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 HOLMBERG II X-1 124.8874 70.7162 123.586257 70.872801 106.845907 49.308193 144.27230635 32.72696637 127.9069 56552.1954398148 2013-09-17 04:41:26 56553.2994212963 2013-09-18 07:11:10 708015010 52.19 50 52.19 52.19 0 52.19 2 2 0 2 1 0 0 48.9852 48.9852 95.376 0 PROCESSED 57612.6731481482 2016-08-12 16:09:20 56954 2014-10-24 00:00:00 56588.6670717593 2013-10-23 16:00:35 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 081251 Recent X-ray observations have produced evidence that a subset of the most extreme ultra-luminous X-ray sources (ULXs) are either intermediate-mass black holes or stellar-mass binaries in an unusual super-Eddington state. Current data are unable to deliver a clear answer, as attempts to model the 0.5-10keV spectra have been plagued by degeneracies resulting from the limited bandpass, owing to the previous lack of focusing hard X-ray telescopes. Combined, Suzaku and NuSTAR will obtain high-quality spectra covering 0.5-30keV, providing powerful probes for understanding the accretion modes and nature of the central BHs. A definitive statement on the existence of either 100-1000Msun black holes or extreme accretion states will be an important legacy of both missions. EXTRAGALACTIC COMPACT SOURCES 7 A DOMINIC WALTON USA 8 AO8 COORDINATED SUZAKU AND NUSTAR OBSERVATIONS OF HOLMBERG II X-1 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/708015010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '708015010'

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