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 ULXs in NGC 1313 49.5245 -66.5352 49.373425 -66.716272 341.380796 -74.178462 283.41323765 -44.63106544 172.6337 53658.556400463 2005-10-15 13:21:13 53659.6252777778 2005-10-16 15:00:24 100032010 32.878 40 32.878 32.878 32.878 32.878 1 1 1 1 1 0 0 30.38 30.38 92.3439 1 PROCESSED 57527.587349537 2016-05-19 14:05:47 54247 2007-05-27 00:00:00 54036.1929398148 2006-10-28 04:37:50 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000032 We propose Suzaku observation of a nearby (4.5 Mpc) galaxy NGC 1313 hosting two prototypical ULXs. These ASCA specta of many ULXs were described with a "high temperature diskbb" model, spectra obtained with XMM (and Chandra) prefer a "power-law plus low-temperature disk" modeling. The superior 5-10 keV sensitivity of Suzaku allows us to examine whether the spectra of luminous ULXs indeed exhibit a turn-over around 5 keV or extend up to 10 keV. CALIBRATION 1 A SWG JAP 0 SWG ULXs in NGC 1313 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100032010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '100032010'

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