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 | HOLMBERG II X-1 | 124.8826 | 70.7169 | 123.581394 | 70.873481 | 106.843254 | 49.308296 | 144.27185866 | 32.72527495 | 119.959 | 56562.4955555556 | 2013-09-27 11:53:36 | 56563.5730324074 | 2013-09-28 13:45:10 | 708015020 | 49.283 | 50 | 49.283 | 49.283 | 0 | 49.283 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 48.206 | 48.206 | 93.0879 | 0 | PROCESSED | 57612.7832986111 | 2016-08-12 18:47:57 | 56954 | 2014-10-24 00:00:00 | 56588.5225462963 | 2013-10-23 12:32:28 | 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/ver3.0/708015020/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '708015020'
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