Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.apo.nmsu.edu/35m_operations/35m_manual/General_Information/Spectra/DIS/OLD_Spectra/callamps2.html
Дата изменения: Wed Jan 24 13:19:54 2007
Дата индексирования: Sun Apr 10 11:00:39 2016
Кодировка:

Поисковые слова: comet tail
APO Lamp Spectra

APO LAMP SPECTRA

These lamp spectra are compiled from imagestaken during February and June 1996. The images were taken with the newest lamp configuration (lamps pointed down toward closedmirror covers). Spectra listed in boldface were taken throughthe 1.6 arcsec slit. All other spectra were taken through the 1.0arcsec slit.

Low Dispersion

High Dispersion

LAMP

BLUE

RED

BLUE

RED

Argon

4400Å

7700Å

4400Å

7300Å
8000Å
8800Å
9600Å

Helium

4400Å

7700Å

Hydrogen

4400Å

7700Å

Krypton

4400Å

7700Å

4400Å

7800Å
5500Å
8600Å

Mercury

4400Å

7700Å

4400Å
5200Å

5600Å

Neon

4400Å

7700Å

5100Å

6000Å
6800Å
7600Å
8400Å

Xenon

4400Å

7700Å

8200Å
9000Å
9800Å


More lamp spectra will be added.
High resolution He spectra can be found on the Old APO LampSpectra page.

In each image ten columns were averagedusing the IRAF combine task. The pixel values wereextracted with the IRAF listpix task. The images have notbeen bias subtracted or flattened. What you see here is what you getout of the spectrograph. Exposure time and counts are listed oneach plot. The plots were created with Kaleidagraph(tm). For eachimage the wavelength listed is the approximate central wavelength.Most of the line identifications for He, Ne, and Ar are from theprevious version of APO lamp spectra, provided by Bruce Balick andAndrew Dolphin


K. Gloria