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 VICINITY OF LMC X-3 83.4844 -63.8863 83.408578 -63.918105 41.435206 -86.187449 273.3865557 -32.64248934 284.6189 53811.6008333333 2006-03-17 14:25:12 53813.9168055556 2006-03-19 22:00:12 500031010 82.0185 80 82.0265 82.0185 82.0265 82.0265 2 2 2 2 1 0 0 74.6148 74.6148 200.0639 2 PROCESSED 57533.2849537037 2016-05-25 06:50:20 54247 2007-05-27 00:00:00 54056.4806828704 2006-11-17 11:32:11 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000043 We propose to observe the vicnity of LMC X-3 for 80 ks. We expectt to determine the OVII and OVIII emission line intensities within 20% errors. Combining these results with the OVII and OVIII absorption lines observed in the energy spectra of LMC X-3 with Chandra LETG-HRC, we can determine the geometrocal extent od the hot gas along the line-of-sight direction. This will answer the long-unanswered question; from where the high lattitude OVII/OVIII emissions come ? GALACTIC DIFFUSE EMISSION 5 A SWG JAP 0 SWG VICINITY OF LMC X-3 XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/500031010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '500031010'

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