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
1 LOW_LATITUDE_86-21 332.3169 30.2173 331.751825 29.971433 347.602182 38.425077 86.0039952 -20.78963339 82.7457 54229.0809259259 2007-05-09 01:56:32 54230.9966898148 2007-05-10 23:55:14 502047010 81.5486 80 81.5486 81.5486 0 81.5486 2 2 0 2 1 0 0 72.2931 72.2931 165.5099 2 PROCESSED 57538.6557986111 2016-05-30 15:44:21 54744 2008-10-05 00:00:00 54244.7948032407 2007-05-24 19:04:31 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 020061 High galactic-latitude Suzaku observations of soft X-ray diffuse emission so far made show general tendency that the OVII emission line becomes stronger with decreasing abs(b). This suggests that the major part of the emission is originating from the halo of our galaxy. However, we cannot rule out the possibility that the data is contaminated by solar wind charge exchange emission from the entire heliosphere. In oder to confirm the abs(b) dependency and to constrain the spatial distribution of the halo emission, we propose to observe diffuse radiation at a low galactic latitude of abs(b) ~ 20 deg, where the galactic absorption still does not affect the line intensity significantly. GALACTIC DIFFUSE EMISSION 5 B TOMOTAKA YOSHINO JAP 2 AO2 SOFT X-RAY DIFFUSE EMISSION AT A LOW GALACTIC LATITUDE XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/502047010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '502047010'

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