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.
observation_id
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
exposure
awarded_exposure
xtend_exposure
xtend_number_modes
xtend_dataclass_file1
xtend_dataclass_file2
xtend_window1_exposure
xtend_window2_exposure
xtend_window1_burst_exposure
xtend_window2_burst_exposure
xtend_code
gen_code
processing_status
processing_date
public_date
distribution_date
processing_version
caldb_version
processing_software
proposal_id
proposal_abstract
proposal_category
proposal_category_code
proposal_priority
pi_name
co_pi_name
proposal_affiliated_country
proposal_cycle
proposal_type
proposal_title
observation_status
data_access_url
ql_access_url
ql_image_url
corner1_ra
corner1_dec
corner2_ra
corner2_dec
corner3_ra
corner3_dec
corner4_ra
corner4_dec
corner1_ra_b1950
corner1_dec_b1950
corner2_ra_b1950
corner2_dec_b1950
corner3_ra_b1950
corner3_dec_b1950
corner4_ra_b1950
corner4_dec_b1950
corner1_ecliptic_lon
corner1_ecliptic_lat
corner2_ecliptic_lon
corner2_ecliptic_lat
corner3_ecliptic_lon
corner3_ecliptic_lat
corner4_ecliptic_lon
corner4_ecliptic_lat
corner1_galactic_lon
corner1_galactic_lat
corner2_galactic_lon
corner2_galactic_lat
corner3_galactic_lon
corner3_galactic_lat
corner4_galactic_lon
corner4_galactic_lat
xtend_data_mode1
xtend_data_mode2
1 201004010 GAMMA_CASSIOPEIAE 14.1806 60.71741 13.42216 60.44712 43.93378 48.81447 123.57851 -2.14771 223.95285 60721.16741 2025-02-15 04:01:04 60722.46185 2025-02-16 11:05:04 59.292 40.000 55.337 2 31100010 320000A0 59.191 55.337 0.000 0.000 11110 11310 PROCESSED 2025-03-20 15:58:57 2026-02-26 00:00:00 2025-02-23 12:27:17 03.00.013.010 gen20241115_xtd20241115_rsl20241115 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000013002 Binary evolution is one of the most fundamental ingredients in astronomy. Binaries consisting of a high-mass star and a compact object constitute an important milestone in the evolution. Gamma Cas and its analogs could be the long-sought missing population of Be/WD binaries, though an alternative scenario exists. The two scenarios (a) Be/WD binary and (b) magnetic disk-star interaction on Be star surface differ most distinctively in the production site of the hard X-rays. We propose two straightforward and fully independent tests with Resolve to distinguish (a) and (b); the test 1 is the RV change of Fe lines as a function of the orbital phase. The test 2 is the line profile of the flurescent Fe Ka lines. Based on our PV experience, the two tests are only possible with Resolve. ACCRETING WHITE DWARFS AND NOVAE 2 A MASAHIRO TSUJIMOTO SEAN GUNDERSON JUS 1 NOR SOLVING THE LONG-STANDING MYSTERY OF GAMMA CASSIOPEIAE WITH RESOLVE archived https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201004010/ Quick Look 14.2089 60.1831 15.11304 60.63996 14.17049 61.08801 13.26629 60.62418 13.45274 59.91285 14.34723 60.37078 13.41034 60.81771 12.5159 60.35287 43.47989 48.37225 44.42727 48.48553 44.25934 49.11727 43.2992 49.00235 123.60358 -2.6816 124.03743 -2.21244 123.56601 -1.77728 123.13163 -2.24694 WINDOW2 WINDOW1

Used SQL

SELECT * FROM xrism_xtend_data WHERE observation_id = '201004010'

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