, the Deputy-Director of the Space Telescope Science Institute, and in 2010 was awarded an honorary Doctor of Science degree at the University of WesternAustralia.
MY INTERESTS BEYOND FAMILY AND WORK My interests beyond family and work. In the few minutes a day that I have for myself, they are dominated by athletics (what Europeans refer to as Sport). It used to be I spent all of my time chasing after a ball. These days my body isn’t so up for all of that contact so I find myself climbing on the tops of mountains instead. There was atime
MY FAMILY TREE
This page contains an index of all the surnames in the database. Selecting a link will lead to a list of individuals in the database with this same surname. KECK HIRES SPECTROGRAPH The xhires control room simulator The xhires program is the user interface which is used at the summit to control the HIRES spectrograph. It can be run in a standalone mode without being atMauna Kea.
ABERRATIONS OF THE HUMAN EYE: STRUCTURE Spatial frequency (c/deg) 1 10 100 Modulation transfer 10 20 30 40 50 60 70 80 90 0 10 20 30 40 50 60 70 80 90 0.0 0.2 0.4 0.6 0.8 1.0 RatioAberration-free
3-METER ALUMINIZING: FEBRUARY 2000 A. 3-M. M. F. 2000. The delicate metalic surface of the mirror at the heart of an astronomical telescope must be renewed periodically. When a telescope is pointed to the sky, its mirror is necessarily exposed to the elements. Oxidation and airborn particles such as dust and pollen gradually reduce the mirror's reflectivity, making thetelescope
UC OBSERVATORIESSUMMER SERIESMOUNT HAMILTON HOMEPAGELICK OBSERVATORY Operates on behalf of the astronomers at all ten UC campuses and is comprised of extensive technical facilities, a business office, telescope and support facilities at the Lick Observatory on Mt Hamilton and a staff of astronomers.LICK OBSERVATORY
Lick Observatory has been at the forefront of astronomy since 1888. Lick Observatory was founded thanks to James Lick, an eccentric California millionaire who dreamed of building a "telescope superior to and more powerful than any telescope yet made."FOBOS
With first-light in 2028, FOBOS will be the premier instrument for deep, high-target-density spectroscopy in the era of deep-imaging surveys, like the Vera C. Rubin Observatory Legacy Survey of Space and Time LSST, Euclid, and the Nancy Grace Roman Space Telescope. KEVIN BUNDY: RESEARCH Kevin Bundy: Research. The MaNGA survey has revealed a new class of galaxies called “red geysers” that harbor supermassive black holes with winds that have the power to keep dormant galaxies quiet. You can read the Nature discovery paper by Edmond Cheung, myself, and the MaNGA team or check out press coverage from the PBS Newshour, the UK'sMY FAMILY TREE
Pedigree. Charles Thomas Maddox Lois Nelle Christen Thomas Michael “Mike” Maddox Susan Lucille Maddox. unknownM Garrity Emily Louise Maddox Anne ElizabethMaddox
DEI, A TRADEMARK OF DABNEY HOVSE DEI Page The letters DEI and their lowercase Greek equivalents have long been associated with Dabney House at Caltech.The origin of this trigraph dates so far back that there is no hard evidence, onlylegends.
