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Hemoglobin F-Caltech

Known as: HBGG g.1369A>C, Hb F-Caltech, Hemoglobin F Caltech 
National Institutes of Health

Related topics

Related topics

3 relations

Broader (2)

Abnormal HemoglobinsFetal Hemoglobin
Hemoglobin Takamatsu

Papers overview

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2009
2009
How and When do Planets Form? The Inner Regions of Planet Forming Disks at High Spatial and Spectral Resolution
The formation of planets is one of the major unsolved problems in modern astrophysics. Planets are believed to form out of the… 
2009
2009
A Caltech Submillimeter Observatory Active Optics System
Active surface correction of the Caltech Submillimeter Observatory (CSO) primary mirror has been accomplished. The Dish Surface… 
2008
2008
Radio source counts at 30 GHz
We observe 1,377 NVSS point sources with the Green Bank Telescope (GBT) and Caltech Continuum Backend (CCB) at 31.25 GHz. We find… 
2008
2008
02 08 44 8 v 1 2 5 A ug 2 00 2 Seeing Statistics at the Upgraded 3 . 8 m UK Infrared Telescope ( UKIRT )
From 1991 until 1997, the 3.8m UK Infrared Telescope (UKIRT) underwent a programme of upgrades aimed at improving its intrinsic… 
2006
2006
To appear in SPIE 6275 ( 2006 ) 1 Instrumentation for the CCAT Telescope
We present a first cut instrument design package for the proposed 25 meter Cornell-Caltech Atacama Telescope (CCAT). The primary… 
2005
2005
350-μ m SHARC-II Imaging of Luminous High-z Radio Galaxies
Using the filled bolometer array SHARC-II on the Caltech Submillimeter Observatory (CSO), we have obtained deep (σrms ∼ 15 mJy… 
2002
2002
Observations of carbon monoxide in the starburst galaxy M82 with a 690 GHz-wide spectral bandwidth receiver
A 690 GHz wide spectral bandwidth heterodyne receiver was developed to observe the J=6-5 rotational emission line of carbon… 
1996
1996
A Submillimeter High Angular Resolution Bolometer Array Camera for the Caltech Submillimeter Observatory
Seventh International Symposium on Space Terahertz Technology, Charlottesville, March 1996 6-4 A Submillimeter High Angular… 
1995
1995
Molecular, atomic, and ionized gas in the NGC 6334 star forming region
NGC 6334 is a nearby (1.7 kpc) giant molecular cloud which contains at least 7 distinct sites of massive star formation. Using… 
1994
1994
High Frequency Effects and Performance of a 600 GHz-635 GHz SIS Receiver Using Nb/A10x/Nb Junctions
A 600 GHz - 635 GHz waveguide SIS heterodyne receiver was built and used for astronomical observations at the Caltech… 
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