“HI巡天”的版本间差异
跳到导航
跳到搜索
| （未显示同一用户的7个中间版本） | |||
| 第1行： | 第1行： | ||
== |
==Blind Survey== |
||
===HIPASS=== |
|||
*The HI Parkes All-Sky Survey (HIPASS) covered 30000 deg2 and produced a final catalog of around 5000 HI detections with a median redshift of 2800 km/s. |
*The HI Parkes All-Sky Survey (HIPASS) covered 30000 deg2 and produced a final catalog of around 5000 HI detections with a median redshift of 2800 km/s. |
||
==ALFALFA== |
===ALFALFA=== |
||
*Arecibo Legacy Fast ALFA Survey (ALFALFA) will map 7000 deg2 and is expected to detect more than 25,000 extragalactic HI line sources out to redshifts of 18,000 km/s. |
*Arecibo Legacy Fast ALFA Survey (ALFALFA) will map 7000 deg2 and is expected to detect more than 25,000 extragalactic HI line sources out to redshifts of 18,000 km/s. |
||
:*the spatial resolution of the grid to 4.3'x3.8' |
|||
:*spectral velocity resolution is 11 km/s after smoothing is applied, |
|||
* Catalog [https://arxiv.org/abs/2011.02588] |
|||
* data webpage [http://egg.astro.cornell.edu/alfalfa/data/index.php] |
|||
*发现了一下Ha dots [[https://arxiv.org/abs/2112.02135] |
|||
== |
==Galaxy== |
||
===AGES=== |
|||
*Arecibo Galaxy Environment Survey (AGES), will cover a total area of 200 deg2 (divided into 13 predesignated regions to sample different environments) to greater depth |
*Arecibo Galaxy Environment Survey (AGES), will cover a total area of 200 deg2 (divided into 13 predesignated regions to sample different environments) to greater depth |
||
== |
===THINGS=== |
||
*The H I Nearby Galaxy Survey (THINGS)," a high spectral (≤5.2 km s–1) and spatial (~6) resolution survey of H I emission in 34 nearby galaxies obtained using the NRAO Very Large Array (VLA). |
|||
*GALEX Arecibo SDSS Survey (GASS), a sample of ~1000 galaxies (randomly selected within the footprint of SDSS spectroscopy, ALFALFA, and [[GALEX]] medium imaging survey) with stellar mass greater than 1010 Msun and gas mass fractions as low as 1.5%. |
|||
*public data [http://www.mpia.de/THINGS/Data.html] |
|||
===COLD GASS=== |
|||
*CO legacy Database for GASS |
|||
===NIBLES=== |
|||
*3666 galaxies randomly from GASS to form COLD GASS |
|||
*Nançay Interstellar Baryons Legacy Extragalactic Survey (NanCay Radio Telescop 100m) |
|||
#Must have both SDSS magnitudes and optical spectrum; |
|||
#Must lie within the [[local volume]] (900<cz<12,000 km s−1); |
|||
#Uniform sampling of each 0.5 magnitude wide bin in absolute z-band magnitude, Mz; |
|||
#Preferentially observe nearby objects; |
|||
#No a priori selection on color. |
|||
*这种on source的观测比ALFALFA这种盲测的好更高信噪比，但是还是有一些星系用了Arecibo做了follow up的定点观测，灵敏度更高，可以到mJy以下，(可以探测Lr < 10^8.5的蓝星系)。参见[http://arxiv.org/abs/1609.06242] |
|||
2021年12月12日 (日) 14:00的最新版本
Blind Survey
HIPASS
- The HI Parkes All-Sky Survey (HIPASS) covered 30000 deg2 and produced a final catalog of around 5000 HI detections with a median redshift of 2800 km/s.
ALFALFA
- Arecibo Legacy Fast ALFA Survey (ALFALFA) will map 7000 deg2 and is expected to detect more than 25,000 extragalactic HI line sources out to redshifts of 18,000 km/s.
- the spatial resolution of the grid to 4.3'x3.8'
- spectral velocity resolution is 11 km/s after smoothing is applied,
Galaxy
AGES
- Arecibo Galaxy Environment Survey (AGES), will cover a total area of 200 deg2 (divided into 13 predesignated regions to sample different environments) to greater depth
THINGS
- The H I Nearby Galaxy Survey (THINGS)," a high spectral (≤5.2 km s–1) and spatial (~6) resolution survey of H I emission in 34 nearby galaxies obtained using the NRAO Very Large Array (VLA).
- public data [4]
NIBLES
- Nançay Interstellar Baryons Legacy Extragalactic Survey (NanCay Radio Telescop 100m)
- Must have both SDSS magnitudes and optical spectrum;
- Must lie within the local volume (900<cz<12,000 km s−1);
- Uniform sampling of each 0.5 magnitude wide bin in absolute z-band magnitude, Mz;
- Preferentially observe nearby objects;
- No a priori selection on color.
- 这种on source的观测比ALFALFA这种盲测的好更高信噪比，但是还是有一些星系用了Arecibo做了follow up的定点观测，灵敏度更高，可以到mJy以下，(可以探测Lr < 10^8.5的蓝星系)。参见[5]