XDF PROJECT
The XDF is the deepest image of the sky taken with Hubble for searching for the earliest galaxies. It includes ALL images taken by Hubble on the small patch of sky first imaged as the Hubble Ultra-Deep Field (HUDF) and subsequently as the HUDF09 and HUDF12. The XDF also adds images that overlapped the HUDF from many other programsincluding
LECTURE 3 ATOMIC SPECTROSCOPY AND ABUNDANCES E m→E n+hν(or E n+hν→ E m)m>n hν= hc λ =E m−E n 1 λ = E m−E n hc = 2π2Z2e4m e h3c 1 n2 − 1 m2 1 λ mn =1.097×105Z2 1 n2 − 1 m2 cm−1 λ mn= 911.6 Z2 1 n2 − 1 m2 −1 Angstroms Radiation in the form of a single quantum (photon) is emittedMY FAMILY TREE
Birth Name: Guy Leslie Leveck Gramps ID: I0605: Gender: male: Age at Death: 23 years, 1 month, 1 day CFAO | AO SOFTWARE | AO SIMUTATION PACKAGE Adaptive Optics (AO) Simulation Package. Synopsis: Software to Simulate an Astronomical Adaptive Optics System. Simulates a system with a telescope, deformable mirror (either piezo stack or bimorph), wavefront sensor (either a curvature wavefront sensor or a Shack-Hartman wavefront sensor) and runs a simulation of the closedloop performance.
UC OBSERVATORIESSUMMER SERIESMOUNT HAMILTON HOMEPAGELICK OBSERVATORY Operates on behalf of the astronomers at all ten UC campuses and is comprised of extensive technical facilities, a business office, telescope and support facilities at the Lick Observatory on Mt Hamilton and a staff of astronomers.LICK OBSERVATORY
Lick Observatory has been at the forefront of astronomy since 1888. Lick Observatory was founded thanks to James Lick, an eccentric California millionaire who dreamed of building a "telescope superior to and more powerful than any telescope yet made."FOBOS
With first-light in 2028, FOBOS will be the premier instrument for deep, high-target-density spectroscopy in the era of deep-imaging surveys, like the Vera C. Rubin Observatory Legacy Survey of Space and Time LSST, Euclid, and the Nancy Grace Roman Space Telescope. KEVIN BUNDY: RESEARCH Kevin Bundy: Research. The MaNGA survey has revealed a new class of galaxies called “red geysers” that harbor supermassive black holes with winds that have the power to keep dormant galaxies quiet. You can read the Nature discovery paper by Edmond Cheung, myself, and the MaNGA team or check out press coverage from the PBS Newshour, the UK'sMY FAMILY TREE
Pedigree. Charles Thomas Maddox Lois Nelle Christen Thomas Michael “Mike” Maddox Susan Lucille Maddox. unknownM Garrity Emily Louise Maddox Anne ElizabethMaddox
DEI, A TRADEMARK OF DABNEY HOVSE DEI Page The letters DEI and their lowercase Greek equivalents have long been associated with Dabney House at Caltech.The origin of this trigraph dates so far back that there is no hard evidence, onlylegends.
XDF PROJECT
The XDF is the deepest image of the sky taken with Hubble for searching for the earliest galaxies. It includes ALL images taken by Hubble on the small patch of sky first imaged as the Hubble Ultra-Deep Field (HUDF) and subsequently as the HUDF09 and HUDF12. The XDF also adds images that overlapped the HUDF from many other programsincluding
LECTURE 3 ATOMIC SPECTROSCOPY AND ABUNDANCES E m→E n+hν(or E n+hν→ E m)m>n hν= hc λ =E m−E n 1 λ = E m−E n hc = 2π2Z2e4m e h3c 1 n2 − 1 m2 1 λ mn =1.097×105Z2 1 n2 − 1 m2 cm−1 λ mn= 911.6 Z2 1 n2 − 1 m2 −1 Angstroms Radiation in the form of a single quantum (photon) is emittedMY FAMILY TREE
Birth Name: Guy Leslie Leveck Gramps ID: I0605: Gender: male: Age at Death: 23 years, 1 month, 1 day CFAO | AO SOFTWARE | AO SIMUTATION PACKAGE Adaptive Optics (AO) Simulation Package. Synopsis: Software to Simulate an Astronomical Adaptive Optics System. Simulates a system with a telescope, deformable mirror (either piezo stack or bimorph), wavefront sensor (either a curvature wavefront sensor or a Shack-Hartman wavefront sensor) and runs a simulation of the closedloop performance.
