H. W. De Vries
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View article: Replication data for: Ursa Major, de Vries (DHT20)
Replication data for: Ursa Major, de Vries (DHT20) Open
Owing to the high latitude of this survey, the longitude spacing of the observations is 0.1429 °, slightly larger than our normal "beamwidth" spacing of 0.125°. For incorporation into the whole-Galaxy cubes presented elsewhere in this arch…
View article: Replication data for: Ursa Major, Heithausen (DHT20)
Replication data for: Ursa Major, Heithausen (DHT20) Open
These are two additional clouds in the Ursa Major region reported by Heithausen et al. (1993). Owing to the high latitude of this survey, the longitude spacing of the observations is 0.1429 °, slightly larger than our normal "beamwidth" sp…
View article: Replication data for: Camelopardalis (DHT19)
Replication data for: Camelopardalis (DHT19) Open
Owing to the high latitude of this survey, the longitude spacing of the observations is 0.1429 °, slightly larger than our normal "beamwidth" spacing of 0.125°. For incorporation into the whole-Galaxy cubes presented elsewhere in this arch…
View article: Replication data for: Polaris Flare (DHT16)
Replication data for: Polaris Flare (DHT16) Open
Owing to the high latitude of this survey, the longitude spacing of the observations is 0.1429 °, slightly larger than our normal "beamwidth" spacing of 0.125°. For incorporation into the whole-Galaxy cubes presented elsewhere in the archi…
View article: DHT16_Polaris_interp.fits
DHT16_Polaris_interp.fits Open
DHT16 v-l-b FITS cube, interpolated. In each spectrum, <= 2 missing channels are filled by linear interpolation. In each spatial plane, single missing pixels are filled by linear interpolation, first in l direction, then b.
View article: DHT19_Camelopardalis_interp.fits
DHT19_Camelopardalis_interp.fits Open
DHT19 v-l-b FITS cube, interpolated. In each spectrum, <= 2 missing channels are filled by linear interpolation. In each spatial plane, single missing pixels are filled by linear interpolation, first in l direction, then b.
View article: DHT20_UrsaMaj_Heithausen_mom.fits
DHT20_UrsaMaj_Heithausen_mom.fits Open
DHT20 (Heithausen) v-l-b FITS cube, moment masked
View article: DHT19.jpg
DHT19.jpg Open
Spatial and longitude-velocity maps of DHT19
View article: DHT20_deVries_raw.jpg
DHT20_deVries_raw.jpg Open
Sampling map for DHT20 (de Vries), raw
View article: DHT20_UrsaMaj_deVries_raw.txt
DHT20_UrsaMaj_deVries_raw.txt Open
FITS header for DHT20 (de Vries)
View article: DHT16_Polaris_raw.txt
DHT16_Polaris_raw.txt Open
FITS header for DHT16
View article: DHT16_raw.jpg
DHT16_raw.jpg Open
Sampling map for DHT16, raw
View article: DHT19_interp.jpg
DHT19_interp.jpg Open
Sampling map for DHT19, interpolated
View article: DHT16.jpg
DHT16.jpg Open
Spatial and velocity-latitude maps of DHT16
View article: DHT16_interp.jpg
DHT16_interp.jpg Open
Sampling map for DHT16, interpolated
View article: DHT16_Polaris_bw_mom.fits
DHT16_Polaris_bw_mom.fits Open
DHT16 v-l-b FITS cube, moment masked. It covers the smaller area with uniform beamwidth sampling.
View article: DHT20_UrsaMaj_Heithausen_raw.txt
DHT20_UrsaMaj_Heithausen_raw.txt Open
FITS header for DHT20 (Heithausen)
View article: DHT20_UrsaMaj_deVries_mom.fits
DHT20_UrsaMaj_deVries_mom.fits Open
DHT20 (de Vries) v-l-b FITS cube, moment masked
View article: DHT19_Camelopardalis_qdeg_mom.fits
DHT19_Camelopardalis_qdeg_mom.fits Open
DHT19 v-l-b FITS cube, moment masked. It covers the whole area with 1/4° sampling.
View article: DHT20_deVries_interp.jpg
DHT20_deVries_interp.jpg Open
Sampling map for DHT20 (de Vries), interpolated
View article: DHT19_raw.jpg
DHT19_raw.jpg Open
Sampling map for DHT19, raw
View article: DHT20_deVries.jpg
DHT20_deVries.jpg Open
Spatial and velocity-latitude maps of DHT20 (de Vries)
View article: DHT16_Polaris_qdeg_mom.fits
DHT16_Polaris_qdeg_mom.fits Open
DHT16 v-l-b FITS cube, moment masked. It covers the whole area with 1/4° sampling.
View article: DHT20_UrsaMaj_deVries_interp.fits
DHT20_UrsaMaj_deVries_interp.fits Open
DHT20 (de Vries) v-l-b FITS cube, interpolated. In each spectrum, <= 2 missing channels are filled by linear interpolation. In each spatial plane, single missing pixels are filled by linear interpolation, first in l direction, then b.
View article: DHT20_UrsaMaj_Heithausen_interp.fits
DHT20_UrsaMaj_Heithausen_interp.fits Open
DHT20 (Heithausen) v-l-b FITS cube, interpolated. In each spectrum, <= 2 missing channels are filled by linear interpolation. In each spatial plane, single missing pixels are filled by linear interpolation, first in l direction, then b.
View article: DHT20_Heith_interp.jpg
DHT20_Heith_interp.jpg Open
Sampling map for DHT20 (Heithausen), interpolated
View article: DHT20_UrsaMaj_Heithausen_raw.fits
DHT20_UrsaMaj_Heithausen_raw.fits Open
DHT20 (Heithausen) v-l-b FITS cube, raw
View article: DHT16_Polaris_raw.fits
DHT16_Polaris_raw.fits Open
DHT16 v-l-b FITS cube, raw
View article: DHT19_Camelopardalis_bw_mom.fits
DHT19_Camelopardalis_bw_mom.fits Open
DHT19 v-l-b FITS cube, moment masked. It covers the smaller area with uniform beamwidth sampling.
View article: DHT20_Heith_raw.jpg
DHT20_Heith_raw.jpg Open
Sampling map for DHT20 (Heithausen), raw