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
|
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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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