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 CAR-D1 162.0244 -59.5887 161.531362 -59.324189 202.52434 -58.576902 287.89332648 -0.36746291 282.973 53891.5567361111 2006-06-05 13:21:42 53892.6343055556 2006-06-06 15:13:24 501099010 76.9074 75 76.924 76.932 76.9314 76.9074 2 2 2 2 1 0 0 64.2576 64.2576 93.0899 0 PROCESSED 57534.5127430556 2016-05-26 12:18:21 54401 2007-10-28 00:00:00 53926.947974537 2006-07-10 22:45:05 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 011257 Soft X-ray emission nebulae with kT =0.1-0.8 keV, log Lx =33-35 ergs/s, and the size of 1-1000 pc accompany a number of giant HII region, but the origin is not understood yet. The Carinae Nebula is 10-100 times more luminous than any other giant HII region in our Galaxy in soft X-rays. From an XMM-Newton observation of the eastern tip of the nebula called Car-D1, we found marginal CVI, CV and OVII lines. If it is real, the carbon abundance should be more than >6 solar, and the OVII line requires more than 2-temperature components. To detect those emission lines clearly and address the origin and environment of the diffuse plasma, we propose a Suzaku observation of the Car-D1 region, optimized for the XIS BI chip. GALACTIC DIFFUSE EMISSION 5 B KENJI HAMAGUCHI USA 1 AO1 ORIGIN OF THE DIFFUSE X-RAY EMISSION AROUND THE CARINA NEBULA, A MASSIVE STAR FORMING REGION XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/501099010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '501099010'

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