Kurt Adelberger | |
|---|---|
| Nationality | American |
| Education | Ph.D. from California Institute of Technology, B.S. in astronomy from Harvey Mudd College, |
| Known for | Astrophysics, Sustainability |
| Spouse | Amy Adelberger |
| Relatives | Theodore Welton (grandfather in law) |
| Awards | Junior Fellow at Harvard University |
Kurt Ludvig Adelberger is an American astrophysicist and sustainability manager, who formerly worked at Google as a principal in energy and sustainability and was previously the Engagement Manager for McKinsey & Company. [1]
He earned his B.S. at Harvey Mudd College and a Ph.D. from the California Institute of Technology, where he was advised by Charles C. Steidel. [2] His thesis was entitled Star formation and structure formation at redshifts 1 < z < 4 and has been cited in 31 other papers. He defended his thesis in 2001. [3]
Prior to working at Mckinsey & Company, Adelberger worked at Carnegie Observatories. [1] He has published 194 papers in the field of astrophysics, and has been cited over 2000 times. [4] In 2000, Adelberger was named a junior fellow of Harvard University. [2]
His notable publications include Lyman-Break Galaxies at z 4 and theEvolution of the Ultraviolet Luminosity Density at High Redshift, cited by 1945 other articles and Spectroscopic confirmation of a population of normal star-forming galaxies at redshifts z> 3 cited by 1766 other articles. He has spoken at GreenBiz on how distributed generation will influence grid evolution. [5] He also holds the patent for a thermostat system which allows the user to specify a range of acceptable temperatures. [6]
In the fields of Big Bang theory and cosmology, reionization is the process that caused electrically neutral atoms in the universe to reionize after the lapse of the "dark ages".
Rychard J. Bouwens is an associate professor at Leiden University. He is also a former member of the Advanced Camera for Surveys Guaranteed Time Observation team and postdoctoral research astronomer at the University of California, Santa Cruz. He obtained his bachelor's degree in physics, chemistry, and mathematics from Hope College. He then went on to earn his Ph.D. in physics at the University of California, Berkeley under the supervision of Joseph Silk and also worked with Tom Broadhurst.
In astronomy, a Lyman-alpha blob (LAB) is a huge concentration of a gas emitting the Lyman-alpha emission line. LABs are some of the largest known individual objects in the Universe. Some of these gaseous structures are more than 400,000 light years across. So far they have only been found in the high-redshift universe because of the ultraviolet nature of the Lyman-alpha emission line. Since Earth's atmosphere is very effective at filtering out UV photons, the Lyman-alpha photons must be redshifted in order to be transmitted through the atmosphere.
GRB 970508 was a gamma-ray burst (GRB) detected on May 8, 1997, at 21:42 UTC; it is historically important as the second GRB with a detected afterglow at other wavelengths, the first to have a direct redshift measurement of the afterglow, and the first to be detected at radio wavelengths.
Lyman-break galaxies are star-forming galaxies at high redshift that are selected using the differing appearance of the galaxy in several imaging filters due to the position of the Lyman limit. The technique has primarily been used to select galaxies at redshifts of z = 3–4 using ultraviolet and optical filters, but progress in ultraviolet astronomy and in infrared astronomy has allowed the use of this technique at lower and higher redshifts using ultraviolet and near-infrared filters.
The SSA22 Protocluster, also known as EQ J221734.0+001701, is a galaxy protocluster located at z=3.1 in the SSA 22 region. It is located at 22h 17m 34.0s +00° 17′ 01″ and was originally discovered in 1998.
Lyman-alpha blob 1 (LAB-1) is a giant cosmic cloud of gas located in the constellation of Aquarius, approximately 11.5 billion light-years from Earth with a redshift (z) of 3.09. It was discovered unexpectedly in 2000 by Charles Steidel and colleagues, who were surveying for high-redshift galaxies using the 200 inch Hale Telescope at the Palomar Observatory. The researchers had been investigating the abundance of galaxies in the young Universe when they came across two objects which would become known as Lyman-alpha blobs—huge concentrations of gases emitting the Lyman-alpha emission line of hydrogen.
Alice Eve Shapley is a professor at the University of California, Los Angeles (UCLA) in the Department of Physics and Astronomy. She was one of the discoverers of the spiral galaxy BX442. Through her time at University of California, Los Angeles (UCLA) she has taught Nature of the Universe, Black Holes and Cosmic Catastrophes, Cosmology: Our Changing Concepts of the Universe, Galaxies, Scientific Writing, AGNs, Galaxies, *and* Writing, and The Formation and Evolution of Galaxies and the IGM. Shapley has committed herself to over a two decades of research and publication in the interest of physics and astronomy.
Benedetta Ciardi is an Italian astrophysicist.
TON 618 is a hyperluminous, broad-absorption-line, radio-loud quasar, and Lyman-alpha blob located near the border of the constellations Canes Venatici and Coma Berenices, with the projected comoving distance of approximately 18.2 billion light-years from Earth. It possesses one of the most massive black holes ever found, at 40.7 billion M☉.
Q2343-BX418 is a young, low-metallicity dwarf galaxy located about 10 billion light years away from Earth. It has a redshift of 2.3052, and a stellar mass of 500 million solar masses.
Dawn K. Erb is an American physicist. She is an associate professor in the department of physics at the University of Wisconsin–Milwaukee.
Marc Alexander Rafelski is an American astrophysicist. Rafelski studied astronomy at the University of California, Los Angeles with Andrea Gehz. He obtained his PhD in physics from the University of California, San Diego, under supervision of Arthur Wolfe, in 2011.
UM 287 known as PHL 868 and LBQS 0049+0045, is a quasar located in the Cetus constellation. Its redshift is 2.267134 estimating the object to be located 10.9 billion light-years away from Earth.
MRC 0316-257 is a radio galaxy located in the constellation Fornax. Its redshift is 3.13, making the object located roughly 11 billion light-years from Earth.
4C +72.26 known as NAME TX J1908+7220, is a radio galaxy located in the constellation Draco. At the redshift of 3.53, the galaxy is located roughly 11.5 billion light-years from Earth.
PKS 0529-549 known as MRC 0529-549 and PKS B0529-549, is a radio galaxy located in the constellation Pictor. At the redshift of 2.57, the object is located nearly 10.8 billion light-years away from Earth.
4C +41.17 is a radio galaxy located in the constellation Auriga. With the redshift of 3.79, it is located nearly 11.7 billion light-years from Earth. At the time of its discovery in 1988, it was one of the most distant galaxies ever seen.
Abell 1942 BCG, also known as PGC 1256558, is a massive elliptical galaxy of type-cD residing as the brightest cluster galaxy of the Abell 1942 galaxy cluster, located in the constellation Virgo. With a redshift of 0.224, the galaxy is located nearly 2.7 billion light-years away from Earth.