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The Arecibo Legacy Fast ALFA Survey

Thoughts on the Next Generation Survey:. Counting Low Mass Dark Matter Halos in Nearby Galaxy Groups. ALFALFA: HI Cosmology in the Local Universe. Solar masses and as high as 10. At the low mass end, ALFALFA has already detected several hundred galaxies with HI masses less than 10. Of ALFALFA (blue) on the Sloan Digital Sky Survey (red). Spin-off surveys inspired by ALFALFA:. A comparison of major blind HI surveys and ALFALFA is presented in Table B.1. A 2-pass drift survey. Greatly aids in the rejection...

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The Arecibo Legacy Fast ALFA Survey | egg.astro.cornell.edu Reviews

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Thoughts on the Next Generation Survey:. Counting Low Mass Dark Matter Halos in Nearby Galaxy Groups. ALFALFA: HI Cosmology in the Local Universe. Solar masses and as high as 10. At the low mass end, ALFALFA has already detected several hundred galaxies with HI masses less than 10. Of ALFALFA (blue) on the Sloan Digital Sky Survey (red). Spin-off surveys inspired by ALFALFA:. A comparison of major blind HI surveys and ALFALFA is presented in Table B.1. A 2-pass drift survey. Greatly aids in the rejection...

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The Arecibo Legacy Fast ALFA Survey | egg.astro.cornell.edu Reviews

https://egg.astro.cornell.edu

Thoughts on the Next Generation Survey:. Counting Low Mass Dark Matter Halos in Nearby Galaxy Groups. ALFALFA: HI Cosmology in the Local Universe. Solar masses and as high as 10. At the low mass end, ALFALFA has already detected several hundred galaxies with HI masses less than 10. Of ALFALFA (blue) on the Sloan Digital Sky Survey (red). Spin-off surveys inspired by ALFALFA:. A comparison of major blind HI surveys and ALFALFA is presented in Table B.1. A 2-pass drift survey. Greatly aids in the rejection...

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The Arecibo Legacy Fast ALFA Survey

http://egg.astro.cornell.edu/index.php/coverage.php

ALFALFA was originially intended to cover 7074 square degrees of the high galactic latitude sky accessible to the Arecibo telescope, i.e. the regions between 0° and 36° in Declination (subdivided into 9 bands of tiles, each 4° wide), 07. In Right Ascension. In the end, some parts of the spring sky were observed only from 08. So that the final coverage is only of about 6300 square degrees. 2004), based largely on primary distances. Figure by mph (01/05).

2

The Arecibo Legacy Fast ALFA Survey

http://egg.astro.cornell.edu/alfalfa/ugrad/twopass.htm

ALFALFA 2 pass strategy. The spacing of the sky tracks of the ALFA beams in the 19 deg rotated configuration. Is about 2.1 arcminutes. For a HPBW of 3.5 arcminutes, we would ideally space the beams closer than 2.1 arcmin to get complete resolution. For the second pass, we want the beams to produce drift scan tracks that are halfway between the ones of the first pass, producing a final spacing of 1.05 arcminutes. Back to ALFA for ALFALFA. Last modified: Sun Oct 7 11:44:33 EST 2007 by martha.

3

The Arecibo Legacy Fast ALFA Survey

http://egg.astro.cornell.edu/alfalfa/people.php

ALFALFA science collaboration guidelines and projects. Below is a list of persons committed to contributing to this effort, including affiliations, level of effort and task assignment. Names highlighted in green indicate members of the ALFALFA Oversight Committee. Software development, simulations. Zw1400 0949; serious flaggbb'ing; undergrad education; coqui recordings. U Wisconsin - Madison. Synthesis observations followup; low mass galaxies. Rotation in low mass galaxies; SDSS photometry. Using ALFALFA...

4

The Arecibo Legacy Fast ALFA Survey

http://egg.astro.cornell.edu/alfalfa/ugrad/observingmode.htm

The observing mode used for ALFALFA is about as simple as it gets. We park the telescope on the meridian, and let the sky drift by. This is called "fixed azimuth drift mode". The seven beams of ALFA. Sweep across seven parallel tracks of sky. We rotate. The array by 19 degrees so that the beams tracks follow lines of constant declination, each offset from the other by 2.1 arcminutes. Beam 0, which is more sensitive (has higher gain) than the others remains at the center of the array.

