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 GALACTIC PLANE 111 347.9369 61.9538 347.407091 61.681886 29.574403 58.088255 111.50111702 1.31488521 81.8498 53892.6499652778 2006-06-06 15:35:57 53893.680775463 2006-06-07 16:20:19 501100010 72.1409 75 72.1649 72.1649 72.1649 72.1409 2 2 2 2 1 0 0 61.025 61.025 89.0349 1 PROCESSED 57534.5221064815 2016-05-26 12:31:50 54401 2007-10-28 00:00:00 53927.3325115741 2006-07-11 07:58:49 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 011258 We propose to observe the line of sight towards (l,b)=(111.5,1.3). This line of sight was observed by XMM because the line of sight is particularly simple, allowing the isolation of the spectrum of the Local Hot Bubble (LHB). The XMM observation did not isolate the LHB, but did reveal the existance of a cool (kT~0.18 keV) X-ray emitting component between 200 and 2000 pcs away that was morphologically unidentifiable in the ROSAT All-Sky Survey. This component may represent the gas responsible for the 3/4 keV "infill problem", and may represent a previously overlooked high filling factor component of the hot ISM. Suzaku observations along this line of sight, coupled with the Suzaku observation towards MBM12, will allow the isolation of this component. GALACTIC DIFFUSE EMISSION 5 B K. KUNTZ USA 1 AO1 BEYOND THE LOCAL HOT BUBBLE TOWARDS L=111 XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/501100010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '501100010'

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