UC OBSERVATORIES
Operates on behalf of the astronomers at all ten UC campuses and is comprised of extensive technical facilities, a business office, telescope and support facilities at the Lick Observatory on Mt Hamilton and a staff of astronomers.FOBOS
With first-light in 2028, FOBOS will be the premier instrument for deep, high-target-density spectroscopy in the era of deep-imaging surveys, like the Vera C. Rubin Observatory Legacy Survey of Space and Time LSST, Euclid, and the Nancy Grace Roman Space Telescope.XDF PROJECT
The XDF is the deepest image of the sky taken with Hubble for searching for the earliest galaxies. It includes ALL images taken by Hubble on the small patch of sky first imaged as the Hubble Ultra-Deep Field (HUDF) and subsequently as the HUDF09 and HUDF12. PROFESSOR PIERO MADAU Educational Background: B.A., Florence University Ph.D., International School for Advanced Studies, Trieste Research Interest: Piero Madau's research interests in the last few years have focused on theoretical cosmology and the high-redshift universe, especially on the physics of the intergalactic medium and the history of star formation ingalaxies.
PEOPLE INVOLVED
John Huchra, Smithsonian Center for Astrophysics . Pauline Barmby, Smithsonian Center for Astrophysics . Katherine Rhode, Wesleyan/Yale WHAT ARE SOME MAJOR CHALLENGES OF HUMAN SPACE EXPLORATION 3) Energy - human settlements will need to create their own energy. Close to the sun (say, within the asteroid belt), solar power is useable. Outside of the asteroid belt, nuclear power would most likely have to be used. There are advantages and disadvantages to each type of power. 4) Radiation - radiation is harmful for people, plants andanimals.
LECTURE 3 ATOMIC SPECTROSCOPY AND ABUNDANCES E m→E n+hν(or E n+hν→ E m)m>n hν= hc λ =E m−E n 1 λ = E m−E n hc = 2π2Z2e4m e h3c 1 n2 − 1 m2 1 λ mn =1.097×105Z2 1 n2 − 1 m2 cm−1 λ mn= 911.6 Z2 1 n2 − 1 m2 −1 Angstroms Radiation in the form of a single quantum (photon) is emittedTHE XIDL CODE
Installation: Installing the code: The code is now distributed via SVN (or you can try to grab a machine-built tarball from above).These notes decribe what do to. LICK OBSERVATORY, CURRENT WEBCAM IMAGES Our webcam images are used for both public outreach and scientific purposes, such as monitoring the weather and the status of the telescope domes and facilities. Hence, the time stamps on our webcam images are always in Pacific Standard Time, even when Pacific Daylight Time is in effect. 2016 APF 2.4-m Telescope Mirror Aluminizing Movies. CFAO | AO SOFTWARE | AO SIMUTATION PACKAGE Adaptive Optics (AO) Simulation Package. Synopsis: Software to Simulate an Astronomical Adaptive Optics System. Simulates a system with a telescope, deformable mirror (either piezo stack or bimorph), wavefront sensor (either a curvature wavefront sensor or a Shack-Hartman wavefront sensor) and runs a simulation of the closedloop performance.
LICK OBSERVATORY
Lick Observatory has been at the forefront of astronomy since 1888. Lick Observatory was founded thanks to James Lick, an eccentric California millionaire who dreamed of building a "telescope superior to and more powerful than any telescope yet made." KEVIN BUNDY: RESEARCH I am the founder and Principal Investigator of MaNGA, one of three programs in the 4th Sloan Digital Sky Survey (SDSS-IV).MaNGA stands for Mappiang Nearby Galaxies at Apache Point Observatory and in Aug 2020 reached its goal of resolved spectroscopy for an unprecedented10,000 galaxies.
UC OBSERVATORIESSEE MORE ON UCOLICK.ORG DEI, A TRADEMARK OF DABNEY HOVSE DEI Page The letters DEI and their lowercase Greek equivalents have long been associated with Dabney House at Caltech.The origin of this trigraph dates so far back that there is no hard evidence, onlylegends.
