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 (L,B)=(0.107,-1.425) 267.8602 -29.5833 267.06157 -29.570962 268.118883 -6.156195 0.10035042 -1.42140103 68.0986 55261.1636226852 2010-03-06 03:55:37 55263.893275463 2010-03-08 21:26:19 504050010 100.3991 100 100.4311 100.3991 0 100.4231 2 2 0 2 1 0 0 80.536 80.536 235.8218 1 PROCESSED 57550.8323726852 2016-06-11 19:58:37 55645 2011-03-25 00:00:00 55278.4832523148 2010-03-23 11:35:53 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 040109 In order to resolve origin of the Galactic bulge/ridge emission, we propose to observe the blank field 1.5 deg from the Galactic center where Chandra recently performed the deepest exposure (900 ksec) aiming to resolve the Galactic "diffuse" emission into point sources. Goals of the present observation are the following: (1) Resolve the three iron emission lines (6.41 keV, 6.67 keV and 6.97 keV) with Suzaku, and compare with the point source population determined by Chandra to clarify what kinds of sources are responsible for which emission line. (2) Study Galactic latitudinal variation of the three emission lines comparing with the existent Suzaku observation at (l,b)=(0.0, -2.0). (3) Constrain the hard-tail emission above 10 keV, and study its Galactic latitudinal variation. GALACTIC DIFFUSE EMISSION 5 B KEN EBISAWA JAP 4 AO4 RESOLVING ORIGIN OF THE IRON EMISSION LINES FROM THE GALACTIC BULGE XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/504050010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '504050010'

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