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 | 3C 59 VICINITY 2 | 31.4351 | 28.9234 | 30.715452 | 28.684984 | 39.296603 | 15.198203 | 141.95387958 | -31.18906496 | 250.3 | 55952.5116435185 | 2012-01-26 12:16:46 | 55957.4238773148 | 2012-01-31 10:10:23 | 506025010 | 173.347 | 50 | 173.347 | 173.355 | 0 | 173.355 | 3 | 2 | 0 | 2 | 1 | 0 | 0 | 0.5479 | 0.5479 | 86.854 | 0 | PROCESSED | 57604.5146759259 | 2016-08-04 12:21:08 | 56526 | 2013-08-22 00:00:00 | 56167.6426388889 | 2012-08-28 15:25:24 | 3.0.22.44 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 060067 | We propose for an observation of the vicinities of 3C 59, in order to study the radial extent of the Galactic hot gas. We have conducted joint analysis of absorption and emission lines toward several targets until now and successfully constrained the temperature, line-of-sight length, and density of the hot gas of the directions. However, all the line-of-sight lengths of the hot gas for the past surveys stay within the Galactic disc with the radius of 10 kpc, therefore the radial extent of the gas is still unknown. Emission analysis of low-latitude and almost anti-center directed 3C 59 will constrain the extent, and the result will be unambiguous when emission and absorption lines are jointly analyzed. | GALACTIC DIFFUSE EMISSION | 5 | C | KAZUHIRO SAKAI | JAP | 6 | AO6 | STUDY OF RADIAL DISTRIBUTION OF THE HOT INTERSTELLAR MEDIUM | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/506025010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '506025010'
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