MY INTERESTS BEYOND FAMILY AND WORK There was a time when I played all sorts of games as well: chess, bridge, xblast, intellivision, stratego, Mao-Mao. You name it. Maybe those days will return as the boys age.FOBOS
With first-light in 2028, FOBOS will be the premier instrument for deep, high-target-density spectroscopy in the era of deep-imaging surveys, like the Vera C. Rubin Observatory Legacy Survey of Space and Time LSST, Euclid, and the Nancy Grace Roman Space Telescope. PROFESSOR PIERO MADAU Educational Background: B.A., Florence University Ph.D., International School for Advanced Studies, Trieste Research Interest: Piero Madau's research interests in the last few years have focused on theoretical cosmology and the high-redshift universe, especially on the physics of the intergalactic medium and the history of star formation ingalaxies.
MY FAMILY TREE
Generated by Gramps 5.0.1 Last change was the 2014-10-12 23:45:11 ©2021 Steve Allen
CFAO | AO SOFTWARE | AO SIMUTATION PACKAGE Adaptive Optics (AO) Simulation Package. Synopsis: Software to Simulate an Astronomical Adaptive Optics System. Simulates a system with a telescope, deformable mirror (either piezo stack or bimorph), wavefront sensor (either a curvature wavefront sensor or a Shack-Hartman wavefront sensor) and runs a simulation of the closedloop performance.
MY FAMILY TREE
Birth Name: Guy Leslie Leveck Gramps ID: I0605: Gender: male: Age at Death: 23 years, 1 month, 1 dayLICK OBSERVATORY
Lick Observatory has been at the forefront of astronomy since 1888. Lick Observatory was founded thanks to James Lick, an eccentric California millionaire who dreamed of building a "telescope superior to and more powerful than any telescope yet made." KEVIN BUNDY: RESEARCH I am the founder and Principal Investigator of MaNGA, one of three programs in the 4th Sloan Digital Sky Survey (SDSS-IV).MaNGA stands for Mappiang Nearby Galaxies at Apache Point Observatory and in Aug 2020 reached its goal of resolved spectroscopy for an unprecedented10,000 galaxies.
UC OBSERVATORIESSEE MORE ON UCOLICK.ORG DEI, A TRADEMARK OF DABNEY HOVSE DEI Page The letters DEI and their lowercase Greek equivalents have long been associated with Dabney House at Caltech.The origin of this trigraph dates so far back that there is no hard evidence, onlylegends.
MY INTERESTS BEYOND FAMILY AND WORK There was a time when I played all sorts of games as well: chess, bridge, xblast, intellivision, stratego, Mao-Mao. You name it. Maybe those days will return as the boys age.FOBOS
With first-light in 2028, FOBOS will be the premier instrument for deep, high-target-density spectroscopy in the era of deep-imaging surveys, like the Vera C. Rubin Observatory Legacy Survey of Space and Time LSST, Euclid, and the Nancy Grace Roman Space Telescope. PROFESSOR PIERO MADAU Educational Background: B.A., Florence University Ph.D., International School for Advanced Studies, Trieste Research Interest: Piero Madau's research interests in the last few years have focused on theoretical cosmology and the high-redshift universe, especially on the physics of the intergalactic medium and the history of star formation ingalaxies.
MY FAMILY TREE
Generated by Gramps 5.0.1 Last change was the 2014-10-12 23:45:11 ©2021 Steve Allen
CFAO | AO SOFTWARE | AO SIMUTATION PACKAGE Adaptive Optics (AO) Simulation Package. Synopsis: Software to Simulate an Astronomical Adaptive Optics System. Simulates a system with a telescope, deformable mirror (either piezo stack or bimorph), wavefront sensor (either a curvature wavefront sensor or a Shack-Hartman wavefront sensor) and runs a simulation of the closedloop performance.
