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 M17 275.2076 -16.1829 274.486266 -16.206429 275.030512 7.16685 15.0906551 -0.7606192 110.1996 53805.8263425926 2006-03-11 19:49:56 53808.5349421296 2006-03-14 12:50:19 501003010 102.7021 100 102.7101 102.7101 102.7021 102.7101 2 2 2 2 1 0 0 92.5661 92.5661 233.9678 4 PROCESSED 57533.2492939815 2016-05-25 05:58:59 54394 2007-10-21 00:00:00 53905.822662037 2006-06-19 19:44:38 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 010066 Recent Chandra observations discovered that HII regions possess a few MK extended plasma, but the origin of the emission is still unknown. We propose to observe M17, which has the most spectacular sample of such emission. A superb soft-band response of XIS will enable us to measure the strengths of O and N emission lines, giving us strong arguments to elucidate the cause of the emission. A 300 ks Chandra observation is planned this year in addition to the existing 40 ks data, which will help us to discriminate the point source contribution. GALACTIC DIFFUSE EMISSION 5 A MASAHIRO TSUJIMOTO JAP 1 AO1 XIS INVESTIGATION FOR THE ORIGIN OF DIFFUSE X-RAY EMISSION IN GALACTIC H II REGIONS XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/501003010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '501003010'

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