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 SGR C BGD 265.7856 -29.8854 264.98542 -29.862996 266.313646 -6.498142 358.90876565 -0.03691694 81.9998 53789.4522106482 2006-02-23 10:51:11 53789.8349421296 2006-02-23 20:02:19 500019010 13.3073 10 13.3153 13.3153 13.3153 13.3073 2 2 2 2 1 0 0 12.2404 12.2404 33.0639 0 PROCESSED 57533.050462963 2016-05-25 01:12:40 54247 2007-05-27 00:00:00 54041.3629166667 2006-11-02 08:42:36 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001079 We propose 100 ksec observation of the Sgr C cloud in the Galactic center region. The cloud emits strong 6.4-keV line, and is a candidate of X-ray reflection nebula; the molecular cloud which emits fluorescence and scattered X-rays irradiated by an external X-ray source. The past activity of Sgr~A$^*$, the Galactic nucleus, may be the origin of 6.4-keV line. We will study 6.4-keV line and verify the X-ray reflection scenario. The second objective is to study the distribution of high ionized and neutral iron lines in the GC region. Chandra observation indicates that H-like iron line is very strong in this region. With the higher energy resolution of XIS, we can confirm the Chandra results. High energy diffuse emission above 10 keV is also a important target by HXD. GALACTIC DIFFUSE EMISSION 5 A HIROSHI MURAKAMI JAP 0 SWG FOSSILS OF THE GALACTIC CENTER ACTIVITY XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/500019010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '500019010'

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