MY FAMILY TREE
Birth Name: Guy Leslie Leveck Gramps ID: I0605: Gender: male: Age at Death: 23 years, 1 month, 1 dayUC OBSERVATORIES
Operates on behalf of the astronomers at all ten UC campuses and is comprised of extensive technical facilities, a business office, telescope and support facilities at the Lick Observatory on Mt Hamilton and a staff of astronomers.FOBOS
With first-light in 2028, FOBOS will be the premier instrument for deep, high-target-density spectroscopy in the era of deep-imaging surveys, like the Vera C. Rubin Observatory Legacy Survey of Space and Time LSST, Euclid, and the Nancy Grace Roman Space Telescope.XDF PROJECT
The XDF is the deepest image of the sky taken with Hubble for searching for the earliest galaxies. It includes ALL images taken by Hubble on the small patch of sky first imaged as the Hubble Ultra-Deep Field (HUDF) and subsequently as the HUDF09 and HUDF12. PROFESSOR PIERO MADAU Educational Background: B.A., Florence University Ph.D., International School for Advanced Studies, Trieste Research Interest: Piero Madau's research interests in the last few years have focused on theoretical cosmology and the high-redshift universe, especially on the physics of the intergalactic medium and the history of star formation ingalaxies.
LECTURE 3 ATOMIC SPECTROSCOPY AND ABUNDANCES E m→E n+hν(or E n+hν→ E m)m>n hν= hc λ =E m−E n 1 λ = E m−E n hc = 2π2Z2e4m e h3c 1 n2 − 1 m2 1 λ mn =1.097×105Z2 1 n2 − 1 m2 cm−1 λ mn= 911.6 Z2 1 n2 − 1 m2 −1 Angstroms Radiation in the form of a single quantum (photon) is emittedTHE XIDL CODE
Installation: Installing the code: The code is now distributed via SVN (or you can try to grab a machine-built tarball from above).These notes decribe what do to. LICK OBSERVATORY, CURRENT WEBCAM IMAGES 2016 APF 2.4-m Telescope Mirror Aluminizing Movies. 2016 Shane 3-m Telescope Mirror Aluminizing Movies. APF Telescope Installation Time Lapse Movie, 2009 April 21 THE STRUCTURE AND EVOLUTION OF COLD DARK MATTER HALOS The structure and evolution of cold dark matter halos Ju¨rg Diemand∗ Hubble Fellow and Astronomy & Astrophysics, University of California, Santa Cruz, CA 95060, U.S.A. WHAT ARE SOME MAJOR CHALLENGES OF HUMAN SPACE EXPLORATION Hello, You've asked for much more information than I could type in a reasonable amount of time, so I hope you don't mind if I point you toward a good resource and CFAO | AO SOFTWARE | AO SIMUTATION PACKAGE Adaptive Optics (AO) Simulation Package. Synopsis: Software to Simulate an Astronomical Adaptive Optics System. Simulates a system with a telescope, deformable mirror (either piezo stack or bimorph), wavefront sensor (either a curvature wavefront sensor or a Shack-Hartman wavefront sensor) and runs a simulation of the closedloop performance.
Fire Emergency: The list of immediate needs is growing and our priorities may need to evolve with circumstances. YOUR GIFT TO THE UCO DIRECTOR’S DISCRETIONARY FUND TODAY WILL PROVIDE THE FLEXIBLE SUPPORT NECESSARY FOR DIRECTOR MAX TO ADDRESS NEEDS AS THEY ARISE IN THIS RAPIDLY CHANGING SITUATION. WELCOME TO UC OBSERVATORIES. THE OLD UCO WEB PAGES HAVE BEEN UPDATED AND NOW CAN BE FOUND AT:The new UC Observatoriesweb pages
TO CONTINUE TO THE LICK OBSERVATORY PAGE:LICK OBSERVATORY
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