DARTS/Astro Query System - SQL Search -
All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".
total 1
No. |
object_name
|
center_ra
|
center_dec
|
center_ra_b1950
|
center_dec_b1950
|
center_ecliptic_lon
|
center_ecliptic_lat
|
center_galactic_lon
|
center_galactic_lat
|
roll_angle
|
observation_start_time_mjd
|
observation_start_time
|
observation_end_time_mjd
|
observation_end_time
|
observation_id
|
exposure
|
awarded_exposure
|
xis0_exposure
|
xis1_exposure
|
xis2_exposure
|
xis3_exposure
|
xis0_observation_mode
|
xis1_observation_mode
|
xis2_observation_mode
|
xis3_observation_mode
|
hxd_observation_mode
|
hxd_coarse_clock_rate_exposure
|
hxd_first_clock_rate_exposure
|
hxd_normal_clock_rate_exposure
|
hxd_all_clock_rate_exposure
|
hxd_wam_exposure
|
quantity_of_hxd_burst
|
processing_status
|
processing_date_mjd
|
processing_date
|
public_date_mjd
|
public_date
|
distribution_date_mjd
|
distribution_date
|
processing_version
|
processing_count
|
processing_software
|
proposal_id
|
proposal_abstract
|
proposal_category
|
proposal_category_code
|
proposal_priority
|
pi_name
|
co_pi_name
|
proposal_affiliated_country
|
proposal_cycle
|
observation_type
|
proposal_title
|
main_instrument
|
has_xis_injection
|
data_access_url
|
ql_access_url
|
ql_image_url
|
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1 | PKS 0558-504 VIC 2 | 88.9376 | -50.5474 | 88.635341 | -50.553317 | 87.569877 | -73.980493 | 257.96524127 | -29.21937587 | 349.9999 | 56822.2473148148 | 2014-06-14 05:56:08 | 56824.093900463 | 2014-06-16 02:15:13 | 809035010 | 60.1523 | 60 | 60.1523 | 62.1728 | 0 | 62.1888 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 56.7476 | 56.7476 | 159.5318 | 2 | PROCESSED | 57615.2572800926 | 2016-08-15 06:10:29 | 57204 | 2015-07-01 00:00:00 | 56835.7714236111 | 2014-06-27 18:30:51 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 090086 | We have conducted joint analysis of absorption and emission lines toward several targets and successfully constrained temperatures, extents, and densities of the hot gas for each directions. The results are all consistent and indicate the disk-like hot gas with its height of a few kpc from the Galactic plane. However, other research group claimed that the hot gas extends to > 100 kpc and can be a reservoir of the missing baryon. We propose for an observation of the vicinities of PKS 0558-504 in order to limit an extent of the hot gas surrounding our Galaxy and to clinch an argument that the hot gas can be a huge reservoir of the missing baryon. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | B | KAZUHIRO SAKAI | JAP | 9 | AO9 | IS GALACTIC HOT GAS REALLY A HUGE RESERVOIR FOR THE MISSING BARYON? | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/809035010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '809035010'
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