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 | (L,B)=(0.25,-0.27) | 266.8068 | -28.8823 | 266.012807 | -28.864862 | 267.181973 | -5.472426 | 0.22878525 | -0.27253682 | 265.3343 | 54343.5232986111 | 2007-08-31 12:33:33 | 54346.7919560185 | 2007-09-03 19:00:25 | 502022010 | 134.7904 | 133 | 134.7984 | 134.8064 | 0 | 134.7904 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 116.8425 | 116.8425 | 282.3759 | 1 | PROCESSED | 57539.9810185185 | 2016-05-31 23:32:40 | 54724 | 2008-09-15 00:00:00 | 54356.5238657407 | 2007-09-13 12:34:22 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 020044 | The Suzaku PV observations found that the diffuse X-rays (6.7 and 6.9 keV-lines) from the GC region can well be explained by a thermal emission from hot plasma with kT=6-7keV (GCDX). The comparison of Suzaku and VLA 90cm images show a hit for special correlation, suggest a magnetic confinement of GCDX. Thus, in order to search for new SNRs and investigate the galactic latitude dependency of the GCDX, we make a GC observation with the aiming point of (l,b)=(0.25, -0.27). We also see the correlation of GCDX with the radio. | GALACTIC DIFFUSE EMISSION | 5 | B | TAKESHI TSURU | JAP | 2 | AO2 | GLOBAL STRUCTURES OF THE GALACTIC CENTER DIFFUSE X-RAY PLASMA (GCDX) | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/502022010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '502022010'
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