5

The Arecibo Legacy Fast ALFA Survey

http://egg.astro.cornell.edu/alfalfa/index.php

Thoughts on the Next Generation Survey:. Counting Low Mass Dark Matter Halos in Nearby Galaxy Groups. ALFALFA: HI Cosmology in the Local Universe. Solar masses and as high as 10. At the low mass end, ALFALFA has already detected several hundred galaxies with HI masses less than 10. Of ALFALFA (blue) on the Sloan Digital Sky Survey (red). Spin-off surveys inspired by ALFALFA:. A comparison of major blind HI surveys and ALFALFA is presented in Table B.1. A 2-pass drift survey. Greatly aids in the rejection...

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nsatlas.org

NASA-Sloan Atlas

http://www.nsatlas.org/documentation

The NASA-Sloan Atlas sample was selected to include virtually all known redshifts out to about. For galaxies with in the coverage of SDSS DR8. For each such galaxy, we have created image mosaics from SDSS and GALEX and rephotometered the. Bands plus the far and near ultraviolet bands in a self-consistent manner. After cleaning a number of suspicious cases the final catalog contains about 140,000 galaxies. Six-degree Field Galaxy Redshift Survey. Two-degree Field Galaxy Redshift Survey. Each galaxy is giv...

nsatlas.org

NASA-Sloan Atlas

http://www.nsatlas.org/data

The NASA-Sloan Atlas data is available in flat-file form, which we document and link to here. See the search. Page for on-line searching and browsing of the galaxies. See the documentation. For a more detailed description of our methods and the caveats. For a list of known problems. Below please find information about how to access the FITS images. For the master file, some source catalog information. The current catalog can be obtained as single FITS format file (0.5 Gb):. Nsa v0 1 2.fits. The full mosa...

rhysy.net

Mapping the Universe

http://www.rhysy.net/mapping-the-universe-1.html

Project I did a lot of things the hard way - downloading the images one at time, manually removing foreground stars. manually setting the images in Blender. About the only bit of automation was a Python code to position and scale the planes correctly. That severely limits the number of galaxies which can be displayed, 'cos any more than a few hundred might break my delicate typin' fingers. To cut a short story into an even more compact and readable format, for this I used the. Sloan Digital Sky Survey.

bret.io

Projects ~ bret.io

http://bret.io/pages/projects

This is a list of personal projects from the past few years. I am still putting the page together, so send a PR. If you spot an error anywhere! There are lots of pictures so that its more interesting to browse. Feel free to let me know if you would like any more info on any of these topics. SEMterface aims to put a Scanning Electron Microscope onto the Internet using websockets. For great good and earn me a masters degree in applied physics. Pictures from webRTC Camp 2013 in Portland, OR. LaTeX Font Sizi...

melissajacquart.com

About Me – Melissa Jacquart

http://melissajacquart.com/about-me

Blogs & Resources. I grew up in Saint Paul, Minnesota and attended the University of Wisconsin – Madison. Where I received my B.S. triple majoring in Astronomy, Philosophy, and Physics. Originally planning to pursue an life as an astronomer, I worked in the astronomy department. With Prof. Eric Wilcots. In Puerto Rico through assisting with the Arecibo Legacy Fast ALFA Survey. ALFALFA), as well as on-site observational experience with the WIYN 0.9m telescope. Directorate. I worked in the MMSTS cluste...

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egg.astro.cornell.edu

The Arecibo Legacy Fast ALFA Survey

Thoughts on the Next Generation Survey:. Counting Low Mass Dark Matter Halos in Nearby Galaxy Groups. ALFALFA: HI Cosmology in the Local Universe. Solar masses and as high as 10. At the low mass end, ALFALFA has already detected several hundred galaxies with HI masses less than 10. Of ALFALFA (blue) on the Sloan Digital Sky Survey (red). Spin-off surveys inspired by ALFALFA:. A comparison of major blind HI surveys and ALFALFA is presented in Table B.1. A 2-pass drift survey. Greatly aids in the rejection...

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