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 DIFFUSE1B 201.171 8.6653 200.545653 8.925438 196.184358 16.273856 327.54408522 69.93225444 119.3004 57014.7841898148 2014-12-23 18:49:14 57015.2196759259 2014-12-24 05:16:20 509059010 20.7335 20 20.7335 20.7415 0 20.7335 2 2 0 2 0 0 0 0 0 0 0 PROCESSED 57617.558275463 2016-08-17 13:23:55 57475 2016-03-28 00:00:00 57107.4265162037 2015-03-26 10:14:11 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 091324 In the course of a program to fit spatial models to the Galactic hot gas content, we discovered a few fields that were highly discrepant in the strength of their O VII and/or O VIII line strengths. These are rare emission regions, occurring in fewer than 1% of the fields and they are not due to known extended emission regions (SNR, galaxy clusters, etc.). These emission anomalies probably signify locations of unusual physics, such as shocks, conductive heating, or local heat injection. We propose observations to determine the angular extent of these unusual regions and to better define the intensities of the O VII and O VIII lines. These observations will help identify the relevant physical process and the nature of the phenomenon causing them. GALACTIC DIFFUSE EMISSION 5 C JOEL BREGMAN USA 9 AO9 UNIDENTIFIED BRIGHT X-RAY BACKGROUND REGIONS XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/509059010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '509059010'

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